Expected sensitivity to galactic/solar axions and bosonic super-WIMPs based on the axio-electric effect in liquid xenon dark matter detectors

Astroparticle Physics

Volumn 44, Issue , 2013, Pages 59-67

  Arisaka, K ^a   Beltrame, P ^a   Ghag, C ^a,b   Kaidi, J ^a   Lung, K ^a   Lyashenko, A ^a   Peccei, R D ^a   Smith, P ^a   Ye, K ^a,c  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY COLLEGE LONDON   (United Kingdom)

^c PEKING UNIVERSITY   (China)

Author keywords

Liquid xenon; Solar axions; SuperWIMPs

Indexed keywords

COUPLING CONSTANTS; DARK MATTER; DARK MATTER DETECTORS; DOUBLE BETA DECAY; GALACTIC AXIONS; LIQUID XENON; LOW-MASS; LOW-RADIOACTIVITY; NEUTRINO BACKGROUND; NUCLEAR RECOIL; SOLAR AXIONS; SOLAR NEUTRINO; SUPERWIMPS; UPPER BOUND; WEAKLY INTERACTING MASSIVE PARTICLES; XENON ATOMS;

BOSONS; DETECTORS; GALAXIES; PARTICLE DETECTORS; RADIOACTIVITY;

LIQUIDS;

EID: 84874711194     PISSN: 09276505     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.astropartphys.2012.12.009     Document Type: Article

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