Cosmology with the Laser Interferometer Space Antenna
Metadatos
Mostrar el registro completo del ítemEditorial
Springer Nature
Materia
Laser Interferometer Space Antenna (LISA) Cosmology
Fecha
2023-08-28Referencia bibliográfica
Auclair, P., Bacon, D., Baker, T. et al. Cosmology with the Laser Interferometer Space Antenna. Living Rev Relativ 26, 5 (2023). [https://doi.org/10.1007/s41114-023-00045-2]
Patrocinador
Atracción de Talento 2019-T1/TIC-13177; Centro de Excelencia Severo Ochoa Program EXC 2118/1, SEV-2016-0597; Contrato de Atracción de Talento 2017-T1/TIC-5520; European Union’s H2020 ERC GRAMS-815673; European Union’s Horizon 2020 Research Council 724659 MassiveCosmo ERC-2016-COG; European Union’s Horizon 2020 programme 860881, ITN HIDDeN; IFT Centro de Excelencia Severo Ochoa; Spanish Ministry MCIU PGC2018-094626-B-C21, PGC2018-096646-A-I00, PID2020-115845GB-I00/AEI/10.13039/501100011033; Horizon 2020 Framework Programme 796961 H2020; Comunidad de Madrid; Eusko Jaurlaritza IT-979-16; Ministerio de Economía y Competitividad 302640 MINECO; Generalitat Valenciana 758792, PROMETEO/2021/083 GVA; Ministerio de Ciencia e Innovación PID2020-113644GB-I00 MICINN; Ministerio de Universidades BG20/00228 MIU; European Union’s H2020 ERC, DarkGRA-757480Resumen
The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravitational-wave backgrounds and their implications for early universe and particle physics, from the MeV to the Planck scale. However, the range of potential cosmological applications of gravitational-wave observations extends well beyond these two objectives. This publication presents a summary of the state of the art in LISA cosmology, theory and methods, and identifies new opportunities to use gravitational-wave observations by LISA to probe the universe.