2017
DOI: 10.1088/1475-7516/2017/03/054
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General calculation of the cross section for dark matter annihilations into two photons

Abstract: Assuming that the underlying model satisfies some general requirements such as renormalizability and CP conservation, we calculate the non-relativistic one-loop cross section for any self-conjugate dark matter particle annihilating into two photons. We accomplish this by carefully classifying all possible one-loop diagrams and, from them, reading off the dark matter interactions with the particles running in the loop. Our approach is general and leads to the same results found in the literature for popular dar… Show more

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Cited by 18 publications
(17 citation statements)
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References 108 publications
(148 reference statements)
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“…The ability to automatically compute loop induced processes would be a great addition to MadDM, as it will allow the user to easy evaluate dark matter annihilation into a pair of photons or γZ or γh (the so-called smoking gun signatures for dark matter), for which the Fermi-LAT satellite is setting strong exclusion bounds [30]. At the moment such loop induced processes need to be evaluated analytically within the specific dark matter model, while there are attempts to analytically provide systematic calculations valid for the most popular dark matter candidates [39]. A fully automatised numerical procedure for any dark matter model is yet a missing block within the dark matter tools world.…”
Section: Computation Of σV In Astrophysical Environmentsmentioning
confidence: 99%
“…The ability to automatically compute loop induced processes would be a great addition to MadDM, as it will allow the user to easy evaluate dark matter annihilation into a pair of photons or γZ or γh (the so-called smoking gun signatures for dark matter), for which the Fermi-LAT satellite is setting strong exclusion bounds [30]. At the moment such loop induced processes need to be evaluated analytically within the specific dark matter model, while there are attempts to analytically provide systematic calculations valid for the most popular dark matter candidates [39]. A fully automatised numerical procedure for any dark matter model is yet a missing block within the dark matter tools world.…”
Section: Computation Of σV In Astrophysical Environmentsmentioning
confidence: 99%
“…One contribution comes from the majoron mixing with the longitudinal component of the Z boson, which then decays into two photons, see figure 2. Notice that only fermion loops contribute to this piece of the amplitude, because similar diagrams with the W boson and its Faddeev-Popov ghosts cancel each other [55]. The additional diagrams that arise from closing the leptonic lines in the W -boson loop of figure 1 b) are much more complicated to calculate, but we expect them to be further suppressed by the W mass or even the heavy neutrino mass, so we will neglect them for now.…”
Section: Jhep05(2017)102mentioning
confidence: 99%
“…Following the general expression given in Ref. [60], we computed the general amplitude for the χ 0 1 χ 0 1 → γγ process. Also, we used FeynArts [53] and FormCalc to reduce the tensor loop integrals to scalar Passarino-Veltman functions [61] and we used Package-X [62] to compute the amplitude of this process.…”
Section: Gamma-ray Signal: Dm Annihilation Into Two Photonsmentioning
confidence: 99%