Analysis of DDM into Gamma Radiation

Authors

  • C. Arellano-Celiz Faculty of Mathematical Physical Sciences, Benemérita Universidad Autónoma de Puebla, Apdo. Postal 1152, Puebla, Pue.-72000, Mexico
  • A. Avilez-Lopez Faculty of Mathematical Physical Sciences, Benemérita Universidad Autónoma de Puebla, Apdo. Postal 1152, Puebla, Pue.-72000, Mexico
  • J. E. Barradas-Guevara Faculty of Mathematical Physical Sciences, Benemérita Universidad Autónoma de Puebla, Apdo. Postal 1152, Puebla, Pue.-72000, Mexico
  • O. Felix-Beltran Faculty of Electronics Sciences, Benemérita Universidad Autónoma de Puebla, Apdo. Postal 542, Puebla, Pue.-72000, Mexico
  • F. Gonzalez-Canales Faculty of Electronics Sciences, Benemérita Universidad Autónoma de Puebla, Apdo. Postal 542, Puebla, Pue.-72000, Mexico

DOI:

https://doi.org/10.15415/jnp.2020.72019

Keywords:

Dark matter, Dipolar dark matter, WIMP, Relic density

Abstract

We are interested in the purpose of a dipolar fermionic particle as a viable candidate of Dark Matter (DDM). Then, we study the annihilation of dark matter into photons, considering it as a neutral particle with non-vanishing magnetic (M) and electric (D) dipolar moments. The total annihilation cross section σ(χchi bar → γgamma bar) is computed by starting from a general form of coupling χchi barγ in a framework beyond to Standard Model (BSM). We found that candidates with O(mχ )∽102GeV, D≈10−16 e cm are required in order to satisfy the current cosmic relic density.

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Published

2020-02-28

How to Cite

(1)
Arellano-Celiz, C. .; Avilez-Lopez, A. .; Barradas-Guevara, J. E. .; Felix-Beltran, O. .; Gonzalez-Canales, F. . Analysis of DDM into Gamma Radiation. J. Nucl. Phy. Mat. Sci. Rad. A. 2020, 7, 153-157.

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