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@INPROCEEDINGS{Brax:295155,
      author       = {Brax, Philippe},
      title        = {{S}olar chameleons: {P}roduction and detection},
      address      = {Hamburg},
      publisher    = {Deutsches Elektronen-Synchrotron, DESY},
      reportid     = {PUBDB-2016-01091, DESY-PROC-2011-04},
      pages        = {116-119},
      year         = {2011},
      abstract     = {Chameleon fields evade gravitational tests in the solar
                      system and the laboratory while playing the role of
                      quintessence on cosmological scales. They could be produced
                      in magnetised regions of the inner sun, e.g. around the
                      tachocline. Once produced, they can be backconverted into
                      X-ray photons in the sun's atmosphere or reach helioscope
                      detectors on earth where the spectrum of photons is
                      typically peaked in the sub-keV region. Dedicated laboratory
                      shining-through-a-wall experiments using powerful X-ray
                      lasers could be used to test the existence of chameleons.},
      month         = {Jun},
      date          = {2011-06-27},
      organization  = {7th Patras Workshop on Axions, WIMPs
                       and WISPs, Mykonos (Greece), 27 Jun
                       2011 - 1 Jul 2011},
      cin          = {L},
      cid          = {I:(DE-H253)L-20120731},
      pnm          = {899 - ohne Topic (POF3-899)},
      pid          = {G:(DE-HGF)POF3-899},
      experiment   = {EXP:(DE-H253)HERA(machine)-20150101},
      typ          = {PUB:(DE-HGF)8 / PUB:(DE-HGF)15},
      doi          = {10.3204/DESY-PROC-2011-04/brax_philippe},
      url          = {https://bib-pubdb1.desy.de/record/295155},
}