Colder freeze-in axinos decaying into photons

被引:10
作者
Bae, Kyu Jung [1 ]
Kamada, Ayuki [1 ]
Liew, Seng Pei [2 ]
Yanagi, Keisuke [3 ]
机构
[1] Inst for Basic Sci Korea, Ctr Theoret Phys Universe, Daejeon 34126, South Korea
[2] Tech Univ Munich, Phys Dept, D-85748 Garching, Germany
[3] Univ Tokyo, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan
关键词
RAY-LINE SIGNAL; DARK-MATTER; CP CONSERVATION; SUPERSYMMETRY; SUPERGRAVITY; SEARCH;
D O I
10.1103/PhysRevD.97.055019
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We point out that 7 keVaxino dark matter (DM) in the R-parity violating (RPV) supersymmetric (SUSY) Dine-Fischler-Srednicki-Zhitnitsky axion model can simultaneously reproduce the 3.5 keV x-ray line excess and evade stringent constraints from the Ly-alpha forest data. Peccei-Quinn symmetry breaking naturally generates both the TeV-scale mu term and the MeV-scale RPV term. The RPV term introduces a tiny axino-neutrino mixing and provides axino DM as a variant of the sterile neutrino DM explaining the 3.5 keV x-ray line excess. Axinos are produced by freeze-in processes via the mu term. The resultant phase space distribution tends to be colder than the Fermi-Dirac distribution. The inherent entropy production from late-time saxion decay makes axinos even colder than those without saxion decay. The resultant axino DM takes the correct relic density and is compatible even with the latest and strongest constraint from the Ly-alpha forest data.
引用
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页数:6
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