% 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{Karuza:408372,
      author       = {Karuza, M.},
      title        = {{O}ptomechanics and astroparticle physics; an (im)possible
                      union},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2018-02825, DESY-PROC-2013-04},
      isbn         = {978-3-935702-83-6},
      series       = {DESY-PROC},
      pages        = {261-264},
      year         = {2013},
      comment      = {Karuza, M. "Optomechanics and astroparticle physics; an
                      (im)possible union" 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     = {Karuza, M. "Optomechanics and
                       astroparticle physics; an (im)possible
                       union" 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     = {In recent year with the advent of optomechanics, physics
                      has gained a new powerful tool for small displacement and
                      small forces sensing. It is based on two key ingredients, a
                      resonant optical cavity and a micro-fabricated mechanical
                      resonator. By coupling the two by radiation pressure a
                      powerful tool, capable of sensing extremely small signals at
                      sensitivity limit imposed by Heisenberg uncertainty
                      principle, can be constructed. Here we will try to exploit
                      it’s extraordinary sensitivity for detection of radiation
                      pressure exerted by hypothetical particles that could be
                      produced in the Sun’s interior.},
      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/karuza_marin},
      url          = {https://bib-pubdb1.desy.de/record/408372},
}