% 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{Coc:408375,
      author       = {Coc, A. and Uzan, J.-P and Vangioni, E.},
      title        = {{M}irror {M}atter, the cosmological {L}ithium {P}roblem and
                      {D}ark {M}atter},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2018-02828, DESY-PROC-2013-04},
      isbn         = {978-3-935702-83-6},
      series       = {DESY-PROC},
      pages        = {277-280},
      year         = {2013},
      comment      = {Coc, A. "Mirror Matter, the cosmological Lithium Problem
                      and Dark Matter" 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     = {Coc, A. "Mirror Matter, the
                       cosmological Lithium Problem and Dark
                       Matter" 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     = {The abundance of lithium-7 confronts cosmology with a long
                      lasting problem between the predictions of standard Big Bang
                      Nucleosynthesis and the baryonic density determined from the
                      Cosmic Microwave Background observations. We investigated
                      the influence of the existence of a mirror world, focusing
                      on models in which miror neutrons can oscillate into
                      ordinary neutrons. Such a mechanism allows for an effective
                      late time neutron injection, which induces an increase of
                      the destruction of beryllium-7 but for mirror baryonic
                      densities much lower than $\Omega_{\mathrm{DM}}$.},
      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/coc_alain},
      url          = {https://bib-pubdb1.desy.de/record/408375},
}