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dc.contributor.authorRicciardone, Angelo
dc.date.accessioned2018-01-05T11:02:41Z
dc.date.available2018-01-05T11:02:41Z
dc.date.created2017-11-30T20:03:55Z
dc.date.issued2017
dc.identifier.citationRicciardone, A. (2017) Primordial Gravitational Waves with LISA. Journal of Physics, Conference Series, 840(1)nb_NO
dc.identifier.issn1742-6588
dc.identifier.urihttp://hdl.handle.net/11250/2475992
dc.description.abstractPrimordial Gravitational Waves are the next target of modern cosmology. They represent a window on the early Universe and the only probe of the physics and microphysics of the inflationary period. When the production of GWs happens in scenarios richer than the standard single-field slow-roll, the GW signal becomes potentially detectable also on scales smaller than the Cosmic Microwave Background. LISA will be extremely complementary to CMB experiments to extract information about primordial inflationary models and in particular to probe phases of the inflationary period for which we have very poor knowledges.nb_NO
dc.language.isoengnb_NO
dc.publisherIOP Publishingnb_NO
dc.rightsNavngivelse 4.0 Internasjonal*
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/deed.no*
dc.subjectfysikknb_NO
dc.subjectgravitasjonsbølgernb_NO
dc.subjectkosmologinb_NO
dc.titlePrimordial Gravitational Waves with LISAnb_NO
dc.typeJournal articlenb_NO
dc.typePeer reviewednb_NO
dc.description.versionacceptedVersionnb_NO
dc.subject.nsiVDP::Mathematics and natural science: 400::Physics: 430nb_NO
dc.source.volume840nb_NO
dc.source.journalJournal of Physics, Conference Seriesnb_NO
dc.source.issue1nb_NO
dc.identifier.doi10.1088/1742-6596/840/1/012030
dc.identifier.cristin1521307
cristin.unitcode217,8,2,0
cristin.unitnameInstitutt for matematikk og naturvitenskap
cristin.ispublishedtrue
cristin.fulltextpostprint
cristin.qualitycode1


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Navngivelse 4.0 Internasjonal
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