Showing 1–8 of 8 results for author: Tong, Y

Stability Analysis of the Possible Consistent Model of Parity Violations in the Symmetric Teleparallel Gravity: Generalized Background Solutions

Authors: Yeheng Tong

Abstract: In this paper, we consider a symmetric teleparallel gravity model that extends the general relativity equivalent model by several parity violating interactions between the gravitational field and a scalar field. We derive three different families of background solutions in flat FRW universe, with three classes of different connections. Through investigations on the linear cosmological perturbation… ▽ More In this paper, we consider a symmetric teleparallel gravity model that extends the general relativity equivalent model by several parity violating interactions between the gravitational field and a scalar field. We derive three different families of background solutions in flat FRW universe, with three classes of different connections. Through investigations on the linear cosmological perturbations, we show that one of the vector modes of this model will evolve into a ghost field at high energy, and the ghost instability can be cancelled only under specific combinations of the coefficients. On two of three families of backgrounds, such combination remains the same as the one we have investigated in our previous work; while on the other family of background, one additional condition should be taken into consider. △ Less

Submitted 21 May, 2025; originally announced May 2025.

Report number: USTC-ICTS/PCFT-25-20

Spacetime perturbations and quasi-teleparallel gravity

Authors: Jian Gao, Yuxuan Kang, Mingzhe Li, Yeheng Tong

Abstract: Gravity is identical to curved spacetime. It is manifested by the curvature of a Riemannian spacetime in general relativity but by torsion or non-metricity in teleparallel gravity models. In this paper, we apply these multiple options to the spacetime perturbation theory and seek the possibilities of representing the gravitation of the background and that of the perturbation in separate ways. We s… ▽ More Gravity is identical to curved spacetime. It is manifested by the curvature of a Riemannian spacetime in general relativity but by torsion or non-metricity in teleparallel gravity models. In this paper, we apply these multiple options to the spacetime perturbation theory and seek the possibilities of representing the gravitation of the background and that of the perturbation in separate ways. We show that the perturbation around a Riemannian background can be described by torsion or non-metricity, so that we have teleparallel like actions for the perturbation. △ Less

Submitted 16 July, 2025; v1 submitted 4 March, 2025; originally announced March 2025.

Comments: 8 pages, no figure. The version to appear in Chinese Physics C

Report number: USTC-ICTS/PCFT-25-07

Progress of the TianQin project

Authors: Jun Luo, Shaojun Bai, Yan-Zheng Bai, Lin Cai, Hao Dang, Qijia Dong, Hui-Zong Duan, Yuanbo Du, Lei Fan, Xinju Fu, Yong Gao, Xingyu Gou, Changlei Guo, Wei Hong, Bin Hu, Heran Hu, Ming Hu, Yi-Ming Hu, Fa Peng Huang, Defeng Gu, Xin Ji, Yuan-Ze Jiang, En-Kun Li, Hongyin Li, Ming Li , et al. (76 additional authors not shown)

Abstract: TianQin is a future space-based gravitational wave observatory targeting the frequency window of $10^{-4}$ Hz $\sim 1$ Hz. A large variety of gravitational wave sources are expected in this frequency band, including the merger of massive black hole binaries, the inspiral of extreme/intermediate mass ratio systems, stellar-mass black hole binaries, Galactic compact binaries, and so on. TianQin will… ▽ More TianQin is a future space-based gravitational wave observatory targeting the frequency window of $10^{-4}$ Hz $\sim 1$ Hz. A large variety of gravitational wave sources are expected in this frequency band, including the merger of massive black hole binaries, the inspiral of extreme/intermediate mass ratio systems, stellar-mass black hole binaries, Galactic compact binaries, and so on. TianQin will consist of three Earth orbiting satellites on nearly identical orbits with orbital radii of about $10^5$ km. The satellites will form a normal triangle constellation whose plane is nearly perpendicular to the ecliptic plane. The TianQin project has been progressing smoothly following the ``0123" technology roadmap. In step ``0", the TianQin laser ranging station has been constructed and it has successfully ranged to all the five retro-reflectors on the Moon. In step ``1", the drag-free control technology has been tested and demonstrated using the TianQin-1 satellite. In step ``2", the inter-satellite laser interferometry technology will be tested using the pair of TianQin-2 satellites. The TianQin-2 mission has been officially approved and the satellites will be launched around 2026. In step ``3", i.e., the TianQin-3 mission, three identical satellites will be launched around 2035 to form the space-based gravitational wave detector, TianQin, and to start gravitational wave detection in space. △ Less

Submitted 16 February, 2025; originally announced February 2025.

Comments: 45 pages, 3 figures

Possible consistent model of parity violations in the symmetric teleparallel gravity

Authors: Mingzhe Li, Yeheng Tong, Dehao Zhao

Abstract: Many parity violating gravity models suffer from the ghost instability problem. In this paper, we consider a symmetric teleparallel gravity model that extends the general relativity equivalent model by several parity violating interactions between the gravitational field and a scalar field. These interactions exclude higher derivatives and are quadratic in the nonmetricity tensor. Through investig… ▽ More Many parity violating gravity models suffer from the ghost instability problem. In this paper, we consider a symmetric teleparallel gravity model that extends the general relativity equivalent model by several parity violating interactions between the gravitational field and a scalar field. These interactions exclude higher derivatives and are quadratic in the nonmetricity tensor. Through investigations on the linear cosmological perturbations, our results show that, in general, this model suffers from the difficulty caused by the existence of ghost mode in the vector perturbations. However, in cases where a special condition is imposed on the coefficients of these parity violating interactions, this model can be ghost free. △ Less

Submitted 18 May, 2022; v1 submitted 14 March, 2022; originally announced March 2022.

Comments: arXiv admin note: text overlap with arXiv:2201.02357

Journal ref: Phys. Rev. D 105, 104002 (2022)

Revisiting a parity violating gravity model without ghost instability: Local Lorentz covariance

Authors: Mingzhe Li, Haomin Rao, Yeheng Tong

Abstract: Recently, based on the theory of teleparallel gravity, a simple and ghost free parity violating gravity model was proposed in [M. Li, H. Rao, and D. Zhao, J. Cosmol. Astropart. Phys. 11 (2020) 023], where the Weitzenböck connection was adopted for simplifying the calculations but breaks the local Lorentz symmetry explicitly. In this paper, we restore the local Lorentz symmetry of this model by giv… ▽ More Recently, based on the theory of teleparallel gravity, a simple and ghost free parity violating gravity model was proposed in [M. Li, H. Rao, and D. Zhao, J. Cosmol. Astropart. Phys. 11 (2020) 023], where the Weitzenböck connection was adopted for simplifying the calculations but breaks the local Lorentz symmetry explicitly. In this paper, we restore the local Lorentz symmetry of this model by giving up the Weitzenböck condition on the spin connection. With full local Lorentz covariance, this model is not a pure tetrad theory any more. We also apply the new version of this model to the universe with general Friedmann-Robertson-Walker background. This further generalizes the studies of [M. Li, H. Rao, and D. Zhao, J. Cosmol. Astropart. Phys. 11 (2020) 023] where only the spatially flat background was considered. Through the investigations of this paper, we confirm the results obtained in [M. Li, H. Rao, and D. Zhao, J. Cosmol. Astropart. Phys. 11 (2020) 023] and in addition get some new results. △ Less

Submitted 31 October, 2021; v1 submitted 12 April, 2021; originally announced April 2021.

Comments: 17 pages, 0 figures

Report number: USTC-ICTS/PCFT-21-17

Ion versus electron heating in compressively driven astrophysical gyrokinetic turbulence

Authors: Y. Kawazura, A. A. Schekochihin, M. Barnes, J. M. TenBarge, Y. Tong, K. G. Klein, W. Dorland

Abstract: The partition of irreversible heating between ions and electrons in compressively driven (but subsonic) collisionless turbulence is investigated by means of nonlinear hybrid gyrokinetic simulations. We derive a prescription for the ion-to-electron heating ratio $Q_\rmi/Q_\rme$ as a function of the compressive-to-Alfvénic driving power ratio $P_\compr/P_\AW$, of the ratio of ion thermal pressure to… ▽ More The partition of irreversible heating between ions and electrons in compressively driven (but subsonic) collisionless turbulence is investigated by means of nonlinear hybrid gyrokinetic simulations. We derive a prescription for the ion-to-electron heating ratio $Q_\rmi/Q_\rme$ as a function of the compressive-to-Alfvénic driving power ratio $P_\compr/P_\AW$, of the ratio of ion thermal pressure to magnetic pressure $β_\rmi$, and of the ratio of ion-to-electron background temperatures $T_\rmi/T_\rme$. It is shown that $Q_\rmi/Q_\rme$ is an increasing function of $P_\compr/P_\AW$. When the compressive driving is sufficiently large, $Q_\rmi/Q_\rme$ approaches $\simeq P_\compr/P_\AW$. This indicates that, in turbulence with large compressive fluctuations, the partition of heating is decided at the injection scales, rather than at kinetic scales. Analysis of phase-space spectra shows that the energy transfer from inertial-range compressive fluctuations to sub-Larmor-scale kinetic Alfvén waves is absent for both low and high $β_\rmi$, meaning that the compressive driving is directly connected to the ion entropy fluctuations, which are converted into ion thermal energy. This result suggests that preferential electron heating is a very special case requiring low $β_\rmi$ and no, or weak, compressive driving. Our heating prescription has wide-ranging applications, including to the solar wind and to hot accretion disks such as M87 and Sgr A*. △ Less

Submitted 23 October, 2020; v1 submitted 10 April, 2020; originally announced April 2020.

Comments: Accepted for publication in Phys. Rev. X

Journal ref: Phys. Rev. X 10, 041050 (2020)

Effects of electron drift on the collisionless damping of kinetic Alfvén waves in the solar wind

Authors: Yuguang Tong, Stuart D. Bale, Christopher H. K. Chen, Chadi S. Salem, Daniel Verscharen

Abstract: The collisionless dissipation of anisotropic Alfvénic turbulence is a promising candidate to solve the solar wind heating problem. Extensive studies examined the kinetic properties of Alfvén waves in simple Maxwellian or bi-Maxwellian plasmas. However, the observed electron velocity distribution functions in the solar wind are more complex. In this study, we analyze the properties of kinetic Alfvé… ▽ More The collisionless dissipation of anisotropic Alfvénic turbulence is a promising candidate to solve the solar wind heating problem. Extensive studies examined the kinetic properties of Alfvén waves in simple Maxwellian or bi-Maxwellian plasmas. However, the observed electron velocity distribution functions in the solar wind are more complex. In this study, we analyze the properties of kinetic Alfvén waves in a plasma with two drifting electron populations. We numerically solve the linearized Maxwell-Vlasov equations and find that the damping rate and the proton-electron energy partition for kinetic Alfvén waves are significantly modified in such plasmas, compared to plasmas without electron drifts. We suggest that electron drift is an important factor to take into account when considering the dissipation of Alfvénic turbulence in the solar wind or other $β\sim 1$ astrophysical plasmas. △ Less

Submitted 9 May, 2015; originally announced May 2015.

Journal ref: The Astrophysical Journal Letters, 804(2015) L36

Dual frequency 230/690 GHz interferometry at the Submillimeter Array

Authors: Todd R. Hunter, John W. Barrett, Raymond Blundell, Robert D. Christensen, Robert S. Kimberk, Steven P. Leiker, Daniel P. Marrone, Scott N. Paine, D. Cosmo Papa, Nimesh Patel, Patricia Riddle, Michael J. Smith, T. K. Sridharan, C. Y. Edward Tong, Ken H. Young, Jun-Hui Zhao

Abstract: The Submillimeter Array (SMA), a collaboration between the Smithsonian Astrophysical Observatory and the Academica Sinica Institute for Astronomy and Astrophysics of Taiwan, is an eight-element radio-interferometer designed to operate throughout the major atmospheric windows from about 180 to 900 GHz. In an effort to mitigate the effects of atmospheric instabilities which limit the phase coheren… ▽ More The Submillimeter Array (SMA), a collaboration between the Smithsonian Astrophysical Observatory and the Academica Sinica Institute for Astronomy and Astrophysics of Taiwan, is an eight-element radio-interferometer designed to operate throughout the major atmospheric windows from about 180 to 900 GHz. In an effort to mitigate the effects of atmospheric instabilities which limit the phase coherence of the array especially in the higher frequency bands, the array was designed to allow simultaneous operation of a low frequency receiver (<350 GHz) with a high frequency receiver (>330 GHz). The overlap region of 330-350 GHz was included to facilitate dual polarization measurements in the frequency range considered to offer the highest sensitivity for continuum observations with the array. So far, the array is equipped with working SIS receivers covering the frequency ranges 176-256 GHz, 260-350 GHz, and 600-700 GHz, and single frequency operation has been routine in the lower two frequency bands for the past year. More recently, with the completion of IF hardware required to make full use of the SMA cross-correlator, dual receiver operation became possible. We have since made a number of Galactic and extra-galactic astronomical observations in dual-band mode with the hopes of using the 230 GHz receiver as a phase reference to enable improved interferometry in the 650 GHz band. We will present the current antenna and receiver performance, some of the first interferometric images in the 650 GHz receiver band, and our initial attempts at phase transfer. △ Less

Submitted 15 September, 2005; originally announced September 2005.

Comments: 6 pages containing text and 11 embedded figures, written in the IEEE Transactions style Latex template, based on an Oral Presentation at the 16th International Symposium on Space Terahertz Technology held at Chalmers University of Technology in Goteborg, Sweden on May 2-4, 2005