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@INPROCEEDINGS{Derbin:408342,
      author       = {Derbin, A. V. and Dratchnev, I. S. and Kayunov, A. S. and
                      Muratova, V. N. and Semenov, D. A. and Unzhakov, E. V.},
      title        = {{S}earch for solar axions produced by {C}ompton process and
                      bremsstrahlung using the resonant absorption and
                      axioelectric effect},
      address      = {Hamburg},
      publisher    = {Verlag Deutsches Elektronen-Synchrotron},
      reportid     = {PUBDB-2018-02795, DESY-PROC-2013-04},
      isbn         = {978-3-935702-83-6},
      series       = {DESY-PROC},
      pages        = {103-107},
      year         = {2013},
      comment      = {Derbin, A.V. "Search for solar axions produced by Compton
                      process and bremsstrahlung using the resonant absorption and
                      axioelectric effect" 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     = {Derbin, A.V. "Search for solar axions
                       produced by Compton process and
                       bremsstrahlung using the resonant
                       absorption and axioelectric effect" 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 search for resonant absorption of Compton and
                      bremsstrahlung solar axions by $^169$Tm nuclei have been
                      performed. Such an absorption should lead to the excitation
                      of low-lying nuclear energy level: $A + ^{169}Tm →
                      ^{169}Tm^∗ → ^{169}Tm + γ$ (8.41 keV). Additionally the
                      axio-electric effect in silicon atoms is sought. The axions
                      are detected using a Si(Li) detectors placed in a
                      low-background setup. As a result, a new model independent
                      restrictions on the axion-electron and the axion-nucleon
                      coupling: $g_{Ae} × |g^{0}_{AN} + g^{3}_{AN}| ≤ 2.1 ×
                      10^{−14}$ and the axion-electron coupling constant:
                      $|g_{Ae}| ≤ 2.2 × 10^{−10}$ has been obtained. The
                      limits leads to the bounds$m_A ≤$ 7.9 eV and $m_A ≤$ 1.3
                      keV for the mass of the axion in the DFSZ and KSVZ models,
                      respectively (90\% C.L.).},
      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/derbin_alexander},
      url          = {https://bib-pubdb1.desy.de/record/408342},
}