Astrophysics with the Laser Interferometer Space Antenna

被引：276

作者：

Amaro-Seoane, Pau ^{[1
,2
,3
,4
,5
,184
]}

Andrews, Jeff ^{[6
,7
]}

Sedda, Manuel Arca ^{[8
]}

Askar, Abbas. ^{[9
]}

Baghi, Quentin ^{[10
]}

Balasov, Razvan ^{[11
,12
]}

Bartos, Imre ^{[13
]}

Bavera, Simone S. ^{[14
,15
]}

Bellovary, Jillian ^{[16
,17
,18
]}

Berry, Christopher P. L. ^{[6
,7
,19
]}

Berti, Emanuele ^{[20
]}

Bianchi, Stefano ^{[21
]}

Blecha, Laura ^{[13
]}

Blondin, Stephane ^{[22
]}

Bogdanovic, Tamara ^{[23
,24
]}

Boissier, Samuel ^{[22
]}

Bonetti, Matteo ^{[25
]}

Bonoli, Silvia ^{[26
,27
]}

Bortolas, Elisa ^{[25
,28
]}

Breivik, Katelyn ^{[178
]}

Capelo, Pedro R. ^{[29
]}

Caramete, Laurentiu ^{[11
]}

Cattorini, Federico ^{[25
,28
,30
]}

Charisi, Maria ^{[31
]}

Chaty, Sylvain ^{[32
]}

Chen, Xian ^{[33
]}

Chruslinska, Martyna ^{[34
]}

Chua, Alvin J. K. ^{[35
]}

Church, Ross ^{[36
]}

Colpi, Monica ^{[37
]}

D'Orazio, Daniel ^{[38
]}

Danielski, Camilla ^{[39
]}

Davies, Melvyn B. ^{[40
]}

Dayal, Pratika ^{[41
]}

De Rosa, Alessandra ^{[42
]}

Derdzinski, Andrea ^{[29
]}

Destounis, Kyriakos ^{[43
]}

Dotti, Massimo ^{[25
,28
,44
]}

Dutan, Ioana ^{[45
]}

Dvorkin, Irina ^{[46
,47
]}

Fabj, Gaia ^{[48
,49
]}

Foglizzo, Thierry ^{[50
]}

Ford, Saavik ^{[51
,52
,53
,54
]}

Fouvry, Jean-Baptiste ^{[55
,56
]}

Franchini, Alessia ^{[25
,28
]}

Fragos, Tassos ^{[15
,57
]}

Fryer, Chris ^{[58
]}

Gaspari, Massimo ^{[59
,60
]}

Gerosa, Davide ^{[25
,28
,61
]}

Graziani, Luca ^{[29
,62
,63
,64
]}

机构：

[1] Univ Politecn Valencia, Inst Multidisciplinary Math, Valencia, Spain

[2] Lanzhou Univ, Sch Phys Sci & Technol, Lanzhou Ctr Theoret Phys, Key Lab Theoret Phys Gansu Prov, Lanzhou 730000, Peoples R China

[3] Lanzhou Univ, Inst Theoret Phys, Lanzhou 730000, Peoples R China

[4] Lanzhou Univ, Res Ctr Gravitat, Lanzhou 730000, Peoples R China

[5] Kavli Inst Astron & Astrophys, Beijing, Peoples R China

[6] CIERA, Evanston, IL USA

[7] Northwestern Univ, Dept Phys & Astron, 1800 Sherman Ave, Evanston, IL 60201 USA

[8] Heidelberg Univ, Astronom Rechen Inst, Heidelberg, Germany

[9] Lund Univ, Dept Astron & Theoret Phys, Lund Observ, Box 43, S-22100 Lund, Sweden

[10] Univ Paris Saclay, IRFU, CEA, F-91191 Gif Sur Yvette, France

[11] Inst Space Sci, Magurele, Romania

[12] Univ Bucharest, Fac Phys, Bucharest, Romania

[13] Univ Florida, Dept Phys, POB 118440, Gainesville, FL 32611 USA

[14] Univ Geneva, Observ Geneva, Chemin Pegasi 51, Geneva, Switzerland

[15] Univ Geneva, GWSC, CH-1211 Geneva, Switzerland

[16] CUNY Queensborough Community Coll, Queens, NY USA

[17] Amer Museum Nat Hist, New York, NY USA

[18] CUNY Grad Ctr, New York, NY USA

[19] Univ Glasgow, Sch Phys & Astron, SUPA, Kelvin Bldg,Univ Ave, Glasgow G12 8QQ, Lanark, Scotland

[20] Johns Hopkins Univ, Baltimore, MD USA

[21] Univ Rome Tre, Dipartimento Matemat & Fis, Via Vasca Navale 84, I-00146 Rome, Italy

[22] Aix Marseille Univ, CNRS, CNES, LAM, Marseille, France

[23] Georgia Inst Technol, Sch Phys, 837 State St NW, Atlanta, GA 30332 USA

[24] Georgia Inst Technol, Ctr Relativist Astrophys, 837 State St NW, Atlanta, GA 30332 USA

[25] Univ Milano Bicocca, Dipartimento Fis G Occhialini, Piazza Sci 3, I-20126 Milan, Italy

[26] DIPC, Paseo Manuel Lardizabal 4, Donostia San Sebastian 20018, Spain

[27] IKERBASQUE, Basque Fdn Sci, Bilbao 48013, Spain

[28] INFN, Sez Milano Bicocca, Piazza Sci 3, I-20126 Milan, Italy

[29] Univ Zurich, Inst Computat Sci, Ctr Theoret Astrophys & Cosmol, Winterthurerstr 190, CH-8057 Zurich, Switzerland

[30] Univ Insubria, DiSAT, Via Valleggio 11, I-22100 Como, Italy

[31] Vanderbilt Univ, Dept Phys & Astron, 2301 Vanderbilt Pl, Nashville, TN 37235 USA

[32] Univ Paris, CNRS, AstroParticule & Cosmol, F-75013 Paris, France

[33] Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China

[34] Radboud Univ Nijmegen, Dept Astrophys IMAPP, POB 9010, NL-6500 GL Nijmegen, Netherlands

[35] CALTECH, Theoret Astrophys Grp, Pasadena, CA 91125 USA

[36] Lund Observ, Lund, Sweden

[37] Univ Milano Bicocca, Dept Phys, Milan, Italy

[38] Niels Bohr Int Acad, Niels Bohr Inst, Blegdamsvej 17, DK-2100 Copenhagen, Denmark

[39] Inst Astrofis Andalucia IAA CSIC, Glorieta Astron S-N, Granada 18008, Spain

[40] Lund Univ, Ctr Math Sci, Box 118, S-22100 Lund, Sweden

[41] Univ Groningen, Kapteyn Astron Inst, POB 800, NL-9700 AV Groningen, Netherlands

[42] INAF Ist Astrofis & Planetol Spaziali, Via Fosso Cavaliere 133, Rome, Italy

[43] Univ Tubingen, Theoret Astrophys, IAAT, D-72076 Tubingen, Germany

[44] INAF, Osservatorio Astron Brera, Via E Bianchi 46, I-23807 Merate, Italy

[45] Inst Space Sci, Atomistilor 409, Magurele 077125, Romania

[46] Sorbonne Univ, Inst Astrophys Paris, 98 Bis Bd Arago, F-75014 Paris, France

[47] CNRS, UMR 7095, 98 Bis Bd Arago, F-75014 Paris, France

[48] Heidelberg Univ, Astronom Rechen Inst, Zentrum Astron, D-69120 Heidelberg, Germany

[49] Amer Museum Nat Hist, Dept Astrophys, New York, NY 10024 USA

[50] Univ Paris Saclay, Univ Paris Diderot, CNRS, AIM,CEA,Sorbonne Paris Cite, F-91191 Gif Sur Yvette, France

来源：

LIVING REVIEWS IN RELATIVITY | 2023年 / 26卷 / 01期

基金：

欧盟地平线“2020”; 澳大利亚研究理事会; 欧洲研究理事会; 瑞士国家科学基金会; 加拿大自然科学与工程研究理事会;

关键词：

Black holes; Gravitational waves; Stellar remnants; Multi-messenger; Extreme mass ratio in-spirals; MASSIVE BLACK-HOLE; X-RAY BINARIES; ACTIVE GALACTIC NUCLEI; MOCCA-SURVEY DATABASE; WHITE-DWARF BINARIES; AM-CVN STARS; GRAVITATIONAL-WAVE SOURCES; COMMON-ENVELOPE EVOLUTION; TIDAL DISRUPTION EVENTS; DOUBLE NEUTRON-STARS;

D O I：

10.1007/s41114-022-00041-y

中图分类号：

O412 [相对论、场论]; O572.2 [粒子物理学];

学科分类号：

摘要：

The Laser Interferometer Space Antenna (LISA) will be a transformative experiment for gravitational wave astronomy, and, as such, it will offer unique opportunities to address many key astrophysical questions in a completely novel way. The synergy with ground-based and space-born instruments in the electromagnetic domain, by enabling multi-messenger observations, will add further to the discovery potential of LISA. The next decade is crucial to prepare the astrophysical community for LISA's first observations. This review outlines the extensive landscape of astrophysical theory, numerical simulations, and astronomical observations that are instrumental for modeling and interpreting the upcoming LISA datastream. To this aim, the current knowledge in three main source classes for LISA is reviewed; ultra-compact stellar-mass binaries, massive black hole binaries, and extreme or interme-diate mass ratio inspirals. The relevant astrophysical processes and the established modeling techniques are summarized. Likewise, open issues and gaps in our understanding of these sources are highlighted, along with an indication of how LISA could help making progress in the different areas. New research avenues that LISA itself, or its joint exploitation with upcoming studies in the electromagnetic domain, will enable, are also illustrated. Improvements in modeling and analysis approaches, such as the combination of numerical simulations and modern data science techniques, are discussed. This review is intended to be a starting point for using LISA as a new discovery tool for understanding our Universe.

引用

页数：328

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