Astrophysics with the Laser Interferometer Space Antenna

Pau Amaro-Seoane; Jeff Andrews; Manuel Arca Sedda; Abbas Askar; Quentin Baghi; Razvan Balasov; Imre Bartos; Simone S. Bavera; Jillian Bellovary; Christopher Philip Luke Berry; Emanuele Berti; Stefano Bianchi; Laura Blecha; Stéphane Blondin; Tamara Bogdanović; Samuel Boissier; Matteo Bonetti; Silvia Bonoli; Elisa Bortolas; Katelyn Breivik; Pedro R. Capelo; Laurentiu Caramete; Federico Cattorini; Maria Charisi; Sylvain Chaty; Xian Chen; Martyna Chruślińska; Alvin J.K. Chua; Ross Church; Monica Colpi; Daniel D’Orazio; Camilla Danielski; Melvyn B. Davies; Pratika Dayal; Alessandra De Rosa; Andrea Derdzinski; Kyriakos Destounis; Massimo Dotti; Ioana Duţan; Irina Dvorkin; Gaia Fabj; Thierry Foglizzo; Saavik Ford; Jean Baptiste Fouvry; Alessia Franchini; Tassos Fragos; Chris Fryer; Massimo Gaspari; Davide Gerosa; Luca Graziani; Paul Groot; Melanie Habouzit; Daryl Haggard; Zoltan Haiman; Wen Biao Han; Alina Istrate; Peter H. Johansson; Fazeel Mahmood Khan; Tomas Kimpson; Kostas Kokkotas; Albert Kong; Valeriya Korol; Kyle Kremer; Thomas Kupfer; Astrid Lamberts; Shane Larson; Mike Lau; Dongliang Liu; Nicole Lloyd-Ronning; Giuseppe Lodato; Alessandro Lupi; Chung Pei Ma; Tomas Maccarone; Ilya Mandel; Alberto Mangiagli; Michela Mapelli; Stéphane Mathis; Lucio Mayer; Sean McGee; Berry McKernan; M. Coleman Miller; David F. Mota; Matthew Mumpower; Syeda S. Nasim; Gijs Nelemans; Scott Noble; Fabio Pacucci; Francesca Panessa; Vasileios Paschalidis; Hugo Pfister; Delphine Porquet; John Quenby; Angelo Ricarte; Friedrich K. Röpke; John Regan; Stephan Rosswog; Ashley Ruiter; Milton Ruiz; Jessie Runnoe; Raffaella Schneider; Jeremy Schnittman; Amy Secunda; Alberto Sesana; Naoki Seto; Lijing Shao; Stuart Shapiro; Carlos Sopuerta; Nicholas C. Stone; Arthur Suvorov; Nicola Tamanini; Tomas Tamfal; Thomas Tauris; Karel Temmink; John Tomsick; Silvia Toonen; Alejandro Torres-Orjuela; Martina Toscani; Antonios Tsokaros; Caner Unal; Verónica Vázquez-Aceves; Rosa Valiante; Maurice van Putten; Jan van Roestel; Christian Vignali; Marta Volonteri; Kinwah Wu; Ziri Younsi; Shenghua Yu; Silvia Zane; Lorenz Zwick; Fabio Antonini; Vishal Baibhav; Enrico Barausse; Alexander Bonilla Rivera; Marica Branchesi; Graziella Branduardi-Raymont; Kevin Burdge; Srija Chakraborty; Jorge Cuadra; Kristen Dage; Benjamin Davis; Selma E. de Mink; Roberto Decarli; Daniela Doneva; Stephanie Escoffier; Poshak Gandhi; Francesco Haardt; Carlos O. Lousto; Samaya Nissanke; Jason Nordhaus; Richard O’Shaughnessy; Simon Portegies Zwart; Adam Pound; Fabian Schussler; Olga Sergijenko; Alessandro Spallicci; Daniele Vernieri; Alejandro Vigna-Gómez

doi:10.1007/s41114-022-00041-y

Astrophysics with the Laser Interferometer Space Antenna

Pau Amaro-Seoane, Jeff Andrews, Manuel Arca Sedda, Abbas Askar, Quentin Baghi, Razvan Balasov, Imre Bartos, Simone S. Bavera, Jillian Bellovary, Christopher Philip Luke Berry, Emanuele Berti, Stefano Bianchi, Laura Blecha, Stéphane Blondin, Tamara Bogdanović, Samuel Boissier, Matteo Bonetti, Silvia Bonoli, Elisa Bortolas, Katelyn BreivikPedro R. Capelo, Laurentiu Caramete, Federico Cattorini, Maria Charisi, Sylvain Chaty, Xian Chen, Martyna Chruślińska, Alvin J.K. Chua, Ross Church, Monica Colpi, Daniel D’Orazio, Camilla Danielski, Melvyn B. Davies, Pratika Dayal, Alessandra De Rosa, Andrea Derdzinski, Kyriakos Destounis, Massimo Dotti, Ioana Duţan, Irina Dvorkin, Gaia Fabj, Thierry Foglizzo, Saavik Ford, Jean Baptiste Fouvry, Alessia Franchini, Tassos Fragos, Chris Fryer, Massimo Gaspari, Davide Gerosa, Luca Graziani, Paul Groot, Melanie Habouzit, Daryl Haggard, Zoltan Haiman, Wen Biao Han, Alina Istrate, Peter H. Johansson, Fazeel Mahmood Khan, Tomas Kimpson, Kostas Kokkotas, Albert Kong, Valeriya Korol, Kyle Kremer, Thomas Kupfer, Astrid Lamberts, Shane Larson, Mike Lau, Dongliang Liu, Nicole Lloyd-Ronning, Giuseppe Lodato, Alessandro Lupi, Chung Pei Ma, Tomas Maccarone, Ilya Mandel, Alberto Mangiagli, Michela Mapelli, Stéphane Mathis, Lucio Mayer^*, Sean McGee, Berry McKernan, M. Coleman Miller, David F. Mota, Matthew Mumpower, Syeda S. Nasim, Gijs Nelemans, Scott Noble, Fabio Pacucci, Francesca Panessa, Vasileios Paschalidis, Hugo Pfister, Delphine Porquet, John Quenby, Angelo Ricarte, Friedrich K. Röpke, John Regan, Stephan Rosswog, Ashley Ruiter, Milton Ruiz, Jessie Runnoe, Raffaella Schneider, Jeremy Schnittman, Amy Secunda, Alberto Sesana, Naoki Seto, Lijing Shao, Stuart Shapiro, Carlos Sopuerta, Nicholas C. Stone, Arthur Suvorov, Nicola Tamanini, Tomas Tamfal, Thomas Tauris, Karel Temmink, John Tomsick, Silvia Toonen, Alejandro Torres-Orjuela, Martina Toscani, Antonios Tsokaros, Caner Unal, Verónica Vázquez-Aceves, Rosa Valiante, Maurice van Putten, Jan van Roestel, Christian Vignali, Marta Volonteri, Kinwah Wu, Ziri Younsi, Shenghua Yu, Silvia Zane, Lorenz Zwick, Fabio Antonini, Vishal Baibhav, Enrico Barausse, Alexander Bonilla Rivera, Marica Branchesi, Graziella Branduardi-Raymont, Kevin Burdge, Srija Chakraborty, Jorge Cuadra, Kristen Dage, Benjamin Davis, Selma E. de Mink, Roberto Decarli, Daniela Doneva, Stephanie Escoffier, Poshak Gandhi, Francesco Haardt, Carlos O. Lousto, Samaya Nissanke, Jason Nordhaus, Richard O’Shaughnessy, Simon Portegies Zwart, Adam Pound, Fabian Schussler, Olga Sergijenko, Alessandro Spallicci, Daniele Vernieri, Alejandro Vigna-Gómez

^*Corresponding author for this work

Research output: Contribution to journal › Review article › peer-review

214 Scopus citations

Abstract

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.

Original language	English (US)
Article number	2
Journal	Living Reviews in Relativity
Volume	26
Issue number	1
DOIs	https://doi.org/10.1007/s41114-022-00041-y
State	Published - Dec 2023

Funding

P. Dayal acknowledges support from the European Research council (ERC-717001) and from the Netherlands Research Council NWO (016.VIDI.189.162). P.H. Johansson acknowledges the support from the European Research Council (ERC-818930). S. Toonen acknowledges support from the Netherlands Research Council NWO (VENI 639.041.645 Grants) C. Unal is supported by European Structural and Investment Funds and the Czech Ministry of Education, Youth and Sports (Project CoGraDS - CZ.02.1.01/0.0/0.0/15_003/0000437). S. Chaty acknowledges the LabEx UnivEarthS for the funding of Interface project I10 \u201CFrom binary evolution towards merging of compact objects\u201D. A. De Rosa acknowledges financial contribution from the agreement ASI-INAF n.2017-14-H.O E. Berti is supported by NSF Grants No. PHY-1912550 and AST-2006538, NASA ATP Grants No. 17-ATP17-0225 and 19-ATP19-0051, NSF-XSEDE Grant No. PHY-090003, and NSF Grant PHY-20043. D. Gerosa is supported by European Union\u2019s H2020 ERC Starting Grant No. 945155\u2013GWmining, Leverhulme Trust Grant No. RPG-2019-350 and Royal Society Grant No. RGS-R2-202004. T. Bogdanovic acknowledges support by the NASA award No. 80NSSC19K0319 and by the NSF award AST-1908042. D. Porquet acknowledges funding support from CNES. C. Danielski acknowledges financial support from the State Agency for Research of the Spanish MCIU through the \u201CCenter of Excellence Severo Ochoa\u201D award to the Instituto de Astrof\u00EDsica de Andaluc\u00EDa (SEV-2017-0709) B.L. Davis acknowledges support from Tamkeen under the NYU Abu Dhabi Research Institute Grant CAP3. F. Pacucci acknowledges support from a Clay Fellowship by the SAO and from the Black Hole Initiative, which is funded by grants from the John Templeton Foundation and the Gordon and Betty Moore Foundation. A.J. Ruiter acknowledges support from the Australian Research Council Future Fellowship Grant FT170100243. V. Paschalidis is supported by NSF Grant PHY-1912619 and NASA Grant 80NSSC20K1542 to the University of Arizona, and NSF-XSEDE Grant TG-PHY190020. D. Haggard acknowledges support from the NSERC Discovery Grant and Canada Research Chairs programs, and the Bob Wares Science Innovation Prospectors Fund. M. Toscani acknowledges European Union\u2019s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie Grant Agreement No. 823823 (RISE DUSTBUSTERS project) and COST Action CA16104 - Gravitational waves, black holes and fundamental physics, supported by COST (European Cooperation in Science and Technology). M. Chruslinska, A. Istrate and G. Nelemans acknowledge support from Netherlands Research Council NWO. T. Fragos and S. Bavera acknowledge support from a Swiss National Science Foundation Professorship Grant (project numbers PP00P2_176868 and PP00P2_211006).

Keywords

Black holes
Extreme mass ratio in-spirals
Gravitational waves
Multi-messenger
Stellar remnants

ASJC Scopus subject areas

Physics and Astronomy (miscellaneous)

Access to Document

10.1007/s41114-022-00041-y

Cite this

Amaro-Seoane, P., Andrews, J., Arca Sedda, M., Askar, A., Baghi, Q., Balasov, R., Bartos, I., Bavera, S. S., Bellovary, J., Berry, C. P. L., Berti, E., Bianchi, S., Blecha, L., Blondin, S., Bogdanović, T., Boissier, S., Bonetti, M., Bonoli, S., Bortolas, E., ... Vigna-Gómez, A. (2023). Astrophysics with the Laser Interferometer Space Antenna. Living Reviews in Relativity, 26(1), Article 2. https://doi.org/10.1007/s41114-022-00041-y

@article{3135838a0a714d7b8600ba8000bbaabc,

title = "Astrophysics with the Laser Interferometer Space Antenna",

abstract = "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{\textquoteright}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.",

keywords = "Black holes, Extreme mass ratio in-spirals, Gravitational waves, Multi-messenger, Stellar remnants",

author = "Pau Amaro-Seoane and Jeff Andrews and {Arca Sedda}, Manuel and Abbas Askar and Quentin Baghi and Razvan Balasov and Imre Bartos and Bavera, {Simone S.} and Jillian Bellovary and Berry, {Christopher Philip Luke} and Emanuele Berti and Stefano Bianchi and Laura Blecha and St{\'e}phane Blondin and Tamara Bogdanovi{\'c} and Samuel Boissier and Matteo Bonetti and Silvia Bonoli and Elisa Bortolas and Katelyn Breivik and Capelo, {Pedro R.} and Laurentiu Caramete and Federico Cattorini and Maria Charisi and Sylvain Chaty and Xian Chen and Martyna Chru{\'s}li{\'n}ska and Chua, {Alvin J.K.} and Ross Church and Monica Colpi and Daniel D{\textquoteright}Orazio and Camilla Danielski and Davies, {Melvyn B.} and Pratika Dayal and {De Rosa}, Alessandra and Andrea Derdzinski and Kyriakos Destounis and Massimo Dotti and Ioana Du{\c t}an and Irina Dvorkin and Gaia Fabj and Thierry Foglizzo and Saavik Ford and Fouvry, {Jean Baptiste} and Alessia Franchini and Tassos Fragos and Chris Fryer and Massimo Gaspari and Davide Gerosa and Luca Graziani and Paul Groot and Melanie Habouzit and Daryl Haggard and Zoltan Haiman and Han, {Wen Biao} and Alina Istrate and Johansson, {Peter H.} and Khan, {Fazeel Mahmood} and Tomas Kimpson and Kostas Kokkotas and Albert Kong and Valeriya Korol and Kyle Kremer and Thomas Kupfer and Astrid Lamberts and Shane Larson and Mike Lau and Dongliang Liu and Nicole Lloyd-Ronning and Giuseppe Lodato and Alessandro Lupi and Ma, {Chung Pei} and Tomas Maccarone and Ilya Mandel and Alberto Mangiagli and Michela Mapelli and St{\'e}phane Mathis and Lucio Mayer and Sean McGee and Berry McKernan and Miller, {M. Coleman} and Mota, {David F.} and Matthew Mumpower and Nasim, {Syeda S.} and Gijs Nelemans and Scott Noble and Fabio Pacucci and Francesca Panessa and Vasileios Paschalidis and Hugo Pfister and Delphine Porquet and John Quenby and Angelo Ricarte and R{\"o}pke, {Friedrich K.} and John Regan and Stephan Rosswog and Ashley Ruiter and Milton Ruiz and Jessie Runnoe and Raffaella Schneider and Jeremy Schnittman and Amy Secunda and Alberto Sesana and Naoki Seto and Lijing Shao and Stuart Shapiro and Carlos Sopuerta and Stone, {Nicholas C.} and Arthur Suvorov and Nicola Tamanini and Tomas Tamfal and Thomas Tauris and Karel Temmink and John Tomsick and Silvia Toonen and Alejandro Torres-Orjuela and Martina Toscani and Antonios Tsokaros and Caner Unal and Ver{\'o}nica V{\'a}zquez-Aceves and Rosa Valiante and {van Putten}, Maurice and {van Roestel}, Jan and Christian Vignali and Marta Volonteri and Kinwah Wu and Ziri Younsi and Shenghua Yu and Silvia Zane and Lorenz Zwick and Fabio Antonini and Vishal Baibhav and Enrico Barausse and {Bonilla Rivera}, Alexander and Marica Branchesi and Graziella Branduardi-Raymont and Kevin Burdge and Srija Chakraborty and Jorge Cuadra and Kristen Dage and Benjamin Davis and {de Mink}, {Selma E.} and Roberto Decarli and Daniela Doneva and Stephanie Escoffier and Poshak Gandhi and Francesco Haardt and Lousto, {Carlos O.} and Samaya Nissanke and Jason Nordhaus and Richard O{\textquoteright}Shaughnessy and {Portegies Zwart}, Simon and Adam Pound and Fabian Schussler and Olga Sergijenko and Alessandro Spallicci and Daniele Vernieri and Alejandro Vigna-G{\'o}mez",

note = "Funding Information: P. Dayal acknowledges support from the European Research council (ERC-717001) and from the Netherlands Research Council NWO (016.VIDI.189.162). P.H. Johansson acknowledges the support from the European Research Council (ERC-818930). S. Toonen acknowledges support from the Netherlands Research Council NWO (VENI 639.041.645 Grants) C. Unal is supported by European Structural and Investment Funds and the Czech Ministry of Education, Youth and Sports (Project CoGraDS - CZ.02.1.01/0.0/0.0/15_003/0000437). S. Chaty acknowledges the LabEx UnivEarthS for the funding of Interface project I10 “From binary evolution towards merging of compact objects”. A. De Rosa acknowledges financial contribution from the agreement ASI-INAF n.2017-14-H.O E. Berti is supported by NSF Grants No. PHY-1912550 and AST-2006538, NASA ATP Grants No. 17-ATP17-0225 and 19-ATP19-0051, NSF-XSEDE Grant No. PHY-090003, and NSF Grant PHY-20043. D. Gerosa is supported by European Union{\textquoteright}s H2020 ERC Starting Grant No. 945155–GWmining, Leverhulme Trust Grant No. RPG-2019-350 and Royal Society Grant No. RGS-R2-202004. T. Bogdanovic acknowledges support by the NASA award No. 80NSSC19K0319 and by the NSF award AST-1908042. D. Porquet acknowledges funding support from CNES. C. Danielski acknowledges financial support from the State Agency for Research of the Spanish MCIU through the “Center of Excellence Severo Ochoa” award to the Instituto de Astrof{\'i}sica de Andaluc{\'i}a (SEV-2017-0709) B.L. Davis acknowledges support from Tamkeen under the NYU Abu Dhabi Research Institute Grant CAP3. F. Pacucci acknowledges support from a Clay Fellowship by the SAO and from the Black Hole Initiative, which is funded by grants from the John Templeton Foundation and the Gordon and Betty Moore Foundation. A.J. Ruiter acknowledges support from the Australian Research Council Future Fellowship Grant FT170100243. V. Paschalidis is supported by NSF Grant PHY-1912619 and NASA Grant 80NSSC20K1542 to the University of Arizona, and NSF-XSEDE Grant TG-PHY190020. D. Haggard acknowledges support from the NSERC Discovery Grant and Canada Research Chairs programs, and the Bob Wares Science Innovation Prospectors Fund. M. Toscani acknowledges European Union{\textquoteright}s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie Grant Agreement No. 823823 (RISE DUSTBUSTERS project) and COST Action CA16104 - Gravitational waves, black holes and fundamental physics, supported by COST (European Cooperation in Science and Technology). M. Chruslinska, A. Istrate and G. Nelemans acknowledge support from Netherlands Research Council NWO. T. Fragos and S. Bavera acknowledge support from a Swiss National Science Foundation Professorship Grant (project numbers PP00P2_176868 and PP00P2_211006). Publisher Copyright: {\textcopyright} 2023, The Author(s).",

year = "2023",

month = dec,

doi = "10.1007/s41114-022-00041-y",

language = "English (US)",

volume = "26",

journal = "Living Reviews in Relativity",

issn = "2367-3613",

publisher = "Albert Einstein Institut",

number = "1",

}

Amaro-Seoane, P, Andrews, J, Arca Sedda, M, Askar, A, Baghi, Q, Balasov, R, Bartos, I, Bavera, SS, Bellovary, J, Berry, CPL, Berti, E, Bianchi, S, Blecha, L, Blondin, S, Bogdanović, T, Boissier, S, Bonetti, M, Bonoli, S, Bortolas, E, Breivik, K, Capelo, PR, Caramete, L, Cattorini, F, Charisi, M, Chaty, S, Chen, X, Chruślińska, M, Chua, AJK, Church, R, Colpi, M, D’Orazio, D, Danielski, C, Davies, MB, Dayal, P, De Rosa, A, Derdzinski, A, Destounis, K, Dotti, M, Duţan, I, Dvorkin, I, Fabj, G, Foglizzo, T, Ford, S, Fouvry, JB, Franchini, A, Fragos, T, Fryer, C, Gaspari, M, Gerosa, D, Graziani, L, Groot, P, Habouzit, M, Haggard, D, Haiman, Z, Han, WB, Istrate, A, Johansson, PH, Khan, FM, Kimpson, T, Kokkotas, K, Kong, A, Korol, V, Kremer, K, Kupfer, T, Lamberts, A, Larson, S, Lau, M, Liu, D, Lloyd-Ronning, N, Lodato, G, Lupi, A, Ma, CP, Maccarone, T, Mandel, I, Mangiagli, A, Mapelli, M, Mathis, S, Mayer, L, McGee, S, McKernan, B, Miller, MC, Mota, DF, Mumpower, M, Nasim, SS, Nelemans, G, Noble, S, Pacucci, F, Panessa, F, Paschalidis, V, Pfister, H, Porquet, D, Quenby, J, Ricarte, A, Röpke, FK, Regan, J, Rosswog, S, Ruiter, A, Ruiz, M, Runnoe, J, Schneider, R, Schnittman, J, Secunda, A, Sesana, A, Seto, N, Shao, L, Shapiro, S, Sopuerta, C, Stone, NC, Suvorov, A, Tamanini, N, Tamfal, T, Tauris, T, Temmink, K, Tomsick, J, Toonen, S, Torres-Orjuela, A, Toscani, M, Tsokaros, A, Unal, C, Vázquez-Aceves, V, Valiante, R, van Putten, M, van Roestel, J, Vignali, C, Volonteri, M, Wu, K, Younsi, Z, Yu, S, Zane, S, Zwick, L, Antonini, F, Baibhav, V, Barausse, E, Bonilla Rivera, A, Branchesi, M, Branduardi-Raymont, G, Burdge, K, Chakraborty, S, Cuadra, J, Dage, K, Davis, B, de Mink, SE, Decarli, R, Doneva, D, Escoffier, S, Gandhi, P, Haardt, F, Lousto, CO, Nissanke, S, Nordhaus, J, O’Shaughnessy, R, Portegies Zwart, S, Pound, A, Schussler, F, Sergijenko, O, Spallicci, A, Vernieri, D & Vigna-Gómez, A 2023, 'Astrophysics with the Laser Interferometer Space Antenna', Living Reviews in Relativity, vol. 26, no. 1, 2. https://doi.org/10.1007/s41114-022-00041-y

TY - JOUR

T1 - Astrophysics with the Laser Interferometer Space Antenna

AU - Amaro-Seoane, Pau

AU - Andrews, Jeff

AU - Arca Sedda, Manuel

AU - Askar, Abbas

AU - Baghi, Quentin

AU - Balasov, Razvan

AU - Bartos, Imre

AU - Bavera, Simone S.

AU - Bellovary, Jillian

AU - Berry, Christopher Philip Luke

AU - Berti, Emanuele

AU - Bianchi, Stefano

AU - Blecha, Laura

AU - Blondin, Stéphane

AU - Bogdanović, Tamara

AU - Boissier, Samuel

AU - Bonetti, Matteo

AU - Bonoli, Silvia

AU - Bortolas, Elisa

AU - Breivik, Katelyn

AU - Capelo, Pedro R.

AU - Caramete, Laurentiu

AU - Cattorini, Federico

AU - Charisi, Maria

AU - Chaty, Sylvain

AU - Chen, Xian

AU - Chruślińska, Martyna

AU - Chua, Alvin J.K.

AU - Church, Ross

AU - Colpi, Monica

AU - D’Orazio, Daniel

AU - Danielski, Camilla

AU - Davies, Melvyn B.

AU - Dayal, Pratika

AU - De Rosa, Alessandra

AU - Derdzinski, Andrea

AU - Destounis, Kyriakos

AU - Dotti, Massimo

AU - Duţan, Ioana

AU - Dvorkin, Irina

AU - Fabj, Gaia

AU - Foglizzo, Thierry

AU - Ford, Saavik

AU - Fouvry, Jean Baptiste

AU - Franchini, Alessia

AU - Fragos, Tassos

AU - Fryer, Chris

AU - Gaspari, Massimo

AU - Gerosa, Davide

AU - Graziani, Luca

AU - Groot, Paul

AU - Habouzit, Melanie

AU - Haggard, Daryl

AU - Haiman, Zoltan

AU - Han, Wen Biao

AU - Istrate, Alina

AU - Johansson, Peter H.

AU - Khan, Fazeel Mahmood

AU - Kimpson, Tomas

AU - Kokkotas, Kostas

AU - Kong, Albert

AU - Korol, Valeriya

AU - Kremer, Kyle

AU - Kupfer, Thomas

AU - Lamberts, Astrid

AU - Larson, Shane

AU - Lau, Mike

AU - Liu, Dongliang

AU - Lloyd-Ronning, Nicole

AU - Lodato, Giuseppe

AU - Lupi, Alessandro

AU - Ma, Chung Pei

AU - Maccarone, Tomas

AU - Mandel, Ilya

AU - Mangiagli, Alberto

AU - Mapelli, Michela

AU - Mathis, Stéphane

AU - Mayer, Lucio

AU - McGee, Sean

AU - McKernan, Berry

AU - Miller, M. Coleman

AU - Mota, David F.

AU - Mumpower, Matthew

AU - Nasim, Syeda S.

AU - Nelemans, Gijs

AU - Noble, Scott

AU - Pacucci, Fabio

AU - Panessa, Francesca

AU - Paschalidis, Vasileios

AU - Pfister, Hugo

AU - Porquet, Delphine

AU - Quenby, John

AU - Ricarte, Angelo

AU - Röpke, Friedrich K.

AU - Regan, John

AU - Rosswog, Stephan

AU - Ruiter, Ashley

AU - Ruiz, Milton

AU - Runnoe, Jessie

AU - Schneider, Raffaella

AU - Schnittman, Jeremy

AU - Secunda, Amy

AU - Sesana, Alberto

AU - Seto, Naoki

AU - Shao, Lijing

AU - Shapiro, Stuart

AU - Sopuerta, Carlos

AU - Stone, Nicholas C.

AU - Suvorov, Arthur

AU - Tamanini, Nicola

AU - Tamfal, Tomas

AU - Tauris, Thomas

AU - Temmink, Karel

AU - Tomsick, John

AU - Toonen, Silvia

AU - Torres-Orjuela, Alejandro

AU - Toscani, Martina

AU - Tsokaros, Antonios

AU - Unal, Caner

AU - Vázquez-Aceves, Verónica

AU - Valiante, Rosa

AU - van Putten, Maurice

AU - van Roestel, Jan

AU - Vignali, Christian

AU - Volonteri, Marta

AU - Wu, Kinwah

AU - Younsi, Ziri

AU - Yu, Shenghua

AU - Zane, Silvia

AU - Zwick, Lorenz

AU - Antonini, Fabio

AU - Baibhav, Vishal

AU - Barausse, Enrico

AU - Bonilla Rivera, Alexander

AU - Branchesi, Marica

AU - Branduardi-Raymont, Graziella

AU - Burdge, Kevin

AU - Chakraborty, Srija

AU - Cuadra, Jorge

AU - Dage, Kristen

AU - Davis, Benjamin

AU - de Mink, Selma E.

AU - Decarli, Roberto

AU - Doneva, Daniela

AU - Escoffier, Stephanie

AU - Gandhi, Poshak

AU - Haardt, Francesco

AU - Lousto, Carlos O.

AU - Nissanke, Samaya

AU - Nordhaus, Jason

AU - O’Shaughnessy, Richard

AU - Portegies Zwart, Simon

AU - Pound, Adam

AU - Schussler, Fabian

AU - Sergijenko, Olga

AU - Spallicci, Alessandro

AU - Vernieri, Daniele

AU - Vigna-Gómez, Alejandro

N1 - Funding Information: P. Dayal acknowledges support from the European Research council (ERC-717001) and from the Netherlands Research Council NWO (016.VIDI.189.162). P.H. Johansson acknowledges the support from the European Research Council (ERC-818930). S. Toonen acknowledges support from the Netherlands Research Council NWO (VENI 639.041.645 Grants) C. Unal is supported by European Structural and Investment Funds and the Czech Ministry of Education, Youth and Sports (Project CoGraDS - CZ.02.1.01/0.0/0.0/15_003/0000437). S. Chaty acknowledges the LabEx UnivEarthS for the funding of Interface project I10 “From binary evolution towards merging of compact objects”. A. De Rosa acknowledges financial contribution from the agreement ASI-INAF n.2017-14-H.O E. Berti is supported by NSF Grants No. PHY-1912550 and AST-2006538, NASA ATP Grants No. 17-ATP17-0225 and 19-ATP19-0051, NSF-XSEDE Grant No. PHY-090003, and NSF Grant PHY-20043. D. Gerosa is supported by European Union’s H2020 ERC Starting Grant No. 945155–GWmining, Leverhulme Trust Grant No. RPG-2019-350 and Royal Society Grant No. RGS-R2-202004. T. Bogdanovic acknowledges support by the NASA award No. 80NSSC19K0319 and by the NSF award AST-1908042. D. Porquet acknowledges funding support from CNES. C. Danielski acknowledges financial support from the State Agency for Research of the Spanish MCIU through the “Center of Excellence Severo Ochoa” award to the Instituto de Astrofísica de Andalucía (SEV-2017-0709) B.L. Davis acknowledges support from Tamkeen under the NYU Abu Dhabi Research Institute Grant CAP3. F. Pacucci acknowledges support from a Clay Fellowship by the SAO and from the Black Hole Initiative, which is funded by grants from the John Templeton Foundation and the Gordon and Betty Moore Foundation. A.J. Ruiter acknowledges support from the Australian Research Council Future Fellowship Grant FT170100243. V. Paschalidis is supported by NSF Grant PHY-1912619 and NASA Grant 80NSSC20K1542 to the University of Arizona, and NSF-XSEDE Grant TG-PHY190020. D. Haggard acknowledges support from the NSERC Discovery Grant and Canada Research Chairs programs, and the Bob Wares Science Innovation Prospectors Fund. M. Toscani acknowledges European Union’s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie Grant Agreement No. 823823 (RISE DUSTBUSTERS project) and COST Action CA16104 - Gravitational waves, black holes and fundamental physics, supported by COST (European Cooperation in Science and Technology). M. Chruslinska, A. Istrate and G. Nelemans acknowledge support from Netherlands Research Council NWO. T. Fragos and S. Bavera acknowledge support from a Swiss National Science Foundation Professorship Grant (project numbers PP00P2_176868 and PP00P2_211006). Publisher Copyright: © 2023, The Author(s).

PY - 2023/12

Y1 - 2023/12

N2 - 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.

AB - 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.

KW - Black holes

KW - Extreme mass ratio in-spirals

KW - Gravitational waves

KW - Multi-messenger

KW - Stellar remnants

UR - http://www.scopus.com/inward/record.url?scp=85150880633&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85150880633&partnerID=8YFLogxK

U2 - 10.1007/s41114-022-00041-y

DO - 10.1007/s41114-022-00041-y

M3 - Review article

AN - SCOPUS:85150880633

SN - 2367-3613

VL - 26

JO - Living Reviews in Relativity

JF - Living Reviews in Relativity

IS - 1

M1 - 2

ER -

Astrophysics with the Laser Interferometer Space Antenna

Abstract

Funding

Keywords

ASJC Scopus subject areas

Access to Document

Other files and links

Fingerprint

Cite this