TY - JOUR
T1 - Anomaly-free flavor models for Nambu-Goldstone bosons and the 3.5 keV X-ray line signal
AU - Nakayama, Kazunori
AU - Takahashi, Fuminobu
AU - Yanagida, Tsutomu T.
N1 - Funding Information:
This work was supported by the Grant-in-Aid for Scientific Research on Innovative Areas (No. 21111006 [K.N. and F.T.], No. 23104008 [F.T.], No. 24111702 [F.T.]), Scientific Research (A) (Nos. 22244030 [K.N. and F.T.], 21244033 [F.T.], 22244021 [T.T.Y.]), JSPS Grant-in-Aid for Young Scientists (B) (No. 24740135 ) [F.T.], and Inoue Foundation for Science [F.T.]. This work was also supported by World Premier International Center Initiative (WPI Program), MEXT , Japan.
PY - 2014/6/27
Y1 - 2014/6/27
N2 - We pursue a possibility that a pseudo-Nambu-Goldstone boson is lurking around or below the intermediate scale. To this end we consider an anomaly-free global flavor symmetry, and construct models where the pseudo-Nambu-Goldstone boson is coupled preferentially to leptons. The experimental and astrophysical bounds derived from couplings to photons and nucleons are significantly relaxed. If sufficiently light, the pseudo-Nambu-Goldstone boson contributes to dark matter, and interestingly, it generally decays into photons through couplings arising from threshold corrections. We show that the recent hint for the X-ray line at about 3.5 keV can be explained by the decay of such pseudo-Nambu-Goldstone boson of mass about 7 keV with the decay constant of order 1010 GeV, if the electron is charged under the flavor symmetry.
AB - We pursue a possibility that a pseudo-Nambu-Goldstone boson is lurking around or below the intermediate scale. To this end we consider an anomaly-free global flavor symmetry, and construct models where the pseudo-Nambu-Goldstone boson is coupled preferentially to leptons. The experimental and astrophysical bounds derived from couplings to photons and nucleons are significantly relaxed. If sufficiently light, the pseudo-Nambu-Goldstone boson contributes to dark matter, and interestingly, it generally decays into photons through couplings arising from threshold corrections. We show that the recent hint for the X-ray line at about 3.5 keV can be explained by the decay of such pseudo-Nambu-Goldstone boson of mass about 7 keV with the decay constant of order 1010 GeV, if the electron is charged under the flavor symmetry.
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U2 - 10.1016/j.physletb.2014.05.035
DO - 10.1016/j.physletb.2014.05.035
M3 - Article
AN - SCOPUS:84901686716
SN - 0370-2693
VL - 734
SP - 178
EP - 182
JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
ER -