Parametric instability induced scalar gravitational waves from a model pulsating neutron star

被引：4
|
作者：
Wang, Charles H. -T. [1 ,2 ]
Bonifacio, Paolo M. [1 ]
Bingham, Robert [2 ,3 ]
Tito Mendonca, J. [2 ,4 ]
机构：
[1] Univ Aberdeen, Kings Coll, SUPA Dept Phys, Aberdeen AB24 3UE, Scotland
[2] STFC Rutherford Appleton Lab, Didcot OX11 0QX, Oxon, England
[3] Univ Strathclyde, SUPA Dept Phys, Glasgow G4 0NG, Lanark, Scotland
[4] Inst Super Tecn, GOLP Ctr Fis Plasmas, P-1049001 Lisbon, Portugal
来源：
PHYSICS LETTERS B | 2011年 / 705卷 / 1-2期
关键词：
Scalar-tensor gravity; Scalar waves; Pulsating stars; General relativity; GENERAL-RELATIVITY; MACHS PRINCIPLE; GRAVITY; INVARIANCE;
D O I：
10.1016/j.physletb.2011.09.111
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We identify a new dynamical mechanism for a strong scalar gravitational field effect. To illustrate this mechanism, we investigate the parametric excitation and emission of scalar gravitational waves by a radially pulsating model neutron star. (C) 2011 Elsevier B.V. All rights reserved.
引用
收藏
页码：148 / 151
页数：4
相关论文
共 50 条
  • [31] Projected constraints on scalarization with gravitational waves from neutron star binaries
    Sampson, Laura
    Yunes, Nicolas
    Cornish, Neil
    Ponce, Marcelo
    Barausse, Enrico
    Klein, Antoine
    Palenzuela, Carlos
    Lehner, Luis
    [J]. PHYSICAL REVIEW D, 2014, 90 (12):
  • [32] FIRST SEARCH FOR GRAVITATIONAL WAVES FROM THE YOUNGEST KNOWN NEUTRON STAR
    Abadie, J.
    Abbott, B. P.
    Abbott, R.
    Abernathy, M.
    Adams, C.
    Adhikari, R.
    Ajith, P.
    Allen, B.
    Allen, G.
    Ceron, E. Amador
    Amin, R. S.
    Anderson, S. B.
    Anderson, W. G.
    Arain, M. A.
    Araya, M.
    Aronsson, M.
    Aso, Y.
    Aston, S.
    Atkinson, D. E.
    Aufmuth, P.
    Aulbert, C.
    Babak, S.
    Baker, P.
    Ballmer, S.
    Barker, D.
    Barnum, S.
    Barr, B.
    Barriga, P.
    Barsotti, L.
    Barton, M. A.
    Bartos, I.
    Bassiri, R.
    Bastarrika, M.
    Bauchrowitz, J.
    Behnke, B.
    Benacquista, M.
    Bertolini, A.
    Betzwieser, J.
    Beveridge, N.
    Beyersdorf, P. T.
    Bilenko, I. A.
    Billingsley, G.
    Birch, J.
    Biswas, R.
    Black, E.
    Blackburn, J. K.
    Blackburn, L.
    Blair, D.
    Bland, B.
    Bock, O.
    [J]. ASTROPHYSICAL JOURNAL, 2010, 722 (02): : 1504 - 1513
  • [33] One-armed spiral instability in neutron star mergers and its detectability in gravitational waves
    Radice, David
    Bernuzzi, Sebastiano
    Ott, Christian D.
    [J]. PHYSICAL REVIEW D, 2016, 94 (06)
  • [34] Cosmic shear from scalar-induced gravitational waves
    Sarkar, Devdeep
    Serra, Paolo
    Cooray, Asantha
    Ichiki, Kiyotomo
    Baumann, Daniel
    [J]. PHYSICAL REVIEW D, 2008, 77 (10):
  • [35] Induced gravitational waves from statistically anisotropic scalar perturbations
    Chen, Chao
    Ota, Atsuhisa
    [J]. PHYSICAL REVIEW D, 2022, 106 (06)
  • [36] Probing the speed of scalar induced gravitational waves from observations
    Li, Jun
    Guo, Guang-Hai
    Zu, Yongcan
    [J]. European Physical Journal C, 2024, 84 (10):
  • [37] Breaking Strain of Neutron Star Crust and Gravitational Waves
    Horowitz, C. J.
    Kadau, Kai
    [J]. PHYSICAL REVIEW LETTERS, 2009, 102 (19)
  • [38] Assessment of Neutron Star Equation of State by Gravitational Waves
    Lee H.K.
    [J]. Physics of Particles and Nuclei Letters, 2018, 15 (4) : 343 - 347
  • [39] Parametric instability in the neutron star extreme matter observatory
    Pan, Juntao
    Zhang, Jue
    Blair, Carl
    Jones, Aaron W.
    Zhao, Chunnong
    Ju, Li
    [J]. CLASSICAL AND QUANTUM GRAVITY, 2022, 39 (08)
  • [40] Inferring neutron star properties with continuous gravitational waves
    Lu, Neil
    Wette, Karl
    Scott, Susan M.
    Melatos, Andrew
    [J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023, 521 (02) : 2103 - 2113
12345