Gravitational waveforms, polarizations, response functions, and energy losses of triple systems in Einstein-aether theory

被引:33
|
作者
Lin, Kai [1 ,2 ]
Zhao, Xiang [3 ,4 ]
Zhang, Chao [3 ,4 ]
Liu, Tan [5 ,6 ]
Wang, Bin [7 ,8 ]
Zhang, Shaojun [4 ]
Zhang, Xing [5 ,6 ]
Zhao, Wen [5 ,6 ]
Zhu, Tao [4 ]
Wang, Anzhong [3 ,4 ]
机构
[1] China Univ Geosci, Inst Geophys & Geomat, Hubei Subsurface Multiscale Imaging Key Lab, Wuhan 430074, Hubei, Peoples R China
[2] Univ Sao Paulo, Escola Engn Lorena, BR-12602810 Lorena, SP, Brazil
[3] Baylor Univ, Dept Phys, CASPER, GCAP, Waco, TX 76798 USA
[4] Zhejiang Univ Technol, Inst Adv Phys & Math, Hangzhou 310032, Zhejiang, Peoples R China
[5] Univ Sci & Technol China, Chinese Acad Sci, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei 230026, Anhui, Peoples R China
[6] Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Anhui, Peoples R China
[7] Yangzhou Univ, Ctr Gravitat & Cosmol, Yangzhou 225009, Jiangsu, Peoples R China
[8] Shanghai Jiao Tong Univ, Sch Phys & Astron, Shanghai 200240, Peoples R China
基金
中国国家自然科学基金;
关键词
GENERAL-RELATIVITY; MASS-DISTRIBUTION; 3-BODY PROBLEM; BLACK-HOLES; PULSAR; PERTURBATIONS; MECHANISM; RADIATION;
D O I
10.1103/PhysRevD.99.023010
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Gravitationally bound hierarchies containing three or more components are very common in our Universe. In this paper we study the periodic gravitational wave (GW) form, its polarizations, the response function, the Fourier transform, and the energy loss rate of a triple system through three different channels of radiation, the scalar, vector, and tensor modes, in the Einstein-aether theory of gravity. The theory violates locally the Lorentz symmetry, and yet satisfies all the theoretical and observational constraints by properly choosing its four coupling constants c(i)'s. In particular, in the weak-field approximations and with the recently obtained constraints of the theory, we first analyze the energy loss rate of a binary system and find that the dipole contributions from the scalar and vector modes could be of the order of O(c(14))O(G(N)m/d)(2), where c(14) (equivalent to c(1) + c(4)) is constrained to c(14) less than or similar to O(10(-5)) by current observations, and G(N), m, and d are, respectively, the Newtonian constant, mass, and size of the source. On the other hand, the "strong-field" effects for a binary system of neutron stars are about 6 orders lower than that of general relativity. So, in this paper we ignore these strong-field effects and first develop the general formulas to the lowest post-Newtonian order, by taking the coupling of the aether field with matter into account. Within this approximation, we find that the scalar breather mode and the scalar longitudinal mode are all suppressed by a factor of O(c(14)) with respect to the transverse-traceless modes (h(+) and h(x)), while the vectorial modes (h(X) and h(Y)) are suppressed by a factor of c(13) less than or similar to O(10(-15)). Applying the general formulas to a triple system with periodic orbits, we find that the corresponding GW form, the response function, and its Fourier transform depend sensitively on the configuration of the triple system, their orientation with respect to the detectors, and the binding energies of the three compact bodies.
引用
收藏
页数:23
相关论文
共 18 条
  • [1] Energy in the Einstein-aether theory
    Eling, C
    PHYSICAL REVIEW D, 2006, 73 (08):
  • [2] Gravitational plane waves in Einstein-aether theory
    Jacob Oost
    Madhurima Bhattacharjee
    Anzhong Wang
    General Relativity and Gravitation, 2018, 50
  • [3] Gravitational plane waves in Einstein-aether theory
    Oost, Jacob
    Bhattacharjee, Madhurima
    Wang, Anzhong
    GENERAL RELATIVITY AND GRAVITATION, 2018, 50 (10)
  • [4] Cylindrical gravitational waves in Einstein-Aether theory
    Chan, R.
    da Silva, M. F. A.
    Satheeshkumar, V. H.
    PHYSICA SCRIPTA, 2025, 100 (02)
  • [5] Numerical simulations of gravitational collapse in Einstein-aether theory
    Garfinkle, David
    Eling, Christopher
    Jacobson, Ted
    PHYSICAL REVIEW D, 2007, 76 (02)
  • [6] Gravitational spectrum of black holes in the Einstein-Aether theory
    Konoplya, R. A.
    Zhidenko, A.
    PHYSICS LETTERS B, 2007, 648 (2-3) : 236 - 239
  • [7] Gravitational quasinormal modes of black holes in Einstein-aether theory
    Ding, Chikun
    NUCLEAR PHYSICS B, 2019, 938 : 736 - 750
  • [8] Gravitational lenses in generalized Einstein-aether theory: The bullet cluster
    Dai, De-Chang
    Matsuo, Reijiro
    Starkman, Glenn
    PHYSICAL REVIEW D, 2008, 78 (10):
  • [9] Gravitational collapse and formation of universal horizons in Einstein-aether theory
    Bhattacharjee, Madhurima
    Mukohyama, Shinji
    Wan, Mew-Bing
    Wang, Anzhong
    PHYSICAL REVIEW D, 2018, 98 (06)
  • [10] Einstein-aether theory as an alternative to dark energy model?
    Meng, Xinhe
    Du, Xiaolong
    PHYSICS LETTERS B, 2012, 710 (4-5) : 493 - 499