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Unveiling the gravitational universe at μ-Hz frequencies

dc.contributor.authorSesana, Alberto
dc.contributor.authorKorsakova, Natalia
dc.contributor.authorSedda, Manuel Arca
dc.contributor.authorBaibhav, Vishal
dc.contributor.authorBarausse, Enrico
dc.contributor.authorBarke, Simon
dc.contributor.authorBerti, Emanuele
dc.contributor.authorBonetti, Matteo
dc.contributor.authorCapelo, Pedro R.
dc.contributor.authorCaprini, Chiara
dc.contributor.authorGarcia-Bellido, Juan
dc.contributor.authorHaiman, Zoltan
dc.contributor.authorJani, Karan
dc.contributor.authorJennrich, Oliver
dc.contributor.authorJohansson, Peter H.
dc.contributor.authorKhan, Fazeel Mahmood
dc.contributor.authorKorol, Valeriya
dc.contributor.authorLamberts, Astrid
dc.contributor.authorLupi, Alessandro
dc.contributor.authorMangiagli, Alberto
dc.contributor.authorMayer, Lucio
dc.contributor.authorNardini, Germano
dc.contributor.authorPacucci, Fabio
dc.contributor.authorPetiteau, Antoine
dc.contributor.authorRaccanelli, Alvise
dc.contributor.authorRajendran, Surjeet
dc.contributor.authorRegan, John
dc.contributor.authorShao, Lijing
dc.contributor.authorSpallicci, Alessandro
dc.contributor.authorTamanini, Nicola
dc.contributor.authorVolonteri, Marta
dc.contributor.authorWarburton, Niels
dc.contributor.authorWong, Kaze
dc.contributor.authorZumalacárregui, Miguel
dc.date.accessioned2022-01-07T10:08:22Z
dc.date.available2022-01-07T10:08:22Z
dc.date.created2021-10-15T13:33:23Z
dc.date.issued2021
dc.identifier.citationSesana, A., Korsakova, N., Sedda, M. A.. Baibhav, V., Barausse, E., Barke, S., Berti, E. Bonetti, M., Capelo, P. R., Caprini, C., Garcia-Bellido, J., Haiman, Z., Jani, K., Jennrich, O., Johansson, P. H., Khan, F. M., Korol, V., Lamberts, A., Lupi, A. (…) , Zumalacárregui, M. (2021) Unveiling the gravitational universe at μ-Hz frequencies. Experimental Astronomy volume 51, 1333–1383en_US
dc.identifier.issn0922-6435
dc.identifier.urihttps://hdl.handle.net/11250/2836466
dc.description.abstractWe propose a space-based interferometer surveying the gravitational wave (GW) sky in the milli-Hz to μ-Hz frequency range. By the 2040s, the μ-Hz frequency band, bracketed in between the Laser Interferometer Space Antenna (LISA) and pulsar timing arrays, will constitute the largest gap in the coverage of the astrophysically relevant GW spectrum. Yet many outstanding questions related to astrophysics and cosmology are best answered by GW observations in this band. We show that a μ-Hz GW detector will be a truly overarching observatory for the scientific community at large, greatly extending the potential of LISA. Conceived to detect massive black hole binaries from their early inspiral with high signal-to-noise ratio, and low-frequency stellar binaries in the Galaxy, this instrument will be a cornerstone for multimessenger astronomy from the solar neighbourhood to the high-redshift Universe.en_US
dc.language.isoengen_US
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.subjectastronomien_US
dc.subjectastrofysikken_US
dc.titleUnveiling the gravitational universe at μ-Hz frequenciesen_US
dc.typePeer revieweden_US
dc.typeJournal articleen_US
dc.description.versionpublishedVersionen_US
dc.rights.holder© The Author(s) 2021en_US
dc.subject.nsiVDP::Matematikk og Naturvitenskap: 400::Fysikk: 430::Astrofysikk, astronomi: 438en_US
dc.source.pagenumber1333–1383en_US
dc.source.volume51en_US
dc.source.journalExperimental astronomyen_US
dc.identifier.doi10.1007/s10686-021-09709-9
dc.identifier.cristin1946231
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1


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