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@INPROCEEDINGS{Davidson:315502,
      author       = {Davidson, Sacha},
      title        = {{T}he {P}ressure of {M}isalignment {A}xions: a {D}ifference
                      from {WIMP}s in {G}alaxy {F}ormation?},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2016-05909},
      isbn         = {978-3-935702-59-1},
      series       = {DESY-PROC},
      pages        = {51-54},
      year         = {2014},
      comment      = {Davidson, Sacha "The Pressure of Misalignment Axions:a
                      Difference from WIMPs in Galaxy Formation?" in Proceedings,
                      10th Patras Workshop on Axions, WIMPs and WISPs (AXION-WIMP
                      2014) / Tsesmelis, Emmanuel, Maroudas, Marios (eds.), Verlag
                      Deutsches Elektronen-Synchrotron : 2014 ; AXION-WIMP 2014 :
                      10th Patras Workshop on Axions, WIMPs and WISPs, 2014-06-29
                      - 2014-07-04, Geneva},
      booktitle     = {Davidson, Sacha "The Pressure of
                       Misalignment Axions:a Difference from
                       WIMPs in Galaxy Formation?" in
                       Proceedings, 10th Patras Workshop on
                       Axions, WIMPs and WISPs (AXION-WIMP
                       2014) / Tsesmelis, Emmanuel, Maroudas,
                       Marios (eds.), Verlag Deutsches
                       Elektronen-Synchrotron : 2014 ;
                       AXION-WIMP 2014 : 10th Patras Workshop
                       on Axions, WIMPs and WISPs, 2014-06-29
                       - 2014-07-04, Geneva},
      abstract     = {Two populations of axions can contribute to cold dark
                      matter: the classical field produced via the misalignment
                      mechanism, and the modes produced in the decay of strings.
                      The classical field has extra pressure, as compared to
                      WIMPs, which could have observable consequences in
                      non-linear galaxy formation.},
      month         = {Jun},
      date          = {2014-06-29},
      organization  = {10th Patras Workshop on Axions, WIMPs
                       and WISPs, Geneva (Switzerland), 29 Jun
                       2014 - 4 Jul 2014},
      typ          = {PUB:(DE-HGF)8 / PUB:(DE-HGF)7},
      doi          = {10.3204/DESY-PROC-2014-03/davidson_sacha},
      url          = {https://bib-pubdb1.desy.de/record/315502},
}