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@INBOOK{Banerjee:410425,
      author       = {Banerjee, Robi and Sigl, Guenter},
      title        = {{C}osmic {M}agnetic {F}ields and their {R}ole in {H}igh
                      {E}nergy {A}strophysics},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2018-03607},
      isbn         = {9783945931219},
      pages        = {387-406},
      year         = {2018},
      comment      = {Banerjee, Robi "Cosmic Magnetic Fields and their Role in
                      High Energy Astrophysics" in Particles, Strings and the
                      Early Universe : The Structure of Matter and Space-Time /
                      Haller, Johannes, Grefe, Michael (eds.), Verlag Deutsches
                      Elektronen-Synchrotron : 2018},
      booktitle     = {Banerjee, Robi "Cosmic Magnetic Fields
                       and their Role in High Energy
                       Astrophysics" in Particles, Strings and
                       the Early Universe : The Structure of
                       Matter and Space-Time / Haller,
                       Johannes, Grefe, Michael (eds.), Verlag
                       Deutsches Elektronen-Synchrotron :
                       2018},
      abstract     = {Magnetic fields play an important role in many
                      astrophysical and cosmological situations. The evolution of
                      primordial seed fields crucially depends on the amount of
                      helicity and the properties of the velocity field. On the
                      other hand, magnetic fields can serve as an agent for
                      possible signatures of dark matter in the form of
                      annihilating weakly interacting massive particles, through
                      induced synchrotron radiation of charged annihilation
                      products, and for a possible mixing of axion-like particles
                      and other light states with photons in scenarios beyond the
                      Standard Model. In the context of project C9 of the SFB 676
                      we investigated both the seeding and evolution of magnetic
                      fields and their effects on other processes.},
      cin          = {UNI/TH / U HH},
      cid          = {$I:(DE-H253)UNI_TH-20120731$ / $I:(DE-H253)U_HH-20120814$},
      pnm          = {611 - Fundamental Particles and Forces (POF3-611) / DFG
                      project 13245592 - SFB 676: Teilchen, Strings und frühes
                      Universum: Struktur von Materie und Raum-Zeit (13245592)},
      pid          = {G:(DE-HGF)POF3-611 / G:(GEPRIS)13245592},
      experiment   = {EXP:(DE-MLZ)NOSPEC-20140101},
      typ          = {PUB:(DE-HGF)7},
      doi          = {10.3204/PUBDB-2018-00782/C9},
      url          = {https://bib-pubdb1.desy.de/record/410425},
}