4.6 Article

Axion searches with the EDELWEISS-II experiment

出版社

IOP PUBLISHING LTD
DOI: 10.1088/1475-7516/2013/11/067

关键词

axions; dark matter detectors; dark matter experiments

资金

  1. French Agence Nationale pour la Recherche [ANR-10-BLAN-0422-03]
  2. P2IO Labex
  3. German ministry of science and education (BMBF) within the Verbundforschung Astroteilchenphysik [05A11VK2]
  4. Helmholtz Alliance for Astroparticle Physics (HAP)
  5. Initiative and Networking Fund of the Helmholtz Association
  6. Russian Foundation for Basic Research (Russia)
  7. Science and Technology Facilities Council (U.K.)
  8. STFC [ST/K006444/1, ST/J000671/1, ST/K003151/1, ST/K003186/1, ST/K00137X/1, ST/K001337/1] Funding Source: UKRI
  9. Science and Technology Facilities Council [ST/K006444/1, ST/K006444/1 DMUK, ST/K00137X/1, ST/K003186/1, ST/J000671/1, ST/K003186/1 DMUK, ST/K001337/1, ST/K003151/1, ST/K003151/1 DMUK] Funding Source: researchfish
  10. Agence Nationale de la Recherche (ANR) [ANR-10-BLAN-0422] Funding Source: Agence Nationale de la Recherche (ANR)

向作者/读者索取更多资源

We present new constraints on the couplings of axions and more generic axion-like particles using data from the EDELWEISS-II experiment. The EDELWEISS experiment, located at the Underground Laboratory of Modane, primarily aims at the direct detection of WIMPs using germanium bolometers. It is also sensitive to the low-energy electron recoils that would be induced by solar or dark matter axions. Using a total exposure of up to 448 kg.d, we searched for axion-induced electron recoils down to 2.5 keV within four scenarios involving different hypotheses on the origin and couplings of axions. We set a 95% CL limit on the coupling to photons gA gamma < 2.15 x 10(-9) GeV-1 in a mass range not fully covered by axion helioscopes. We also constrain the coupling to electrons, g(Ae) < 2.59 x 10(-11), similar to the more indirect solar neutrino bound. Finally we place a limit on g(Ae) x g(AN)(eff) < 4.82 x 10(-17), where g(AN)(eff) is the effective axion-nucleon coupling for Fe-57. Combining these results we fully exclude the mass range 0.92 eV < m(A) < 80 keV for DFSZ axions and 5.78 eV < m(A) < 40 keV for KSVZ axions.

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