001     460300
005     20240105113126.0
024 7 _ |2 INSPIRETeX
|a Cicoli:2021yhb
024 7 _ |2 inspire
|a inspire:1879700
024 7 _ |2 arXiv
|a arXiv:2107.03391
024 7 _ |2 datacite_doi
|a 10.3204/PUBDB-2021-02869
037 _ _ |a PUBDB-2021-02869
041 _ _ |a English
082 _ _ |a 530
088 _ _ |2 DESY
|a DESY-21-106
088 _ _ |2 arXiv
|a arXiv:2107.03391
100 1 _ |0 P:(DE-H253)PIP1010796
|a Cicoli, Michele
|b 0
245 _ _ |a On the choice of entropy variables in multifield inflation
260 _ _ |c 2021
336 7 _ |0 PUB:(DE-HGF)25
|2 PUB:(DE-HGF)
|a Preprint
|b preprint
|m preprint
|s 1660288412_20094
336 7 _ |2 ORCID
|a WORKING_PAPER
336 7 _ |0 28
|2 EndNote
|a Electronic Article
336 7 _ |2 DRIVER
|a preprint
336 7 _ |2 BibTeX
|a ARTICLE
336 7 _ |2 DataCite
|a Output Types/Working Paper
520 _ _ |a We discuss the usefulness and theoretical consistency of different entropy variables used in the literature to describe isocurvature perturbations in multifield inflationary models with a generic curved field space. We clarify which is the proper entropy variable to be used to match the evolution of isocurvature modes during inflation to the one after the reheating epoch in order to compare with observational constraints. In particular, we find that commonly used variables, as the relative entropy perturbation or the one associated to the decomposition in tangent and normal perturbations with respect to the inflationary trajectory, even if more useful to perform numerical studies, can lead to results which are wrong by several orders of magnitude, or even to apparent destabilisation effects which are unphysical for cases with light kinetically coupled spectator fields.
536 _ _ |0 G:(DE-HGF)POF4-611
|a 611 - Fundamental Particles and Forces (POF4-611)
|c POF4-611
|f POF IV
|x 0
588 _ _ |a Dataset connected to INSPIRE
650 _ 7 |2 INSPIRE
|a entropy, perturbation
650 _ 7 |2 INSPIRE
|a inflation, model
650 _ 7 |2 INSPIRE
|a isocurvature, perturbation
650 _ 7 |2 INSPIRE
|a trajectory
650 _ 7 |2 INSPIRE
|a reheating
650 _ 7 |2 INSPIRE
|a spectator
693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
|5 EXP:(DE-MLZ)NOSPEC-20140101
|e No specific instrument
|x 0
700 1 _ |0 P:(DE-H253)PIP1087239
|a Guidetti, Veronica
|b 1
|e Corresponding author
700 1 _ |0 P:(DE-HGF)0
|a Muia, Francesco
|b 2
700 1 _ |0 P:(DE-H253)PIP1018307
|a Pedro, Francisco
|b 3
700 1 _ |0 P:(DE-HGF)0
|a Paolo, Vacca Gian
|b 4
856 4 _ |u https://bib-pubdb1.desy.de/record/460300/files/HTML-Approval_of_scientific_publication.html
856 4 _ |u https://bib-pubdb1.desy.de/record/460300/files/PDF-Approval_of_scientific_publication.pdf
856 4 _ |u https://bib-pubdb1.desy.de/record/460300/files/Main_draft.pdf
|y OpenAccess
856 4 _ |u https://bib-pubdb1.desy.de/record/460300/files/Main_draft.pdf?subformat=pdfa
|x pdfa
|y OpenAccess
909 C O |o oai:bib-pubdb1.desy.de:460300
|p openaire
|p open_access
|p VDB
|p driver
|p dnbdelivery
|q ec_fundedresources
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-H253)PIP1010796
|a University of Bologna
|b 0
910 1 _ |0 I:(DE-588b)2008985-5
|6 P:(DE-H253)PIP1087239
|a Deutsches Elektronen-Synchrotron
|b 1
|k DESY
910 1 _ |0 I:(DE-HGF)0
|6 P:(DE-H253)PIP1018307
|a University of Bologna
|b 3
913 1 _ |0 G:(DE-HGF)POF4-611
|1 G:(DE-HGF)POF4-610
|2 G:(DE-HGF)POF4-600
|3 G:(DE-HGF)POF4
|4 G:(DE-HGF)POF
|a DE-HGF
|b Forschungsbereich Materie
|l Matter and the Universe
|v Fundamental Particles and Forces
|x 0
914 1 _ |y 2021
915 _ _ |0 StatID:(DE-HGF)0200
|2 StatID
|a DBCoverage
|b SCOPUS
|d 2021-01-30
915 _ _ |0 LIC:(DE-HGF)CCBYNV
|2 V:(DE-HGF)
|a Creative Commons Attribution CC BY (No Version)
|b DOAJ
|d 2021-01-30
915 _ _ |0 StatID:(DE-HGF)0600
|2 StatID
|a DBCoverage
|b Ebsco Academic Search
|d 2021-01-30
915 _ _ |0 StatID:(DE-HGF)0100
|2 StatID
|a JCR
|b J HIGH ENERGY PHYS : 2019
|d 2021-01-30
915 _ _ |0 StatID:(DE-HGF)0160
|2 StatID
|a DBCoverage
|b Essential Science Indicators
|d 2021-01-30
915 _ _ |0 StatID:(DE-HGF)0501
|2 StatID
|a DBCoverage
|b DOAJ Seal
|d 2021-01-30
915 _ _ |0 StatID:(DE-HGF)0500
|2 StatID
|a DBCoverage
|b DOAJ
|d 2021-01-30
915 _ _ |0 StatID:(DE-HGF)0113
|2 StatID
|a WoS
|b Science Citation Index Expanded
|d 2021-01-30
915 _ _ |0 StatID:(DE-HGF)0199
|2 StatID
|a DBCoverage
|b Clarivate Analytics Master Journal List
|d 2021-01-30
915 _ _ |0 StatID:(DE-HGF)0150
|2 StatID
|a DBCoverage
|b Web of Science Core Collection
|d 2021-01-30
915 _ _ |0 StatID:(DE-HGF)0510
|2 StatID
|a OpenAccess
915 _ _ |0 StatID:(DE-HGF)0030
|2 StatID
|a Peer Review
|b DOAJ : Blind peer review
|d 2021-01-30
915 _ _ |0 StatID:(DE-HGF)1150
|2 StatID
|a DBCoverage
|b Current Contents - Physical, Chemical and Earth Sciences
|d 2021-01-30
915 _ _ |0 StatID:(DE-HGF)0300
|2 StatID
|a DBCoverage
|b Medline
|d 2021-01-30
915 _ _ |0 StatID:(DE-HGF)9905
|2 StatID
|a IF >= 5
|b J HIGH ENERGY PHYS : 2019
|d 2021-01-30
915 _ _ |0 StatID:(DE-HGF)0420
|2 StatID
|a Nationallizenz
|d 2021-01-30
|w ger
915 _ _ |0 StatID:(DE-HGF)0571
|2 StatID
|a DBCoverage
|b SCOAP3 sponsored Journal
|d 2021-01-30
915 _ _ |0 StatID:(DE-HGF)0580
|2 StatID
|a Published
920 1 _ |0 I:(DE-H253)T-20120731
|k T
|l Theorie-Gruppe
|x 0
980 _ _ |a preprint
980 _ _ |a VDB
980 _ _ |a I:(DE-H253)T-20120731
980 _ _ |a UNRESTRICTED
980 1 _ |a FullTexts


LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21