Approximate universal relations for neutron stars and quark stars

被引：288

作者：

Yagi, Kent ^{[1
,2
]}

Yunes, Nicolas ^{[2
]}

机构：

[1] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA

[2] Montana State Univ, Dept Phys, eXtreme Grav Inst, Bozeman, MT 59717 USA

来源：

PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS | 2017年 / 681卷

基金：

美国国家科学基金会;

关键词：

Neutron stars; Universal relations; No-hair theorem; X-ray; Gravitational wave; EQUATION-OF-STATE; ROTATING RELATIVISTIC STARS; INSPIRALING COMPACT BINARIES; TOROIDAL MAGNETIC-FIELDS; BLACK-HOLE CANDIDATES; GENERAL-RELATIVITY; GRAVITATIONAL-WAVES; MULTIPOLE MOMENTS; NUCLEAR-MATTER; DIFFERENTIAL ROTATION;

D O I：

10.1016/j.physrep.2017.03.002

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

Neutron stars and quark stars are ideal laboratories to study fundamental physics at supra nuclear densities and strong gravitational fields. Astrophysical observables, however, depend strongly on the star's internal structure, which is currently unknown due to uncertainties in the equation of state. Universal relations, however, exist among certain stellar observables that do not depend sensitively on the star's internal structure. One such set of relations is between the star's moment of inertia (I), its tidal Love number (Love) and its quadrupole moment (Q), the so-called I-Love-Q relations. Similar relations hold among the star's multipole moments, which resemble the well-known black hole no-hair theorems. Universal relations break degeneracies among astrophysical observables, leading to a variety of applications: (i) X-ray measurements of the nuclear matter equation of state, (ii) gravitational wave measurements of the intrinsic spin of inspiraling compact objects, and (iii) gravitational and astrophysical tests of General Relativity that are independent of the equation of state. We here review how the universal relations come about and all the applications that have been devised to date. (C) 2017 Elsevier B.V. All rights reserved.

引用

页码：1 / 72

页数：72

共 479 条

[1] Properties of the Binary Black Hole Merger GW150914 [J].

Abbott, B. P. ;

Abbott, R. ;

Abbott, T. D. ;

Abernathy, M. R. ;

Acernese, F. ;

Ackley, K. ;

Adams, C. ;

Adams, T. ;

Addesso, P. ;

Adhikari, R. X. ;

Adya, V. B. ;

Affeldt, C. ;

Agathos, M. ;

Agatsuma, K. ;

Aggarwal, N. ;

Aguiar, O. D. ;

Aiello, L. ;

Ain, A. ;

Ajith, P. ;

Allen, B. ;

Allocca, A. ;

Altin, P. A. ;

Anderson, S. B. ;

Anderson, W. G. ;

Arai, K. ;

Araya, M. C. ;

Arceneaux, C. C. ;

Areeda, J. S. ;

Arnaud, N. ;

Arun, K. G. ;

Ascenzi, S. ;

Ashton, G. ;

Ast, M. ;

Aston, S. M. ;

Astone, P. ;

Aufmuth, P. ;

Aulbert, C. ;

Babak, S. ;

Bacon, P. ;

Bader, M. K. M. ;

Baker, P. T. ;

Baldaccini, F. ;

Ballardin, G. ;

Ballmer, S. W. ;

Barayoga, J. C. ;

Barclay, S. E. ;

Barish, B. C. ;

Barker, D. ;

Barone, F. ;

Barr, B. .

PHYSICAL REVIEW LETTERS, 2016, 116 (24)

[2]

Abbott BP, 2018, PHYS REV LETT, V121, DOI [10.1103/PhysRevLett.121.129902, 10.1103/PhysRevLett.123.011102]

[3] Binary Black Hole Mergers in the First Advanced LIGO Observing Run [J].

Abbott, B. P. ;

Abbott, R. ;

Abbott, T. D. ;

Abernathy, M. R. ;

Acernese, F. ;

Ackley, K. ;

Adams, C. ;

Adams, T. ;

Addesso, P. ;

Adhikari, R. X. ;

Adya, V. B. ;

Affeldt, C. ;

Agathos, M. ;

Agatsuma, K. ;

Aggarwal, N. ;

Aguiar, O. D. ;

Aiello, L. ;

Ain, A. ;

Ajith, P. ;

Allen, B. ;

Allocca, A. ;

Altin, P. A. ;

Anderson, S. B. ;

Anderson, W. G. ;

Arai, K. ;

Araya, M. C. ;

Arceneaux, C. C. ;

Areeda, J. S. ;

Arnaud, N. ;

Arun, K. G. ;

Ascenzi, S. ;

Ashton, G. ;

Ast, M. ;

Aston, S. M. ;

Astone, P. ;

Aufmuth, P. ;

Aulbert, C. ;

Babak, S. ;

Bacon, P. ;

Bader, M. K. M. ;

Baker, P. T. ;

Baldaccini, F. ;

Ballardin, G. ;

Ballmer, S. W. ;

Barayoga, J. C. ;

Barclay, S. E. ;

Barish, B. C. ;

Barker, D. ;

Barone, F. ;

Barr, B. .

PHYSICAL REVIEW X, 2016, 6 (04)

[4] LIGO: the Laser Interferometer Gravitational-Wave Observatory [J].

Abbott, B. P. ;

Abbott, R. ;

Adhikari, R. ;

Ajith, P. ;

Allen, B. ;

Allen, G. ;

Amin, R. S. ;

Anderson, S. B. ;

Anderson, W. G. ;

Arain, M. A. ;

Araya, M. ;

Armandula, H. ;

Armor, P. ;

Aso, Y. ;

Aston, S. ;

Aufmuth, P. ;

Aulbert, C. ;

Babak, S. ;

Baker, P. ;

Ballmer, S. ;

Barker, C. ;

Barker, D. ;

Barr, B. ;

Barriga, P. ;

Barsotti, L. ;

Barton, M. A. ;

Bartos, I. ;

Bassiri, R. ;

Bastarrika, M. ;

Behnke, B. ;

Benacquista, M. ;

Betzwieser, J. ;

Beyersdorf, P. T. ;

Bilenko, I. A. ;

Billingsley, G. ;

Biswas, R. ;

Black, E. ;

Blackburn, J. K. ;

Blackburn, L. ;

Blair, D. ;

Bland, B. ;

Bodiya, T. P. ;

Bogue, L. ;

Bork, R. ;

Boschi, V. ;

Bose, S. ;

Brady, P. R. ;

Braginsky, V. B. ;

Brau, J. E. ;

Bridges, D. O. .

REPORTS ON PROGRESS IN PHYSICS, 2009, 72 (07)

[5]

Abbott B.P., 2016, Phys. Rev. Lett., V116, DOI DOI 10.1103/PHYSREVLETT.116.061102

[6] LIGO - THE LASER-INTERFEROMETER-GRAVITATIONAL-WAVE-OBSERVATORY [J].

ABRAMOVICI, A ;

ALTHOUSE, WE ;

DREVER, RWP ;

GURSEL, Y ;

KAWAMURA, S ;

RAAB, FJ ;

SHOEMAKER, D ;

SIEVERS, L ;

SPERO, RE ;

THORNE, KS ;

VOGT, RE ;

WEISS, R ;

WHITCOMB, SE ;

ZUCKER, ME .

SCIENCE, 1992, 256 (5055) :325-333

[7] Advanced Virgo: a second-generation interferometric gravitational wave detector [J].

Acernese, F. ;

Agathos, M. ;

Agatsuma, K. ;

Aisa, D. ;

Allemandou, N. ;

Allocca, A. ;

Amarni, J. ;

Astone, P. ;

Balestri, G. ;

Ballardin, G. ;

Barone, F. ;

Baronick, J-P ;

Barsuglia, M. ;

Basti, A. ;

Basti, F. ;

Bauer, Th S. ;

Bavigadda, V. ;

Bejger, M. ;

Beker, M. G. ;

Belczynski, C. ;

Bersanetti, D. ;

Bertolini, A. ;

Bitossi, M. ;

Bizouard, M. A. ;

Bloemen, S. ;

Blom, M. ;

Boer, M. ;

Bogaert, G. ;

Bondi, D. ;

Bondu, F. ;

Bonelli, L. ;

Bonnand, R. ;

Boschi, V. ;

Bosi, L. ;

Bouedo, T. ;

Bradaschia, C. ;

Branchesi, M. ;

Briant, T. ;

Brillet, A. ;

Brisson, V. ;

Bulik, T. ;

Bulten, H. J. ;

Buskulic, D. ;

Buy, C. ;

Cagnoli, G. ;

Calloni, E. ;

Campeggi, C. ;

Canuel, B. ;

Carbognani, F. ;

Cavalier, F. .

CLASSICAL AND QUANTUM GRAVITY, 2015, 32 (02)

[8]

Adam J, 2016, PHYS REV LETT, V116, DOI [10.1103/PhysRevLett.116.222302, 10.1103/PhysRevLett.116.241103]

[9] Planck 2015 results XIII. Cosmological parameters [J].

Ade, P. A. R. ;

Aghanim, N. ;

Arnaud, M. ;

Ashdown, M. ;

Aumont, J. ;

Baccigalupi, C. ;

Banday, A. J. ;

Barreiro, R. B. ;

Bartlett, J. G. ;

Bartolo, N. ;

Battaner, E. ;

Battye, R. ;

Benabed, K. ;

Benoit, A. ;

Benoit-Levy, A. ;

Bernard, J. -P. ;

Bersanelli, M. ;

Bielewicz, P. ;

Bock, J. J. ;

Bonaldi, A. ;

Bonavera, L. ;

Bond, J. R. ;

Borrill, J. ;

Bouchet, F. R. ;

Boulanger, F. ;

Bucher, M. ;

Burigana, C. ;

Butler, R. C. ;

Calabrese, E. ;

Cardoso, J. -F. ;

Catalano, A. ;

Challinor, A. ;

Chamballu, A. ;

Chary, R. -R. ;

Chiang, H. C. ;

Chluba, J. ;

Christensen, P. R. ;

Church, S. ;

Clements, D. L. ;

Colombi, S. ;

Colombo, L. P. L. ;

Combet, C. ;

Coulais, A. ;

Crill, B. P. ;

Curto, A. ;

Cuttaia, F. ;

Danese, L. ;

Davies, R. D. ;

Davis, R. J. ;

de Bernardis, P. .

ASTRONOMY & ASTROPHYSICS, 2016, 594

[10] Gravitational radiation detection with laser interferometry [J].

Adhikari, Rana X. .

REVIEWS OF MODERN PHYSICS, 2014, 86 (01) :121-151

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