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000408366 0247_ $$2datacite_doi$$a10.3204/DESY-PROC-2013-04/cembranos_jose
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000408366 1001_ $$0P:(DE-HGF)0$$aJ. A. R. Cembranos, $$b0$$eCorresponding author
000408366 1112_ $$0C13-06-24.5$$2inspire$$a9th Patras Workshop on Axions, WIMPs and WISPs$$cMainz$$d2013-06-24 - 2013-06-28$$gAXION-WIMP 2013$$wGermany
000408366 245__ $$aSolution to the Isotropy Problem for Cosmological Hidden Vector Models
000408366 260__ $$aHamburg$$bVerlag Deutsches Elektronen-Synchrotron$$c2013
000408366 29510 $$aCembranos, 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
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000408366 520__ $$aGauge bosons associated to new gauge symmetries under which the standard model particles are not charged are predicted in many extensions of the standard model of particles and interactions. We show that under very general conditions, the average energy-momentum tensor of these rapidly oscillating vector fields is isotropic for any locally inertial observer. This result has a fundamental importance in order to consider coherent vector fields as a viable alternative to support models of dark matter, dark energy or inflation.
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000408366 7001_ $$0P:(DE-HGF)0$$aMaroto, A. L.$$b1
000408366 7001_ $$0P:(DE-HGF)0$$aNúñez Jareño, S. J.$$b2
000408366 7870_ $$0PUBDB-2015-05816$$aOberlack, Uwe et. al.$$iisPartOf$$rDESY-PROC-2013-04$$tProceedings, 9th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP 2013)
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