Home > Publications database > Solution to the Isotropy Problem for Cosmological Hidden Vector Models > print

001     408366
005     20211110151246.0
010 _ _ |a
020 _ _ |a 978-3-935702-83-6
024 7 _ |a 10.3204/DESY-PROC-2013-04/cembranos_jose
|2 datacite_doi
024 7 _ |a 1435-8077
|2 ISSN
037 _ _ |a PUBDB-2018-02819
041 _ _ |a English
088 1 _ |a DESY-PROC-2013-04
088 _ _ |a DESY-PROC-2013-04
|2 DESY
100 1 _ |a J. A. R. Cembranos,
|0 P:(DE-HGF)0
|b 0
|e Corresponding author
111 2 _ |a 9th Patras Workshop on Axions, WIMPs and WISPs
|c Mainz
|d 2013-06-24 - 2013-06-28
|g AXION-WIMP 2013
|0 C13-06-24.5
|2 inspire
|w Germany
245 _ _ |a Solution to the Isotropy Problem for Cosmological Hidden Vector Models
260 _ _ |a Hamburg
|c 2013
|b Verlag Deutsches Elektronen-Synchrotron
295 1 0 |a Cembranos, J.A.R. "Solution to the Isotropy Problem for Cosmological Hidden Vector Models" in Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013) / Oberlack, Uwe, Sissol, Pierre (eds.), 2013 ; AXION-WIMP 2013 : 9th Patras Workshop on Axions, WIMPs and WISPs , 2013-06-23 - 2013-06-28, Mainz
300 _ _ |a 231-234
336 7 _ |a CONFERENCE_PAPER
|2 ORCID
336 7 _ |a Conference Paper
|0 33
|2 EndNote
336 7 _ |a INPROCEEDINGS
|2 BibTeX
336 7 _ |a conferenceObject
|2 DRIVER
336 7 _ |a Report
|0 PUB:(DE-HGF)29
|2 PUB:(DE-HGF)
|m report
336 7 _ |a Output Types/Conference Paper
|2 DataCite
336 7 _ |a Contribution to a conference proceedings
|b contrib
|m contrib
|0 PUB:(DE-HGF)8
|s 1534165943_22823
|2 PUB:(DE-HGF)
336 7 _ |a Contribution to a book
|0 PUB:(DE-HGF)7
|2 PUB:(DE-HGF)
|m contb
490 0 _ |a DESY-PROC
|0 PERI:(DE-600)2450075-6
520 _ _ |a Gauge bosons associated to new gauge symmetries under which the standard model particles are not charged are predicted in many extensions of the standard model of particles and interactions. We show that under very general conditions, the average energy-momentum tensor of these rapidly oscillating vector fields is isotropic for any locally inertial observer. This result has a fundamental importance in order to consider coherent vector fields as a viable alternative to support models of dark matter, dark energy or inflation.
536 _ _ |a 899 - ohne Topic (POF3-899)
|0 G:(DE-HGF)POF3-899
|c POF3-899
|f POF III
|x 0
588 _ _ |a Dataset connected to GVK
650 _ 7 |a Hypothetisches Teilchen
|0 (DE-588)4220935-3
|2 gnd
693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
|5 EXP:(DE-MLZ)NOSPEC-20140101
|e No specific instrument
|x 0
700 1 _ |a Maroto, A. L.
|0 P:(DE-HGF)0
|b 1
700 1 _ |a Núñez Jareño, S. J.
|0 P:(DE-HGF)0
|b 2
787 0 _ |a Oberlack, Uwe et. al.
|0 PUBDB-2015-05816
|r DESY-PROC-2013-04
|i isPartOf
|t Proceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013)
856 4 _ |u https://bib-pubdb1.desy.de/record/408366/files/fulltext.pdf
|y OpenAccess
909 C O |o oai:bib-pubdb1.desy.de:408366
|p openaire
|p open_access
|p VDB
|p driver
|p dnbdelivery
913 1 _ |a DE-HGF
|b Programmungebundene Forschung
|l ohne Programm
|1 G:(DE-HGF)POF3-890
|0 G:(DE-HGF)POF3-899
|2 G:(DE-HGF)POF3-800
|v ohne Topic
|x 0
|4 G:(DE-HGF)POF
|3 G:(DE-HGF)POF3
915 _ _ |a OpenAccess
|0 StatID:(DE-HGF)0510
|2 StatID
915 _ _ |a Creative Commons Attribution CC BY 4.0
|0 LIC:(DE-HGF)CCBY4
|2 HGFVOC
920 1 _ |0 I:(DE-H253)L-20120731
|k L
|l Bibliothek und Dokumentation
|x 0
980 _ _ |a contrib
980 _ _ |a VDB
980 _ _ |a UNRESTRICTED
980 _ _ |a report
980 _ _ |a contb
980 _ _ |a I:(DE-H253)L-20120731
980 1 _ |a FullTexts

LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21