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@INPROCEEDINGS{Banik:316749,
      author       = {Banik, Nilanjan and Christopherson, Adam and Sikivie,
                      Pierre and Todarello, Elisa Maria},
      title        = {{T}he {R}ethermalizing {B}ose-{E}instein {C}ondensate
                      of{D}ark {M}atter {A}xions},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2017-00147},
      isbn         = {978-3-935702-43-0},
      series       = {DESY-PROC},
      pages        = {134-139},
      year         = {2015},
      comment      = {Banik, Nilanjan "The Rethermalizing Bose-Einstein
                      Condensate ofDark Matter Axions" in Proceedings, 11th Patras
                      Workshop on Axions, WIMPs and WISPs (Axion-WIMP 2015) /
                      Irastorza, Igor G., Redondo, Javier, Carmona, José Manuel,
                      Cebrian, Susana, Dafni, Theopisti, Iguaz, Francisco J.,
                      Luzon, Gloria (eds.), Verlag Deutsches
                      Elektronen-Synchrotron : 2015 ; AXION-WIMP 2015 : 11th
                      Patras Workshop on Axions, WIMPs and WISPs, 2015-06-22 -
                      2015-06-26, Zaragoza},
      booktitle     = {Banik, Nilanjan "The Rethermalizing
                       Bose-Einstein Condensate ofDark Matter
                       Axions" in Proceedings, 11th Patras
                       Workshop on Axions, WIMPs and WISPs
                       (Axion-WIMP 2015) / Irastorza, Igor G.,
                       Redondo, Javier, Carmona, José Manuel,
                       Cebrian, Susana, Dafni, Theopisti,
                       Iguaz, Francisco J., Luzon, Gloria
                       (eds.), Verlag Deutsches
                       Elektronen-Synchrotron : 2015 ;
                       AXION-WIMP 2015 : 11th Patras Workshop
                       on Axions, WIMPs and WISPs, 2015-06-22
                       - 2015-06-26, Zaragoza},
      abstract     = {The axions produced during the QCD phase transition by
                      vacuum realignment, string decay and domain wall decay
                      thermalize as a result of their gravitational
                      self-interactions when the photon temperature is
                      approximately 500 eV. They then form a Bose-Einstein
                      condensate (BEC). Because the axion BEC rethermalizes on
                      time scales shorter than the age of the universe, it has
                      properties that distinguish it from other forms of cold dark
                      matter. The observational evidence for caustic rings of dark
                      matter in galactic halos is explained if the dark matter is
                      axions, at least in part, but not if the dark matter is
                      entirely WIMPs or sterile neutrinos.},
      month         = {Jun},
      date          = {2015-06-22},
      organization  = {11th Patras Workshop on Axions, WIMPs
                       and WISPs, Zaragoza (Spain), 22 Jun
                       2015 - 26 Jun 2015},
      typ          = {PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.3204/DESY-PROC-2015-02/sikivie_pierre},
      url          = {https://bib-pubdb1.desy.de/record/316749},
}