English

$SU(2)_X$ Vector DM and Galactic Center Gamma-Ray Excess

High Energy Physics - Phenomenology 2015-06-11 v3 High Energy Astrophysical Phenomena

Abstract

An unbroken Z3Z_3 symmetry remains when local SU(2)XSU(2)_X is broken spontaneously by one quadruplet. The gauge boson χμ(χˉμ)\chi_\mu (\bar \chi_\mu ) carries the dark charge and is the candidate of dark matter (DM). By the mixture of scalar boson ϕr\phi_r of quadruplet and standard model (SM) Higgs, the DM can annihilate to SM particles through Higgs portal. For investigating the implications of vector DM, we study the relic density of DM, the direct detection of DM-nucleon scattering and the excess of gamma-ray spectrum, which is supported by the data from {\it Fermi} Gamma-Ray Space Telescope. We find that with the DM mass of around 7070 GeV in our model, the excess of gamma-ray could be fitted well with the data.

Keywords

Cite

@article{arxiv.1501.07413,
  title  = {$SU(2)_X$ Vector DM and Galactic Center Gamma-Ray Excess},
  author = {Chuan-Hung Chen and Takaaki Nomura},
  journal= {arXiv preprint arXiv:1501.07413},
  year   = {2015}
}

Comments

17 pages, 12 figures, final version published in physics letters B

R2 v1 2026-06-22T08:15:40.281Z