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@INPROCEEDINGS{Meyer:315514,
      author       = {Meyer, Manuel},
      title        = {{M}odelling $\gamma$-ray-axion-like particle oscillations
                      in turbulent magnetic fields: relevance for observations
                      with {C}herenkov telescopes},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2016-05921},
      isbn         = {978-3-935702-59-1},
      series       = {DESY-PROC},
      pages        = {108-112},
      year         = {2014},
      comment      = {Meyer, Manuel "Modelling $\gamma$-ray-axion-like particle
                      oscillations in turbulent magnetic fields: relevance for
                      observations with Cherenkov telescopes" 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     = {Meyer, Manuel "Modelling
                       $\gamma$-ray-axion-like particle
                       oscillations in turbulent magnetic
                       fields: relevance for observations with
                       Cherenkov telescopes" 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     = {Axion-like particles (ALPs) are a common prediction of
                      certain theories beyond the Standard Model and couple to
                      photons in the presence of external magnetic fields. As a
                      consequence, photon-ALP conversion could lead to an
                      enhancement of the flux of extragalactic $\gamma$-ray
                      sources that is otherwise attenuated due to the interactions
                      with background radiation fields. The magnetic fields
                      traversed by the $\gamma$ rays are often turbulent and
                      frequently modelled with a simple domain-like structure.
                      Given a maximum mixing between photons and ALPs, we show
                      that in such models realisations of the fields exist for
                      which the photon-ALP oscillation probability vanishes. This
                      behaviour does not occur in more sophisticated
                      magnetic-field models.},
      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/meyer_manuel},
      url          = {https://bib-pubdb1.desy.de/record/315514},
}