Accès ouvert déclaré
2022
preprint
Astrophysics with the Laser Interferometer Space Antenna
Pau Amaro‐Seoane, Jeff J. Andrews, Manuel Arca Sedda, Abbas Askar, Razvan Balasov, I. Bartos, Simone S. Bavera, Jillian Bellovary, C. P. L. Berry, Emanuele Berti, S. Bianchi, Laura Blecha, S. Blondin, Tamara Bogdanović, S. Boissier, Matteo Bonetti, Silvia Bonoli, Elisa Bortolas, Pedro R. Capelo, Maria Charisi, S. Chaty, Xian Chen, Martyna Chruślińska, Alvin J. K. Chua, Ross P. Church, Monica Colpi, Camilla Danielski, M. B. Davies, Pratika Dayal, Alessandra De Rosa, Andrea Derdzinski, Kyriakos Destounis, Massimo Dotti, I. Duţan, Irina Dvorkin, Gaia Fabj, T. Foglizzo, K. E. Saavik Ford, Jean-Baptiste Fouvry, Chris L. Fryer, M. Gaspari, Davide Gerosa, Luca Graziani, P. Groot, Mélanie Habouzit, Daryl Haggard, Zoltán Haiman, Wen-Biao Han, Alina Istrate, Peter H. Johansson, Fazeel Mahmood Khan, T. Kimpson, Kostas D. Kokkotas, A. K. H. Kong, Valeriya Korol, Kyle Kremer, Thomas Kupfer, A. Lamberts, Shane L. Larson, Mike Lau, Dongliang Liu, Nicole Lloyd-Ronning, Giuseppe Lodato, Alessandro Lupi, Chung‐Pei Ma, Tomas Maccarone, Ilya Mandel, Alberto Mangiagli, Michela Mapelli, Lucio Mayer, Sean McGee, M. Coleman Miller, David F. Mota, Matthew R. Mumpower, Syeda S. Nasim, G. Nelemans, Scott C. Noble, Fabio Pacucci, F. Panessa, Hugo Pfister, D. Porquet, J. J. Quenby, John W. Regan, Stephan Rosswog, Ashley J. Ruiter, Milton Ruiz, Jessie C. Runnoe, Jeremy D. Schnittman, Amy Secunda, Alberto Sesana, Naoki Seto, Lijing Shao, Stuart L. Shapiro, Carlos F. Sopuerta, Arthur G. Suvorov, Nicola Tamanini, Tomas Tamfal, Thomas M. Tauris, Karel Temmink, John A. Tomsick, Silvia Toonen, Alejandro Torres-Orjuela, Martina Toscani, Antonios Tsokaros, Caner Ünal, 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, M. Branchesi, G. Branduardi‐Raymont, Kevin B. Burdge, Srija Chakraborty, Jorge Cuadra, Kristen C. Dage, Benjamin L. Davis, S. E. de Mink, Roberto Decarli, Daniela D. Doneva, S. Escoffier, P. Gandhi, Francesco Haardt, Carlos O. Lousto, S. Nissanke, Jason Nordhaus, R. O’Shaughnessy, Simon Portegies Zwart, Adam Pound, F. Schüßler, O. Sergijenko, A. Spallicci, Alejandro Vigna-Gómez
21Citations signalées, ce qui n’est pas une note de qualité
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Le résumé fourni par la source
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; ultracompact stellar-mass binaries, massive black hole binaries, and extreme or intermediate 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.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
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