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Picosecond-resolved entanglement distribution over an urban free-space channel
Authors:
Alessandro Laneve,
Fabrizio Cienzo,
Santiago Gomez,
Paolo Barigelli,
Philip Menz,
Mattia Beccaceci,
Giuseppe Ronco,
Giorgia Grossi,
Ievgen Brytavskyi,
Thomas Oberleitner,
Markus Wiener,
Christian Weidinger,
Tobias M. Krieger,
Ailton Garcia Jr.,
Saimon Filipe Covre da Silva,
Michele B. Rota,
Nicolò Spagnolo,
Henning Weier,
Fabio Sciarrino,
Armando Rastelli,
Rinaldo Trotta
Abstract:
Time-evolving entangled states describe quantum particles whose correlations evolve in time according to a well-defined dynamics. Such states can be generated in a variety of physical systems and are promising resources for several quantum technologies, ranging from quantum clock synchronization to quantum communication. However, their full potential is currently limited by the fact that the entan…
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Time-evolving entangled states describe quantum particles whose correlations evolve in time according to a well-defined dynamics. Such states can be generated in a variety of physical systems and are promising resources for several quantum technologies, ranging from quantum clock synchronization to quantum communication. However, their full potential is currently limited by the fact that the entanglement dynamics often occur on timescales comparable to the achievable synchronization precision, especially in experiments aimed at distributing entanglement through noisy urban channels. In this context, accurate timing is not merely a technical detail, but a fundamental requirement for faithfully observing and exploiting the underlying quantum correlations. Here, we demonstrate the faithful distribution of a fast-evolving entangled state over a 270 m free-space channel connecting two buildings in the center of Rome. The developed system incorporates a synchronization device capable of achieving sub-50 ps timing accuracy between the two ends of the link while simultaneously supporting channel stabilization. Our results demonstrate that time-evolving entanglement can be reliably transmitted through a noisy urban free-space channel, representing an important benchmark toward long-distance free-space quantum communication and the future implementation of time-correlated entangled states in demanding scenarios such as satellite-based quantum networks.
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Submitted 23 July, 2026;
originally announced July 2026.
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Dark Matter Sensitivity of the CYGNO Detector with HFO-1234ze Enhanced Gas Mixtures
Authors:
F. D. Amaro,
R. Antonietti,
E. Baracchini,
L. Benussi,
F. M. Brunbauer,
C. Capoccia,
M. Caponero,
L. G. M. de Carvalho,
G. Cavoto,
I. A. Costa,
A. Croce,
M. D'Astolfo,
G. D'Imperio,
E. Dane',
G. Dho,
E. Di Marco,
J. M. F. dos Santos,
D. Fiorina,
F. Iacoangeli,
Z. Islam,
E. Kemp,
H. P. Lima Jr,
G. Maccarrone,
R. D. P. Mano,
D. J. G. Marques
, et al. (20 additional authors not shown)
Abstract:
The CYGNO collaboration introduces an innovative approach to direct dark matter detection, proposing a high-resolution optical Time Projection Chamber. It operates at atmospheric pressure with a He:CF$_{4}$ (60:40) gas mixture and uses a triple Gas Electron Multiplier stage for signal amplification. A key feature is its optical readout system, which captures the scintillation light produced during…
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The CYGNO collaboration introduces an innovative approach to direct dark matter detection, proposing a high-resolution optical Time Projection Chamber. It operates at atmospheric pressure with a He:CF$_{4}$ (60:40) gas mixture and uses a triple Gas Electron Multiplier stage for signal amplification. A key feature is its optical readout system, which captures the scintillation light produced during the electron avalanche. This setup allows 3D event reconstruction by combining the time profile of the light detected by photomultiplier tubes with high-granularity, pixelated X-Y tracking recorded by a scientific camera. The CYGNO experiment's projected sensitivity to both spin-independent and spin-dependent interactions is competitive in the framework of directional dark matter detectors. However, incorporating a hydrogen-based gas would introduce an even lighter target, further improving the detection potential at low dark matter masses. In this work, we present the performance characterization of one of the CYGNO experiment prototypes, MANGO, operated with the standard gas mixture enriched with varying concentrations of HFO-1234ze, a gas with a promising low global warming potential. The study includes measurements of the detector charge gain and scintillation yield for each configuration. In addition, to evaluate the impact of HFO-1234ze on scintillation light quenching, the secondary scintillation spectrum was collected for each gas mixture tested.
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Submitted 23 July, 2026; v1 submitted 22 July, 2026;
originally announced July 2026.
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High Resolution Optical Methane Linelist from observations of Titan for Cross-Correlation studies
Authors:
Rafael Rianço-Silva,
Pedro Machado,
Clara Sousa Silva,
Sergey Yurchenko,
Giovanna Tinetti
Abstract:
Exoplanet atmosphere characterization heavily relies on molecular spectroscopic data. Despite efforts to obtain comprehensive spectral libraries for the chemical characterization of exoplanet atmospheres, large gaps remain, particularly for larger molecules and higher frequencies at high spectral resolution. One key example is the methane (CH4) optical spectrum. CH4, the simplest hydrocarbon, is a…
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Exoplanet atmosphere characterization heavily relies on molecular spectroscopic data. Despite efforts to obtain comprehensive spectral libraries for the chemical characterization of exoplanet atmospheres, large gaps remain, particularly for larger molecules and higher frequencies at high spectral resolution. One key example is the methane (CH4) optical spectrum. CH4, the simplest hydrocarbon, is a crucial species for exoplanet atmosphere characterization and a possible biosignature. However, until now, high-resolution linelists at optical wavelengths for CH4 have been very challenging to obtain either experimentally or computationally, leaving the high resolution spectrum of CH4 uncharacterised across most of the visible spectrum. This restricts exploration of CH4 absorption in the optical regime, as upcoming instruments such as ELT-ANDES and VLT-RISTRETTO will start probing the atmospheres of ever smaller exoplanets in optical wavelengths. To address this spectroscopic data limitation, we observed Titan's optical spectrum, dominated by CH4 absorption, at the highest spectral resolution to date with VLT-ESPRESSO. From it, we produced an empirical, low-temperature high-resolution (R ~ 190000) linelist of CH4 in optical wavelengths which we present here, with thousands of previously unidentified lines. We employ this CH4 linelist (RRS-2026) to build a template suitable for high resolution cross-correlation spectroscopy (HRCCS) studies, a first for CH4 in optical wavelengths. With this new linelist, we performed the first HRCCS detection of CH4 in the atmospheres of Titan and Jupiter using optical high resolution spectra. This work sets the stage for the search for CH4 in exoplanet atmospheres through HRCCS with current and future ground-based high-resolution optical spectrographs, showcasing how Solar System observations provide useful products for exoplanet research.
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Submitted 11 July, 2026;
originally announced July 2026.
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Detection of scintillation light in noble gases with wavelength-shifting optical fibers
Authors:
S. R. Soleti,
S. Torelli,
G. Martínez-Lema,
H. Almazán,
A. Beck,
A. Castillo,
M. del Barrio-Torregrosa,
P. Dietz,
C. Echeverria,
L. Gurriana,
Y. Ifergan,
I. Israelashvili,
F. Lopez,
F. Monrabal,
E. Oblak,
J. Pelegrin,
J. G. M. Saraiva,
M. Seemann,
L. Arazi,
J. J. Gómez-Cadenas,
V. Álvarez,
I. J. Arnquist,
F. Auria-Luna,
S. Ayet,
Y. Ayyad
, et al. (88 additional authors not shown)
Abstract:
Wavelength-shifting (WLS) techniques enable particle detectors based on noble gases, whose scintillation light is predominantly emitted in the vacuum-ultraviolet. We investigate WLS fibers coated with tetraphenyl butadiene (TPB) for scintillation light detection in gaseous xenon and argon at pressures up to 8.5 bar, motivated by future high-pressure xenon time-projection chambers of the NEXT progr…
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Wavelength-shifting (WLS) techniques enable particle detectors based on noble gases, whose scintillation light is predominantly emitted in the vacuum-ultraviolet. We investigate WLS fibers coated with tetraphenyl butadiene (TPB) for scintillation light detection in gaseous xenon and argon at pressures up to 8.5 bar, motivated by future high-pressure xenon time-projection chambers of the NEXT program. Two detector configurations are studied: an elongated high-pressure vessel with four PTFE panels equipped with WLS fibers read by temperature-stabilized SiPMs, and a compact box-shaped detector operated at 1 bar Xe with WLS fibers read out by PMTs. Both operate with continuous gas purification. The detector response is characterized using cosmic muons and alpha particles from a $^{241}$Am source. With the SiPM setup, we measure a light collection efficiency (LCE) of ${1.18 \pm 0.01~\mathrm{(sta.)}~^{+0.07}_{-0.09}~\mathrm{(sys.)}~\%}$ for xenon and ${1.07 \pm 0.01~\mathrm{(sta.)}~^{+0.06}_{-0.08}~\mathrm{(sys.)}~\%}$ for argon. With PMT readout, we measure a LCE of ${0.45 \pm 0.01~\mathrm{(sta.)} \pm 0.05~\mathrm{(sys.)}~\%}$ in xenon, in agreement with the SiPM result once photon detection efficiency is accounted for. Average scintillation waveforms in xenon and argon are studied to assess the time structure of the emitted light. Cosmic-muon measurements yield a mean energy required to produce a scintillation photon $45\pm7~\mathrm{(sta.)}~^{+4}_{-5}~\mathrm{(sys.)}~\mathrm{eV}$ at 1.5 bar, in agreement with the literature. The results demonstrate that TPB-coated WLS fiber systems can reliably detect scintillation light in high-pressure gaseous noble detectors, with a LCE representing an upper limit for realistic large-scale TPCs, where additional photon losses from materials and fiber attenuation are expected.
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Submitted 6 July, 2026;
originally announced July 2026.
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Automated Vector-Scanning Spectroscopy for Large-Scale Characterization of Single Quantum Emitters
Authors:
William Eshbaugh,
Ashish Chanana,
Edgar Perez,
Junyeob Song,
Craig R. Copeland,
Sulaiman Al Ghadani,
Daniel McBride,
Prasiddha Siwakoti,
Maria Carolina Volpato,
Armando Rastelli,
Saimon Filipe Covre da Silva,
Ignacio Segovia-Dominguez,
Sadhvikas Addamane,
Kartik Srinivasan,
Edward B. Flagg,
Marcelo Davanco
Abstract:
The inherent spatial randomness and broad spectral heterogeneity of epitaxial quantum dots (QDs) -- one of the most mature classes of solid-state quantum emitters -- remains a major obstacle to their scalable deployment in integrated photonic quantum technologies. Overcoming this challenge requires deterministic fabrication strategies capable of precisely aligning nanophotonic structures with high…
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The inherent spatial randomness and broad spectral heterogeneity of epitaxial quantum dots (QDs) -- one of the most mature classes of solid-state quantum emitters -- remains a major obstacle to their scalable deployment in integrated photonic quantum technologies. Overcoming this challenge requires deterministic fabrication strategies capable of precisely aligning nanophotonic structures with high-quality emitters, which in turn demands efficient and automated single-QD characterization. Despite substantial progress in optical measurement techniques, a platform capable of autonomous, data-efficient, and sufficiently versatile characterization of single quantum dots at the chip scale remains lacking. Here, we introduce an automated cryogenic measurement platform that combines wide-field photoluminescence imaging with vector-stage-scanning confocal spectroscopy to enable high-throughput, chip-scale targeted optical characterization of individual QDs. Using this platform, we automatically acquire photoluminescence data from thousands of GaAs/AlGaAs QDs on a single chip. We demonstrate how this extensive dataset enables identification of high-performance emitters for future deterministic device fabrication, while simultaneously revealing statistical trends across the QD ensemble. By uniting data-efficient targeted measurements with scalable automation, our platform establishes a foundation for large-scale quantum photonic integration and the high throughput characterization framework needed to accelerate materials optimization.
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Submitted 26 June, 2026;
originally announced June 2026.
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Low Complexity Kolmogorov-Arnold Network-based DPD for Analog RoF Fronthaul
Authors:
Carlos Daniel Fontes da Silva,
Tianyu Jiang,
Lu Zhang,
Vjaceslavs Bobrovs,
Xianbin Yu,
Xiaodan Pang,
Oskars Ozolins,
Edson Porto da Silva
Abstract:
This paper proposes and demonstrates experimentally for the first time a Kolmogorov-Arnold Network (KAN)-based digital predistortion (DPD) model, named envelope time-delay KAN (ETDKAN), for mitigating nonlinear distortions in analog radio-over-fiber (A-RoF) systems. The ETDKAN model incorporates physical constraints of radio-frequency (RF) nonlinear devices and, through KAN symbolization, achieves…
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This paper proposes and demonstrates experimentally for the first time a Kolmogorov-Arnold Network (KAN)-based digital predistortion (DPD) model, named envelope time-delay KAN (ETDKAN), for mitigating nonlinear distortions in analog radio-over-fiber (A-RoF) systems. The ETDKAN model incorporates physical constraints of radio-frequency (RF) nonlinear devices and, through KAN symbolization, achieves a significant reduction in computational complexity while improving interpretability. The proposed model is numerically implemented and optimized alongside multilayer perceptron (MLP) and memory-polynomial-based DPDs. Results show that the resulting symbolic ETDKAN (symbETDKAN) attains ACLR and EVM performance comparable to neural network-based models, while maintaining a computational complexity close to that of memory polynomials. Experimental validation using an A-RoF system confirms the practical feasibility of the proposed approach, which resulted in a 4-5 dB reduction in ACLR in the analyzed scenario.
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Submitted 25 June, 2026;
originally announced June 2026.
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OSOG: A Differentiable, Physics-Informed Synthetic Data Engine for Micro-Optical Environments
Authors:
Caio Silva
Abstract:
Deep learning in computational microscopy is severely constrained by the scarcity of densely annotated datasets. While synthetic data generation has bridged this gap in macroscopic computer vision, traditional graphics engines rely on geometric ray-tracing, failing to capture the micro-optical phenomena required for microscopy. Conversely, while wave-optics formulations exist, rendering them compu…
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Deep learning in computational microscopy is severely constrained by the scarcity of densely annotated datasets. While synthetic data generation has bridged this gap in macroscopic computer vision, traditional graphics engines rely on geometric ray-tracing, failing to capture the micro-optical phenomena required for microscopy. Conversely, while wave-optics formulations exist, rendering them computationally tractable at the scale required for deep learning remains a massive systems challenge. To address this, we introduce the Optical Synthetic Object Generator (OSOG), a high-performance, fully differentiable forward-modeling engine. Drawing on established physical models of diffraction and phase retardation, OSOG maps continuous Optical Path Difference (OPD) calculations into a highly optimized, PyTorch-native Structure-of-Arrays (SoA) architecture. We validate this computational framework across three axes: First, object detection models (YOLOv11-OBB) trained purely on OSOG-generated data achieve robust zero-shot transfer to real-world highly occluded Lysozyme micrographs. Second, we introduce DiffOSOG, demonstrating that the engine's end-to-end differentiability allows for the exact recovery of continuous optical parameters via curriculum-guided inverse rendering. Finally, OSOG bypasses the $\mathcal{O}(N)$ bottlenecks of sequential ray-tracing, demonstrating sub-linear scaling by synthesizing 40,000 complex wave-optic particles in under 50 milliseconds (\>20 FPS). By providing a fast, scalable, and physically grounded tensor pipeline, OSOG enables true real-time, on-the-fly dataset generation.
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Submitted 19 June, 2026;
originally announced June 2026.
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State estimation of Rayleigh-Bénard convection with reduced-order models
Authors:
Enrique Flores-Montoya,
André F. C. da Silva,
André V. G. Cavalieri
Abstract:
In this work, we develop a state estimation framework for two-dimensional Rayleigh-Bénard (RB) convection that combines a stable Galerkin reduced-order model (ROM) with an extended Kalman filter (EKF). The ROM, constructed from controllability modes of the linearised Boussinesq equations, provides the nonlinear dynamical model for the filter prediction step. Direct numerical simulations (DNS) are…
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In this work, we develop a state estimation framework for two-dimensional Rayleigh-Bénard (RB) convection that combines a stable Galerkin reduced-order model (ROM) with an extended Kalman filter (EKF). The ROM, constructed from controllability modes of the linearised Boussinesq equations, provides the nonlinear dynamical model for the filter prediction step. Direct numerical simulations (DNS) are used to generate synthetic measurements for data assimilation. We assess filter performance across periodic, quasiperiodic, and chaotic regimes, demonstrating that the filter tracks the most energetic modes with high fidelity and achieves time-averaged reconstruction errors below $14\%$ for velocity and $9\%$ for temperature. We apply the ROM-based EKF to a hybrid simulation scenario where the system state is assimilated from coarse PIV-like velocity measurements. It is shown that velocity observations alone suffice to reconstruct the state, including the temperature field. Finally, we exploit the Kalman gain matrix to develop a greedy sensor placement strategy that progressively removes the least informative sensors. The algorithm reveals a clear hierarchy among sensor types and can be used to derive skeletal observation configurations. It also provides guidance on which measurement variables and spatial locations are most informative for state correction. The present framework is general, and may be applied to other quadratic Galerkin ROMs for state estimation.
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Submitted 19 June, 2026; v1 submitted 18 June, 2026;
originally announced June 2026.
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Influence of CeO$_2$MnO$_x$ heterostructure on Hydrogen Peroxide Electrogeneration on Carbon-Based Catalysts
Authors:
Caroline de O. Carrilho,
Juliana M. S. de Jesus,
João Paulo C. Moura,
Dara Silva Santos,
Aline B. Trench,
Caio Machado Fernandes,
Aila O. Santos,
Odivaldo C. Alves,
Júlio C. M. Silva,
Mauro C. dos Santos
Abstract:
The sustainable electrogeneration of hydrogen peroxide (H2O2) via the two-electron oxygen reduction reaction (2e$^-$ ORR) represents a promising alternative to conventional production methods. In this study, CeO2 and CeO2MnOx nanoparticles were synthesized and supported on Vulcan XC-72 carbon at varying loadings (1, 3, and 5%), aiming to assess the lowest metal loading and high H2O2 electrosynthes…
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The sustainable electrogeneration of hydrogen peroxide (H2O2) via the two-electron oxygen reduction reaction (2e$^-$ ORR) represents a promising alternative to conventional production methods. In this study, CeO2 and CeO2MnOx nanoparticles were synthesized and supported on Vulcan XC-72 carbon at varying loadings (1, 3, and 5%), aiming to assess the lowest metal loading and high H2O2 electrosynthesis. Physicochemical characterizations confirmed the successful formation of CeO2 nanowires and the effectiveness of the MnOx surface modification. XRD, TEM, XPS, EPR, and contact angle analyses revealed that CeO2 loading increased surface hydrophilicity through the presence of oxygenated functional groups, thereby favoring electrochemical activity. On the other hand, all CeO2MnOx loadings were statistically equivalent to Vulcan XC-72 in terms of contact angle. Electrochemical evaluations using a rotating ring-disk electrode (RRDE) demonstrated enhanced ORR activity and high H2O2 selectivity for the 1% CeO2MnOx/C and 3% CeO2/C catalysts, achieving up to 90% selectivity and elevated ring currents. The results suggest that low metal loading and surface modification via MnOx improve the balance between active site exposure, oxygen adsorption, and intermediate stabilization, thus favoring the selective 2e$^-$ pathway. These findings support the development of cost-effective, non-noble-metal catalysts for green H2O2 production via electrosynthesis.
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Submitted 9 June, 2026;
originally announced June 2026.
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He-CF4-CH4 ternary mixtures as target gas for the CYGNO directional dark matter experiment
Authors:
F. D. Amaro,
R. Antonietti,
E. Baracchini,
L. Benussi,
C. Capoccia,
M. Caponero,
L. G. M de Carvalho,
G. Cavoto,
I. A. Costa,
A. Croce,
M. D'Astolfo,
G. D'Imperio,
G. Dho,
E. Di Marco,
J. M. F. dos Santos,
D. Fiorina,
F. Iacoangeli,
Z. Islam,
H. P. Lima Jr,
G. Maccarrone,
R. D. P. Mano,
D. J. G. Marques,
L. G. M. de Carvalho,
G. Mazzitelli,
P. Meloni
, et al. (19 additional authors not shown)
Abstract:
The CYGNO collaboration is advancing a high-resolution optical Time Projection Chamber (TPC) for directional dark matter searches and solar neutrino spectroscopy at LNGS. The detector uses a He-40%CF4 gas mixture at atmospheric pressure and a triple-GEM cascade for ionization signal amplification. Scintillation light from GEM electron avalanches is read out using sCMOS cameras, enabling high sensi…
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The CYGNO collaboration is advancing a high-resolution optical Time Projection Chamber (TPC) for directional dark matter searches and solar neutrino spectroscopy at LNGS. The detector uses a He-40%CF4 gas mixture at atmospheric pressure and a triple-GEM cascade for ionization signal amplification. Scintillation light from GEM electron avalanches is read out using sCMOS cameras, enabling high sensitivity to interactions in the few keV range, alongside precise ionization event tracking and particle identification. This study investigates the effects of adding 3-10% methane to the He-40%CF4 mixture. Methane improves the electrical stability of the TPC, allowing for higher GEM voltages before discharge onset, which compensates for its scintillation quenching and leads to enhanced overall scintillation yield. Compared to prior studies performed with isobutane, methane demonstrates a lower quenching effect on visible and UV photons while maintaining good energy resolution. Importantly, the inclusion of methane lowers the dark matter detection threshold by providing a lighter target and extending track lengths of light nuclear recoils, thus enhancing directional discrimination. These results establish methane as a promising additive for optimizing CYGNO's performance in detecting low-mass dark matter candidates.
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Submitted 31 May, 2026;
originally announced June 2026.
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Two-point enstrophy dynamics in homogeneous isotropic turbulence
Authors:
Gabriele Boga,
Carlos B. da Silva,
Sergio Chibbaro,
Andrea Cimarelli
Abstract:
In the present work we investigate the multiscale dynamics of enstrophy in homogeneous isotropic turbulence by exploiting the two-point formalism provided by the Kármán-Howarth-Monin-Hill approach. The study is conducted on direct numerical simulations with a Taylor-based Reynolds number in the range of $140 \lesssim Re_λ \lesssim 400$. The two-point enstrophy budget at scales $r > 10 η$ appears t…
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In the present work we investigate the multiscale dynamics of enstrophy in homogeneous isotropic turbulence by exploiting the two-point formalism provided by the Kármán-Howarth-Monin-Hill approach. The study is conducted on direct numerical simulations with a Taylor-based Reynolds number in the range of $140 \lesssim Re_λ \lesssim 400$. The two-point enstrophy budget at scales $r > 10 η$ appears to be entirely determined by production via vortex stretching, which balances enstrophy destruction, and to be dominated by the diffusive transport at smaller scales, thus preventing the emergence of a range dominated by the inertial transport of enstrophy. The decomposition in longitudinal and transverse contributions also highlights a dual nature of the inertial enstrophy flux. In particular, enstrophy appears to be transferred across scales through a non-trivial combination of direct and reverse interscale transfer. It is shown that the dual nature of this transfer is strictly related to the vortex stretching mechanism, which, in addition to producing enstrophy through vorticity amplification, also transfers longitudinal vorticity towards larger scales (by stretching the vortical elements) and transverse vorticity towards smaller scales (by contracting these vortical elements in the radial direction). The sum of these two contributions results in an overall transfer of enstrophy from large towards small scales. We propose the use of the pressure transport term as a proxy to obtain some information on the dynamics of relevant events of inertial energy and enstrophy transport. The new findings highlight the relevance of inertial compression events in longitudinal energy transport. At the same time, a good correlation between transverse energy transport events and the radial contraction of vortical elements due to vortex stretching mechanisms is also found.
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Submitted 19 May, 2026;
originally announced May 2026.
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Physics in the Public Square: University Extension as a Strategy for Integrating Physics Education and Science Communication
Authors:
Andre A. A. Marinho,
Gisele B. Freitas,
Camila B. C. da Silva
Abstract:
University extension activities play a fundamental role in bridging the gap between academia and society by fostering the socialization of scientific knowledge. This study reports and analyzes an outreach activity conducted in a public space, involving undergraduate students enrolled in Physics I, Physics III, and Physics IV courses within the Physics Teacher Education Program at the State Univers…
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University extension activities play a fundamental role in bridging the gap between academia and society by fostering the socialization of scientific knowledge. This study reports and analyzes an outreach activity conducted in a public space, involving undergraduate students enrolled in Physics I, Physics III, and Physics IV courses within the Physics Teacher Education Program at the State University of the Tocantina Region of Maranhao (UEMASUL). The activity was developed through the design and presentation of didactic experiments using low-cost materials. Its main objectives were to disseminate fundamental physics concepts to the community, stimulate public interest in science, and provide pre-service teachers with a formative experience integrating theory, practice, and social responsibility. Data were collected from questionnaires adminisvelopment of communication skills, and the strengthening of the university's social role, while also fostering scientific curitered to visitors (n = 52). The results indicate that the activity significantly contributed to student learning, the deosity among participants.
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Submitted 18 May, 2026;
originally announced May 2026.
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Electroluminescence Yield Measurements in Xenon Gas with the NEXT-DEMO++ Detector
Authors:
NEXT Collaboration,
J. Renner,
J. D. Villamil,
N. López-March,
K. Mistry,
P. Novella,
A. Simón,
V. Álvarez,
J. M. Benlloch-Rodríguez,
M. Cid,
C. Cortes-Parra,
R. Esteve,
F. Kellerer,
J. Martín-Albo,
A. Martínez,
G. Martínez-Lema,
M. Martínez-Vara,
M. Querol,
P. Saharia,
M. Sorel,
S. Teruel-Pardo,
H. Almazán,
L. Arazi,
I. J. Arnquist,
F. Auria-Luna
, et al. (89 additional authors not shown)
Abstract:
The NEXT-DEMO++ detector, a high-pressure xenon gas time projection chamber serving as a prototype for the NEXT-100 experiment, was used to measure the electroluminescence (EL) yield as a function of reduced electric field ($E/p$) across pressures from 2.0 to 9.4 bar, utilizing the 41.5 keV de-excitation peak of $^{83m}$Kr. These measurements were made to examine the pressure dependence of the slo…
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The NEXT-DEMO++ detector, a high-pressure xenon gas time projection chamber serving as a prototype for the NEXT-100 experiment, was used to measure the electroluminescence (EL) yield as a function of reduced electric field ($E/p$) across pressures from 2.0 to 9.4 bar, utilizing the 41.5 keV de-excitation peak of $^{83m}$Kr. These measurements were made to examine the pressure dependence of the slope of the reduced EL yield $Y/p$, which has shown inconsistencies in the literature. The reduced yield was fitted with a linear model, revealing a modest ($\sim$5%) change in slope, beginning around 5 bar and increasing with pressure up to 9.4 bar.
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Submitted 17 April, 2026;
originally announced April 2026.
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Pushing the Limits of Pulse Shape Discrimination in a Large Liquid Xenon Detector
Authors:
D. S. Akerib,
A. K. Al Musalhi,
F. Alder,
B. J. Almquist,
C. S. Amarasinghe,
A. Ames,
T. J. Anderson,
N. Angelides,
H. M. Araújo,
J. E. Armstrong,
M. Arthurs,
A. Baker,
S. Balashov,
J. Bang,
J. W. Bargemann,
E. E. Barillier,
K. Beattie,
A. Bhatti,
T. P. Biesiadzinski,
H. J. Birch,
E. Bishop,
G. M. Blockinger,
C. A. J. Brew,
P. Brás,
S. Burdin
, et al. (186 additional authors not shown)
Abstract:
The LUX-ZEPLIN (LZ) experiment is a direct-detection dark matter experiment, optimized to search for weakly interacting massive particles (WIMPs) through WIMP-nucleon interactions. The main challenge in dark matter detection is differentiating between WIMP signals and background events. In LZ, the ratio of ionization to scintillation signals (charge-to-light) is the primary method for rejecting el…
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The LUX-ZEPLIN (LZ) experiment is a direct-detection dark matter experiment, optimized to search for weakly interacting massive particles (WIMPs) through WIMP-nucleon interactions. The main challenge in dark matter detection is differentiating between WIMP signals and background events. In LZ, the ratio of ionization to scintillation signals (charge-to-light) is the primary method for rejecting electronic recoil (ER) background. Pulse shape discrimination (PSD) offers a method for additional ER backgrounds rejection in liquid xenon detectors. In this paper, the discrimination power of PSD with the LZ experiment is discussed. To precisely characterize the scintillation pulse shape, an analysis framework is developed to reconstruct the detection time of individual photons. Using LZ calibration data, the photon-timing prompt fraction discriminator is optimized and achieves ER leakage as low as $15\%$. For specific background processes such as $^{124}$Xe double electron capture, the leakage is reduced further to about $5\%$. PSD is combined with charge-to-light to form two-factor discrimination (TFD). The optimized TFD performance is compared with the performance of the charge-to-light method, with the corresponding false positive rate reduced by up to a factor of two for large scintillation pulses. Finally, PSD and TFD are applied to data from LZ's WS2024 run and their performance is summarized.
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Submitted 21 August, 2026; v1 submitted 27 March, 2026;
originally announced March 2026.
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Cascaded Metasurface Interferometer for Multipath Interference with Classical and Quantum Light
Authors:
Rebecca Aschwanden,
Nicolás Claro-Rodríguez,
Ruizhe Zhao,
Patricia Kallert,
Tobias Krieger,
Quirin Buchinger,
Saimon F. Covre da Silva,
Sandra Stroj,
Michele Rota,
Sven Höfling,
Tobias Huber-Loyola,
Armando Rastelli,
Rinaldo Trotta,
Lingling Huang,
Tim Bartley,
Klaus D. Jöns,
Thomas Zentgraf
Abstract:
Beamsplitters represent fundamental components in both classical and quantum optical systems, enabling the distribution of light, as well as the generation of interference, superposition and entanglement. However, optical networks constructed from conventional bulk 2x2-beamsplitters encounter inherent scalability issues, as the number of required beamsplitters scales quadratically with the number…
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Beamsplitters represent fundamental components in both classical and quantum optical systems, enabling the distribution of light, as well as the generation of interference, superposition and entanglement. However, optical networks constructed from conventional bulk 2x2-beamsplitters encounter inherent scalability issues, as the number of required beamsplitters scales quadratically with the number of optical modes for a fully connected network. Metasurfaces offer a promising route to overcome these constraints. By manipulating light at the wavelength scale compact optical components with advanced functionalities can be constructed, which address several modes simultaneously. In this work, we design and experimentally utilize a metasurface as a multiport beamsplitter. Furthermore, we realize a multimode interferometer composed of two cascaded metasurfaces. We characterize the individual and cascaded metasurfaces using classical light, showing controllable splitting ratios through tunable phase relations. We then expand the approach to quantum light, employing single photons to demonstrate second- and third-order photon correlations, as well as single photon interference across multiple spatial paths. These results establish metasurface-based multiport beamsplitters as a scalable and reconfigurable platform bridging classical and quantum photonics.
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Submitted 26 March, 2026;
originally announced March 2026.
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KATRIN Sensitivity to keV Sterile Neutrinos with the TRISTAN Detector Upgrade
Authors:
H. Acharya,
M. Aker,
D. Batzler,
A. Beglarian,
J. Beisenkötter,
M. Biassoni,
B. Bieringer,
Y. Biondi,
B. Bornschein,
L. Bornschein,
M. Böttcher,
M. Carminati,
A. Chatrabhuti,
S. Chilingaryan,
B. A. Daniel,
M. Descher,
D. Díaz Barrero,
P. J. Doe,
O. Dragoun,
G. Drexlin,
E. Ellinger,
R. Engel,
K. Erhardt,
L. Fallböhmer,
A. Felden
, et al. (105 additional authors not shown)
Abstract:
Sterile neutrinos in the keV mass range are a well-motivated extension of the Standard Model and viable dark matter candidates. Their existence can be probed in laboratory experiments, as the admixture of a sterile state would induce a characteristic kink-like distortion in the $β$-decay electron energy spectrum. The KATRIN experiment is designed to measure the effective electron neutrino mass wit…
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Sterile neutrinos in the keV mass range are a well-motivated extension of the Standard Model and viable dark matter candidates. Their existence can be probed in laboratory experiments, as the admixture of a sterile state would induce a characteristic kink-like distortion in the $β$-decay electron energy spectrum. The KATRIN experiment is designed to measure the effective electron neutrino mass with sub-eV sensitivity by analyzing the endpoint region of the tritium $β$-decay spectrum. Following the completion of its neutrino mass program, KATRIN will extend its physics reach to the search for keV-scale sterile neutrinos. This effort will be enabled by the TRISTAN detector, a newly developed silicon drift detector array optimized for differential measurements at high rates and energies well below the endpoint. In this article, we present the projected sensitivity of KATRIN to keV-scale sterile neutrinos using a dedicated simulation framework. With four months of detector livetime, KATRIN has the statistical power to probe mixing amplitudes at the level of $|U_{e4}|^2 \sim 10^{-6}$ for sterile neutrino masses in the (4$-$13) keV range, significantly extending the reach of previous laboratory searches. The major experimental systematic uncertainties investigated in this work reduces the sensitivity by a factor of 10$-$50 over the same mass range.
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Submitted 15 April, 2026; v1 submitted 24 March, 2026;
originally announced March 2026.
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The CYGNO experiment: a gaseous TPC with optical readout for rare events searches
Authors:
F. D. Amaro,
R. Antonietti,
E. Baracchini,
L. Benussi,
C. Capoccia,
M. Caponero,
L. G. M de Carvalho,
G. Cavoto,
I. A. Costa,
A. Croce,
M. D'Astolfo,
G. D'Imperio,
G. Dho,
E. Di Marco,
J. M. F. dos Santos,
D. Fiorina,
F. Iacoangeli,
Z. Islam,
H. P. Lima Jr,
G. Maccarrone,
R. D. P. Mano,
D. J. G. Marques,
G. Mazzitelli,
P. Meloni,
A. Messina
, et al. (17 additional authors not shown)
Abstract:
The CYGNO collaboration is developing a novel strategy for directional Dark Matter searches based on a gaseous Time Projection Chamber (TPC). The detector is optimized for the exploration of light (0.5-50 GeV) WIMPs-like particles and employs a He/CF4 gas mixture at atmospheric pressure, sensitive to both spin-dependent and spin-independent interactions. A key feature of the project is its optical…
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The CYGNO collaboration is developing a novel strategy for directional Dark Matter searches based on a gaseous Time Projection Chamber (TPC). The detector is optimized for the exploration of light (0.5-50 GeV) WIMPs-like particles and employs a He/CF4 gas mixture at atmospheric pressure, sensitive to both spin-dependent and spin-independent interactions. A key feature of the project is its optical readout, which relies on photon detection rather than charge collection. In CYGNO detectors, electrons released by ionizing tracks drift toward an amplification stage of three Gas Electron Multipliers (GEMs). The electron avalanches generate scintillation light that is captured by scientific CMOS (sCMOS) cameras for high-resolution two-dimensional imaging and by Photomultiplier Tubes (PMTs) that provide a precise time profile along the drift direction. This allows a 3D event reconstruction, detailed energy deposition mapping, and effective topology and head-to-tail discrimination. Building on the achievements of the 50 L prototype (LIME), which successfully operated underground at LNGS, the next step is the deployment of a 0.4 m3 demonstrator, CYGNO-04, to be completed in 2026. The demonstrator will validate scalability and confirm the advantages of the proposed technique. Recent results from LIME highlight strong progress in 3D tracking and particle identification. The current status of CYGNO-04 and its role in advancing the program will be presented as well.
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Submitted 23 March, 2026;
originally announced March 2026.
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A Framework for Closed-Loop Robotic Assembly, Alignment and Self-Recovery of Precision Optical Systems
Authors:
Seou Choi,
Sachin Vaidya,
Caio Silva,
Shiekh Zia Uddin,
Sajib Biswas Shuvo,
Shrish Choudhary,
Marin Soljačić
Abstract:
Robotic automation has transformed scientific workflows in domains such as chemistry and materials science, yet free-space optics, which is a high precision domain, remains largely manual. Optical systems impose strict spatial and angular tolerances, and their performance is governed by tightly coupled physical parameters, making generalizable automation particularly challenging. In this work, we…
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Robotic automation has transformed scientific workflows in domains such as chemistry and materials science, yet free-space optics, which is a high precision domain, remains largely manual. Optical systems impose strict spatial and angular tolerances, and their performance is governed by tightly coupled physical parameters, making generalizable automation particularly challenging. In this work, we present a robotics framework for the autonomous construction, alignment, and maintenance of precision optical systems. Our approach integrates hierarchical computer vision systems, optimization routines, and custom-built tools to achieve this functionality. As a representative demonstration, we perform the fully autonomous construction of a tabletop laser cavity from randomly distributed components. The system performs several tasks such as laser beam centering, spatial alignment of multiple beams, resonator alignment, laser mode selection, and self-recovery from induced misalignment and disturbances. By achieving closed-loop autonomy for highly sensitive optical systems, this work establishes a foundation for autonomous optical experiments for applications across technical domains.
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Submitted 22 March, 2026;
originally announced March 2026.
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Upgrade of the Trigger and Data Acquisition System for Continuous Imaging and Multi-Camera Operation in CYGNO
Authors:
F. D. Amaro,
R. Antonietti,
E. Baracchini,
L. Benussi,
C. Capoccia,
M. Caponero,
L. G. M. de Carvalho,
G. Cavoto,
I. A. Costa,
A. Croce,
M. D'Astolfo,
G. D'Imperio,
G. Dho,
E. Di Marco,
J. M. F. dos Santos,
D. Fiorina,
F. Iacoangeli,
Z. Islam,
E. Kemp,
H. P. Lima Jr,
G. Maccarrone,
R. D. P. Mano,
D. J. G. Marques,
G. Mazzitelli,
P. Meloni
, et al. (19 additional authors not shown)
Abstract:
The CYGNO experiment employs an optical readout to image particle interactions in a gaseous Time Projection Chamber (TPC), combining cameras and photomultiplier tubes (PMTs) to achieve high spatial resolution and timing information. This approach enables detailed track reconstruction but poses significant challenges for data acquisition, particularly in view of the next experimental phase, CYGNO-0…
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The CYGNO experiment employs an optical readout to image particle interactions in a gaseous Time Projection Chamber (TPC), combining cameras and photomultiplier tubes (PMTs) to achieve high spatial resolution and timing information. This approach enables detailed track reconstruction but poses significant challenges for data acquisition, particularly in view of the next experimental phase, CYGNO-04, which will operate multiple cameras simultaneously. In this paper, we present an upgrade of the CYGNO Trigger and Data Acquisition (T-DAQ) system, developed starting from the LIME configuration and validated on the MANGO prototype. The upgrade introduces a continuous imaging acquisition mode, substantially reducing the camera dead time, together with an extended trigger time-tagging scheme that provides a robust global time reference for PMT signals. A synchronous multi-camera DAQ architecture is also implemented and tested, enabling coordinated operation of multiple optical sensors without a master camera. The performance of the upgraded system is validated through dedicated tests, demonstrating stable continuous acquisition, reliable time-tagging, and consistent synchronization across multiple cameras. These results establish a solid and scalable foundation for the CYGNO-04 DAQ and represent a key step toward efficient data acquisition in future large-scale optical TPC detectors.
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Submitted 30 April, 2026; v1 submitted 16 March, 2026;
originally announced March 2026.
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First Optical Observation of Negative Ion Drift at Surface Pressure
Authors:
F. D. Amaro,
R. Antonietti,
E. Baracchini,
L. Benussi,
C. Capoccia,
M. Caponero,
L. G. M. de Carvalho,
G. Cavoto,
I. A. Costa,
A. Croce,
M. D'Astolfo,
G. D'Imperio,
G. Dho,
F. Di Giambattista,
E. Di Marco,
J. M. F. dos Santos,
D. Fiorina,
F. Iacoangeli,
Z. Islam,
H. P. Lima Jr.,
G. Maccarrone,
R. D. P. Mano,
D. J. G. Marques,
G. Mazzitelli,
P. Meloni
, et al. (19 additional authors not shown)
Abstract:
We report the first observation of Negative Ion Drift (NID) at surface pressure of $900 \pm 7$ mbar at Laboratori Nazionali del Gran Sasso in a He:CF$_4$:SF$_6$ mixture using an optically read out Time Projection Chamber (TPC) within the CYGNO/INITIUM project. We present the first PMT waveform analysis in the NID regime, interpreting the temporal light pattern through a model that combines track g…
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We report the first observation of Negative Ion Drift (NID) at surface pressure of $900 \pm 7$ mbar at Laboratori Nazionali del Gran Sasso in a He:CF$_4$:SF$_6$ mixture using an optically read out Time Projection Chamber (TPC) within the CYGNO/INITIUM project. We present the first PMT waveform analysis in the NID regime, interpreting the temporal light pattern through a model that combines track geometry and charge transport. The inferred drift velocities correspond to mobilities of O(cm$^2$ V$^{-1}$ s$^{-1}$), consistent with negative ion transport. The observed linear scaling of the time extension mean with drift distance reveals the presence of a faster minority charge carrier population in addition to the dominant SF$_6^-$ species, drifting at a $\sim$25\% higher velocity under external inputs. These results demonstrate multi-species negative ion drift operation at surface pressure in a He:CF$_4$:SF$_6$ mixture and open a concrete path toward large scale, low diffusion optical TPCs for rare event searches.
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Submitted 6 March, 2026;
originally announced March 2026.
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Low-Energy Radon Backgrounds from Electrode Grids in Dual-Phase Xenon TPCs
Authors:
D. S. Akerib,
A. K. Al Musalhi,
F. Alder,
B. J. Almquist,
S. Alsum,
C. S. Amarasinghe,
A. Ames,
T. J. Anderson,
N. Angelides,
H. M. Araújo,
J. E. Armstrong,
M. Arthurs,
X. Bai,
A. Baker,
J. Balajthy,
S. Balashov,
J. Bang,
J. W. Bargemann,
E. E. Barillier,
A. Baxter,
K. Beattie,
T. Benson,
E. P. Bernard,
A. Bernstein,
A. Bhatti
, et al. (242 additional authors not shown)
Abstract:
The dual-phase xenon time projection chamber (TPC) is a powerful technology to detect rare interactions such as scatters of dark matter particles on nuclei. In particular, the built-in gain of ionization signals in a dual-phase TPC makes it sensitive to events in the few-electron regime, as expected from low-mass dark matter interactions. The pursuit of this low-energy sensitivity through ionizati…
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The dual-phase xenon time projection chamber (TPC) is a powerful technology to detect rare interactions such as scatters of dark matter particles on nuclei. In particular, the built-in gain of ionization signals in a dual-phase TPC makes it sensitive to events in the few-electron regime, as expected from low-mass dark matter interactions. The pursuit of this low-energy sensitivity through ionization-only signal detection has so far been hindered by excessive electron backgrounds observed across experiments. Much of this background is attributed to the plate-out of $^{222}$Rn decay chain isotopes on the high voltage electrode grid surfaces that span the full cross section of the TPC. This work presents a first-principle model constructed for this background, the predictions of which are consistent with data from the LZ and LUX experiments. We then discuss mitigation strategies of this background in future dual-phase TPCs and the possibility of applying this grid background model to ionization-only dark matter searches.
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Submitted 24 February, 2026;
originally announced February 2026.
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Production of GEM-like structures for cryogenic applications, using laser-cutting techniques
Authors:
D. Rodas-Rodríguez,
A. F. V. Cortez,
M. Kuźniak,
D. González-Díaz,
P. A. O. C. Silva,
A. Gnat,
G. Nieradka,
T. Sworobowicz,
E. Alario,
C. D. R. Azevedo,
K. T. Floethner,
P. Gasik,
J. Llerena,
C. M. B. Monteiro,
R. Oliveira,
A. Pallas,
D. Tenreiro,
V. Peskov,
J. M. F. dos Santos
Abstract:
A novel concept for electroluminescence (EL) structures was recently proposed. In it, a wavelength-shifting material is deposited inside the holes of GEM-like structures which, after suitable optical treatment of its electrodes, improves the light collection and detection efficiency in noble gas TPCs. This new development directly addresses problems related with the scalability of future dual-phas…
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A novel concept for electroluminescence (EL) structures was recently proposed. In it, a wavelength-shifting material is deposited inside the holes of GEM-like structures which, after suitable optical treatment of its electrodes, improves the light collection and detection efficiency in noble gas TPCs. This new development directly addresses problems related with the scalability of future dual-phase TPCs for rare-event searches, matching (and potentially exceeding) the performance of conventional EL techniques.
We report the newest developments on the production of such structures using laser-based techniques, namely the manufacture of a first batch of the so-called FAT-GEMs. This process allows low-cost and reproducible manufacturing of a high volume of such structures.
In addition to the detailed description of the production, we present a performance assessment in pure argon, at a gas density close to the one expected in LAr conditions. An energy resolution of 23.5$\pm$1~\% (FWHM) at 5.9~keV was obtained, indicating a consistent improvement over previous batch. The optical treatment of the electrode surfaces has been greatly simplified and modestly improved, while charging-up effects arising from the use of laminates eliminated.
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Submitted 3 February, 2026;
originally announced February 2026.
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Trigger Optimization and Event Classification for Dark Matter Searches in the CYGNO Experiment Using Machine Learning
Authors:
F. D. Amaro,
R. Antonietti,
E. Baracchini,
L. Benussi,
C. Capoccia,
M. Caponero,
L. G. M. de Carvalho,
G. Cavoto,
I. A. Costa,
A. Croce,
M. D'Astolfo,
G. D'Imperio,
G. Dho,
E. Di Marco,
J. M. F. dos Santos,
D. Fiorina,
F. Iacoangeli,
Z. Islam,
E. Kemp,
H. P. Lima Jr,
G. Maccarrone,
R. D. P. Mano,
D. J. G. Marques,
G. Mazzitelli,
P. Meloni
, et al. (18 additional authors not shown)
Abstract:
The CYGNO experiment employs an optical-readout Time Projection Chamber (TPC) to search for rare low-energy interactions using finely resolved scintillation images. While the optical readout provides rich topological information, it produces large, sparse megapixel images that challenge real-time triggering, data reduction, and background discrimination.
We summarize two complementary machine-le…
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The CYGNO experiment employs an optical-readout Time Projection Chamber (TPC) to search for rare low-energy interactions using finely resolved scintillation images. While the optical readout provides rich topological information, it produces large, sparse megapixel images that challenge real-time triggering, data reduction, and background discrimination.
We summarize two complementary machine-learning approaches developed within CYGNO. First, we present a fast and fully unsupervised strategy for online data reduction based on reconstruction-based anomaly detection. A convolutional autoencoder trained exclusively on pedestal images (i.e. frames acquired with GEM amplification disabled) learns the detector noise morphology and highlights particle-induced structures through localized reconstruction residuals, from which compact Regions of Interest (ROIs) are extracted. On real prototype data, the selected configuration retains (93.0 +/- 0.2)% of reconstructed signal intensity while discarding (97.8 +/- 0.1)% of the image area, with ~25 ms per-frame inference time on a consumer GPU.
Second, we report a weakly supervised application of the Classification Without Labels (CWoLa) framework to data acquired with an Americium--Beryllium neutron source. Using only mixed AmBe and standard datasets (no event-level labels), a convolutional classifier learns to identify nuclear-recoil-like topologies. The achieved performance approaches the theoretical limit imposed by the mixture composition and isolates a high-score population with compact, approximately circular morphologies consistent with nuclear recoils.
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Submitted 23 March, 2026; v1 submitted 28 January, 2026;
originally announced January 2026.
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Large-scale real-time signal processing in physics experiments: The ALICE TPC FPGA pipeline
Authors:
J. Alme,
T. Alt,
C. Andrei,
V. Anguelov,
H. Appelshäuser,
M. Arslandok,
R. Averbeck,
M. Ball,
G. G. Barnaföldi,
P. Becht,
R. Bellwied,
A. Berdnikova,
B. Blidaru,
L. Boldizsár,
L. Bratrud,
P. Braun-Munzinger,
M. Bregant,
C. L. Britton,
H. Büsching,
H. Caines,
P. Chatzidaki,
P. Christiansen,
T. M. Cormier,
L. Döpper,
R. Ehlers
, et al. (97 additional authors not shown)
Abstract:
For LHC Run 3, the ALICE Time Projection Chamber was upgraded to operate in continuous readout mode. Interaction rates of up to 50 kHz in Pb-Pb collisions require real-time processing of more than 3 TB/s of raw detector data. This requirement is met by a custom FPGA-based processing pipeline that performs the complete front-end data treatment fully in-stream, including common-mode correction, pede…
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For LHC Run 3, the ALICE Time Projection Chamber was upgraded to operate in continuous readout mode. Interaction rates of up to 50 kHz in Pb-Pb collisions require real-time processing of more than 3 TB/s of raw detector data. This requirement is met by a custom FPGA-based processing pipeline that performs the complete front-end data treatment fully in-stream, including common-mode correction, pedestal subtraction, ion-tail filtering, zero suppression, and dense data packing.
A central element of the design is a highly parallel common-mode correction algorithm operating directly on the streaming data. It robustly identifies signal-free readout channels on a time-bin basis and applies pad-dependent scaling to compensate for local variations in capacitive coupling in the GEM readout. In combination with pedestal subtraction and ion-tail filtering, this enables accurate baseline restoration under extreme high-occupancy conditions, preventing signal loss while efficiently suppressing noise prior to zero suppression.
The pipeline operates continuously at the full detector bandwidth and reduces the raw input rate to about 900 GB/s for Pb-Pb collisions at the target interaction rate. Overall, it represents a large-scale FPGA-based real-time signal-processing implementation for high-energy physics detector readout.
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Submitted 17 March, 2026; v1 submitted 22 January, 2026;
originally announced January 2026.
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Simulation of the CYGNO Gaseous TPC Optical Readout
Authors:
F. D. Amaro,
R. Antonietti,
E. Baracchini,
L. Benussi,
S. Bianco,
C. Capoccia,
M. Caponero,
L. G. M de Carvalho,
G. Cavoto,
I. A. Costa,
A. Croce,
M. D'Astolfo,
G. D'Imperio,
G. Dho,
E. Di Marco,
J. M. F. dos Santos,
D. Fiorina,
F. Iacoangeli,
Z. Islam,
E. Kemp,
H. P. Lima Jr,
G. Maccarrone,
R. D. P. Mano,
D. J. G. Marques,
G. Mazzitelli
, et al. (19 additional authors not shown)
Abstract:
Gaseous Time Projection Chambers with Optical Readout are sensitive detectors suitable for 3D measurement of low-energy O(1 keV) particles and are proposed for detecting rare events such as Dark Matter particle interactions. The CYGNO collaboration is developing such a detector with a high spatial and energy resolution, leveraging an innovative optical readout system. A reliable simulation of the…
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Gaseous Time Projection Chambers with Optical Readout are sensitive detectors suitable for 3D measurement of low-energy O(1 keV) particles and are proposed for detecting rare events such as Dark Matter particle interactions. The CYGNO collaboration is developing such a detector with a high spatial and energy resolution, leveraging an innovative optical readout system. A reliable simulation of the detector response is needed to properly assess the physics reach of this technique and to better understand the performance of the detector in the development phase. Such a simulation cannot entirely rely on existing software packages; indeed, none of the available tools is capable of properly and reliably treating the different phenomena occurring in the detector, from the primary interaction in the gas volume throughout the whole detector response model, including charge transport, light production and propagation, and the response of the optical sensors. In this paper, we present a modeling of the detector response tuned on the CYGNO Optical TPC case; a description of the method is reported together with comparisons with experimental data from the LIME prototype to demonstrate the simulation performances.
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Submitted 10 May, 2026; v1 submitted 4 January, 2026;
originally announced January 2026.
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Fast reconstruction-based ROI triggering via anomaly detection in the CYGNO optical TPC
Authors:
F. D. Amaro,
R. Antonietti,
E. Baracchini,
L. Benussi,
C. Capoccia,
M. Caponero,
L. G. M. de Carvalho,
G. Cavoto,
I. A. Costa,
A. Croce,
M. D'Astolfo,
G. D'Imperio,
G. Dho,
E. Di Marco,
J. M. F. dos Santos,
D. Fiorina,
F. Iacoangeli,
Z. Islam,
E. Kemp,
H. P. Lima Jr.,
G. Maccarrone,
R. D. P. Mano,
D. J. G. Marques,
G. Mazzitelli,
P. Meloni
, et al. (19 additional authors not shown)
Abstract:
Optical-readout Time Projection Chambers (TPCs) produce megapixel-scale images whose fine-grained topological information is essential for rare-event searches, but whose size challenges real-time data selection. We present an unsupervised, reconstruction-based anomaly-detection strategy for fast Region-of-Interest (ROI) extraction that operates directly on minimally processed camera frames. A conv…
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Optical-readout Time Projection Chambers (TPCs) produce megapixel-scale images whose fine-grained topological information is essential for rare-event searches, but whose size challenges real-time data selection. We present an unsupervised, reconstruction-based anomaly-detection strategy for fast Region-of-Interest (ROI) extraction that operates directly on minimally processed camera frames. A convolutional autoencoder trained exclusively on pedestal images learns the detector noise morphology without labels, simulation, or fine-grained calibration. Applied to standard data-taking frames, localized reconstruction residuals identify particle-induced structures, from which compact ROIs are extracted via thresholding and spatial clustering. Using real data from the CYGNO optical TPC prototype, we compare two pedestal-trained autoencoder configurations that differ only in their training objective, enabling a controlled study of its impact. The best configuration retains (93.0 +/- 0.2)% of reconstructed signal intensity while discarding (97.8 +/- 0.1)% of the image area, with an inference time of approximately 25 ms per frame on a consumer GPU. The results demonstrate that careful design of the training objective is critical for effective reconstruction-based anomaly detection and that pedestal-trained autoencoders provide a transparent and detector-agnostic baseline for online data reduction in optical TPCs.
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Submitted 8 April, 2026; v1 submitted 30 December, 2025;
originally announced December 2025.
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Gate-controlled analog memcapacitance in LaAlO3/SrTiO3 interface-based devices
Authors:
Soumen Pradhan,
Victor Lopez-Richard,
Igor Ricardo Filgueira e Silva,
Fabian Hartmann,
Ana Luiza Costa Silva,
Leonardo K. Castelano,
Merit Spring,
Silke Kuhn,
Michael Sing,
Ralph Claessen,
Sven Höfling
Abstract:
Current memcapacitor implementations typically demand complex fabrication processes or depend on organic materials exhibiting poor environmental stability and reproducibility. Here, we demonstrate memcapacitor structures utilizing a quasi 2-dimensional electron gas, formed at the crystalline LaAlO3/SrTiO3 heterointerface, as electrodes and SiO2/SrTiO3 as dielectric layer. The observed memcapacitan…
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Current memcapacitor implementations typically demand complex fabrication processes or depend on organic materials exhibiting poor environmental stability and reproducibility. Here, we demonstrate memcapacitor structures utilizing a quasi 2-dimensional electron gas, formed at the crystalline LaAlO3/SrTiO3 heterointerface, as electrodes and SiO2/SrTiO3 as dielectric layer. The observed memcapacitance originates from the charge localization in a lateral floating gate, while an applied gate voltage enables reversible tuning of the device capacitance. Furthermore, preprogrammed or erased gate biases enable controllable shifts of the capacitance hysteresis window toward positive or negative bias, leading to an enlarged capacitance gap at zero bias. A memcapacitor model developed for this system reproduces the main features of the experimental capacitance hysteresis, capturing the effects of charge fluctuations and dielectric frequency modulation within the oxide layer. The demonstrated low-voltage operation and gate tunability of oxide interface-based memcapacitors highlight their potential for power-efficient, capacitor-based neuromorphic and synaptic electronic architectures.
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Submitted 11 December, 2025;
originally announced December 2025.
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All-photonic entanglement swapping with remote quantum dots
Authors:
Mattia Beccaceci,
Giuseppe Ronco,
Fabrizio Cienzo,
Pierpaolo Bassetti,
Alessandro Laneve,
Francesco Basso Basset,
Tobias M. Krieger,
Qurin Buchinger,
Francesco Salusti,
Barbara Souza Damasceno,
Silke Kuhn,
Saimon F. Covre da Silva,
Sandra Stroj,
Klaus D. Jöns,
Sven Höfling,
Tobias Huber-Loyola,
Armando Rastelli,
Michele B. Rota,
Rinaldo Trotta
Abstract:
Entanglement swapping is a protocol that details how to create entanglement between previously uncorrelated particles. Its all-photonic version - mediated by the interference of photon pairs generated by separate quantum systems-finds disparate applications in quantum networks. So far, all-photonic entanglement swapping between remote systems has been implemented only using sources that operate pr…
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Entanglement swapping is a protocol that details how to create entanglement between previously uncorrelated particles. Its all-photonic version - mediated by the interference of photon pairs generated by separate quantum systems-finds disparate applications in quantum networks. So far, all-photonic entanglement swapping between remote systems has been implemented only using sources that operate probabilistically. However, the scaling up of quantum networks requires deterministic quantum emitters that do not suffer from a trade-off between degree of entanglement and photonpair generation rate. Here, we demonstrate all-photonic entanglement swapping using photon-pairs generated by two separate GaAs quantum dots. The emitters are deterministically embedded in hybrid semiconductor-piezoelectric devices that make the entangled-photons from two dissimilar quantum dots nearly identical. Entanglement swapping is demonstrated with a fidelity as high as 0.71(2), more than 10 standard deviations above the classical limit. The experimental data are quantitatively explained by a theoretical model that also suggests how to boost the protocol performances. Our work opens the path to the exploitation of quantum dot entangled-photon sources in quantum repeater networks.
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Submitted 11 December, 2025;
originally announced December 2025.
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In-series Multimode Interference Sensors and Fabry-Perot Interferometers for Enhanced Wavelength Shift Resolving Capabilities
Authors:
João G. M. de Carvalho,
Luiz D. C. Silva,
Flavio A. M. Marques,
Alexandre A. C. Cotta,
Jefferson E. Tsuchida,
Julio C. Ugucioni,
Silésia C. da Silva,
Leomar S. Marques,
Diego C. Fuzatto,
Alexandre Bessa dos Santos,
Cristiano M. B. Cordeiro,
Limin Xiao,
Jonas H. Osório
Abstract:
We report on the development of a refractive index sensor obtained by using a singlemode-multimode-singlemode (SMS) structure and a Fabry-Perot interferometer (FPI) set into an in-series configuration. Due to the self-imaging phenomenon, the SMS structure - formed by splicing a no-core fiber between two singlemode fibers -, provides a broad spectral peak whose central wavelength position is sensit…
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We report on the development of a refractive index sensor obtained by using a singlemode-multimode-singlemode (SMS) structure and a Fabry-Perot interferometer (FPI) set into an in-series configuration. Due to the self-imaging phenomenon, the SMS structure - formed by splicing a no-core fiber between two singlemode fibers -, provides a broad spectral peak whose central wavelength position is sensitive to variations in the refractive index of the medium surrounding the fiber. In turn, thanks to the in-series SMS-FPI configuration, the sensor's reflection spectrum exhibits the SMS spectral signature modulated by FPI fringes. This readily allows for reducing the width of the spectral features monitored during the sensing measurements, thus enhancing the capabilities of adequately resolving the corresponding spectral shifts. The FPIs reported in this investigation have been fabricated by using two different methods, namely by forming an air-gap FPI between the cleaved ends of two singlemode optical fibers, and by casting a polymeric film onto a connectorized fiber end tip. In the first configuration, the distance between the two cleaved fiber ends could be varied to tune the FPI's free spectral range, hence allowing for tailoring the widths of the spectral oscillations to be monitored during the sensing measurements. Alternatively, the second configuration, while avoiding the use of motorized translation stages, provides a more versatile option for applications. Thus, we understand that our work expands the application of multimode interference and FPIs in sensing scenarios, providing new opportunities for probing physical and chemical parameters by exploring their combined response.
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Submitted 6 December, 2025;
originally announced December 2025.
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Characterization of cutting-edge CMOS Active Pixel sensors within the CYGNO Experiment
Authors:
B. D. Almeida,
F. D. Amaro,
R. Antonietti,
E. Baracchini,
L. Benussi,
S. Bianco,
C. Capoccia,
M. Caponero,
L. G. M. de Carvalho,
G. Cavoto,
I. A. Costa,
A. Croce,
M. D'Astolfo,
G. D'Imperio,
E. Dane,
G. Dho,
E. Di Marco,
J. M. F. Dos Santos,
D. Fiorina,
F. Iacoangeli,
Z. Islam,
E. Kemp,
H. P. Lima Jr.,
G. Maccarrone,
R. D. P. Mano
, et al. (21 additional authors not shown)
Abstract:
Time Projection Chambers equipped with Gas Electron Multipliers and optical readout by scientific CMOS cameras are a promising technology for low-energy particle detection, as demonstrated by the CYGNO experiment. To help identify the optimal CYGNO detector configuration, we performed a detailed characterization of two state-of-the-art scientific CMOS sensors, focusing on dark-signal behavior acro…
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Time Projection Chambers equipped with Gas Electron Multipliers and optical readout by scientific CMOS cameras are a promising technology for low-energy particle detection, as demonstrated by the CYGNO experiment. To help identify the optimal CYGNO detector configuration, we performed a detailed characterization of two state-of-the-art scientific CMOS sensors, focusing on dark-signal behavior across different exposure times and on detection sensitivity, assessed using the well-defined X-ray emissions from a 55Fe source, which reproduce the low-light conditions expected in CYGNO.
CYGNO currently employs a very low-noise Hamamatsu sensor, the ORCA-Fusion, for testing and validation of its detection system. Hamamatsu has recently introduced two new sensors that may be of interest for future upgrades. The first is an improved version of the current model, the ORCA-Fusion-BT, featuring a back-illuminated design that reaches a quantum efficiency of up to 95% at 550 nm. The second is a next-generation sensor, the ORCA-Quest. Although its peak quantum efficiency is not as high as that of the Fusion-BT, it offers high sensitivity over a broader spectral range, extending into the ultraviolet region, and provides ultra-low readout noise of 0.27 electrons, about 2.6 times lower than that of the Fusion family.
These two sensors therefore represent a significant opportunity to enhance the performance of scientific experiments, including those conducted by the CYGNO collaboration. This document presents a comprehensive characterization of these sensors to evaluate their relevance for experiments operating in photon-limited environments and their suitability for integration into the CYGNO detector system.
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Submitted 1 December, 2025;
originally announced December 2025.
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A multiresolution weather dataset for the Southwestern South Atlantic (2017-2018)
Authors:
Luan C. V. Silva,
Lívia Sancho,
Mauricio S. Silva,
Elisa Passos,
Larissa F. R. Jacinto,
Rebeca S. Lyra,
Nilton O. Moraes,
Carina S. Bock,
Douglas M. Nehme,
Raquel Toste,
Jacques Honigbaum,
Rodrigo S. Luna,
Carlos H. Beisl,
Patricia M. Silva,
Adriano O. Vasconcelos,
Rian C. Ferreira,
Cédric Eneau,
Fernando A. Rochinha,
Luiz P. F. Assad,
Alvaro L. G. A. Coutinho,
Laura Bahiense,
Alexandre G. Evsukoff
Abstract:
The Southwestern South Atlantic (SWSA) is a key region for climate research and renewable energy assessment, yet high-resolution meteorological data are scarce. We present a multiresolution dataset spanning February 2017--November 2018, combining Weather Research and Forecasting (WRF) simulations with Sentinel-1A/B Synthetic Aperture Radar (SAR) wind fields processed using the CMOD5 model. WRF out…
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The Southwestern South Atlantic (SWSA) is a key region for climate research and renewable energy assessment, yet high-resolution meteorological data are scarce. We present a multiresolution dataset spanning February 2017--November 2018, combining Weather Research and Forecasting (WRF) simulations with Sentinel-1A/B Synthetic Aperture Radar (SAR) wind fields processed using the CMOD5 model. WRF outputs were generated every 30 minutes for three nested domains (9 km, 3 km, 1 km) through 975 short-term simulations. SAR/CMOD5 wind fields are provided at 500 m and 1 km resolution across 104 acquisition dates. Validation shows strong agreement: daily spatial averages of 10 m wind speed yield RMSE and MAE below 3 m/s on over 93% of acquisition days, while more than 91.5% of pixel-level residuals fall within $\pm$3 m/s. In situ measurements from the Itajaí buoy further confirmed the reliability of both sources. The dataset supports regional climate studies, wind energy resource assessment, and machine-learning applications in forecasting and downscaling, with usage examples included to aid practical adoption.
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Submitted 23 November, 2025;
originally announced November 2025.
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Exploring the production of Terbium-161 in the Brazilian Multipurpose Reactor
Authors:
Fernando Cozim Melges,
Jhonatha Ricardo Santos,
Luiz Paulo de Oliveira,
Alexandre Pinho dos Santos Souza,
Carlos Gabriel Santos da Silva,
Iberê Souza Ribeiro Júnior,
Barbara Perez Gonçalves Silva,
Marco Antonio Stanojev Pereira,
Frederico Antonio Genezini
Abstract:
The Brazilian Multipurpose Reactor (RMB) was conceived to meet national needs for radioisotope production, materials irradiation testing, and neutron beam applications. In addition to its 30~MW pool-type reactor, the RMB complex will include additional facilities for radioisotope production and related applications. $^{161}Tb$ is a promising radionuclide for radiopharmaceutical therapy, offering d…
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The Brazilian Multipurpose Reactor (RMB) was conceived to meet national needs for radioisotope production, materials irradiation testing, and neutron beam applications. In addition to its 30~MW pool-type reactor, the RMB complex will include additional facilities for radioisotope production and related applications. $^{161}Tb$ is a promising radionuclide for radiopharmaceutical therapy, offering decay properties similar to $^{177}Lu$ but with additional conversion and Auger electrons that enhance dose delivery to cancer cells. In light of this emerging radioisotope, this study explores the potential production of $^{161}Tb$ in the RMB through neutron irradiation of enriched $Gd_{2}O_{3}$ targets. Monte Carlo (MCNP) simulations provided detailed neutron flux distributions, which were used as input for ORIGEN calculations of isotope buildup. Assuming 10 mg targets enriched to 97.5% in $^{160}Gd$, a 40-day irradiation, and a thermal flux of $2 \cdot 10^{14}$ $n/cm^{2}s$, the results indicate that $^{161}Tb$ activity reaches approximately 4.5 GBq after 14 days ($\approx 450 GBq/g$), in agreement with data from other research reactors. Building on prior studies that demonstrated the RMB's capability to irradiate larger targets, terabecquerel-scale yields appear feasible. These findings highlight the RMB's potential to support domestic production of emerging therapeutic radionuclides such as $^{161}Tb$. The potential for isotopic enrichment of $^{160}Gd$ using the AVLIS method is also discussed.
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Submitted 17 November, 2025;
originally announced November 2025.
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Impacts of bridging nodes on the epidemic activation mechanisms
Authors:
José Carlos M. Silva,
Diogo H. Silva,
Wesley Cota,
Francisco A. Rodrigues,
Silvio C. Ferreira
Abstract:
Bridging nodes, which connect critical components of a network, play an important role in maintaining structural integrity and facilitating communication within the network, representing indirect yet relevant connections. Epidemic triggering mechanisms in networks often involve long-range mutual activation of hubs, mediated by paths composed of low-degree nodes. While low-degree nodes are abundant…
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Bridging nodes, which connect critical components of a network, play an important role in maintaining structural integrity and facilitating communication within the network, representing indirect yet relevant connections. Epidemic triggering mechanisms in networks often involve long-range mutual activation of hubs, mediated by paths composed of low-degree nodes. While low-degree nodes are abundant in networks, their role in bridging central nodes in epidemic activation mechanisms has not been thoroughly analyzed. Starting with a backbone network with a power-law degree distribution, we investigate the role of adding degree-2 bridging nodes that are preferentially attached to hubs. Our findings reveal that bridging nodes can mediate an indirect feedback interaction between hubs that modifies the epidemic localization and activation mechanisms of the epidemic processes with recurrent infections. In particular, the collective activation observed in the presence of waning immunity, which produces a finite epidemic threshold in power-law networks with degree exponent $γ>3$, is altered to a localized activation with a vanishing threshold. Our numerical results are analytically supported by the non-backtracking matrix properties that emerge in the recurrent dynamical message-passing theory.
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Submitted 25 April, 2026; v1 submitted 16 November, 2025;
originally announced November 2025.
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Demonstration of Sub-Percent Energy Resolution in the NEXT-100 Detector
Authors:
NEXT Collaboration,
M. Pérez Maneiro,
M. Martínez-Vara,
S. Torelli,
G. Martínez-Lema,
P. Novella,
J. A. Hernando Morata,
J. J. Gómez-Cadenas,
C. Adams,
H. Almazán,
V. Álvarez,
A. I. Aranburu,
L. Arazi,
I. J. Arnquist,
F. Auria-Luna,
S. Ayet,
Y. Ayyad,
C. D. R. Azevedo,
K. Bailey,
F. Ballester,
J. E. Barcelon,
M. del Barrio-Torregrosa,
A. Bayo,
J. M. Benlloch-Rodríguez,
F. I. G. M. Borges
, et al. (89 additional authors not shown)
Abstract:
NEXT-100 is a high-pressure xenon time projection chamber with electroluminescent amplification, designed to operate with up to approximately 70.5 kg at 13.5 bar. It is the most recent detector developed by the NEXT collaboration to search for the neutrinoless double-beta decay ($ββ0ν$) of Xe-136. The NEXT gas TPC technology offers the best energy resolution near the Q-value of the decay (…
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NEXT-100 is a high-pressure xenon time projection chamber with electroluminescent amplification, designed to operate with up to approximately 70.5 kg at 13.5 bar. It is the most recent detector developed by the NEXT collaboration to search for the neutrinoless double-beta decay ($ββ0ν$) of Xe-136. The NEXT gas TPC technology offers the best energy resolution near the Q-value of the decay ($Q_{ββ}$ = 2458 keV) among xenon detectors, which is set by design to be <1% FWHM. We report here the high-energy calibration of the detector using a Th-228 source, demonstrating linear response and an energy resolution of $(0.90 \pm 0.02)$% FWHM at the Tl-208 photopeak (2615 keV). This performance extrapolates to a resolution at the double-beta decay end-point of $R(Q_{ββ})$ = $(0.93 \pm 0.02)$% FWHM, confirming the detector's capability for precision energy measurement in the search for $ββ0ν$.
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Submitted 12 January, 2026; v1 submitted 4 November, 2025;
originally announced November 2025.
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First results of the NEXT-100 detector using $^{83m}$Kr decays
Authors:
NEXT Collaboration,
G. Martínez-Lema,
C. Hervés Carrete,
S. Torelli,
M. Cid Laso,
P. Vázquez Cabaleiro,
B. Palmeiro,
J. A. Hernando Morata,
J. J. Gómez-Cadenas,
C. Adams,
H. Almazán,
V. Álvarez,
A. I. Aranburu,
L. Arazi,
I. J. Arnquist,
F. Auria-Luna,
S. Ayet,
Y. Ayyad,
C. D. R. Azevedo,
K. Bailey,
F. Ballester,
J. E. Barcelon,
M. del Barrio-Torregrosa,
A. Bayo,
J. M. Benlloch-Rodríguez
, et al. (91 additional authors not shown)
Abstract:
The NEXT collaboration is investigating the double beta decay of $^{136}$Xe using high-pressure gas electroluminescent time projection chambers, which provide excellent energy resolution together with a robust topological signature. Operating at the Laboratorio Subterráneo de Canfranc (LSC) and building on the success of the NEXT-White detector, the NEXT-100 apparatus began commissioning in May 20…
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The NEXT collaboration is investigating the double beta decay of $^{136}$Xe using high-pressure gas electroluminescent time projection chambers, which provide excellent energy resolution together with a robust topological signature. Operating at the Laboratorio Subterráneo de Canfranc (LSC) and building on the success of the NEXT-White detector, the NEXT-100 apparatus began commissioning in May 2024 and started operation with xenon at a pressure of 4 bar in October 2024.
We report here the first results obtained with NEXT-100 using low-energy calibration data from $^{83m}$Kr decays, which allow mapping of the detector response in the active volume and monitoring of its stability over time. After homogenizing the light response, we achieve an energy resolution of 4.37% FWHM at 41.5 keV for $^{83m}$Kr point-like energy deposits contained in a radius of 425 mm. In a fiducial region representing the operating conditions of NEXT-100 at 10 bar we obtain an improved energy resolution of 4.16% FWHM. These results are in good agreement with that obtained in NEXT-White, and an $E^{-1/2}$ extrapolation to $Q_{ββ}$ yields an energy resolution close to 0.5% FWHM, well below the 1% FWHM design target.
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Submitted 8 January, 2026; v1 submitted 3 November, 2025;
originally announced November 2025.
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GEDICorrect: A Scalable Python Tool for Orbit-, Beam-, and Footprint-Level GEDI Geolocation Correction
Authors:
Leonel Corado,
Sérgio Godinho,
Carlos Alberto Silva,
Juan Guerra-Hernández,
Francesco Valérioa,
Teresa Gonçalves,
Pedro Salgueiro
Abstract:
Accurate geolocation is essential for the reliable use of GEDI LiDAR data in footprint-scale applications such as aboveground biomass modeling, data fusion, and ecosystem monitoring. However, residual geolocation errors arising from both systematic biases and random ISS-induced jitter can significantly affect the accuracy of derived vegetation and terrain metrics. The main goal of this study is to…
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Accurate geolocation is essential for the reliable use of GEDI LiDAR data in footprint-scale applications such as aboveground biomass modeling, data fusion, and ecosystem monitoring. However, residual geolocation errors arising from both systematic biases and random ISS-induced jitter can significantly affect the accuracy of derived vegetation and terrain metrics. The main goal of this study is to develop and evaluate a flexible, computationally efficient framework (GEDICorrect) that enables geolocation correction of GEDI data at the orbit, beam, and footprint levels. The framework integrates existing GEDI Simulator modules (gediRat and gediMetrics) and extends their functionality with flexible correction logic, multiple similarity metrics, adaptive footprint clustering, and optimized I/O handling. Using the Kullback--Leibler divergence as the waveform similarity metric, GEDICorrect improved canopy height (RH95) accuracy from $R^2 = 0.61$ (uncorrected) to 0.74 with the orbit-level correction, and up to $R^2 = 0.78$ with the footprint-level correction, reducing RMSE from 2.62~m ($rRMSE = 43.13\%$) to 2.12~m ($rRMSE = 34.97\%$) at the orbit level, and 2.01~m ($rRMSE = 33.05\%$) at the footprint level. Terrain elevation accuracy also improved, decreasing RMSE by 0.34~m relative to uncorrected data and by 0.37~m compared to the GEDI Simulator baseline. In terms of computational efficiency, GEDICorrect achieved a $\sim2.4\times$ speedup over the GEDI Simulator in single-process mode (reducing runtime from $\sim84$~h to $\sim35$~h) and scaled efficiently to 24 cores, completing the same task in $\sim4.3$~h -- an overall $\sim19.5\times$ improvement. GEDICorrect offers a robust and scalable solution for improving GEDI geolocation accuracy while maintaining full compatibility with standard GEDI data products.
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Submitted 31 October, 2025;
originally announced November 2025.
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Characterization of field cage and cathode for low radioactivity operation with the CYGNO experiment
Authors:
F. D. Amaro,
R. Antonietti,
E. Baracchini,
L. Benussi,
S. Bianco,
A. Biondi,
C. Capoccia,
M. Caponero,
L. G. M. de Carvalho,
G. Cavoto,
I. A. Costa,
A. Croce,
M. D'Astolfo,
G. D'Imperio,
E. Danè,
G. Dho,
E. Di Marco,
J. M. F. dos Santos,
D. Fiorina,
F. Iacoangeli,
Z. Islam,
E. Kemp,
H. P. Lima Jr,
G. Maccarrone,
R. D. P. Mano
, et al. (26 additional authors not shown)
Abstract:
Dark matter, which is considered to account for approximately the 27% of the Universe's energy-mass content, remains an open issue in modern particle physics along with its composition. The CYGNO Experiment aims to exploit an innovative approach applied to the direct detection search of low energy nuclear recoils possibly induced by cold particle-like dark matter candidates. CYGNO employs a direct…
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Dark matter, which is considered to account for approximately the 27% of the Universe's energy-mass content, remains an open issue in modern particle physics along with its composition. The CYGNO Experiment aims to exploit an innovative approach applied to the direct detection search of low energy nuclear recoils possibly induced by cold particle-like dark matter candidates. CYGNO employs a directional detector based on a Time Projection Chamber (TPC) filled with a He:CF$_{4}$ gas mixture and equipped with an optical readout. Currently, the CYGNO Collaboration is constructing the detector demonstrator, CYGNO-04, in Hall F at Laboratori Nazionali del Gran Sasso (LNGS). This 0.4 m$^3$ detector has the goal of proving the scalability of the technology and assessing the physics and radiopurity capabilities. Given the low radioactivity requirements, especially in internal components such as field cage and cathode, the reduction of material while keeping the correct electrical behavior is paramount. In this paper, we present the validation of several internal components, mainly focusing on the field cage material and support structure. The tests included geometrical asymmetries in the electric field response, collection efficiency as well as measurement of known physical quantities. A preferred configuration is found with a structure based on Nylon material which supports a PET or Kapton sheet with copper strips deposited on.
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Submitted 28 April, 2026; v1 submitted 27 October, 2025;
originally announced October 2025.
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Exciton and biexciton preparation via coherent swing-up excitation in a GaAs quantum dot embedded in micropillar cavity
Authors:
Claudia Piccinini,
Aleksander Rodek,
Abdulmalik A. Madigawa,
Ailton Garcia Jr.,
Saimon F. Covre da Silva,
Martin A. Jacobsen,
Luca Vannucci,
Gregor Weihs,
Armando Rastelli,
Vikas Remesh,
Niels Gregersen,
Battulga Munkhbat
Abstract:
Coherent control of quantum emitters is essential for scalable quantum photonic technologies. The recently proposed swing-up of quantum emitter (SUPER) scheme allows efficient and coherent preparation of single photons via off-resonant, red-detuned laser pulses, simplifying laser suppression and enhancing photon collection. We present a systematic study of SUPER excitation applied to a single GaAs…
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Coherent control of quantum emitters is essential for scalable quantum photonic technologies. The recently proposed swing-up of quantum emitter (SUPER) scheme allows efficient and coherent preparation of single photons via off-resonant, red-detuned laser pulses, simplifying laser suppression and enhancing photon collection. We present a systematic study of SUPER excitation applied to a single GaAs quantum dot in a low-Q micropillar cavity. We perform a comparison of the key figures of merit against the well-established two-photon excitation (TPE). Despite requiring higher excitation powers, SUPER achieves near-unity population inversion of the exciton state ($\sim$95%) and high single-photon purity ($g^{(2)}=0.03$) comparable to that under TPE, while also exhibiting a shortened decay time ($\sim$200 ps) reducing the time jitter in the exciton population. A polarization-resolved analysis reveals that when both excitation and collection are aligned with one of the exciton dipoles, SUPER results in polarized single-photon emission, exceeding the resonant TPE saturation by a factor of 1.45. Under optimized excitation conditions, we also observe biexciton preparation via a distinct SUPER resonance, confirmed by the appearance of the biexciton emission line, constituting the first experimental demonstration of biexciton preparation using SUPER. These findings are in good agreement with a proposed four-level theoretical model that incorporates the biexciton state. We also report that a slight misalignment of laser polarization induces an additional SUPER resonance that selectively populates the orthogonal exciton dipole, without altering the nominal excitation polarization. This unexpected behavior reveals a new degree of freedom for coherent state preparation. Our findings establish the SUPER scheme as a versatile tool for state-selective exciton and biexciton control.
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Submitted 2 December, 2025; v1 submitted 24 October, 2025;
originally announced October 2025.
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Study of few-electron backgrounds in the LUX-ZEPLIN detector
Authors:
D. S. Akerib,
A. K. Al Musalhi,
F. Alder,
B. J. Almquist,
C. S. Amarasinghe,
A. Ames,
T. J. Anderson,
N. Angelides,
H. M. Araújo,
J. E. Armstrong,
M. Arthurs,
A. Baker,
S. Balashov,
J. Bang,
J. W. Bargemann,
E. E. Barillier,
K. Beattie,
T. Benson,
A. Bhatti,
T. P. Biesiadzinski,
H. J. Birch,
E. Bishop,
G. M. Blockinger,
B. Boxer,
C. A. J. Brew
, et al. (182 additional authors not shown)
Abstract:
The LUX-ZEPLIN (LZ) experiment aims to detect rare interactions between dark matter particles and xenon. Although the detector is designed to be the most sensitive to GeV/$c^2$--TeV/$c^2$ Weakly Interacting Massive Particles (WIMPs), it is also capable of measuring low-energy ionization signals down to a single electron that may be produced by scatters of sub-GeV/$c^2$ dark matter. The major chall…
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The LUX-ZEPLIN (LZ) experiment aims to detect rare interactions between dark matter particles and xenon. Although the detector is designed to be the most sensitive to GeV/$c^2$--TeV/$c^2$ Weakly Interacting Massive Particles (WIMPs), it is also capable of measuring low-energy ionization signals down to a single electron that may be produced by scatters of sub-GeV/$c^2$ dark matter. The major challenge in exploiting this sensitivity is to understand and suppress the ionization background in the few-electron regime. We report a characterization of the delayed electron backgrounds following energy depositions in the LZ detector under different detector conditions. In addition, we quantify the probability for photons to be emitted in coincidence with electron emission from the high voltage grids. We then demonstrate that spontaneous grid electron emission can be identified and rejected with a high efficiency using a coincident photon tag, which provides a tool to improve the sensitivity of future dark matter searches.
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Submitted 18 March, 2026; v1 submitted 7 October, 2025;
originally announced October 2025.
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Chiral Pt(Me-BPCH): Synthesis and theoretical investigation of parity violation sensitivity
Authors:
Eduardus,
J. Wietze J. van Boven,
Charles Silva,
Philip Karageorghis,
D. Scott Bohle,
Benoît Darquié,
Anastasia Borschevsky,
Lukáš F. Pašteka
Abstract:
A complex of platinum and the tetra-coordinate chelating ligand, R,R'-6,6'-dimethyl-N,N'-bis(2'-pyridine-carboxamide)-1-cyclohexane (Me-BPCH) is investigated as a potential candidate for measurement of parity violation (PV) in chiral molecules. The synthesis of Pt(Me-BPCH) is presented alongside computational investigation of PV sensitivity in its vibrational spectrum. Pt(Me-BPCH) is compared to o…
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A complex of platinum and the tetra-coordinate chelating ligand, R,R'-6,6'-dimethyl-N,N'-bis(2'-pyridine-carboxamide)-1-cyclohexane (Me-BPCH) is investigated as a potential candidate for measurement of parity violation (PV) in chiral molecules. The synthesis of Pt(Me-BPCH) is presented alongside computational investigation of PV sensitivity in its vibrational spectrum. Pt(Me-BPCH) is compared to other two derivatives of this complex, Au(Me-BPCH) and Pt(CF$_3$-BPCH) in terms of their PV response and suitability for measurement. We identify the most promising vibrational transitions based on their enhanced PV effects and practical experimental considerations and analyze the relationship between the vibrational structure and the corresponding PV sensitivity for all three molecules.
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Submitted 30 September, 2025;
originally announced September 2025.
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Low-energy nuclear recoil calibration of the LUX-ZEPLIN experiment with a photoneutron source
Authors:
J. Aalbers,
D. S. Akerib,
A. K. Al Musalhi,
F. Alder,
C. S. Amarasinghe,
A. Ames,
T. J. Anderson,
N. Angelides,
H. M. Araújo,
J. E. Armstrong,
M. Arthurs,
A. Baker,
S. Balashov,
J. Bang,
J. W. Bargemann,
E. E. Barillier,
K. Beattie,
T. Benson,
A. Bhatti,
T. P. Biesiadzinski,
H. J. Birch,
E. Bishop,
G. M. Blockinger,
B. Boxer,
C. A. J. Brew
, et al. (185 additional authors not shown)
Abstract:
The LZ experiment is a liquid xenon time-projection chamber (TPC) searching for evidence of particle dark matter interactions. In the simplest assumption of elastic scattering, many dark matter models predict an energy spectrum which rises quasi-exponentially with decreasing energy transfer to a target atom. LZ expects to detect coherent neutrino-nucleus scattering of $^{8}$B solar neutrinos, the…
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The LZ experiment is a liquid xenon time-projection chamber (TPC) searching for evidence of particle dark matter interactions. In the simplest assumption of elastic scattering, many dark matter models predict an energy spectrum which rises quasi-exponentially with decreasing energy transfer to a target atom. LZ expects to detect coherent neutrino-nucleus scattering of $^{8}$B solar neutrinos, the signal from which is very similar to a dark matter particle with mass of about 5.5 GeV/$c^{2}$, which result in typical nuclear recoil energies of $<$5 keV$_{\text{nr}}$. Therefore, it is of crucial importance to calibrate the response of recoiling xenon nuclei to keV-energy recoils. This analysis details the first in situ photoneutron calibration of the LZ detector and probes its response in this energy regime.
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Submitted 18 September, 2025;
originally announced September 2025.
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Flow-dependent tagging of $^{214}$Pb decays in the LZ dark matter detector
Authors:
J. Aalbers,
D. S. Akerib,
A. K. Al Musalhi,
F. Alder,
C. S. Amarasinghe,
A. Ames,
T. J. Anderson,
N. Angelides,
H. M. Araújo,
J. E. Armstrong,
M. Arthurs,
A. Baker,
S. Balashov,
J. Bang,
J. W. Bargemann,
E. E. Barillier,
K. Beattie,
T. Benson,
A. Bhatti,
T. P. Biesiadzinski,
H. J. Birch,
E. Bishop,
G. M. Blockinger,
B. Boxer,
C. A. J. Brew
, et al. (183 additional authors not shown)
Abstract:
The LUX-ZEPLIN (LZ) experiment is searching for dark matter interactions in a liquid xenon time projection chamber (LXe-TPC). This article demonstrates how control of the flow state in the LXe-TPC enables the identification of pairs of sequential alpha-decays, which are used to map fluid flow and ion drift in the liquid target. The resulting transport model is used to tag \UChPb~ beta-decays, a le…
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The LUX-ZEPLIN (LZ) experiment is searching for dark matter interactions in a liquid xenon time projection chamber (LXe-TPC). This article demonstrates how control of the flow state in the LXe-TPC enables the identification of pairs of sequential alpha-decays, which are used to map fluid flow and ion drift in the liquid target. The resulting transport model is used to tag \UChPb~ beta-decays, a leading background to dark matter signals in LZ. Temporally evolving volume selections, at a cost of 9.0\% of exposure, target the decay of each \UChPb~ atom up to 81 minutes after production, resulting in (63~$\pm$~6$_{(\mathrm{stat})}$~$\pm$~7$_{(\mathrm{sys})}$)\% identification of \UChPb~decays to ground state. We also demonstrate how flow-based tagging techniques enable a novel calibration side band that is concurrent with science data. Finally we report updated estimates of radon-chain charge branching fractions in liquid xenon, finding branching to $^{218}$Po$^+$ at $0.49 \pm 0.01$, $^{214}$Pb$^+$ at $0.48 \pm 0.12$, and $^{214}$Bi$^+$ at $0.74 \pm 0.05$, with a mean charged ion lifetime in the LZ TPC of $49 \pm 4$ min.
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Submitted 19 August, 2026; v1 submitted 26 August, 2025;
originally announced August 2025.
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Estimation of nanometer-thickness layer of 6B graphite: an experimental activity to study Ohm's law in higher education
Authors:
Paulo Henrique Eleuterio Falsetti,
André Coelho da Silva,
Leonardo Geraldino da Silva,
Douglas Mendes da Silva Del Duque,
Murilo Antonio Menegati,
Bruno Fernando Gianelli,
Vagner Romito de Mendonça,
Idelma Aparecida Alves Terra
Abstract:
Ohm's law is crucial for understanding electrical circuits and conductive materials. Formulated by Georg Simon Ohm in the 19th century, it describes the direct proportional relationship between electric voltage and electric current in ohmic conductors. Despite its apparent simplicity, the literature has pointed out that students at different educational levels have difficulty understanding it, esp…
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Ohm's law is crucial for understanding electrical circuits and conductive materials. Formulated by Georg Simon Ohm in the 19th century, it describes the direct proportional relationship between electric voltage and electric current in ohmic conductors. Despite its apparent simplicity, the literature has pointed out that students at different educational levels have difficulty understanding it, especially due to the abstraction associated with the concepts of electric voltage, electric current, and electrical resistance. In order to provide possibilities to overcome this abstraction and the associated learning difficulties, the present work proposes an experimental activity that applies Ohm's law to determine the nanometer-scale thickness of 6B graphite traces deposited on tracing paper. The employed methodology is based on measuring physical quantities such as electric voltage, electric current, and length, and on analyzing the collected data. The thickness of the graphite traces determined by this method was also compared with values obtained using a scanning probe microscope (SPM). Based on the proposed methodology, the thickness of the traces was determined to be 456.5(34)~nm, while SPM measurements yielded an average thickness of 440(50)~nm. Thus, the results show good agreement between the measurements within experimental uncertainties, validating the effectiveness of the suggested methodology and indicating that it is a viable proposal for electricity courses in higher education and, with adaptations, even for high school.
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Submitted 11 August, 2025;
originally announced August 2025.
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Low-density InGaAs/AlGaAs Quantum Dots in Droplet-Etched Nanoholes
Authors:
Saimon F. Covre Da Silva,
Ailton J. Garcia Jr,
Maximilian Aigner,
Christian Weidinger,
Tobias M. Krieger,
Gabriel Undeutsch,
Christoph Deneke,
Ishrat Bashir,
Santanu Manna,
Melina Peter,
Ievgen Brytavskyi,
Johannes Aberl,
Armando Rastelli
Abstract:
Over the past two decades, epitaxial semiconductor quantum dots (QDs) have demonstrated very promising properties as sources of single photons and entangled photons on-demand. Among different growth methods, droplet etching epitaxy has allowed the growth of almost strain-free QDs, with low and controllable surface densities, small excitonic fine structure splitting (FSS), and fast radiative decays…
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Over the past two decades, epitaxial semiconductor quantum dots (QDs) have demonstrated very promising properties as sources of single photons and entangled photons on-demand. Among different growth methods, droplet etching epitaxy has allowed the growth of almost strain-free QDs, with low and controllable surface densities, small excitonic fine structure splitting (FSS), and fast radiative decays. Here, we extend the local droplet etching technique to In(Ga)As QDs in AlGaAs, thereby increasing the achievable emission wavelength range beyond that accessible to GaAs/AlGaAs QDs, while benefiting from the aforementioned advantages of this growth method. We observe QD densities of $\sim 0.2\ μ\mathrm{m}^{-2}$, FSS values as small as $3\ μ\mathrm{eV}$, and short radiative lifetimes of $\sim 300\ \mathrm{ps}$, while extending the achievable emission range to $\sim 920\ \mathrm{nm}$ at cryogenic temperatures. We envision these QDs to be particularly suitable for integrated quantum photonics applications.
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Submitted 11 August, 2025;
originally announced August 2025.
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Bayesian network 3D event reconstruction in the Cygno optical TPC for dark matter direct detection
Authors:
Fernando Domingues Amaro,
Rita Antonietti,
Elisabetta Baracchini,
Luigi Benussi,
Stefano Bianco,
Francesco Borra,
Cesidio Capoccia,
Michele Caponero,
Gianluca Cavoto,
Igor Abritta Costa,
Antonio Croce,
Emiliano Dané,
Melba D'Astolfo,
Giorgio Dho,
Flaminia Di Giambattista,
Emanuele Di Marco,
Giulia D'Imperio,
Matteo Folcarelli,
Joaquim Marques Ferreira dos Santos,
Davide Fiorina,
Francesco Iacoangeli,
Zahoor Ul Islam,
Herman Pessoa Lima Júnior,
Ernesto Kemp,
Giovanni Maccarrone
, et al. (28 additional authors not shown)
Abstract:
The CYGNO experiment is developing a high-resolution gaseous Time Projection Chamber with optical readout for directional dark matter searches. The detector uses a helium-tetrafluoromethane (He:CF$_4$ 60:40) gas mixture at atmospheric pressure and a triple Gas Electron Multiplier amplification stage, coupled with a scientific camera for high-resolution 2D imaging and fast photomultipliers for time…
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The CYGNO experiment is developing a high-resolution gaseous Time Projection Chamber with optical readout for directional dark matter searches. The detector uses a helium-tetrafluoromethane (He:CF$_4$ 60:40) gas mixture at atmospheric pressure and a triple Gas Electron Multiplier amplification stage, coupled with a scientific camera for high-resolution 2D imaging and fast photomultipliers for time-resolved scintillation light detection. This setup enables 3D event reconstruction: photomultipliers signals provide depth information, while the camera delivers high-precision transverse resolution. In this work, we present a Bayesian Network-based algorithm designed to reconstruct the events using only the photomultipliers signals, yielding a full 3D description of the particle trajectories. The algorithm models the light collection process probabilistically and estimates spatial and intensity parameters on the Gas Electron Multiplier plane, where light emission occurs. It is implemented within the Bayesian Analysis Toolkit and uses Markov Chain Monte Carlo sampling for posterior inference. Validation using data from the CYGNO LIME prototype shows accurate reconstruction of localized and extended tracks. Results demonstrate that the Bayesian approach enables robust 3D description and, when combined with camera data, further improves the precision of track reconstruction. This methodology represents a significant step forward in directional dark matter detection, enhancing the identification of nuclear recoil tracks with high spatial resolution.
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Submitted 11 November, 2025; v1 submitted 5 June, 2025;
originally announced June 2025.
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The NEXT-100 Detector
Authors:
NEXT Collaboration,
C. Adams,
H. Almazán,
V. Álvarez,
A. I. Aranburu,
L. Arazi,
I. J. Arnquist,
F. Auria-Luna,
S. Ayet,
Y. Ayyad,
C. D. R. Azevedo,
K. Bailey,
F. Ballester,
J. E. Barcelon,
M. del Barrio-Torregrosa,
A. Bayo,
J. M. Benlloch-Rodríguez,
F. I. G. M. Borges,
A. Brodoline,
N. Byrnes,
A. Castillo,
E. Church,
L. Cid,
M. Cid,
X. Cid
, et al. (92 additional authors not shown)
Abstract:
The NEXT collaboration is dedicated to the study of double beta decays of $^{136}$Xe using a high-pressure gas electroluminescent time projection chamber. This advanced technology combines exceptional energy resolution ($\leq 1\%$ FWHM at the $Q_{ββ}$ value of the neutrinoless double beta decay) and powerful topological event discrimination. Building on the achievements of the NEXT-White detector,…
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The NEXT collaboration is dedicated to the study of double beta decays of $^{136}$Xe using a high-pressure gas electroluminescent time projection chamber. This advanced technology combines exceptional energy resolution ($\leq 1\%$ FWHM at the $Q_{ββ}$ value of the neutrinoless double beta decay) and powerful topological event discrimination. Building on the achievements of the NEXT-White detector, the NEXT-100 detector started taking data at the Laboratorio Subterráneo de Canfranc (LSC) in May of 2024. Designed to operate with xenon gas at 13.5 bar, NEXT-100 consists of a time projection chamber where the energy and the spatial pattern of the ionising particles in the detector are precisely retrieved using two sensor planes (one with photo-multiplier tubes and the other with silicon photo-multipliers). The detector has been operating at stable conditions using argon and xenon gases at $\sim$4 bar and drift fields of 74 V/cm and 118 V/cm, respectively. Alpha decays from the $^{222}$Rn chain have been used to test and monitor the stability of the detector, showing a constant electron lifetime in the drift volume. In this paper, in addition to reporting the results of the commissioning run, we provide a detailed description of the NEXT-100 detector, describe its assembly, and present the current estimation of the radiopurity budget.
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Submitted 10 December, 2025; v1 submitted 23 May, 2025;
originally announced May 2025.
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Enhanced ammonia electro-oxidation reaction on platinum-iron oxide catalyst assisted by MagnetoElectroCatalysis
Authors:
Caio Machado Fernandes,
Eduardo M. Rodrigues,
Odivaldo C. Alves,
Flavio Garcia,
Yutao Xing,
Mauro C. Santos,
Julio Cesar M. Silva
Abstract:
Ammonia poses significant environmental challenges due to its role in water pollution, contributing to eutrophication and several detrimental environmental and ecological issues. Addressing the efficient removal or conversion of ammonia is, therefore, critical. Among various methods, the ammonia electro-oxidation reaction stands out due to its potential for direct energy conversion and environment…
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Ammonia poses significant environmental challenges due to its role in water pollution, contributing to eutrophication and several detrimental environmental and ecological issues. Addressing the efficient removal or conversion of ammonia is, therefore, critical. Among various methods, the ammonia electro-oxidation reaction stands out due to its potential for direct energy conversion and environment remediation. Here, we synthesize platinum-iron oxide magnetic nanoparticles (Pt-MNP) as electrocatalysts and apply an alternating magnetic field (AMF) to enhance their activity.. The AMF generates localized heat via Néel relaxation, accelerating ammonia oxidation kinetics at the catalytic surface.. Compared to conventional electro-oxidation methods, this technique demonstrates superior efficiency and stability, offering a promising alternative for ammonia treatment. This work uses the concept of MagnetoElectroCatalysis, showcasing the synergy between magnetic fields and the electrochemical process, leveraging the AMF to induce localized heating within the nanocatalyst, thereby improving its catalytic activity as shown in cyclic voltammetry and chronoamperometry experiments. By combining nanocatalyst design with innovative AMF application, this study provides a new avenue for enhancing electrochemical reactions, with broad implications for environmental remediation and sustainable energy solutions.
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Submitted 19 May, 2025;
originally announced May 2025.
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Magnetic field-enhanced two-electron oxygen reduction reaction using CeMnCo nanoparticles supported on different carbonaceous matrices
Authors:
Caio Machado Fernandes,
Joao Paulo C. Moura,
Aline B. Trench,
Odivaldo C. Alves,
Yutao Xing,
Marcos R. V. Lanza,
Julio Cesar M. Silva,
Mauro C. Santos
Abstract:
The current study illustrates the successful synthesis of Ce$_{1.0}$Mn$_{0.9}$Co$_{0.1}$ nanoparticles, characterized through XRD, EPR, magnetization curves, and TEM/HRTEM/EDX analyses. These nanoparticles were then loaded into the carbon Vulcan XC72 and the carbon Printex L6 matrices in varying amounts (1, 3, 5, and 10% w/w) via wet impregnation method to fabricate electrocatalysts for the 2-elec…
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The current study illustrates the successful synthesis of Ce$_{1.0}$Mn$_{0.9}$Co$_{0.1}$ nanoparticles, characterized through XRD, EPR, magnetization curves, and TEM/HRTEM/EDX analyses. These nanoparticles were then loaded into the carbon Vulcan XC72 and the carbon Printex L6 matrices in varying amounts (1, 3, 5, and 10% w/w) via wet impregnation method to fabricate electrocatalysts for the 2-electron ORR. Before experimentation, the material was characterized via XPS and contact angle measurements. The electrochemical results produced significant findings, indicating that the electrocatalysts with the nanostructures modifying both carbon blacks notably augmented currents in rotating ring-disk electrode measurements, signifying enhanced selectivity for H$_2$O$_2$ production. Moreover, our research underscored the significant impact of Magnetic Field-Enhanced Electrochemistry, employing a constant magnetic field strength of 2000 Oe, on 2-electron ORR experiments. Particularly noteworthy were the observed results surpassing the ones without the magnetic field, demonstrating heightened currents and improved selectivity for H$_2$O$_2$ production (more than 90 %) facilitated by CeMnCo nanoparticles. These significant findings in electrocatalytic efficiency have practical implications, suggesting the potential for developing more efficient and selective catalysts for the 2-electron ORR.
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Submitted 19 May, 2025;
originally announced May 2025.
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Magnetic field-enhanced oxygen reduction reaction for electrochemical hydrogen peroxide production with different cerium oxide nanostructures
Authors:
Caio Machado Fernandes,
Aila O. Santos,
Vanessa S. Antonin,
Joao Paulo C. Moura,
Aline B. Trench,
Odivaldo C. Alves,
Yutao Xing,
Julio Cesar M. Silva,
Mauro C. Santos
Abstract:
We investigated cerium oxide nanoparticles of various morphologies (nanosheets, nanocubes, and nanoparticles) supported on carbon Vulcan XC-72 for the two-electron oxygen reduction reaction (ORR). It was used a continuous magnetic field (2000 Oe) for the first time in the literature. The best results were for 5% (w/w) CeO2 for all three different morphologies, more than doubling the ring current,…
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We investigated cerium oxide nanoparticles of various morphologies (nanosheets, nanocubes, and nanoparticles) supported on carbon Vulcan XC-72 for the two-electron oxygen reduction reaction (ORR). It was used a continuous magnetic field (2000 Oe) for the first time in the literature. The best results were for 5% (w/w) CeO2 for all three different morphologies, more than doubling the ring current, enhancing the hydrogen peroxide selectivity from 51% (Vulcan XC-72) to 84-89%, and modifying the onset potential to lesser negative values. The presence of the magnetic field led to even higher ring currents with 5% (w/w) CeO$_2$, H$_2$O$_2$ selectivity from 54% (Vulcan XC-72) to 88-96% and changing even more the onset potential. Those results were correlated with the Zeeman effect, the Lorentz force, generating magnetohydrodynamic effects, the Kelvin force, and the formation of Bound Magnetic Polarons. This pioneering research introduces an innovative approach, highlighting the potential of an external continuous magnetic field.
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Submitted 19 May, 2025;
originally announced May 2025.
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Modeling the light response of an optically readout GEM based TPC for the CYGNO experiment
Authors:
Fernando Dominques Amaro,
Rita Antonietti,
Elisabetta Baracchini,
Luigi Benussi,
Stefano Bianco,
Roberto Campagnola,
Cesidio Capoccia,
Michele Caponero,
Gianluca Cavoto,
Igor Abritta Costa,
Antonio Croce,
Emiliano Danè,
Melba D'Astolfo,
Giorgio Dho,
Flaminia Di Giambattista,
Emanuele Di Marco,
Giulia D'Imperio,
Joaquim Marques Ferreira dos Santos,
Davide Fiorina,
Francesco Iacoangeli,
Zahoor Ul Islam,
Herman Pessoa Lima Junior,
Ernesto Kemp,
Francesca Lewis,
Giovanni Maccarrone
, et al. (34 additional authors not shown)
Abstract:
The use of gaseous Time Projection Chambers enables the detection and the detailed study of rare events due to particles interactions with the atoms of the gas with energy releases as low as a few keV. Due to this capability, these instruments are being developed for applications in the field of astroparticle physics, such as the study of dark matter and neutrinos. To readout events occurring in t…
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The use of gaseous Time Projection Chambers enables the detection and the detailed study of rare events due to particles interactions with the atoms of the gas with energy releases as low as a few keV. Due to this capability, these instruments are being developed for applications in the field of astroparticle physics, such as the study of dark matter and neutrinos. To readout events occurring in the sensitive volume with a high granularity, the CYGNO collaboration is developing a solution where the light generated during the avalanche processes occurring in a multiplication stage based on Gas Electron Multiplier (GEM) is read out by optical sensors with very high sensitivity and spatial resolution. To achieve a high light output, gas gain values of the order of $10^5\text{-}10^6$ are needed. Experimentally, a dependence of the detector response on the spatial density of the charge collected in the GEM holes has been observed, indicating a gain-reduction effect likely caused by space-charge buildup within the multiplication channels. This paper presents data collected with a prototype featuring a sensitive volume of about two liters, together with a model developed by the collaboration to describe and predict the gain dependence on charge density. A comparison with experimental data shows that the model accurately reproduces the gain behaviour over nearly one order of magnitude, with a percent-level precision.
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Submitted 19 February, 2026; v1 submitted 9 May, 2025;
originally announced May 2025.