% IMPORTANT: The following is UTF-8 encoded.  This means that in the presence
% of non-ASCII characters, it will not work with BibTeX 0.99 or older.
% Instead, you should use an up-to-date BibTeX implementation like “bibtex8” or
% “biber”.

@INPROCEEDINGS{Weltman:408374,
      author       = {Weltman, A.},
      title        = {{C}hameleon {F}ields {N}ear and {F}ar},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2018-02827, DESY-PROC-2013-04},
      isbn         = {978-3-935702-83-6},
      series       = {DESY-PROC},
      pages        = {271-276},
      year         = {2013},
      comment      = {Weltman, A. "Chameleon Fields Near and Far" 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     = {Weltman, A. "Chameleon Fields Near and
                       Far" 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     = {In this presentation we contemplate the problem of dark
                      energy and advocate for a multi-faceted approach to studying
                      its solution. Indeed it may be that, like the philosophers
                      described above, we too cannot understand the nature of our
                      beast by only touching one side of the problem. In
                      particular we will study chameleon fields as a candidate for
                      driving the observed acceleration of the universe and we
                      will look how to test this theory through a varied approach
                      as advocated here.},
      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/weltman_amanda},
      url          = {https://bib-pubdb1.desy.de/record/408374},
}