Please use this identifier to cite or link to this item: http://dspace.chitkarauniversity.edu.in/xmlui/handle/123456789/372
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dc.contributor.authorBarradas-Guevara, E.-
dc.contributor.authorDiaz-Cruz, J. L.-
dc.contributor.authorFelix Beltran, O. G.-
dc.contributor.authorArellano Celiz, C.-
dc.date.accessioned2022-04-15T05:15:03Z-
dc.date.available2022-04-15T05:15:03Z-
dc.date.issued2018-08-06-
dc.identifier.issn2321-8649-
dc.identifier.issn2321-9289-
dc.identifier.urihttp://dspace.chitkarauniversity.edu.in/xmlui/handle/123456789/372-
dc.description.abstractIn this work we study the annihilation of dark matter, considering it as a neutral particle with magnetic and/or electric moments not null. The calculation of the effective section of the process χχbar→γγ is made starting from a general form of coupling χ χbar γ in the framework of an extension of the Standard Model. We found, when taking into account an annihilation of DDM-antiDDM to monoenergetic photons, that for small masses, mχ ≤ 0 GeV, an electric dipole moment ~10–6 e cm is required to satisfy the current residual density, while for the range of greater sensitivity of HAWC, 10 TeV < Eg < 20 TeV, the electrical dipole moment must be of the order of 10–8 e cm.en_US
dc.language.isoenen_US
dc.relation.ispartofseries;CHAENG/2013/51628-
dc.subjectdark matter annihilationen_US
dc.subjectgamma-ray signaturesen_US
dc.subjectdark matter annihilationen_US
dc.subjectrelic densityen_US
dc.subjectannihilationen_US
dc.subjectnuclear physicsen_US
dc.titleAnnihilation of Dipolar Dark Matter: χχ→γγen_US
dc.typeArticleen_US
Appears in Collections:VOL.6.NO 1(2018)

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