Exploring the sensitivity of gravitational wave detectors to neutron star physics

被引：85

作者：

Martynov, Denis ^{[1
,2
]}

Miao, Haixing ^{[1
,2
]}

Yang, Huan ^{[3
,4
]}

Vivanco, Francisco Hernandez ^{[5
,6
]}

Thrane, Eric ^{[5
,6
]}

Smith, Rory ^{[5
,6
]}

Lasky, Paul ^{[5
,6
]}

East, William E. ^{[3
]}

Adhikari, Rana ^{[7
]}

Bauswein, Andreas ^{[8
,9
]}

Brooks, Aidan ^{[7
]}

Chen, Yanbei ^{[7
]}

Corbitt, Thomas ^{[10
]}

Freise, Andreas ^{[1
,2
]}

Grote, Hartmut ^{[11
]}

Levin, Yuri ^{[12
,13
,14
]}

Zhao, Chunnong ^{[6
,15
]}

Vecchio, Alberto ^{[1
,2
]}

机构：

[1] Univ Birmingham, Sch Phys & Astron, Birmingham B15 2TT, W Midlands, England

[2] Univ Birmingham, Inst Gravitat Wave Astron, Birmingham B15 2TT, W Midlands, England

[3] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada

[4] Univ Guelph, Guelph, ON N2L 3G1, Canada

[5] Monash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia

[6] OzGrav ARC Ctr Excellence Gravitat Wave Discovery, Clayton, Vic 3800, Australia

[7] CALTECH, LIGO, Pasadena, CA 91125 USA

[8] GSI Helmholtzzentrum Schwerionenforsch, Planckstrae 1, D-64291 Darmstadt, Germany

[9] Heidelberg Inst Theoret Studies, Schloss Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany

[10] Louisiana State Univ, Dept Phys & Astron, Baton Rouge, LA 70803 USA

[11] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales

[12] Columbia Univ, Dept Phys, 538 W 120th St, New York, NY 10027 USA

[13] Columbia Univ, Columbia Astrophys Lab, 538 W 120th St, New York, NY 10027 USA

[14] Flatiron Inst, Ctr Computat Astrophys, New York, NY 10010 USA

[15] Univ Western Australia, ARC Ctr Excellence Gravitat Wave Discovery, Crawley, WA 6009, Australia

来源：

PHYSICAL REVIEW D | 2019年 / 99卷 / 10期

基金：

加拿大自然科学与工程研究理事会; 欧洲研究理事会; 澳大利亚研究理事会; 美国国家科学基金会;

关键词：

ARMED SPIRAL INSTABILITY; MICHELSON INTERFEROMETER; DYNAMICAL INSTABILITIES; RADIATION-PRESSURE; LIGO; NOISE; EQUATION; MATTER;

D O I：

10.1103/PhysRevD.99.102004

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The physics of neutron stars can be studied with gravitational waves emitted from coalescing binary systems. Tidal effects become significant during the last few orbits and can be visible in the gravitational wave spectrum above 500 Hz. After the merger, the neutron star remnant oscillates at frequencies above 1 kHz and can collapse into a black hole. Gravitational wave detectors with a sensitivity of similar or equal to 10(-24) strain/root Hz at 2-4 kHz can observe these oscillations from a source which is approximately 100 Mpc away. The current observatories, such as LIGO and Virgo, are limited by shot noise at high frequencies and have a sensitivity of greater than or equal to 2 x 10(-23) strain/root Hz at 3 kHz. In this paper, we propose an optical configuration of gravitational wave detectors, which can be set up in present facilities using the current interferometer topology. This scheme has the potential to reach 7 x 10(-25) strain/root Hz at 2.5 kHz without compromising the detector sensitivity to black hole binaries. We argue that the proposed instruments have the potential to detect similar amount of postmerger neutron star oscillations as the next generation detectors, such as Cosmic Explorer and Einstein Telescope. We also optimize the arm length of the future detectors for neutron star physics and find that the optimal arm length is approximate to 20 km. These instruments have the potential to observe neutron star postmerger oscillations at a rate of approximately 30 events per year with a signal-to-noise ratio of 5 or more.

引用

页数：17

共 120 条

[1] Measurement of the Soft-Drop Jet Mass in pp Collisions at √s=13 TeV with the ATLAS Detector
Aaboud, M.
Aad, G.
Abbott, B.
Abdinov, O.
Abeloos, B.
Abidi, S. H.
AbouZeid, O. S.
Abraham, N. L.
Abramowicz, H.
Abreu, H.
Abreu, R.
Abulaiti, Y.
Acharya, B. S.
Adachi, S.
Adamczyk, L.
Adelman, J.
Adersberger, M.
Adye, T.
Affolder, A. A.
Afik, Y.
Agheorghiesei, C.
Aguilar-Saavedra, J. A.
Ahlen, S. P.
Ahmadov, F.
Aielli, G.
Akatsuka, S.
Akerstedt, H.
Akesson, T. P. A.
Akilli, E.
Akimov, A., V
Alberghi, G. L.
Albert, J.
Albicocco, P.
Alconada Verzini, M. J.
Alderweireldt, S. C.
Aleksa, M.
Aleksandrov, I. N.
Alexa, C.
Alexander, G.
Alexopoulos, T.
Alhroob, M.
Ali, B.
Aliev, M.
Alimonti, G.
Alison, J.
Alkire, S. P.
Allbrooke, B. M. M.
Allen, B. W.
Allport, P. P.
Aloisio, A.
[J]. PHYSICAL REVIEW LETTERS, 2018, 121 (09)
[2] Advanced LIGO
Aasi, J.
Abbott, B. P.
Abbott, R.
Abbott, T.
Abernathy, M. R.
Ackley, K.
Adams, C.
Adams, T.
Addesso, P.
Adhikari, R. X.
Adya, V.
Affeldt, C.
Aggarwal, N.
Aguiar, O. D.
Ain, A.
Ajith, P.
Alemic, A.
Allen, B.
Amariutei, D.
Anderson, S. B.
Anderson, W. G.
Arai, K.
Araya, M. C.
Arceneaux, C.
Areeda, J. S.
Ashton, G.
Ast, S.
Aston, S. M.
Aufmuth, P.
Aulbert, C.
Aylott, B. E.
Babak, S.
Baker, P. T.
Ballmer, S. W.
Barayoga, J. C.
Barbet, M.
Barclay, S.
Barish, B. C.
Barker, D.
Barr, B.
Barsotti, L.
Bartlett, J.
Barton, M. A.
Bartos, I.
Bassiri, R.
Batch, J. C.
Baune, C.
Behnke, B.
Bell, A. S.
Bell, C.
[J]. CLASSICAL AND QUANTUM GRAVITY, 2015, 32 (07)
[3] Aasi J, 2013, NAT PHOTONICS, V7, P613, DOI [10.1038/nphoton.2013.177, 10.1038/NPHOTON.2013.177]
[4] Abadie J, 2011, NAT PHYS, V7, P962, DOI [10.1038/NPHYS2083, 10.1038/nphys2083]
[5] Properties of the Binary Neutron Star Merger GW170817
Abbott, B. P.
Abbott, R.
Abbott, T. D.
Acernese, F.
Ackley, K.
Adams, C.
Adams, T.
Addesso, P.
Adhikari, R. X.
Adya, V. B.
Affeldt, C.
Agarwal, B.
Agathos, M.
Agatsuma, K.
Aggarwal, N.
Aguiar, O. D.
Aiello, L.
Ain, A.
Ajith, P.
Allen, B.
Allen, G.
Allocca, A.
Aloy, M. A.
Altin, P. A.
Amato, A.
Ananyeva, A.
Anderson, S. B.
Anderson, W. G.
Angelova, S., V
Antier, S.
Appert, S.
Arai, K.
Araya, M. C.
Areeda, J. S.
Arene, M.
Arnaud, N.
Arun, K. G.
Ascenzi, S.
Ashton, G.
Ast, M.
Aston, S. M.
Astone, P.
Atallah, D., V
Aubin, F.
Aufmuth, P.
Aulbert, C.
AultONeal, K.
Austin, C.
Avila-Alvarez, A.
Babak, S.
[J]. PHYSICAL REVIEW X, 2019, 9 (01):
[6] A gravitational-wave standard siren measurement of the Hubble constant
Abbott, B. P.
Abbott, R.
Abbott, T. D.
Acernese, F.
Ackley, K.
Adams, C.
Adams, T.
Addesso, P.
Adhikari, R. X.
Adya, V. B.
Affeldt, C.
Afrough, M.
Agarwal, B.
Agathos, M.
Agatsuma, K.
Aggarwal, N.
Aguiar, O. D.
Aiello, L.
Ain, A.
Ajith, P.
Allen, B.
Allen, G.
Allocca, A.
Altin, P. A.
Amato, A.
Ananyeva, A.
Anderson, S. B.
Anderson, W. G.
Angelova, S. V.
Antier, S.
Appert, S.
Arai, K.
Araya, M. C.
Areeda, J. S.
Arnaud, N.
Arun, K. G.
Ascenzi, S.
Ashton, G.
Ast, M.
Aston, S. M.
Astone, P.
Atallah, D. V.
Aufmuth, P.
Aulbert, C.
AultO'Neal, K.
Austin, C.
Avila-Alvarez, A.
Babak, S.
Bacon, P.
Bader, M. K. M.
[J]. NATURE, 2017, 551 (7678) : 85 - +
[7] Multi-messenger Observations of a Binary Neutron Star Merger
Abbott, B. P.
Abbott, R.
Abbott, T. D.
Acernese, F.
Ackley, K.
Adams, C.
Adams, T.
Addesso, P.
Adhikari, R. X.
Adya, V. B.
Affeldt, C.
Afrough, M.
Agarwal, B.
Agathos, M.
Agatsuma, K.
Aggarwal, N.
Aguiar, O. D.
Aiello, L.
Ain, A.
Ajith, P.
Allen, B.
Allen, G.
Allocca, A.
Altin, P. A.
Amato, A.
Ananyeva, A.
Anderson, S. B.
Anderson, W. G.
Angelova, S. V.
Antier, S.
Appert, S.
Arai, K.
Araya, M. C.
Areeda, J. S.
Arnaud, N.
Arun, K. G.
Ascenzi, S.
Ashton, G.
Ast, M.
Aston, S. M.
Astone, P.
Atallah, D. V.
Aufmuth, P.
Aulbert, C.
AultONeal, K.
Austin, C.
Avila-Alvarez, A.
Babak, S.
Bacon, P.
Bader, M. K. M.
[J]. ASTROPHYSICAL JOURNAL LETTERS, 2017, 848 (02)
[8] Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
Abbott, B. P.
Abbott, R.
Abbott, T. D.
Acernese, F.
Ackley, K.
Adams, C.
Adams, T.
Addesso, P.
Adhikari, R. X.
Adya, V. B.
Affeldt, C.
Afrough, M.
Agarwal, B.
Agathos, M.
Agatsuma, K.
Aggarwal, N.
Aguiar, O. D.
Aiello, L.
Ain, A.
Ajith, P.
Allen, B.
Allen, G.
Allocca, A.
Aloy, M. A.
Altin, P. A.
Amato, A.
Ananyeva, A.
Anderson, S. B.
Anderson, W. G.
Angelova, S. V.
Antier, S.
Appert, S.
Arai, K.
Araya, M. C.
Areeda, J. S.
Arnaud, N.
Arun, K. G.
Ascenzi, S.
Ashton, G.
Ast, M.
Aston, S. M.
Astone, P.
Atallah, D. V.
Aufmuth, P.
Aulbert, C.
AultONeal, K.
Austin, C.
Avila-Alvarez, A.
Babak, S.
Bacon, P.
[J]. ASTROPHYSICAL JOURNAL LETTERS, 2017, 848 (02)
[9] Exploring the sensitivity of next generation gravitational wave detectors
Abbott, B. P.
Abbott, R.
Abbott, T. D.
Abernathy, M. R.
Ackley, K.
Adams, C.
Addesso, P.
Adhikari, R. X.
Adya, V. B.
Affeldt, C.
Aggarwal, N.
Aguiar, O. D.
Ain, A.
Ajith, P.
Allen, B.
Altin, P. A.
Anderson, S. B.
Anderson, W. G.
Arai, K.
Araya, M. C.
Arceneaux, C. C.
Areeda, J. S.
Arun, K. G.
Ashton, G.
Ast, M.
Aston, S. M.
Aufmuth, P.
Aulbert, C.
Babak, S.
Baker, P. T.
Ballmer, S. W.
Barayoga, J. C.
Barclay, S. E.
Barish, B. C.
Barker, D.
Barr, B.
Barsotti, L.
Bartlett, J.
Bartos, I.
Bassiri, R.
Batch, J. C.
Baune, C.
Bell, A. S.
Berger, B. K.
Bergmann, G.
Berry, C. P. L.
Betzwieser, J.
Bhagwat, S.
Bhandare, R.
Bilenko, I. A.
[J]. CLASSICAL AND QUANTUM GRAVITY, 2017, 34 (04)
[10] Advanced Virgo: a second-generation interferometric gravitational wave detector
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.
[J]. CLASSICAL AND QUANTUM GRAVITY, 2015, 32 (02)

← 1 2 3 4 5 6 7 8 9 10 →