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Ontology-Grounded Project Memory for Coding Agents
Authors:
James Adam
Abstract:
Coding agents have become the primary means of generating new code in many software projects, and the resulting velocity of changes makes keeping track of the reasons behind those changes challenging. This paper introduces MOOSEDev, a system designed to give coding agents structured, ontology-grounded project memory. The system captures architectural decisions, lessons, constraints, and rationales…
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Coding agents have become the primary means of generating new code in many software projects, and the resulting velocity of changes makes keeping track of the reasons behind those changes challenging. This paper introduces MOOSEDev, a system designed to give coding agents structured, ontology-grounded project memory. The system captures architectural decisions, lessons, constraints, and rationales in a knowledge graph exposed to agents via a Model Context Protocol (MCP) interface. Records carry lifecycle status, provenance, and supersession links, queryable via MOOSE, a proprietary neurosymbolic engine that treats the symbolic layer as the primary reasoning substrate. We compared MOOSEDev against a production vector-memory tool on a neutral public corpus of 835 typed records. MOOSEDev returned the expected answer set essentially in full (0.98-1.00) on supersession, set-completeness, and negation questions, whereas the baseline's top-k retrieval surfaced between 6% and 27%. Conversely, relevance recall and token cost were largely equivalent between the two systems. We also describe a temporal commit-history bootstrap of our own codebase, a pre-registered live trial, and lessons learned.
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Submitted 13 August, 2026;
originally announced August 2026.
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ePIC Early Science Report
Authors:
D. Abbott,
N. Abdelrahman,
S. Abhijit,
I. Abualrob,
R. B. Achari,
J. Adam,
L. Adamczyk,
K. Adkins,
A. Affolder,
K. Agarwal,
J. Agarwala,
N. Agrawal,
C. A. Aidala,
W. Akers,
A. Al-bataineh,
S. N. Alam,
M. Alekseev,
P. R. Altieri,
J. -S. Alvarado Gallenao,
S. B. L. Amar,
R. Ammendola,
I. Amos Cali,
G. An,
D. Anderson,
E. Anderssen
, et al. (774 additional authors not shown)
Abstract:
This Early Science Report from the ePIC Collaboration outlines the compelling physics program achievable during the first years of operation of the Electron-Ion Collider (EIC), prior to the establishment of the full design luminosity and energy range. The analyses are based on realistic early-running beam configurations and detailed Geant4 ePIC detector simulations, hit digitization and data recon…
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This Early Science Report from the ePIC Collaboration outlines the compelling physics program achievable during the first years of operation of the Electron-Ion Collider (EIC), prior to the establishment of the full design luminosity and energy range. The analyses are based on realistic early-running beam configurations and detailed Geant4 ePIC detector simulations, hit digitization and data reconstruction. The projected studies from the physics working groups of ePIC span inclusive, semi-inclusive, exclusive, diffractive and tagging, as well as jet and heavy flavor measurements in both electron-proton and electron-ion collisions. Even before the collider reaches its full design performance, these measurements will constrain parton distribution functions in nucleons and nuclei, access transverse-momentum-dependent and spin-dependent observables, probe gluon dynamics in nuclei, and initiate a program of imaging of quarks and gluons. Each measurement is directly connected to the core science pillars of the EIC, identified in the 2018 report by the National Academy of Sciences: understanding the origin of the nucleon mass, unraveling the spin structure of the nucleon, and exploring the emergent properties of dense gluonic matter. The results presented here provide examples that demonstrate that the early years of EIC running with ePIC will deliver novel world-leading insights into Quantum Chromodynamics. In addition, the early science program will establish measurement and analysis methodologies that will pave the way to the subsequent full EIC physics program.
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Submitted 5 August, 2026;
originally announced August 2026.
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Spin-wave softening across the uniform-to-stripe domain transition in iron garnet film
Authors:
Titiksha Srivastava,
Victor Leroy,
Nessrine Benaziz,
Nathaniel Findling,
Ludovic Largeau,
Jamal Ben Youssef,
Jean-Paul Adam,
Thibaut Devolder,
Joo-Von Kim
Abstract:
Spin-wave spectra across transitions between uniform and textured phases can offer deep insight into both symmetry-breaking physics and self-assembled magnonic bands. However, experiments require a material platform that combines low damping, well-defined textures, and spectroscopic access. Here, we study a Bi-doped iron-garnet film with perpendicular magnetic anisotropy (PMA), which undergoes a u…
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Spin-wave spectra across transitions between uniform and textured phases can offer deep insight into both symmetry-breaking physics and self-assembled magnonic bands. However, experiments require a material platform that combines low damping, well-defined textures, and spectroscopic access. Here, we study a Bi-doped iron-garnet film with perpendicular magnetic anisotropy (PMA), which undergoes a uniform-to-stripe-domain transition as a function of in-plane magnetic field. Real-space imaging by magnetic force microscopy reveals field-reorientable stripe domains aligned with the in-plane field, while reciprocal-space measurements using thermal microfocused Brillouin light scattering ($μ$-BLS) reveal the softening of a low-frequency spin-wave branch near the transition and the appearance of additional modes in the stripe-domain state. Calculated dispersion relations identify finite-$k$ softening in the Damon-Eshbach geometry ($k \perp M$), with the corresponding wavelength matching the stripe periodicity at the transition. In addition, a $μ$-BLS spectral model reproduces the measured mode frequencies and relative intensities at selected fixed fields. Micromagnetic simulations capture the field-driven formation of the stripe state and reproduce the experimental thermal $μ$-BLS spectra. Our findings establish BiYIG with PMA as a model low-damping platform for studying spin-wave freezing, stripe-domain modes, and reconfigurable magnonic band structures.
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Submitted 22 July, 2026;
originally announced July 2026.
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Kani: A Model Checker for Rust
Authors:
Rémi Delmas,
Zyad Hassan,
Qinheping Hu,
Rahul Kumar,
Felipe R. Monteiro,
Thanh Nguyen,
Adrián Palacios,
Celina Val,
Michael Tautschnig,
Justus Adam,
Daniel Schwartz-Narbonne,
Carolyn Zech
Abstract:
Rust's ownership type system prevents memory errors in safe code, but certain desirable properties remain orthogonal to compilation: the soundness of unsafe operations (e.g., raw pointer dereferences), functional correctness, and absence of runtime panics. We present Kani, an open-source model checker for Rust that pushes bounded model checking beyond bug-finding to provide correctness guarantees…
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Rust's ownership type system prevents memory errors in safe code, but certain desirable properties remain orthogonal to compilation: the soundness of unsafe operations (e.g., raw pointer dereferences), functional correctness, and absence of runtime panics. We present Kani, an open-source model checker for Rust that pushes bounded model checking beyond bug-finding to provide correctness guarantees for these properties. Kani compiles proof harnesses from Rust's Mid-level Intermediate Representation (MIR) into CBMC's bit-precise verification engine, automatically checking a comprehensive set of safety properties with no user annotation. To extend verification from bounded to unbounded, Kani provides a specification language comprising function contracts, loop contracts, quantifiers, and function stubbing. We demonstrate feasibility through case studies on industrial Rust projects, where contracts upgraded verification from panic-freedom to functional correctness, uncovering six previously unknown bugs. Kani operates at scale in production CI, with over 16,000 harnesses verified per code change in the Rust standard library verification campaign.
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Submitted 1 July, 2026;
originally announced July 2026.
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Reprogrammable magnonic logic in a multiferroic heterostructure via magnetoelectric coupling
Authors:
Ping Che,
Amr Abdelsamie,
Ádám Papp,
Sali Salama,
André Thiaville,
Romain Lebrun,
Stéphane Fusil,
Vincent Garcia,
Aymeric Vecchiola,
Karim Bouzehouane,
Manuel Bibes,
Agnès Barthélémy,
Jean-Paul Adam,
Vladislav Demidov,
Paolo Bortolotti,
Abdelmadjid Anane,
Isabella Boventer
Abstract:
The realization of fully reconfigurable, voltage-controlled, and programmable on-chip magnonic devices is essential to fully harness the potential of spin waves for signal processing, logic and neuromorphic computing. Yet, existing demonstrations of electrical tuning of magnonic responses are either volatile, current-driven and thus energy-inefficient, or rely on local strain modification limiting…
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The realization of fully reconfigurable, voltage-controlled, and programmable on-chip magnonic devices is essential to fully harness the potential of spin waves for signal processing, logic and neuromorphic computing. Yet, existing demonstrations of electrical tuning of magnonic responses are either volatile, current-driven and thus energy-inefficient, or rely on local strain modification limiting their scalability for wafer-scale integration. Here, we address this challenge using a BiFeO3/La0.67Sr0.33MnO3 multiferroic thin film heterostructure. We show that ferroelectric domain engineering in BiFeO3 enables deterministic tuning of the magnon dispersion of La0.67Sr0.33MnO3, producing frequency shifts up to $\sim 150 MHz$ and allowing reconfigurable waveguiding. Micro-focused Brillouin light scattering directly images these effects, revealing electrically defined magnonic waveguides and spatially programmable dispersion. Compared to conventional approaches, this method provides non-volatile and reversible control. Furthermore, using an inverse-design simulation code, we demonstrate the capability of our platform to perform advanced magnonic functions such as frequency demultiplexing. Our results open a new avenue for using magnetoelectric heterostructures for magnonic logic, with further applicability to reservoir and neuromorphic computing and AI driven magnonic devices.
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Submitted 16 May, 2026;
originally announced May 2026.
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Control of relaxation properties of a macroscopic nuclear spin ensemble
Authors:
János Ádám,
Andrew J. Winter,
Deniz Aybas,
Dmitry Budker,
Derek F. Jackson Kimball,
Arne Wickenbrock,
Alexander O. Sushkov
Abstract:
Macroscopic spin ensembles in solids are powerful platforms for quantum sensing and precision metrology. A key challenge is controlling the nuclear spin population relaxation time $T_1$, which can become prohibitively long at cryogenic temperatures due to phonon freeze-out. We demonstrate optical control of the $T_1$ relaxation time of the $^{207}$Pb nuclear spin ensemble in lead-containing ferroe…
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Macroscopic spin ensembles in solids are powerful platforms for quantum sensing and precision metrology. A key challenge is controlling the nuclear spin population relaxation time $T_1$, which can become prohibitively long at cryogenic temperatures due to phonon freeze-out. We demonstrate optical control of the $T_1$ relaxation time of the $^{207}$Pb nuclear spin ensemble in lead-containing ferroelectric crystals PbTiO$_3$ (PT) and (PbMg$_{1/3}$Nb$_{2/3}$O$_3$)$_{2/3}$-(PbTiO$_3$)$_{1/3}$ (PMN-PT). Using X-band electron paramagnetic resonance (EPR) spectroscopy at 10 K, we characterize light-induced paramagnetic centers created by 405 nm laser illumination. In PT, we observe paramagnetic Pb$^{3+}$ centers and their hyperfine interaction with nearby nuclear spins. In PMN-PT, we identify two populations: isotropic Pb$^{3+}$ centers and anisotropic Ti$^{3+}$ centers occupying $d$-orbitals, with spin number densities of $(2.5 \pm 1.0) \times 10^{17}$ cm$^{-3}$ and $(4.1 \pm 1.7) \times 10^{17}$ cm$^{-3}$, respectively. Power-dependent EPR measurements enable extraction of spin relaxation times. We investigate the ionization and recombination dynamics of these transient paramagnetic centers. Using saturation-recovery nuclear magnetic resonance, we demonstrate that laser illumination reduces the $^{207}$Pb nuclear $T_1$ by approximately a factor of two, from $(17 \pm 2)$ s to $(7 \pm 1)$ s at 4.6 MHz, and from $(1550 \pm 40)$ s to $(850 \pm 70)$ s at 40 MHz. We develop a model relating the nuclear relaxation rate to the density of photoinduced paramagnetic centers. This optical control of nuclear spin relaxation provides a pathway toward accelerated thermal polarization and dynamic nuclear polarization in solid-state NMR-based precision measurements, including searches for axion-like dark matter.
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Submitted 28 April, 2026;
originally announced April 2026.
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Inclusive jet cross section in $pp$ collisions at $\sqrt{s} = 200$ and $510$ GeV
Authors:
STAR Collaboration,
B. E. Aboona,
J. Adam,
L. Adamczyk,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
A. K. Alshammri,
E. C. Aschenauer,
S. Aslam,
J. Atchison,
V. Bairathi,
X. Bao,
P. Barik,
K. Barish,
S. Behera,
R. Bellwied,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
J. Bielcik,
J. Bielcikova,
J. D. Brandenburg,
C. Broodo
, et al. (379 additional authors not shown)
Abstract:
Jets are collimated clusters of particles formed by the hadronization of partons following a hard interaction. In proton-proton ($pp$) collisions at the Relativistic Heavy Ion Collider (RHIC), jet production is dominated by $gg$ and $qg$ partonic processes, allowing us to directly probe the gluon parton distribution function (PDF) in the proton in a way complementary to deep inelastic scattering.…
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Jets are collimated clusters of particles formed by the hadronization of partons following a hard interaction. In proton-proton ($pp$) collisions at the Relativistic Heavy Ion Collider (RHIC), jet production is dominated by $gg$ and $qg$ partonic processes, allowing us to directly probe the gluon parton distribution function (PDF) in the proton in a way complementary to deep inelastic scattering. In this paper, we report the double-differential inclusive-jet cross sections as a function of jet transverse momentum, $p_{\rm T}$, and pseudorapidity, $η$, at center-of-mass energies $\sqrt{s} = 200$ and $510$~GeV, from $pp$ collisions studied with the STAR detector. The jet $p_{\rm T}$ is corrected for underlying event contributions by applying an off-axis cone method. At mid-pseudorapidity, $|η| < 0.9$, the kinematic coverage of our data extends to $0.07 < x_{\rm T} \text{ (}= 2p_{\rm T}{} / \sqrt{s} \text{)} < 0.5$ and $0.03 < x_{\rm T} < 0.31$ at $\sqrt{s} = 200$~and 510 GeV, respectively, where the gluon PDF is poorly constrained by the TeV-scale $pp$~($p\bar{p}$) colliders. The inclusive jet cross sections are compared to the next-to-next-to-leading order perturbative quantum chromodynamics calculations using several recent PDF sets as inputs. These results will further constrain the gluon PDF, help tune Monte Carlo generators, and provide critical reference data needed to study the quark-gluon plasma.
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Submitted 24 June, 2026; v1 submitted 30 March, 2026;
originally announced March 2026.
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Guidelines for interpreting microfocused Brillouin light scattering spectra
Authors:
Nessrine Benaziz,
Thibaut Devolder,
Stéphane Andrieu,
Jamal Ben Youssef,
Jean-Paul Adam
Abstract:
We present an analysis of the influence of spin wave dispersion relations and profiles on microfocused Brillouin Light Scattering spectra. Three archetypal magnetic materials are reported: a 51-nm thick Bi-substituted YIG, a 25-nm thick Heusler compound and 50-nm thick CoFeB alloy. These samples were chosen because they exhibit strongly contrasting spectral features -peak frequencies, linewidth, s…
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We present an analysis of the influence of spin wave dispersion relations and profiles on microfocused Brillouin Light Scattering spectra. Three archetypal magnetic materials are reported: a 51-nm thick Bi-substituted YIG, a 25-nm thick Heusler compound and 50-nm thick CoFeB alloy. These samples were chosen because they exhibit strongly contrasting spectral features -peak frequencies, linewidth, skewness. The shapes of these spectral features reflect the underlying spin wave dispersion relations and the thickness profile of the related spin wave modes. While analytical expressions of the dispersion relations provide a satisfactory description of the spectra if the modes are in separate frequency domains, the exact dispersion relations and the exact mode profiles are required for a correct description of the spectra not only when mode hybridization is present in the range or near the range of frequencies and wavevector accessed by the experiment. Our examples of microfocused BLS spectra are handy references that can be used as interpretation guidelines for BLS spectra recorded on a broader range of materials.
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Submitted 12 March, 2026;
originally announced March 2026.
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Mitigating crosstalk errors for simultaneous single-qubit gates on a superconducting quantum processor
Authors:
Jaap J. Wesdorp,
Eric Hyyppä,
Joona Andersson,
Janos Adam,
Rohit Beriwal,
Ville Bergholm,
Saga Dahl,
Simone Diego Fasciati,
Alejandro Gomez Friero,
Zheming Gao,
Daria Gusenkova,
Andrew Guthrie,
Johannes Heinsoo,
Tuukka Hiltunen,
Keiran Holland,
Amin Hosseinkhani,
Sinan Inel,
Joni Ikonen,
Shan W. Jolin,
Kristinn Juliusson,
Seung-Goo Kim,
Anton Komlev,
Roope Kokkoniemi,
Otto Koskinen,
Joonas Kylmälä
, et al. (39 additional authors not shown)
Abstract:
Single-qubit gates on superconducting quantum processors are typically implemented using microwave pulses applied through dedicated control lines. However, these microwave pulses may also drive other qubits due to crosstalk arising from capacitive coupling and wavefunction overlap in systems with closely spaced transition frequencies. Crosstalk and frequency crowding increase errors during simulta…
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Single-qubit gates on superconducting quantum processors are typically implemented using microwave pulses applied through dedicated control lines. However, these microwave pulses may also drive other qubits due to crosstalk arising from capacitive coupling and wavefunction overlap in systems with closely spaced transition frequencies. Crosstalk and frequency crowding increase errors during simultaneous single-qubit operations relative to isolated gates, thus forming a major bottleneck for scaling superconducting quantum processors. In this work, we combine model-based qubit frequency optimization with pulse shaping to demonstrate crosstalk error mitigation in single-qubit gates on a 49-qubit superconducting quantum processor. We introduce and experimentally verify an analytical model of simultaneous single-qubit gate error caused by microwave crosstalk that depends on a given pulse shape. By employing a model-based optimization strategy of qubit frequencies, we minimize the crosstalk-induced error across the processor and achieve a mean simultaneous single-qubit gate fidelity of 99.96% for a 16-ns gate duration, approaching the mean individual gate fidelity. To further reduce the simultaneous error and required qubit frequency bandwidth on high-crosstalk qubit pairs, we introduce a crosstalk transition suppression (CTS) pulse shaping technique that minimizes the spectral energy around transitions inducing leakage and crosstalk errors. Finally, we combine CTS with model-based frequency optimization across the device and experimentally show a systematic reduction in the required qubit frequency bandwidth for high-fidelity simultaneous gates, supported by simulations of systems with up to 1000 qubits. By alleviating constraints on qubit frequency bandwidth for parallel single-qubit operations, this work represents an important step for scaling towards larger quantum processors.
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Submitted 11 March, 2026;
originally announced March 2026.
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Probing Late-Stage Hadronic Interactions at High Baryon Density via $K^{*0}$ Production in the RHIC Beam Energy Scan Program
Authors:
STAR Collaboration,
B. E. Aboona,
J. Adam,
G. Agakishiev,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
A. Aitbayev,
I. Alekseev,
E. Alpatov,
A. K. Alshammri,
A. Aparin,
S. Aslam,
J. Atchison,
G. S. Averichev,
V. Bairathi,
X. Bao,
P. Barik,
K. Barish,
S. Behera,
P. Bhagat,
A. Bhasin,
S. Bhatta,
I. G. Bordyuzhin,
J. D. Brandenburg
, et al. (363 additional authors not shown)
Abstract:
A precision measurement of the $K^{*0}$ meson yield is reported in Au+Au collisions at $\sqrt{s_{NN}} = 7.7,\; 11.5,\; 14.6,\; 19.6,$ and $27~\mathrm{GeV}$ using the high-statistics data sample collected by the STAR experiment during the Beam Energy Scan II (BES-II) program at RHIC. The transeverse momentum ($p_{T}$)-integrated yield ratios $(K^{*0} + \overline{K^{*0}})/(K^{+} + K^{-})$ in central…
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A precision measurement of the $K^{*0}$ meson yield is reported in Au+Au collisions at $\sqrt{s_{NN}} = 7.7,\; 11.5,\; 14.6,\; 19.6,$ and $27~\mathrm{GeV}$ using the high-statistics data sample collected by the STAR experiment during the Beam Energy Scan II (BES-II) program at RHIC. The transeverse momentum ($p_{T}$)-integrated yield ratios $(K^{*0} + \overline{K^{*0}})/(K^{+} + K^{-})$ in central collisions show a suppression relative to peripheral collisions at the $(1.7\text{-}3.6)\,σ$ level, while a thermal model without final-stage rescattering overpredicts this ratio with a deviation of $(6.9\text{-}8.2)\,σ$. These results indicate a loss of the measured $K^{*0}$ signal in central collisions due to re-scattering of its hadronic decay products in the hadronic phase. The $p_{T}$-integrated yield of charged kaons exhibits an approximate scaling with charged-particle multiplicity, independent of collision energy and system size. A similar trend is observed for the short-lived $K^{*0}$ resonance, although significant deviations emerge at lower energies. At BES energies, the $K^{*0}/K$ ratio shows stronger suppression than at the highest RHIC and LHC energies within a given multiplicity bin, particularly in central and mid-central collisions. This behavior is consistent with changes in the effective hadronic interaction cross section and is supported by transport model calculations, which indicate dominant meson-baryon interactions at lower energies and meson-meson interactions at higher energies.
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Submitted 28 April, 2026; v1 submitted 21 January, 2026;
originally announced January 2026.
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Multiple three-magnon splittings in bismuth yttrium iron garnet nanostructures
Authors:
Sali Salama,
Joo-Von Kim,
Maryam Massouras,
Jamal Ben Youssef,
Abdelmadjid Anane,
Jean-Paul Adam
Abstract:
We experimentally demonstrate the generation of multiple three-magnon splitting processes in an in-plane magnetized submicron Bi-YIG disk using micro-focused Brillouin light scattering. The low magnetic damping and strong magneto-optical response of BiYIG enable the detection of nonlinear spin-wave interactions at low threshold powers. By tuning the in-plane static magnetic field, excitation frequ…
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We experimentally demonstrate the generation of multiple three-magnon splitting processes in an in-plane magnetized submicron Bi-YIG disk using micro-focused Brillouin light scattering. The low magnetic damping and strong magneto-optical response of BiYIG enable the detection of nonlinear spin-wave interactions at low threshold powers. By tuning the in-plane static magnetic field, excitation frequency, and power, we observe the generation of three pairs of secondary modes symmetrically distributed around half the excitation frequency. Time-resolved BLS measurements present temporal dynamics and threshold behavior associated with the successive activation of three-magnon pairs.
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Submitted 14 January, 2026;
originally announced January 2026.
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Identified charged hadron production in Au+Au collisions at $\sqrt{s_\mathrm{NN}}$ = 54.4 GeV with the STAR detector
Authors:
STAR Collaboration,
B. E. Aboona,
J. Adam,
G. Agakishiev,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
A. Aitbayev,
I. Alekseev,
E. Alpatov,
A. K. Alshammri,
A. Aparin,
S. Aslam,
J. Atchison,
G. S. Averichev,
V. Bairathi,
X. Bao,
P. Barik,
K. Barish,
S. Behera,
P. Bhagat,
A. Bhasin,
S. Bhatta,
I. G. Bordyuzhin,
J. D. Brandenburg
, et al. (363 additional authors not shown)
Abstract:
We present results on the production of $π^{\pm}$, $K^{\pm}$, $p$, and $\bar{p}$ in Au+Au collisions at $\sqrt{s_\mathrm{NN}}$ = 54.4~GeV using the STAR detector at RHIC, at midrapidity ($|y| <$ 0.1). Invariant yields of these particles as a function of transverse momentum are shown. We determine bulk properties such as integrated particle yields ($dN/dy$), mean transverse momentum (…
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We present results on the production of $π^{\pm}$, $K^{\pm}$, $p$, and $\bar{p}$ in Au+Au collisions at $\sqrt{s_\mathrm{NN}}$ = 54.4~GeV using the STAR detector at RHIC, at midrapidity ($|y| <$ 0.1). Invariant yields of these particles as a function of transverse momentum are shown. We determine bulk properties such as integrated particle yields ($dN/dy$), mean transverse momentum ($\langle p_{T} \rangle$), particle ratios, which provide insight into the particle production mechanisms. Additionally, the kinetic freezeout parameters ($T_\text{kin}$ and $\langle β_{T} \rangle$), which provide information about the dynamics of the system at the time of freezeout, are obtained. The Bjorken energy density ($ε_{\rm{BJ}}$), which gives an estimate of the energy density in the central rapidity region of the collision zone at the formation time $τ$, is calculated and presented as a function of multiplicity for various energies. The results are compared with those from the models such as A Multi-Phase Transport (AMPT) and Heavy Ion Jet INteraction Generator (HIJING) for further insights.
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Submitted 21 May, 2026; v1 submitted 6 December, 2025;
originally announced December 2025.
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Study of Central Exclusive Production of $π^+π^-$, $K^+K^-$ and $p \bar{p}$ Pairs in Proton-Proton Collisions at $\sqrt{s} = 510$ GeV with the STAR Detector at RHIC
Authors:
STAR Collaboration,
B. E. Aboona,
J. Adam,
L. Adamczyk,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
A. K. Alshammri,
E. C. Aschenauer,
S. Aslam,
J. Atchison,
V. Bairathi,
X. Bao,
P. Barik,
K. Barish,
S. Behera,
R. Bellwied,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
J. Bielcik,
J. Bielcikova,
J. D. Brandenburg,
C. Broodo
, et al. (380 additional authors not shown)
Abstract:
We report on the first measurement of the Central Exclusive Production process in proton-proton collisions: $pp \ \rightarrow \ p h^+ h^- p$ (where $h = π, K, p$) at the center-of-mass energy $\sqrt{s} = 510$ GeV with the STAR experiment at RHIC. At this energy, the process is dominated by a double Pomeron exchange mechanism. Hence, it provides a clean environment for investigating Pomeron interac…
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We report on the first measurement of the Central Exclusive Production process in proton-proton collisions: $pp \ \rightarrow \ p h^+ h^- p$ (where $h = π, K, p$) at the center-of-mass energy $\sqrt{s} = 510$ GeV with the STAR experiment at RHIC. At this energy, the process is dominated by a double Pomeron exchange mechanism. Hence, it provides a clean environment for investigating Pomeron interactions by measuring fully reconstructed final states involving only two hadrons and two forward scattered protons. The oppositely charged hadron pairs are measured within the central detector of STAR. The forward scattered protons are measured in the Roman Pot system allowing the verification of the event's exclusivity. Differential fiducial cross sections within the STAR acceptance are presented as a function of the difference in the azimuthal angle between the outgoing protons. The invariant masses of the charged hadron pairs are measured up to approximately 3 GeV and the square of the four-momentum transfer ($t_1$ and $t_2$) of the two forward-scattered protons in the range $0.3 \text{ GeV}^2 < -t_1 , -t_2 < 1.6 \text{ GeV}^2$. The differential fiducial cross sections of the forward protons as a function of the $|t_1 + t_2|$ are also presented. All results for the $π^+π^-$ pair are presented in three mass ranges. A comparison with GRANIITTI Monte Carlo predictions are also presented, where the spectra include continuum and resonant contributions. The observed spectra are consistent with double Pomeron exchange, including resonances seen in previous studies.
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Submitted 2 June, 2026; v1 submitted 31 October, 2025;
originally announced October 2025.
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Measurement of transverse polarization of $Λ$ and $\barΛ$ hyperons inside jets in $pp$ collisions at $\sqrt{s}=200$ GeV
Authors:
STAR Collaboration,
B. E. Aboona,
J. Adam,
G. Agakishiev,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
A. Aitbayev,
I. Alekseev,
E. Alpatov,
A. K. Alshammri,
A. Aparin,
S. Aslam,
J. Atchison,
G. S. Averichev,
V. Bairathi,
X. Bao,
P. Barik,
K. Barish,
S. Behera,
P. Bhaga t,
A. Bhasin,
S. Bhatta,
I. G. Bordyuzhin,
J. D. Brandenburg
, et al. (365 additional authors not shown)
Abstract:
A surprisingly large transverse polarization of $Λ$ hyperons in unpolarized hadron-nucleon/nucleus collisions has been observed for 50 years, and the origin of this polarization remains an important open question. Recently, theoretical frameworks have advanced in describing this puzzle with the polarizing fragmentation function (PFF). We report the first measurement of $Λ$ and $\overlineΛ$ transve…
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A surprisingly large transverse polarization of $Λ$ hyperons in unpolarized hadron-nucleon/nucleus collisions has been observed for 50 years, and the origin of this polarization remains an important open question. Recently, theoretical frameworks have advanced in describing this puzzle with the polarizing fragmentation function (PFF). We report the first measurement of $Λ$ and $\overlineΛ$ transverse polarization inside jets in unpolarized proton-proton collisions, which is directly attributed to the PFF. The polarization is measured as a function of the jet transverse momentum, the fraction of the jet momentum carried by $Λ$($\overlineΛ$) hyperons, and the transverse momentum of $Λ(\overlineΛ)$ hyperons relative to the jet axis. Covering a wide jet-energy range, these data provide the first constraints on the gluon PFF and allow tests of TMD evolution and its universality.
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Submitted 13 May, 2026; v1 submitted 22 September, 2025;
originally announced September 2025.
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Observation of charmonium sequential suppression in heavy-ion collisions at the Relativistic Heavy Ion Collider
Authors:
STAR Collaboration,
B. E. Aboona,
J. Adam,
L. Adamczyk,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
A. K. Alshammri,
E. C. Aschenauer,
S. Aslam,
J. Atchison,
V. Bairathi,
X. Bao,
P. Barik,
K. Barish,
S. Behera,
R. Bellwied,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
J. Bielcik,
J. Bielcikova,
J. D. Brandenburg,
C. Broodo
, et al. (372 additional authors not shown)
Abstract:
We report measurements of charmonium sequential suppression in Ru+Ru and Zr+Zr collisions at $\sqrt{s_{\mathrm {NN}}}$ = 200 GeV with the STAR experiment at the Relativistic Heavy Ion Collider (RHIC). The inclusive yield ratio of $ψ$(2S) to J/$ψ$ as a function of transverse momentum is reported, along with the centrality dependence of the double ratio, defined as the $ψ$(2S) to J/$ψ$ ratio in heav…
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We report measurements of charmonium sequential suppression in Ru+Ru and Zr+Zr collisions at $\sqrt{s_{\mathrm {NN}}}$ = 200 GeV with the STAR experiment at the Relativistic Heavy Ion Collider (RHIC). The inclusive yield ratio of $ψ$(2S) to J/$ψ$ as a function of transverse momentum is reported, along with the centrality dependence of the double ratio, defined as the $ψ$(2S) to J/$ψ$ ratio in heavy-ion collisions relative to that in $p$+$p$ collisions. In the 0-80% centrality class, the double ratio is found to be 0.41 $\pm$ 0.10 (stat) $\pm$ 0.03 (syst) $\pm$ 0.02 (ref), lower than unity with a significance of 5.6 standard deviations. This provides experimental evidence that $ψ$(2S) is significantly more suppressed than J/$ψ$ in heavy-ion collisions at RHIC. This sequential suppression pattern seems to increase from peripheral to central collisions, but with no significant dependence on the transverse momentum.
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Submitted 9 March, 2026; v1 submitted 16 September, 2025;
originally announced September 2025.
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Probing the Cosmological Principle with CMB lensing and cosmic shear
Authors:
James Adam,
Roy Maartens,
Julien Larena,
Chris Clarkson,
Ruth Durrer
Abstract:
The standard cosmological model assumes the Cosmological Principle. However, recent observations hint at possible violations of isotropy on large scales, possibly through late-time anisotropic expansion. Here we investigate the potential of cross-correlations between CMB lensing convergence $κ$ and galaxy cosmic shear $B$-modes as a novel probe of such late-time anisotropies. Our signal-to-noise f…
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The standard cosmological model assumes the Cosmological Principle. However, recent observations hint at possible violations of isotropy on large scales, possibly through late-time anisotropic expansion. Here we investigate the potential of cross-correlations between CMB lensing convergence $κ$ and galaxy cosmic shear $B$-modes as a novel probe of such late-time anisotropies. Our signal-to-noise forecasts reveal that information from the $κ$-$B$ cross-correlation is primarily contained on large angular scales ($\ell \lesssim 200$). We find that this cross-correlation for a Euclid-like galaxy survey is sensitive to anisotropy at the percent level. Making use of tomography yields a modest improvement of $\sim 20\%$ in detection power. Incorporating the galaxy $E$-$B$ cross-correlations would further enhance these constraints.
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Submitted 14 November, 2025; v1 submitted 8 September, 2025;
originally announced September 2025.
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Above 99.9% Fidelity Single-Qubit Gates, Two-Qubit Gates, and Readout in a Single Superconducting Quantum Device
Authors:
Fabian Marxer,
Jakub Mrożek,
Joona Andersson,
Leonid Abdurakhimov,
Janos Adam,
Ville Bergholm,
Rohit Beriwal,
Chun Fai Chan,
Saga Dahl,
Soumya Ranjan Das,
Frank Deppe,
Olexiy Fedorets,
Zheming Gao,
Alejandro Gomez Frieiro,
Daria Gusenkova,
Andrew Guthrie,
Tuukka Hiltunen,
Hao Hsu,
Eric Hyyppä,
Joni Ikonen,
Sinan Inel,
Shan W. Jolin,
Azad Karis,
Seung-Goo Kim,
William Kindel
, et al. (42 additional authors not shown)
Abstract:
Achieving high-fidelity single-qubit gates, two-qubit gates, and qubit readout is critical for building scalable, error-corrected quantum computers. However, device parameters that enhance one operation often degrade the others, making simultaneous optimization challenging. Here, we demonstrate that careful tuning of qubit-coupler coupling strengths in a superconducting circuit with two transmon q…
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Achieving high-fidelity single-qubit gates, two-qubit gates, and qubit readout is critical for building scalable, error-corrected quantum computers. However, device parameters that enhance one operation often degrade the others, making simultaneous optimization challenging. Here, we demonstrate that careful tuning of qubit-coupler coupling strengths in a superconducting circuit with two transmon qubits coupled via a tunable coupler enables high-fidelity single- and two-qubit gates, without compromising readout performance. As a result, we achieve a 40h-averaged CZ gate fidelity of 99.93%, simultaneous single-qubit gate fidelities of 99.98%, and readout fidelities over 99.94% in a single device. These results are enabled by optimized coupling parameters, an efficient CZ gate calibration experiment based on our new Phased-Averaged Leakage Error Amplification (PALEA) protocol, and a readout configuration compatible with high coherence qubits. Our results demonstrate a viable path toward scaling up superconducting quantum processors while maintaining consistently high fidelities across all core operations.
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Submitted 22 August, 2025;
originally announced August 2025.
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Experimental determination and micromagnetic analysis of spin wave modes in cylindrical nanowires
Authors:
Niklas Martin,
Laura Álvaro-Gómez,
Lucas Perez,
André Thiaville,
Jean-Paul Adam,
Olivier Fruchart,
Aurélien Masseboeuf
Abstract:
We report an experimental study of spin wave modes in individual cylindrical nanowires, a textbook situation of confined spin waves in 3D nanomagnetism. We observe discrete modes of thermal spin waves with micro-Brillouin light scattering, whose frequencies $f$ shift to higher values as the applied longitudinal induction magnetic field $B_z$ increases. Micromagnetic simulations allowed us to assoc…
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We report an experimental study of spin wave modes in individual cylindrical nanowires, a textbook situation of confined spin waves in 3D nanomagnetism. We observe discrete modes of thermal spin waves with micro-Brillouin light scattering, whose frequencies $f$ shift to higher values as the applied longitudinal induction magnetic field $B_z$ increases. Micromagnetic simulations allowed us to associate every $f(B_z)$ curve to a given spatial mode, labeled with radial and azimuthal indices $\ell$ and $m$.
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Submitted 21 August, 2025;
originally announced August 2025.
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Metalens-coupled terahertz NbN hot electron bolometer mixer
Authors:
D. Ren,
J. R. G. Silva,
S. Cremasco,
Z. Zhao,
W. Ji,
J. de Graaff,
A. J. L. Adam,
J. R. Gao
Abstract:
Enabled by planarized phase engineering, metalenses based on metasurfaces offer compact and scalable solutions for applications such as sensing, imaging, and virtual reality. They are particularly attractive for multi-pixel, large-scale heterodyne focal plane arrays in space observatories, where a flat metalens array on a silicon wafer can replace individual lenses, greatly simplifying system inte…
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Enabled by planarized phase engineering, metalenses based on metasurfaces offer compact and scalable solutions for applications such as sensing, imaging, and virtual reality. They are particularly attractive for multi-pixel, large-scale heterodyne focal plane arrays in space observatories, where a flat metalens array on a silicon wafer can replace individual lenses, greatly simplifying system integration and beam alignment. In this work, we demonstrate, for the first time, a superconducting niobium nitride (NbN) hot electron bolometer (HEB) mixer coupled with a silicon-based metalens operating at terahertz frequencies. The metalens phase profile was derived from a finite-size Gaussian beam source using the Rayleigh-Sommerfeld diffraction integral, and its focusing behavior was validated through 2D simulation. Experimentally, the metalens-coupled NbN HEB receiver exhibited a noise temperature of 1800 K at 1.63 THz. The power coupling efficiency from free space to the mixer via the metalens was measured to be 25 %. Measured far-field beam profiles are Gaussian-like with sidelobes below -14 dB. These results demonstrate the feasibility of integrating metalenses with HEB mixers for THz detection, offering a scalable path for compact focal plane arrays in space-based THz instrumentation.
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Submitted 22 July, 2025;
originally announced July 2025.
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Energy Independence of the Collins Asymmetry in $p^{\uparrow}p$ Collisions
Authors:
STAR Collaboration,
B. E. Aboona,
J. Adam,
L. Adamczyk,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
A. K. Alshammri,
E. C. Aschenauer,
S. Aslam,
J. Atchison,
V. Bairathi,
X. Bao,
P. Barik,
K. Barish,
S. Behera,
R. Bellwied,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
J. Bielcik,
J. Bielcikova,
J. D. Brandenburg,
C. Broodo
, et al. (368 additional authors not shown)
Abstract:
The STAR experiment reports new, high-precision measurements of the transverse single-spin asymmetries for $π^{\pm}$ within jets, namely the Collins asymmetries, from transversely polarized ${p^{\uparrow}p}$ collisions at $\sqrt{s}$ = 510 GeV. The energy-scaled distribution of jet transverse momentum, $x_{\mathrm{T}} = 2p_{\mathrm{T,jet}}/\sqrt s$, shows a remarkable consistency for Collins asymme…
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The STAR experiment reports new, high-precision measurements of the transverse single-spin asymmetries for $π^{\pm}$ within jets, namely the Collins asymmetries, from transversely polarized ${p^{\uparrow}p}$ collisions at $\sqrt{s}$ = 510 GeV. The energy-scaled distribution of jet transverse momentum, $x_{\mathrm{T}} = 2p_{\mathrm{T,jet}}/\sqrt s$, shows a remarkable consistency for Collins asymmetries of $π^{\pm}$ in jets between $\sqrt{s}$ = 200 GeV and 510 GeV. This indicates that the Collins asymmetries are nearly energy independent with, at most, a very weak scale dependence in $p^{\uparrow}p$ collisions. These results extend to high-momentum scales ($Q^2 \leq 3400$ GeV$^2$) and enable unique tests of evolution and universality in the transverse-momentum-dependent formalism, thus providing important constraints for the Collins fragmentation functions.
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Submitted 24 January, 2026; v1 submitted 22 July, 2025;
originally announced July 2025.
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Spin waves involved in three-magnon splitting in synthetic antiferromagnets
Authors:
Asma Mouhoub,
Nathalie Bardou,
Jean-Paul Adam,
Aurélie Solignac,
Thibaut Devolder
Abstract:
An important nonlinear effect in magnonics is the 3-magnon splitting where a high frequency magnon splits into two magnons of lower frequencies. Here, we study the 3-magnon splitting in spin wave conduits made from synthetic antiferromagnets. By combining inductive excitation, inductive detection, Brillouin Light Scattering imaging of the spin waves and analytical modeling based on conservation la…
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An important nonlinear effect in magnonics is the 3-magnon splitting where a high frequency magnon splits into two magnons of lower frequencies. Here, we study the 3-magnon splitting in spin wave conduits made from synthetic antiferromagnets. By combining inductive excitation, inductive detection, Brillouin Light Scattering imaging of the spin waves and analytical modeling based on conservation laws, we elucidate the nature of the spin waves involved in this process. We show in particular that low order optical spin waves propagating along the conduit can split in doublets of non-degenerate acoustic spin waves that have a standing wave character in the confined direction and unsymmetrical wavevectors in the direction of the spin wave conduit. Generally, several splitting channels run in parallel. The rules governing the three-magnon splitting and its interplay with the mode confinement have consequences for the applications in non-linear microwave signal processing based on spin waves.
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Submitted 27 March, 2026; v1 submitted 23 June, 2025;
originally announced June 2025.
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Method of analysis of the spectra obtained by microfocused Brillouin light scattering
Authors:
Nessrine Benaziz,
Thibaut Devolder,
Jean-Paul Adam
Abstract:
Brillouin Light Scattering is a powerful technique to measure the microwave excitations present in a magnetic system. In microfocused mode, the light is focused on the sample using a microscope objective. This accelerates substantially the measurement but results in mixing the response of all microwave excitations into a single spectrum, such that modeling is required to disentangle the contributi…
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Brillouin Light Scattering is a powerful technique to measure the microwave excitations present in a magnetic system. In microfocused mode, the light is focused on the sample using a microscope objective. This accelerates substantially the measurement but results in mixing the response of all microwave excitations into a single spectrum, such that modeling is required to disentangle the contribution of each spin wave. By assuming that a spectrum collected in microfocused mode can be approximated by the sum of all back-scattering spectra that can be collected by the microscope objective, we develop a simple and direct way of interpreting spectra. The model is compared to experimental data collected on a 50 nm thick CoFeB magnetic film. The model allows the understanding of the influence of the optical properties of a sample, of the dispersion relation of the spin wave eigenexcitations and of their thickness profiles, as well as of their populations onto the magnitudes and the lineshapes of the characteristic features of a spectrum
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Submitted 27 June, 2025; v1 submitted 12 June, 2025;
originally announced June 2025.
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Role of non-reciprocity in spin-wave channeling
Authors:
Jean-Paul Adam,
Nathalie Bardou,
Aurélie Solignac,
Joo-Von Kim,
Thibaut Devolder
Abstract:
The extent to which non-reciprocal waves can be guided in arbitrary directions is an interesting question. We address one aspect of this problem by studying the propagation of acoustic spin waves in a narrow physical conduit made of a synthetic antiferromagnet. Through a combination of Brillouin Light Scattering microscopy and modeling, we demonstrate that even when attempting to guide waves in th…
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The extent to which non-reciprocal waves can be guided in arbitrary directions is an interesting question. We address one aspect of this problem by studying the propagation of acoustic spin waves in a narrow physical conduit made of a synthetic antiferromagnet. Through a combination of Brillouin Light Scattering microscopy and modeling, we demonstrate that even when attempting to guide waves in the reciprocal direction of the material, the system still exhibits strong signatures of non-reciprocity. This includes the excitation of high wavevector waves in the direction perpendicular to the intended channeling, as well as energy transfer in directions that often neither aligns with the physical conduit nor with the symmetry axes of the magnetic properties. These findings have implications for the modeling of propagating wave spectroscopy in non-reciprocal materials and their potential applications.
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Submitted 12 May, 2025;
originally announced May 2025.
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Self-Supervision Enhances Instance-based Multiple Instance Learning Methods in Digital Pathology: A Benchmark Study
Authors:
Ali Mammadov,
Loic Le Folgoc,
Julien Adam,
Anne Buronfosse,
Gilles Hayem,
Guillaume Hocquet,
Pietro Gori
Abstract:
Multiple Instance Learning (MIL) has emerged as the best solution for Whole Slide Image (WSI) classification. It consists of dividing each slide into patches, which are treated as a bag of instances labeled with a global label. MIL includes two main approaches: instance-based and embedding-based. In the former, each patch is classified independently, and then the patch scores are aggregated to pre…
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Multiple Instance Learning (MIL) has emerged as the best solution for Whole Slide Image (WSI) classification. It consists of dividing each slide into patches, which are treated as a bag of instances labeled with a global label. MIL includes two main approaches: instance-based and embedding-based. In the former, each patch is classified independently, and then the patch scores are aggregated to predict the bag label. In the latter, bag classification is performed after aggregating patch embeddings. Even if instance-based methods are naturally more interpretable, embedding-based MILs have usually been preferred in the past due to their robustness to poor feature extractors. However, recently, the quality of feature embeddings has drastically increased using self-supervised learning (SSL). Nevertheless, many authors continue to endorse the superiority of embedding-based MIL. To investigate this further, we conduct 710 experiments across 4 datasets, comparing 10 MIL strategies, 6 self-supervised methods with 4 backbones, 4 foundation models, and various pathology-adapted techniques. Furthermore, we introduce 4 instance-based MIL methods never used before in the pathology domain. Through these extensive experiments, we show that with a good SSL feature extractor, simple instance-based MILs, with very few parameters, obtain similar or better performance than complex, state-of-the-art (SOTA) embedding-based MIL methods, setting new SOTA results on the BRACS and Camelyon16 datasets. Since simple instance-based MIL methods are naturally more interpretable and explainable to clinicians, our results suggest that more effort should be put into well-adapted SSL methods for WSI rather than into complex embedding-based MIL methods.
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Submitted 2 May, 2025;
originally announced May 2025.
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Onset of Constituent Quark Number Scaling in Heavy-Ion Collisions at RHIC
Authors:
STAR Collaboration,
B. E. Aboona,
J. Adam,
L. Adamczyk,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
A. K. Alshammri,
E. C. Aschenauer,
S. Aslam,
J. Atchison,
V. Bairathi,
X. Bao,
K. Barish,
S. Behera,
R. Bellwied,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
J. Bielcik,
J. Bielcikova,
J. D. Brandenburg,
C. Broodo,
X. Z. Cai
, et al. (347 additional authors not shown)
Abstract:
Partonic collectivity is one of the necessary signatures for the formation of quark-gluon plasma in high-energy nuclear collisions. Number of constituent quarks (NCQ) scaling has been observed for hadron elliptic flow $v_2$ in top energy nuclear collisions at the Relativistic Heavy Ion Collider and the LHC, and this has been theoretically suggested as strong evidence for partonic collectivity. In…
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Partonic collectivity is one of the necessary signatures for the formation of quark-gluon plasma in high-energy nuclear collisions. Number of constituent quarks (NCQ) scaling has been observed for hadron elliptic flow $v_2$ in top energy nuclear collisions at the Relativistic Heavy Ion Collider and the LHC, and this has been theoretically suggested as strong evidence for partonic collectivity. In this Letter, a systematic analysis of $v_2$ of $π^{\pm}$, $K^{\pm}$, $K^{0}_{S}$, $p$, and $Λ$ in Au+Au collisions at ${\sqrt{s_{_{\rm{NN}}}}}$ = 3.2, 3.5, 3.9, and 4.5 GeV, with the STAR experiment at the Relativistic Heavy Ion Collider, is presented. NCQ scaling is markedly violated at 3.2 GeV, consistent with a hadronic-interaction dominated equation of state. However, as the collision energy increases, a gradual evolution to NCQ scaling is observed. This beam-energy dependence of $v_2$ for all hadrons studied provides evidence for the onset of dominant partonic interactions by ${\sqrt{s_{_{\rm{NN}}}}}$ = 4.5 GeV.
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Submitted 11 August, 2025; v1 submitted 2 April, 2025;
originally announced April 2025.
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Measurement of Kaon Directed Flow in Au+Au Collisions in the High Baryon Density Region
Authors:
STAR Collaboration,
B. E. Aboona,
J. Adam,
G. Agakishiev,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
A. Aitbayev,
I. Alekseev,
E. Alpatov,
A. K. Alshammri,
A. Aparin,
S. Aslam,
J. Atchison,
G. S. Averichev,
V. Bairathi,
X. Bao,
P. Barik,
K. Barish,
S. Behera,
P. Bhagat,
A. Bhasin,
S. Bhatta,
I. G. Bordyuzhin,
J. D. Brandenburg
, et al. (363 additional authors not shown)
Abstract:
Rapidity-odd directed flow $v_1$ measurements are presented for $K^{\pm}$ and $K^0_S$ in Au$+$Au collisions at $\sqrt{s_{\text{NN}}}$ = 3.0, 3.2, 3.5, and 3.9 GeV with the STAR experiment. For comparison, $v_1$ of $π^{\pm}$, protons, and $Λ$ from the same collisions are also discussed. The mid-rapidity $v_1$ slope $\text{d}v_1/\text{d}y|_{y=0}$ for protons and $Λ$ is positive in these collisions.…
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Rapidity-odd directed flow $v_1$ measurements are presented for $K^{\pm}$ and $K^0_S$ in Au$+$Au collisions at $\sqrt{s_{\text{NN}}}$ = 3.0, 3.2, 3.5, and 3.9 GeV with the STAR experiment. For comparison, $v_1$ of $π^{\pm}$, protons, and $Λ$ from the same collisions are also discussed. The mid-rapidity $v_1$ slope $\text{d}v_1/\text{d}y|_{y=0}$ for protons and $Λ$ is positive in these collisions. On the other hand, $v_1$ slope of kaons exhibits a strong $p_\text{T}$ dependence: negative at $p_\text{T} <$ 0.6 GeV/$c$ and positive at higher $p_\text{T}$. A similar $p_\text{T}$ dependence is also evident for the $v_1$ slope of charged pions. Compared to the spectator-removed calculations in Au$+$Au collisions at $\sqrt{s_{\text{NN}}} =$ 3.0-3.9 GeV, the JAM model demonstrates a pronounced shift of the $v_1$ slopes of mesons towards the negative direction. It suggests that the shadowing effect of the spectators plays an important role in the observed kaon anti-flow at low $p_\text{T}$ in the high baryon density region of non-central collisions.
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Submitted 31 May, 2026; v1 submitted 30 March, 2025;
originally announced March 2025.
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Large frequency nonreciprocity of azimuthal spin wave modes in submicron vortex state disks
Authors:
Sali Salama,
Joo-Von Kim,
Abdelmadjid Anane,
Jean-Paul Adam
Abstract:
Vortex states in thin film disks host spin-wave modes that are geometrically quantized according to their radial and azimuthal indices. Previous studies have shown that hybridization between these modes and the vortex core results in a sizable frequency nonreciprocity between low-order clockwise and counterclockwise propagating azimuthal modes. Here, we present a computational study of these spin-…
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Vortex states in thin film disks host spin-wave modes that are geometrically quantized according to their radial and azimuthal indices. Previous studies have shown that hybridization between these modes and the vortex core results in a sizable frequency nonreciprocity between low-order clockwise and counterclockwise propagating azimuthal modes. Here, we present a computational study of these spin-wave modes in submicron disks in which the spatial extension of the vortex core becomes comparable to the wavelength of certain modes. In such cases, we find that the frequency nonreciprocity can be large even for higher order radial and azimuthal indices, reaching several GHz and comparable to the mode frequencies themselves.
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Submitted 7 May, 2025; v1 submitted 30 January, 2025;
originally announced January 2025.
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Probing the Cosmological Principle with weak lensing shear
Authors:
James Adam,
Roy Maartens,
Julien Larena,
Chris Clarkson
Abstract:
The Cosmological Principle is a cornerstone of the standard model of cosmology and shapes how we view the Universe and our place within it. It is imperative, then, to devise multiple observational tests which can identify and quantify possible violations of this foundational principle. One possible method of probing large-scale anisotropies involves the use of weak gravitational lensing. We revisi…
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The Cosmological Principle is a cornerstone of the standard model of cosmology and shapes how we view the Universe and our place within it. It is imperative, then, to devise multiple observational tests which can identify and quantify possible violations of this foundational principle. One possible method of probing large-scale anisotropies involves the use of weak gravitational lensing. We revisit this approach in order to analyse the imprint of late-time anisotropic expansion on cosmic shear. We show that the cross-correlation of shear $E$- and $B$-modes on large scales can be used to constrain the magnitude (and possibly direction) of anisotropic expansion. We estimate the signal to noise for multipoles $10\lesssim \ell\lesssim 100$ that is achievable by a Euclid-like survey. Our findings suggest that such a survey could detect the $E$-$B$ signal for reasonable values of the late-time anisotropy parameter.
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Submitted 12 February, 2025; v1 submitted 13 November, 2024;
originally announced November 2024.
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Technology and Performance Benchmarks of IQM's 20-Qubit Quantum Computer
Authors:
Leonid Abdurakhimov,
Janos Adam,
Hasnain Ahmad,
Olli Ahonen,
Manuel Algaba,
Guillermo Alonso,
Ville Bergholm,
Rohit Beriwal,
Matthias Beuerle,
Clinton Bockstiegel,
Alessio Calzona,
Chun Fai Chan,
Daniele Cucurachi,
Saga Dahl,
Rakhim Davletkaliyev,
Olexiy Fedorets,
Alejandro Gomez Frieiro,
Zheming Gao,
Johan Guldmyr,
Andrew Guthrie,
Juha Hassel,
Hermanni Heimonen,
Johannes Heinsoo,
Tuukka Hiltunen,
Keiran Holland
, et al. (89 additional authors not shown)
Abstract:
Quantum computing has tremendous potential to overcome some of the fundamental limitations present in classical information processing. Yet, today's technological limitations in the quality and scaling prevent exploiting its full potential. Quantum computing based on superconducting quantum processing units (QPUs) is among the most promising approaches towards practical quantum advantage.
In thi…
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Quantum computing has tremendous potential to overcome some of the fundamental limitations present in classical information processing. Yet, today's technological limitations in the quality and scaling prevent exploiting its full potential. Quantum computing based on superconducting quantum processing units (QPUs) is among the most promising approaches towards practical quantum advantage.
In this article the basic technological approach of IQM Quantum Computers is described covering both the QPU and the rest of the full-stack quantum computer. In particular, the focus is on a 20-qubit quantum computer featuring the Garnet QPU and its architecture, which we will scale up to 150 qubits. We also present QPU and system-level benchmarks, including a median 2-qubit gate fidelity of 99.5% and genuinely entangling all 20 qubits in a Greenberger-Horne-Zeilinger (GHZ) state.
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Submitted 22 August, 2024;
originally announced August 2024.
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Entropy and thermodynamical stability of white dwarfs
Authors:
Jiří Adam, Jr.,
Emil Truhlík
Abstract:
A structure of spherical white dwarfs is calculated for a non-zero temperature. It is shown that the thermodynamical stability of the white dwarf stars can be described naturally within the concept of the Helmholtz free energy of the Coulomb fully ionized electron-ion plasma.
A structure of spherical white dwarfs is calculated for a non-zero temperature. It is shown that the thermodynamical stability of the white dwarf stars can be described naturally within the concept of the Helmholtz free energy of the Coulomb fully ionized electron-ion plasma.
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Submitted 24 July, 2024; v1 submitted 11 June, 2024;
originally announced June 2024.
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Correlations of event activity with hard and soft processes in $p$ + Au collisions at $\sqrt{s_\mathrm{NN}}$ = 200 GeV at STAR
Authors:
STAR Collaboration,
M. I. Abdulhamid,
B. E. Aboona,
J. Adam,
L. Adamczyk,
J. R. Adams,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
E. C. Aschenauer,
S. Aslam,
J. Atchison,
V. Bairathi,
J. G. Ball Cap,
K. Barish,
R. Bellwied,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
J. Bielcik,
J. Bielcikova,
J. D. Brandenburg,
C. Broodo,
X. Z. Cai
, et al. (338 additional authors not shown)
Abstract:
With the STAR experiment at the BNL Relativisic Heavy Ion Collider, we characterize $\sqrt{s_\mathrm{NN}}$ = 200 GeV p+Au collisions by event activity (EA) measured within the pseudorapidity range $eta$ $in$ [-5, -3.4] in the Au-going direction and report correlations between this EA and hard- and soft- scale particle production at midrapidity ($η$ $\in$ [-1, 1]). At the soft scale, charged partic…
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With the STAR experiment at the BNL Relativisic Heavy Ion Collider, we characterize $\sqrt{s_\mathrm{NN}}$ = 200 GeV p+Au collisions by event activity (EA) measured within the pseudorapidity range $eta$ $in$ [-5, -3.4] in the Au-going direction and report correlations between this EA and hard- and soft- scale particle production at midrapidity ($η$ $\in$ [-1, 1]). At the soft scale, charged particle production in low-EA p+Au collisions is comparable to that in p+p collisions and increases monotonically with increasing EA. At the hard scale, we report measurements of high transverse momentum (pT) jets in events of different EAs. In contrast with the soft particle production, high-pT particle production and EA are found to be inversely related. To investigate whether this is a signal of jet quenching in high-EA events, we also report ratios of pT imbalance and azimuthal separation of dijets in high- and low-EA events. Within our measurement precision, no significant differences are observed, disfavoring the presence of jet quenching in the highest 30% EA p+Au collisions at $\sqrt{s_\mathrm{NN}}$ = 200 GeV.
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Submitted 21 October, 2024; v1 submitted 12 April, 2024;
originally announced April 2024.
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Measurement of flow coefficients in high-multiplicity $p$+Au, $d$+Au and $^{3}$He$+$Au collisions at $\sqrt{s_{_{\mathrm{NN}}}}$=200 GeV
Authors:
STAR Collaboration,
M. I. Abdulhamid,
B. E. Aboona,
J. Adam,
L. Adamczyk,
J. R. Adams,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
E. C. Aschenauer,
S. Aslam,
J. Atchison,
V. Bairathi,
J. G. Ball Cap,
K. Barish,
R. Bellwied,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
J. Bielcik,
J. Bielcikova,
J. D. Brandenburg,
C. Broodo,
X. Z. Cai
, et al. (343 additional authors not shown)
Abstract:
Flow coefficients ($v_2$ and $v_3$) are measured in high-multiplicity $p$+Au, $d$+Au, and $^{3}$He$+$Au collisions at a center-of-mass energy of $\sqrt{s_{_{\mathrm{NN}}}}$ = 200 GeV using the STAR detector. The measurements utilize two-particle correlations with a pseudorapidity requirement of $|η| <$ 0.9 and a pair gap of $|Δη|>1.0$. The primary focus is on analysis methods, particularly the sub…
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Flow coefficients ($v_2$ and $v_3$) are measured in high-multiplicity $p$+Au, $d$+Au, and $^{3}$He$+$Au collisions at a center-of-mass energy of $\sqrt{s_{_{\mathrm{NN}}}}$ = 200 GeV using the STAR detector. The measurements utilize two-particle correlations with a pseudorapidity requirement of $|η| <$ 0.9 and a pair gap of $|Δη|>1.0$. The primary focus is on analysis methods, particularly the subtraction of non-flow contributions. Four established non-flow subtraction methods are applied to determine $v_n$, validated using the HIJING event generator. $v_n$ values are compared across the three collision systems at similar multiplicities; this comparison cancels the final state effects and isolates the impact of initial geometry. While $v_2$ values show differences among these collision systems, $v_3$ values are largely similar, consistent with expectations of subnucleon fluctuations in the initial geometry. The ordering of $v_n$ differs quantitatively from previous measurements using two-particle correlations with a larger rapidity gap, which, according to model calculations, can be partially attributed to the effects of longitudinal flow decorrelations. The prospects for future measurements to improve our understanding of flow decorrelation and subnucleonic fluctuations are also discussed.
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Submitted 6 November, 2024; v1 submitted 12 December, 2023;
originally announced December 2023.
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Production of Protons and Light Nuclei in Au+Au Collisions at $\sqrt{s_{\mathrm{NN}}}$ = 3 GeV with the STAR Detector
Authors:
STAR Collaboration,
M. I. Abdulhamid,
B. E. Aboona,
J. Adam,
L. Adamczyk,
J. R. Adams,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
E. C. Aschenauer,
S. Aslam,
J. Atchison,
V. Bairathi,
J. G. Ball Cap,
K. Barish,
R. Bellwied,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
J. Bielcik,
J. Bielcikova,
J. D. Brandenburg,
C. Broodo,
X. Z. Cai
, et al. (342 additional authors not shown)
Abstract:
We report the systematic measurement of protons and light nuclei production in Au+Au collisions at $\sqrt{s_{\mathrm{NN}}}$ = 3 GeV by the STAR experiment at the Relativistic Heavy Ion Collider (RHIC). The transverse momentum ($p_{T}$) spectra of protons ($p$), deuterons ($d$), tritons ($t$), $^{3}\mathrm{He}$, and $^{4}\mathrm{He}$ are measured from mid-rapidity to target rapidity for different c…
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We report the systematic measurement of protons and light nuclei production in Au+Au collisions at $\sqrt{s_{\mathrm{NN}}}$ = 3 GeV by the STAR experiment at the Relativistic Heavy Ion Collider (RHIC). The transverse momentum ($p_{T}$) spectra of protons ($p$), deuterons ($d$), tritons ($t$), $^{3}\mathrm{He}$, and $^{4}\mathrm{He}$ are measured from mid-rapidity to target rapidity for different collision centralities. We present the rapidity and centrality dependence of particle yields ($dN/dy$), average transverse momentum ($\langle p_{T}\rangle$), yield ratios ($d/p$, $t/p$,$^{3}\mathrm{He}/p$, $^{4}\mathrm{He}/p$), as well as the coalescence parameters ($B_2$, $B_3$). The 4$π$ yields for various particles are determined by utilizing the measured rapidity distributions, $dN/dy$. Furthermore, we present the energy, centrality, and rapidity dependence of the compound yield ratios ($N_{p} \times N_{t} / N_{d}^{2}$) and compare them with various model calculations. The physics implications of those results on the production mechanism of light nuclei and on QCD phase structure are discussed.
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Submitted 23 October, 2024; v1 submitted 18 November, 2023;
originally announced November 2023.
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Measurements of charged-particle multiplicity dependence of higher-order net-proton cumulants in $p$+$p$ collisions at $\sqrt{s} =$ 200 GeV from STAR at RHIC
Authors:
STAR Collaboration,
M. I. Abdulhamid,
B. E. Aboona,
J. Adam,
L. Adamczyk,
J. R. Adams,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
E. C. Aschenauer,
S. Aslam,
J. Atchison,
V. Bairathi,
J. G. Ball Cap,
K. Barish,
R. Bellwied,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
J. Bielcik,
J. Bielcikova,
J. D. Brandenburg,
C. Broodo,
X. Z. Cai
, et al. (338 additional authors not shown)
Abstract:
We report on the charged-particle multiplicity dependence of net-proton cumulant ratios up to sixth order from $\sqrt{s}=200$ GeV $p$+$p$ collisions at the Relativistic Heavy Ion Collider (RHIC). The measured ratios $C_{4}/C_{2}$, $C_{5}/C_{1}$, and $C_{6}/C_{2}$ decrease with increased charged-particle multiplicity and rapidity acceptance. Neither the Skellam baselines nor PYTHIA8 calculations ac…
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We report on the charged-particle multiplicity dependence of net-proton cumulant ratios up to sixth order from $\sqrt{s}=200$ GeV $p$+$p$ collisions at the Relativistic Heavy Ion Collider (RHIC). The measured ratios $C_{4}/C_{2}$, $C_{5}/C_{1}$, and $C_{6}/C_{2}$ decrease with increased charged-particle multiplicity and rapidity acceptance. Neither the Skellam baselines nor PYTHIA8 calculations account for the observed multiplicity dependence. In addition, the ratios $C_{5}/C_{1}$ and $C_{6}/C_{2}$ approach negative values in the highest-multiplicity events, which implies that thermalized QCD matter may be formed in $p$+$p$ collisions.
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Submitted 4 September, 2024; v1 submitted 1 November, 2023;
originally announced November 2023.
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Estimate of Background Baseline and Upper Limit on the Chiral Magnetic Effect in Isobar Collisions at $\sqrt{s_{\text{NN}}}=200$ GeV at the Relativistic Heavy-Ion Collider
Authors:
STAR Collaboration,
M. I. Abdulhamid,
B. E. Aboona,
J. Adam,
J. R. Adams,
G. Agakishiev,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
A. Aitbaev,
I. Alekseev,
E. Alpatov,
A. Aparin,
S. Aslam,
J. Atchison,
G. S. Averichev,
V. Bairathi,
J. G. Ball Cap,
K. Barish,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
I. G. Bordyuzhin,
J. D. Brandenburg
, et al. (333 additional authors not shown)
Abstract:
For the search of the chiral magnetic effect (CME), STAR previously presented the results from isobar collisions (${^{96}_{44}\text{Ru}}+{^{96}_{44}\text{Ru}}$, ${^{96}_{40}\text{Zr}}+{^{96}_{40}\text{Zr}}$) obtained through a blind analysis. The ratio of results in Ru+Ru to Zr+Zr collisions for the CME-sensitive charge-dependent azimuthal correlator ($Δγ$), normalized by elliptic anisotropy (…
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For the search of the chiral magnetic effect (CME), STAR previously presented the results from isobar collisions (${^{96}_{44}\text{Ru}}+{^{96}_{44}\text{Ru}}$, ${^{96}_{40}\text{Zr}}+{^{96}_{40}\text{Zr}}$) obtained through a blind analysis. The ratio of results in Ru+Ru to Zr+Zr collisions for the CME-sensitive charge-dependent azimuthal correlator ($Δγ$), normalized by elliptic anisotropy ($v_{2}$), was observed to be close to but systematically larger than the inverse multiplicity ratio. The background baseline for the isobar ratio, $Y = \frac{(Δγ/v_{2})^{\text{Ru}}}{(Δγ/v_{2})^{\text{Zr}}}$, is naively expected to be $\frac{(1/N)^{\text{Ru}}}{(1/N)^{\text{Zr}}}$; however, genuine two- and three-particle correlations are expected to alter it. We estimate the contributions to $Y$ from those correlations, utilizing both the isobar data and HIJING simulations. After including those contributions, we arrive at a final background baseline for $Y$, which is consistent with the isobar data. We extract an upper limit for the CME fraction in the $Δγ$ measurement of approximately $10\%$ at a $95\%$ confidence level on in isobar collisions at $\sqrt{s_{\text{NN}}} = 200$ GeV, with an expected $15\%$ difference in their squared magnetic fields.
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Submitted 17 July, 2024; v1 submitted 19 October, 2023;
originally announced October 2023.
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Observation of the Antimatter Hypernucleus $^4_{\barΛ}\overline{\hbox{H}}$
Authors:
STAR Collaboration,
M. I. Abdulhamid,
B. E. Aboona,
J. Adam,
L. Adamczyk,
J. R. Adams,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
E. C. Aschenauer,
S. Aslam,
J. Atchison,
V. Bairathi,
J. G. Ball Cap,
K. Barish,
R. Bellwied,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
J. Bielcik,
J. Bielcikova,
J. D. Brandenburg,
C. Broodo,
X. Z. Cai
, et al. (342 additional authors not shown)
Abstract:
At the origin of the Universe, asymmetry between the amount of created matter and antimatter led to the matter-dominated Universe as we know today. The origins of this asymmetry remain not completely understood yet. High-energy nuclear collisions create conditions similar to the Universe microseconds after the Big Bang, with comparable amounts of matter and antimatter. Much of the created antimatt…
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At the origin of the Universe, asymmetry between the amount of created matter and antimatter led to the matter-dominated Universe as we know today. The origins of this asymmetry remain not completely understood yet. High-energy nuclear collisions create conditions similar to the Universe microseconds after the Big Bang, with comparable amounts of matter and antimatter. Much of the created antimatter escapes the rapidly expanding fireball without annihilating, making such collisions an effective experimental tool to create heavy antimatter nuclear objects and study their properties, hoping to shed some light on existing questions on the asymmetry between matter and antimatter. Here we report the first observation of the antimatter hypernucleus \hbox{$^4_{\barΛ}\overline{\hbox{H}}$}, composed of a $\barΛ$ , an antiproton and two antineutrons. The discovery was made through its two-body decay after production in ultrarelativistic heavy-ion collisions by the STAR experiment at the Relativistic Heavy Ion Collider. In total, 15.6 candidate \hbox{$^4_{\barΛ}\overline{\hbox{H}}$} antimatter hypernuclei are obtained with an estimated background count of 6.4. The lifetimes of the antihypernuclei \hbox{$^3_{\barΛ}\overline{\hbox{H}}$} and \hbox{$^4_{\barΛ}\overline{\hbox{H}}$} are measured and compared with the lifetimes of their corresponding hypernuclei, testing the symmetry between matter and antimatter. Various production yield ratios among (anti)hypernuclei and (anti)nuclei are also measured and compared with theoretical model predictions, shedding light on their production mechanisms.
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Submitted 8 June, 2024; v1 submitted 19 October, 2023;
originally announced October 2023.
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Wavefront shaping through a free-form scattering object
Authors:
Alfredo Rates,
Ad Lagendijk,
Aurèle J. L. Adam,
Wilbert L. IJzerman,
Willem L. Vos
Abstract:
Wavefront shaping is a technique to study and control light transport inside scattering media. Wavefront shaping is considered to be applicable to any complex material, yet in most previous studies, the only sample geometries that are studied are slabs or wave-guides. In this paper, we study how macroscopic changes in the sample shape affect light scattering using the wavefront shaping technique.…
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Wavefront shaping is a technique to study and control light transport inside scattering media. Wavefront shaping is considered to be applicable to any complex material, yet in most previous studies, the only sample geometries that are studied are slabs or wave-guides. In this paper, we study how macroscopic changes in the sample shape affect light scattering using the wavefront shaping technique. Using a flexible scattering material, we optimize the intensity of light in a focusing spot using wavefront shaping and record the optimized pattern, comparing the enhancement for different curvatures and beam radii. We validate our hypothesis that wavefront shaping has a similar enhancement regardless of the free-form shape of the sample and thus offers relevant potential for industrial applications. We propose a new figure of merit to evaluate the performance of wavefront shaping for different shapes. Surprisingly, based on this figure of merit, we observe that for this particular sample, wavefront shaping has a slightly better performance for a free-form shape than for a slab shape.
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Submitted 11 December, 2023; v1 submitted 7 October, 2023;
originally announced October 2023.
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Results on Elastic Cross Sections in Proton-Proton Collisions at $\sqrt{s} = 510$ GeV with the STAR Detector at RHIC
Authors:
STAR Collaboration,
M. I. Abdulhamid,
B. E. Aboona,
J. Adam,
L. Adamczyk,
J. R. Adams,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
E. C. Aschenauer,
S. Aslam,
J. Atchison,
V. Bairathi,
J. G. Ball Cap,
K. Barish,
R. Bellwied,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
J. Bielcik,
J. Bielcikova,
J. D. Brandenburg,
C. Broodo,
X. Z. Cai
, et al. (343 additional authors not shown)
Abstract:
We report results on an elastic cross section measurement in proton-proton collisions at a center-of-mass energy $\sqrt{s}=510$ GeV, obtained with the Roman Pot setup of the STAR experiment at the Relativistic Heavy Ion Collider (RHIC). The elastic differential cross section is measured in the four-momentum transfer squared range $0.23 \leq -t \leq 0.67$ GeV$^2$. We find that a constant slope $B$…
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We report results on an elastic cross section measurement in proton-proton collisions at a center-of-mass energy $\sqrt{s}=510$ GeV, obtained with the Roman Pot setup of the STAR experiment at the Relativistic Heavy Ion Collider (RHIC). The elastic differential cross section is measured in the four-momentum transfer squared range $0.23 \leq -t \leq 0.67$ GeV$^2$. We find that a constant slope $B$ does not fit the data in the aforementioned $t$ range, and we obtain a much better fit using a second-order polynomial for $B(t)$. The $t$ dependence of $B$ is determined using six subintervals of $t$ in the STAR measured $t$ range, and is in good agreement with the phenomenological models. The measured elastic differential cross section $\mathrm{d}σ/\mathrm{dt}$ agrees well with the results obtained at $\sqrt{s} = 546$ GeV for proton--antiproton collisions by the UA4 experiment. We also determine that the integrated elastic cross section within the STAR $t$-range is $σ^\mathrm{fid}_\mathrm{el} = 462.1 \pm 0.9 (\mathrm{stat.}) \pm 1.1 (\mathrm {syst.}) \pm 11.6 (\mathrm {scale})$~$μ\mathrm{b}$.
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Submitted 6 May, 2024; v1 submitted 28 September, 2023;
originally announced September 2023.
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Longitudinal and transverse spin transfer to $Λ$ and $\overlineΛ$ hyperons in polarized $p$+$p$ collisions at $\sqrt{s} = 200$ GeV
Authors:
STAR Collaboration,
M. I. Abdulhamid,
B. E. Aboona,
J. Adam,
L. Adamczyk,
J. R. Adams,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
D. M. Anderson,
E. C. Aschenauer,
S. Aslam,
J. Atchison,
V. Bairathi,
W. Baker,
J. G. Ball Cap,
K. Barish,
R. Bellwied,
P. Bhagat,
A. Bhasin,
S. Bhatta,
J. Bielcik,
J. Bielcikova,
J. D. Brandenburg,
X. Z. Cai
, et al. (357 additional authors not shown)
Abstract:
The longitudinal and transverse spin transfers to $Λ$ ($\overlineΛ$) hyperons in polarized proton-proton collisions are expected to be sensitive to the helicity and transversity distributions, respectively, of (anti-)strange quarks in the proton, and to the corresponding polarized fragmentation functions. We report improved measurements of the longitudinal spin transfer coefficient, $D_{LL}$, and…
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The longitudinal and transverse spin transfers to $Λ$ ($\overlineΛ$) hyperons in polarized proton-proton collisions are expected to be sensitive to the helicity and transversity distributions, respectively, of (anti-)strange quarks in the proton, and to the corresponding polarized fragmentation functions. We report improved measurements of the longitudinal spin transfer coefficient, $D_{LL}$, and the transverse spin transfer coefficient, $D_{TT}$, to $Λ$ and $\overlineΛ$ in polarized proton-proton collisions at $\sqrt{s}$ = 200 GeV by the STAR experiment at RHIC. The data set includes longitudinally polarized proton-proton collisions with an integrated luminosity of 52 pb$^{-1}$, and transversely polarized proton-proton collisions with a similar integrated luminosity. Both data sets have about twice the statistics of previous results and cover a kinematic range of $|η_{Λ(\overlineΛ)}|$ $<$ 1.2 and transverse momentum $p_{T,{Λ(\overlineΛ)}}$ up to 8 GeV/$c$. We also report the first measurements of the hyperon spin transfer coefficients $D_{LL}$ and $D_{TT}$ as a function of the fractional jet momentum $z$ carried by the hyperon, which can provide more direct constraints on the polarized fragmentation functions.
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Submitted 7 December, 2023; v1 submitted 25 September, 2023;
originally announced September 2023.
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Reaction plane correlated triangular flow in Au+Au collisions at $\sqrt{s_{NN}}=3$ GeV
Authors:
STAR Collaboration,
M. I. Abdulhamid,
B. E. Aboona,
J. Adam,
L. Adamczyk,
J. R. Adams,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
E. C. Aschenauer,
S. Aslam,
J. Atchison,
V. Bairathi,
J. G. Ball Cap,
K. Barish,
R. Bellwied,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
J. Bielcik,
J. Bielcikova,
J. D. Brandenburg,
C. Broodo,
X. Z. Cai
, et al. (341 additional authors not shown)
Abstract:
We measure triangular flow relative to the reaction plane at 3 GeV center-of-mass energy in Au+Au collisions at the BNL Relativistic Heavy Ion Collider. A significant $v_3$ signal for protons is observed, which increases for higher rapidity, higher transverse momentum, and more peripheral collisions. The triangular flow is essentially rapidity-odd with a slope at mid-rapidity, $dv_3/dy|_{(y=0)}$,…
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We measure triangular flow relative to the reaction plane at 3 GeV center-of-mass energy in Au+Au collisions at the BNL Relativistic Heavy Ion Collider. A significant $v_3$ signal for protons is observed, which increases for higher rapidity, higher transverse momentum, and more peripheral collisions. The triangular flow is essentially rapidity-odd with a slope at mid-rapidity, $dv_3/dy|_{(y=0)}$, opposite in sign compared to the slope for directed flow. No significant $v_3$ signal is observed for charged pions and kaons. Comparisons with models suggest that a mean field potential is required to describe these results, and that the triangular shape of the participant nucleons is the result of stopping and nuclear geometry.
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Submitted 19 April, 2024; v1 submitted 21 September, 2023;
originally announced September 2023.
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Compact Metasurface Terahertz Spectrometer
Authors:
Wenye Ji,
Jin Chang,
Behnam Mirzaei,
Marcel Ridder,
Willem Jellema,
Wilt Kao,
Alan Lee,
Jian Rong Gao,
Paul Urbach,
Aurele J. L. Adam
Abstract:
The electromagnetic spectrum in the terahertz frequency region is of significant importance for understanding the formation and evolution of galaxies and stars throughout the history of the universe and the process of planet formation. Within the star forming clouds the constituent atoms and molecules are excited to produce characteristic emission and absorption lines, many of which happen at the…
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The electromagnetic spectrum in the terahertz frequency region is of significant importance for understanding the formation and evolution of galaxies and stars throughout the history of the universe and the process of planet formation. Within the star forming clouds the constituent atoms and molecules are excited to produce characteristic emission and absorption lines, many of which happen at the terahertz frequencies. Thus, detecting the spectral signatures as unique fingerprints of molecules and atoms require terahertz spectrometers, which need to be operated in a space observatory because of the water vapor absorption in the earth atmosphere. However, current terahertz spectrometers face several challenges that limit their performances and applications, including a low resolution, limited bandwidth, large volume, and complexity. In this paper, we address the last two issues by demonstrating a concept of a compact terahertz spectrometer using metasurface. We start by modelling, designing, and fabricating a metasurface, aiming to optimize its performance within a band from 1.7 to 2.5 THz. Next, we make use of an array of quantum cascade lasers that operate at slightly different frequencies around 2.1 THz to validate the performance of the spectrometer. Finally, we apply the spectrum inversion method to analyse the measured data to confirm a resolution R of at least 273. Our results demonstrated a miniaturized terahertz spectrometer concept successfully.
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Submitted 5 September, 2023;
originally announced September 2023.
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Upper Limit on the Chiral Magnetic Effect in Isobar Collisions at the Relativistic Heavy-Ion Collider
Authors:
STAR Collaboration,
M. I. Abdulhamid,
B. E. Aboona,
J. Adam,
J. R. Adams,
G. Agakishiev,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
A. Aitbaev,
I. Alekseev,
E. Alpatov,
A. Aparin,
S. Aslam,
J. Atchison,
G. S. Averichev,
V. Bairathi,
J. G. Ball Cap,
K. Barish,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
I. G. Bordyuzhin,
J. D. Brandenburg
, et al. (333 additional authors not shown)
Abstract:
The chiral magnetic effect (CME) is a phenomenon that arises from the QCD anomaly in the presence of an external magnetic field. The experimental search for its evidence has been one of the key goals of the physics program of the Relativistic Heavy-Ion Collider. The STAR collaboration has previously presented the results of a blind analysis of isobar collisions (…
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The chiral magnetic effect (CME) is a phenomenon that arises from the QCD anomaly in the presence of an external magnetic field. The experimental search for its evidence has been one of the key goals of the physics program of the Relativistic Heavy-Ion Collider. The STAR collaboration has previously presented the results of a blind analysis of isobar collisions (${^{96}_{44}\text{Ru}}+{^{96}_{44}\text{Ru}}$, ${^{96}_{40}\text{Zr}}+{^{96}_{40}\text{Zr}}$) in the search for the CME. The isobar ratio ($Y$) of CME-sensitive observable, charge separation scaled by elliptic anisotropy, is close to but systematically larger than the inverse multiplicity ratio, the naive background baseline. This indicates the potential existence of a CME signal and the presence of remaining nonflow background due to two- and three-particle correlations, which are different between the isobars. In this post-blind analysis, we estimate the contributions from those nonflow correlations as a background baseline to $Y$, utilizing the isobar data as well as Heavy Ion Jet Interaction Generator simulations. This baseline is found consistent with the isobar ratio measurement, and an upper limit of 10% at 95% confidence level is extracted for the CME fraction in the charge separation measurement in isobar collisions at $\sqrt{s_{\rm NN}}=200$ GeV.
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Submitted 17 July, 2024; v1 submitted 31 August, 2023;
originally announced August 2023.
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Jet-hadron correlations with respect to the event plane in $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV Au+Au collisions in STAR
Authors:
STAR Collaboration,
M. I. Abdulhamid,
B. E. Aboona,
J. Adam,
L. Adamczyk,
J. R. Adams,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
E. C. Aschenauer,
S. Aslam,
J. Atchison,
V. Bairathi,
J. G. Ball Cap,
K. Barish,
R. Bellwied,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
J. Bielcik,
J. Bielcikova,
J. D. Brandenburg,
X. Z. Cai,
H. Caines
, et al. (340 additional authors not shown)
Abstract:
Angular distributions of charged particles relative to jet axes are studied in $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV Au+Au collisions as a function of the jet orientation with respect to the event plane. This differential study tests the expected path-length dependence of energy loss experienced by a hard-scattered parton as it traverses the hot and dense medium formed in heavy-ion collisions. A seco…
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Angular distributions of charged particles relative to jet axes are studied in $\sqrt{s_{\mathrm{NN}}}$ = 200 GeV Au+Au collisions as a function of the jet orientation with respect to the event plane. This differential study tests the expected path-length dependence of energy loss experienced by a hard-scattered parton as it traverses the hot and dense medium formed in heavy-ion collisions. A second-order event plane is used in the analysis as an experimental estimate of the reaction plane formed by the collision impact parameter and the beam direction. Charged-particle jets with $15 < p_{\rm T, jet} <$ 20 and $20 < p_{\rm T, jet} <$ 40 GeV/$c$ were reconstructed with the anti-$k_{\rm T}$ algorithm with radius parameter setting of (R=0.4) in the 20-50\% centrality bin to maximize the initial-state eccentricity of the interaction region. The reaction plane fit method is implemented to remove the flow-modulated background with better precision than prior methods. Yields and widths of jet-associated charged-hadron distributions are extracted in three angular bins between the jet axis and the event plane. The event-plane (EP) dependence is further quantified by ratios of the associated yields in different EP bins. No dependence on orientation of the jet axis with respect to the event plane is seen within the uncertainties in the kinematic regime studied. This finding is consistent with a similar experimental observation by ALICE in $\sqrt{s_{\mathrm{NN}}}$ = 2.76 TeV Pb+Pb collision data.
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Submitted 20 March, 2024; v1 submitted 25 July, 2023;
originally announced July 2023.
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Recent Advances in Metasurface Design and Quantum Optics Applications with Machine Learning, Physics-Informed Neural Networks, and Topology Optimization Methods
Authors:
Wenye Ji,
Jin Chang2,
He-Xiu Xu,
Jian Rong Gao,
Simon Gröblacher,
Paul Urbach,
Aurèle J. L. Adam
Abstract:
As a two-dimensional planar material with low depth profile, a metasurface can generate non-classical phase distributions for the transmitted and reflected electromagnetic waves at its interface. Thus, it offers more flexibility to control the wave front. A traditional metasurface design process mainly adopts the forward prediction algorithm, such as Finite Difference Time Domain, combined with ma…
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As a two-dimensional planar material with low depth profile, a metasurface can generate non-classical phase distributions for the transmitted and reflected electromagnetic waves at its interface. Thus, it offers more flexibility to control the wave front. A traditional metasurface design process mainly adopts the forward prediction algorithm, such as Finite Difference Time Domain, combined with manual parameter optimization. However, such methods are time-consuming, and it is difficult to keep the practical meta-atom spectrum being consistent with the ideal one. In addition, since the periodic boundary condition is used in the meta-atom design process, while the aperiodic condition is used in the array simulation, the coupling between neighboring meta-atoms leads to inevitable inaccuracy. In this review, representative intelligent methods for metasurface design are introduced and discussed, including machine learning, physics-information neural network, and topology optimization method. We elaborate on the principle of each approach, analyze their advantages and limitations, and discuss their potential applications. We also summarise recent advances in enabled metasurfaces for quantum optics applications. In short, this paper highlights a promising direction for intelligent metasurface designs and applications for future quantum optics research and serves as an up-to-date reference for researchers in the metasurface and metamaterial fields.
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Submitted 18 July, 2023;
originally announced July 2023.
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Unidirectionality of spin waves in Synthetic Antiferromagnets
Authors:
F. Millo,
J. -P. Adam,
C. Chappert,
J. -V. Kim,
A. Mouhoub,
A. Solignac,
T. Devolder
Abstract:
We study the frequency non-reciprocity of the spin waves in symmetric CoFeB/Ru/CoFeB synthetic antiferromagnets stacks set in the scissors state by in-plane applied fields. Using a combination of Brillouin Light Scattering and propagating spin wave spectroscopy experiments, we show that the acoustical spin waves in synthetic antiferromagnets possess a unique feature if their wavevector is parallel…
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We study the frequency non-reciprocity of the spin waves in symmetric CoFeB/Ru/CoFeB synthetic antiferromagnets stacks set in the scissors state by in-plane applied fields. Using a combination of Brillouin Light Scattering and propagating spin wave spectroscopy experiments, we show that the acoustical spin waves in synthetic antiferromagnets possess a unique feature if their wavevector is parallel to the applied field: the frequency non-reciprocity due to layer-to-layer dipolar interactions can be so large that the acoustical spin waves transfer energy in a unidirectional manner for a wide and bipolar interval of wavevectors. Analytical modeling and full micromagnetic calculations are conducted to account for the dispersion relations of the optical and acoustical spin waves for arbitrary field orientations. Our formalism provides a simple and direct method to understand and design devices harnessing unidirectional propagation of spin waves in synthetic antiferromagnets.
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Submitted 21 September, 2023; v1 submitted 8 June, 2023;
originally announced June 2023.
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Pixel-based tracking detectors for a Low Q2 Tagger at EIC -- status report
Authors:
Simon Gardner,
Derek I. Glazier,
Kenneth Livingston,
Dzmitry Maneuski,
Daria Sokhan,
Jaroslav Adam
Abstract:
The design of pixel-based tracking detectors for a Low Q2 Tagger in the Far Backward region of the ePIC detector at EIC is presented. The physics case is outlined, together with estimates of rates and resolutions, and the current design based on Timepix4 technology is introduced.
The design of pixel-based tracking detectors for a Low Q2 Tagger in the Far Backward region of the ePIC detector at EIC is presented. The physics case is outlined, together with estimates of rates and resolutions, and the current design based on Timepix4 technology is introduced.
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Submitted 11 May, 2023; v1 submitted 3 May, 2023;
originally announced May 2023.
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Collision-energy Dependence of Deuteron Cumulants and Proton-deuteron Correlations in Au+Au collisions at RHIC
Authors:
STAR Collaboration,
M. I. Abdulhamid,
B. E. Aboona,
J. Adam,
L. Adamczyk,
J. R. Adams,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
E. C. Aschenauer,
S. Aslam,
J. Atchison,
V. Bairathi,
J. G. Ball Cap,
K. Barish,
R. Bellwied,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
J. Bielcik,
J. Bielcikova,
J. D. Brandenburg,
C. Broodo,
X. Z. Cai
, et al. (343 additional authors not shown)
Abstract:
We report the first measurements of cumulants, up to $4^{th}$ order, of deuteron number distributions and proton-deuteron correlations in Au+Au collisions recorded by the STAR experiment in phase-I of Beam Energy Scan (BES) program at the Relativistic Heavy Ion Collider. Deuteron cumulants, their ratios, and proton-deuteron mixed cumulants are presented for different collision centralities coverin…
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We report the first measurements of cumulants, up to $4^{th}$ order, of deuteron number distributions and proton-deuteron correlations in Au+Au collisions recorded by the STAR experiment in phase-I of Beam Energy Scan (BES) program at the Relativistic Heavy Ion Collider. Deuteron cumulants, their ratios, and proton-deuteron mixed cumulants are presented for different collision centralities covering a range of center-of-mass energy per nucleon pair $\sqrt{s_{NN}}$~=~7.7 to 200~GeV. It is found that the cumulant ratios at lower collision energies favor a canonical ensemble over a grand canonical ensemble in thermal models. An anti-correlation between proton and deuteron multiplicity is observed across all collision energies and centralities, consistent with the expectation from global baryon number conservation. The UrQMD model coupled with a phase-space coalescence mechanism qualitatively reproduces the collision-energy dependence of cumulant ratios and proton-deuteron correlations.
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Submitted 28 June, 2024; v1 submitted 21 April, 2023;
originally announced April 2023.
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Event-by-event correlations between $Λ$ ($\barΛ$) hyperon global polarization and handedness with charged hadron azimuthal separation in Au+Au collisions at $\sqrt{s_{\text{NN}}} = 27 \text{ GeV}$ from STAR
Authors:
STAR Collaboration,
M. I. Abdulhamid,
B. E. Aboona,
J. Adam,
J. R. Adams,
G. Agakishiev,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
A. Aitbaev,
I. Alekseev,
D. M. Anderson,
A. Aparin,
S. Aslam,
J. Atchison,
G. S. Averichev,
V. Bairathi,
W. Baker,
J. G. Ball Cap,
K. Barish,
P. Bhagat,
A. Bhasin,
S. Bhatta,
I. G. Bordyuzhin,
J. D. Brandenburg
, et al. (333 additional authors not shown)
Abstract:
Global polarizations ($P$) of $Λ$ ($\barΛ$) hyperons have been observed in non-central heavy-ion collisions. The strong magnetic field primarily created by the spectator protons in such collisions would split the $Λ$ and $\barΛ$ global polarizations ($ΔP = P_Λ - P_{\barΛ} < 0$). Additionally, quantum chromodynamics (QCD) predicts topological charge fluctuations in vacuum, resulting in a chirality…
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Global polarizations ($P$) of $Λ$ ($\barΛ$) hyperons have been observed in non-central heavy-ion collisions. The strong magnetic field primarily created by the spectator protons in such collisions would split the $Λ$ and $\barΛ$ global polarizations ($ΔP = P_Λ - P_{\barΛ} < 0$). Additionally, quantum chromodynamics (QCD) predicts topological charge fluctuations in vacuum, resulting in a chirality imbalance or parity violation in a local domain. This would give rise to an imbalance ($Δn = \frac{N_{\text{L}} - N_{\text{R}}}{\langle N_{\text{L}} + N_{\text{R}} \rangle} \neq 0$) between left- and right-handed $Λ$ ($\barΛ$) as well as a charge separation along the magnetic field, referred to as the chiral magnetic effect (CME). This charge separation can be characterized by the parity-even azimuthal correlator ($Δγ$) and parity-odd azimuthal harmonic observable ($Δa_{1}$). Measurements of $ΔP$, $Δγ$, and $Δa_{1}$ have not led to definitive conclusions concerning the CME or the magnetic field, and $Δn$ has not been measured previously. Correlations among these observables may reveal new insights. This paper reports measurements of correlation between $Δn$ and $Δa_{1}$, which is sensitive to chirality fluctuations, and correlation between $ΔP$ and $Δγ$ sensitive to magnetic field in Au+Au collisions at 27 GeV. For both measurements, no correlations have been observed beyond statistical fluctuations.
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Submitted 22 July, 2023; v1 submitted 19 April, 2023;
originally announced April 2023.
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Observation of the electromagnetic field effect via charge-dependent directed flow in heavy-ion collisions at the Relativistic Heavy Ion Collider
Authors:
STAR Collaboration,
M. I. Abdulhamid,
B. E. Aboona,
J. Adam,
J. R. Adams,
G. Agakishiev,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
A. Aitbaev,
I. Alekseev,
E. Alpatov,
A. Aparin,
S. Aslam,
J. Atchison,
G. S. Averichev,
V. Bairathi,
J. G. Ball Cap,
K. Barish,
P. Bhagat,
A. Bhasin,
S. Bhatta,
S. R. Bhosale,
I. G. Bordyuzhin,
J. D. Brandenburg
, et al. (331 additional authors not shown)
Abstract:
The deconfined quark-gluon plasma (QGP) created in relativistic heavy-ion collisions enables the exploration of the fundamental properties of matter under extreme conditions. Non-central collisions can produce strong magnetic fields on the order of $10^{18}$ Gauss, which offers a probe into the electrical conductivity of the QGP. In particular, quarks and anti-quarks carry opposite charges and rec…
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The deconfined quark-gluon plasma (QGP) created in relativistic heavy-ion collisions enables the exploration of the fundamental properties of matter under extreme conditions. Non-central collisions can produce strong magnetic fields on the order of $10^{18}$ Gauss, which offers a probe into the electrical conductivity of the QGP. In particular, quarks and anti-quarks carry opposite charges and receive contrary electromagnetic forces that alter their momenta. This phenomenon can be manifested in the collective motion of final-state particles, specifically in the rapidity-odd directed flow, denoted as $v_1(\mathsf{y})$. Here we present the charge-dependent measurements of $dv_1/d\mathsf{y}$ near midrapidities for $π^{\pm}$, $K^{\pm}$, and $p(\bar{p})$ in Au+Au and isobar ($_{44}^{96}$Ru+$_{44}^{96}$Ru and $_{40}^{96}$Zr+$_{40}^{96}$Zr) collisions at $\sqrt{s_{\rm NN}}=$ 200 GeV, and in Au+Au collisions at 27 GeV, recorded by the STAR detector at the Relativistic Heavy Ion Collider. The combined dependence of the $v_1$ signal on collision system, particle species, and collision centrality can be qualitatively and semi-quantitatively understood as several effects on constituent quarks. While the results in central events can be explained by the $u$ and $d$ quarks transported from initial-state nuclei, those in peripheral events reveal the impacts of the electromagnetic field on the QGP. Our data put valuable constraints on the electrical conductivity of the QGP in theoretical calculations.
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Submitted 22 February, 2024; v1 submitted 6 April, 2023;
originally announced April 2023.
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Hyperon polarization along the beam direction relative to the second and third harmonic event planes in isobar collisions at $\sqrt{s_{NN}}$ = 200 GeV
Authors:
STAR Collaboration,
M. I. Abdulhamid,
B. E. Aboona,
J. Adam,
J. R. Adams,
G. Agakishiev,
I. Aggarwal,
M. M. Aggarwal,
Z. Ahammed,
A. Aitbaev,
I. Alekseev,
D. M. Anderson,
A. Aparin,
S. Aslam,
J. Atchison,
G. S. Averichev,
V. Bairathi,
W. Baker,
J. G. Ball Cap,
K. Barish,
P. Bhagat,
A. Bhasin,
S. Bhatta,
I. G. Bordyuzhin,
J. D. Brandenburg
, et al. (338 additional authors not shown)
Abstract:
The polarization of $Λ$ and $\barΛ$ hyperons along the beam direction has been measured relative to the second and third harmonic event planes in isobar Ru+Ru and Zr+Zr collisions at $\sqrt{s_{NN}}$ = 200 GeV. This is the first experimental evidence of the hyperon polarization by the triangular flow originating from the initial density fluctuations. The amplitudes of the sine modulation for the se…
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The polarization of $Λ$ and $\barΛ$ hyperons along the beam direction has been measured relative to the second and third harmonic event planes in isobar Ru+Ru and Zr+Zr collisions at $\sqrt{s_{NN}}$ = 200 GeV. This is the first experimental evidence of the hyperon polarization by the triangular flow originating from the initial density fluctuations. The amplitudes of the sine modulation for the second and third harmonic results are comparable in magnitude, increase from central to peripheral collisions, and show a mild $p_T$ dependence. The azimuthal angle dependence of the polarization follows the vorticity pattern expected due to elliptic and triangular anisotropic flow, and qualitatively disagree with most hydrodynamic model calculations based on thermal vorticity and shear induced contributions. The model results based on one of existing implementations of the shear contribution lead to a correct azimuthal angle dependence, but predict centrality and $p_T$ dependence that still disagree with experimental measurements. Thus, our results provide stringent constraints on the thermal vorticity and shear-induced contributions to hyperon polarization. Comparison to previous measurements at RHIC and the LHC for the second-order harmonic results shows little dependence on the collision system size and collision energy.
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Submitted 16 November, 2023; v1 submitted 16 March, 2023;
originally announced March 2023.