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Cosmology with the Laser Interferometer Space Antenna

dc.contributor.authorAuclair, Pierre
dc.contributor.authorBacon, David
dc.contributor.authorBaker, Tessa
dc.contributor.authorBarreiro, Tiago
dc.contributor.authorBartolo, Nicola
dc.contributor.authorBelgacem, Enis
dc.contributor.authorBellomo, Nicola
dc.contributor.authorBen-Dayan, Ido
dc.contributor.authorBertacca, Daniele
dc.contributor.authorBesancon, Marc
dc.contributor.authorBlanco-Pillado, Jose J.
dc.contributor.authorBlas, Diego
dc.contributor.authorBoileau, Guillaume
dc.contributor.authorCalcagni, Gianluca
dc.contributor.authorCaldwell, Robert
dc.contributor.authorCaprini, Chiara
dc.contributor.authorCarbone, Carmelita
dc.contributor.authorChang, Chia-Feng
dc.date.accessioned2023-10-06T19:14:16Z
dc.date.available2023-10-06T19:14:16Z
dc.date.issued2023-08-28
dc.identifier.urihttps://hdl.handle.net/1721.1/152389
dc.description.abstractAbstract 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.en_US
dc.publisherSpringer International Publishingen_US
dc.relation.isversionofhttps://doi.org/10.1007/s41114-023-00045-2en_US
dc.rightsCreative Commons Attributionen_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.sourceSpringer International Publishingen_US
dc.titleCosmology with the Laser Interferometer Space Antennaen_US
dc.typeArticleen_US
dc.identifier.citationLiving Reviews in Relativity. 2023 Aug 28;26(1):5en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physics
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Research
dc.identifier.mitlicensePUBLISHER_CC
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2023-09-03T03:08:58Z
dc.language.rfc3066en
dc.rights.holderSpringer Nature Switzerland AG
dspace.embargo.termsN
dspace.date.submission2023-09-03T03:08:57Z
mit.licensePUBLISHER_CC
mit.metadata.statusAuthority Work and Publication Information Neededen_US


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