001     472023
005     20250724175815.0
024 7 _ |a 10.1088/1475-7516/2021/08/020
|2 doi
024 7 _ |a Dorsch:2021ubz
|2 INSPIRETeX
024 7 _ |a inspire:1868302
|2 inspire
024 7 _ |a 1475-7508
|2 ISSN
024 7 _ |a 1475-7516
|2 ISSN
024 7 _ |a arXiv:2106.06547
|2 arXiv
024 7 _ |a altmetric:111856556
|2 altmetric
024 7 _ |a 10.3204/PUBDB-2021-04790
|2 datacite_doi
024 7 _ |a WOS:000686656000006
|2 WOS
024 7 _ |a openalex:W3210767361
|2 openalex
037 _ _ |a PUBDB-2021-04790
041 _ _ |a English
082 _ _ |a 530
088 _ _ |a arXiv:2106.06547
|2 arXiv
088 _ _ |a DESY-21-089
|2 DESY
100 1 _ |a Dorsch, Glauber C.
|0 P:(DE-HGF)0
|b 0
|e Corresponding author
245 _ _ |a On the wall velocity dependence of electroweak baryogenesis
260 _ _ |a London
|c 2021
|b IOP
336 7 _ |a article
|2 DRIVER
336 7 _ |a Output Types/Journal article
|2 DataCite
336 7 _ |a Journal Article
|b journal
|m journal
|0 PUB:(DE-HGF)16
|s 1719328951_2887561
|2 PUB:(DE-HGF)
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a JOURNAL_ARTICLE
|2 ORCID
336 7 _ |a Journal Article
|0 0
|2 EndNote
520 _ _ |a We re-evaluate the status of supersonic electroweak baryogenesis using a generalized fluid Ansatz for the non-equilibrium distribution functions. Instead of truncating the expansion to first order in momentum, we allow for higher order terms as well, including up to 21 fluctuations. The collision terms are computed analytically at leading-log accuracy. We also point out inconsistencies in the standard treatments of transport in electroweak baryogenesis, arguing that one cannot do without specifying an Ansatz for the distribution function. We present the first analysis of baryogenesis using the fluid approximation to higher orders. Our results support the recent findings that baryogenesis may indeed be possible even in the presence of supersonic wall velocities.
536 _ _ |a 611 - Fundamental Particles and Forces (POF4-611)
|0 G:(DE-HGF)POF4-611
|c POF4-611
|f POF IV
|x 0
536 _ _ |a DFG project 390833306 - EXC 2121: Quantum Universe (390833306)
|0 G:(GEPRIS)390833306
|c 390833306
|x 1
588 _ _ |a Dataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de
650 _ 7 |a approximation: fluid
|2 INSPIRE
650 _ 7 |a baryogenesis
|2 INSPIRE
650 _ 7 |a electroweak interaction
|2 INSPIRE
650 _ 7 |a higher-order
|2 INSPIRE
650 _ 7 |a distribution function
|2 INSPIRE
650 _ 7 |a fluctuation
|2 INSPIRE
650 _ 7 |a velocity dependence
|2 INSPIRE
693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
|5 EXP:(DE-MLZ)NOSPEC-20140101
|e No specific instrument
|x 0
700 1 _ |a Huber, Stephan J.
|0 P:(DE-HGF)0
|b 1
|e Corresponding author
700 1 _ |a Konstandin, Thomas
|0 P:(DE-H253)PIP1015746
|b 2
|e Corresponding author
773 _ _ |a 10.1088/1475-7516/2021/08/020
|g Vol. 08, no. 08, p. 020 -
|0 PERI:(DE-600)2104147-7
|n 08
|p 020
|t Journal of cosmology and astroparticle physics
|v 08
|y 2021
|x 1475-7508
787 0 _ |a Dorsch, Glauber C. et.al.
|d 2021
|i IsParent
|0 PUBDB-2021-02610
|r DESY-21-089 ; arXiv:2106.06547
|t On the wall velocity dependence of electroweak baryogenesis
856 4 _ |u https://bib-pubdb1.desy.de/record/472023/files/2106.06547v2.pdf
|y OpenAccess
856 4 _ |u https://bib-pubdb1.desy.de/record/472023/files/Dorsch_2021_J._Cosmol._Astropart._Phys._2021_020.pdf
|y Restricted
856 4 _ |u https://bib-pubdb1.desy.de/record/472023/files/2106.06547v2.pdf?subformat=pdfa
|x pdfa
|y OpenAccess
856 4 _ |u https://bib-pubdb1.desy.de/record/472023/files/Dorsch_2021_J._Cosmol._Astropart._Phys._2021_020.pdf?subformat=pdfa
|x pdfa
|y Restricted
909 C O |o oai:bib-pubdb1.desy.de:472023
|p openaire
|p open_access
|p VDB
|p driver
|p dnbdelivery
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 2
|6 P:(DE-H253)PIP1015746
913 1 _ |a DE-HGF
|b Forschungsbereich Materie
|l Matter and the Universe
|1 G:(DE-HGF)POF4-610
|0 G:(DE-HGF)POF4-611
|3 G:(DE-HGF)POF4
|2 G:(DE-HGF)POF4-600
|4 G:(DE-HGF)POF
|v Fundamental Particles and Forces
|x 0
914 1 _ |y 2021
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0200
|2 StatID
|b SCOPUS
|d 2021-01-29
915 _ _ |a JCR
|0 StatID:(DE-HGF)0100
|2 StatID
|b J COSMOL ASTROPART P : 2019
|d 2021-01-29
915 _ _ |a IF >= 5
|0 StatID:(DE-HGF)9905
|2 StatID
|b J COSMOL ASTROPART P : 2019
|d 2021-01-29
915 _ _ |a WoS
|0 StatID:(DE-HGF)0113
|2 StatID
|b Science Citation Index Expanded
|d 2021-01-29
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0150
|2 StatID
|b Web of Science Core Collection
|d 2021-01-29
915 _ _ |a OpenAccess
|0 StatID:(DE-HGF)0510
|2 StatID
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)1150
|2 StatID
|b Current Contents - Physical, Chemical and Earth Sciences
|d 2021-01-29
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0160
|2 StatID
|b Essential Science Indicators
|d 2021-01-29
915 _ _ |a Nationallizenz
|0 StatID:(DE-HGF)0420
|2 StatID
|d 2021-01-29
|w ger
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0199
|2 StatID
|b Clarivate Analytics Master Journal List
|d 2021-01-29
920 1 _ |0 I:(DE-H253)T-20120731
|k T
|l Theorie-Gruppe
|x 0
980 _ _ |a journal
980 _ _ |a VDB
980 _ _ |a I:(DE-H253)T-20120731
980 _ _ |a UNRESTRICTED
980 1 _ |a FullTexts


LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21