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@INPROCEEDINGS{JARCembranos:408366,
      author       = {J. A. R. Cembranos, and Maroto, A. L. and Núñez Jareño,
                      S. J.},
      title        = {{S}olution to the {I}sotropy {P}roblem for {C}osmological
                      {H}idden {V}ector {M}odels},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2018-02819, DESY-PROC-2013-04},
      isbn         = {978-3-935702-83-6},
      series       = {DESY-PROC},
      pages        = {231-234},
      year         = {2013},
      comment      = {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},
      booktitle     = {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},
      abstract     = {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.},
      month         = {Jun},
      date          = {2013-06-24},
      organization  = {9th Patras Workshop on Axions, WIMPs
                       and WISPs, Mainz (Germany), 24 Jun 2013
                       - 28 Jun 2013},
      keywords     = {Hypothetisches Teilchen (gnd)},
      cin          = {L},
      cid          = {I:(DE-H253)L-20120731},
      pnm          = {899 - ohne Topic (POF3-899)},
      pid          = {G:(DE-HGF)POF3-899},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)29 / PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.3204/DESY-PROC-2013-04/cembranos_jose},
      url          = {https://bib-pubdb1.desy.de/record/408366},
}