2026-06-28T04:47:41Zhttps://docta.ucm.es/rest/oai/request

oai:docta.ucm.es:20.500.14352/437322023-08-26T19:31:50Zcom_20.500.14352_14col_20.500.14352_15

00925njm 22002777a 4500 dc Ruiz Cembranos, José Alberto author Cruz Dombriz, Álvaro de la author Dobado González, Antonio author Lineros, R. author López Maroto, Antonio author 2011 Annihilation of different dark matter (DM) candidates into Standard Model (SM) particles could be detected through their contribution to the gamma ray fluxes that are measured on the Earth. The magnitude of such contributions depends on the particular DM candidate, but certain imprints of produced photon spectra may be analyzed in a model-independent fashion. In this work we provide the fitting formulae for the photon spectra generated by WIMP annihilation into quarks, leptons and gauge bosons channels in a wide range of WIMP masses. 1742-6588 10.1088/1742-6596/314/1/012063 https://hdl.handle.net/20.500.14352/43732 http://dx.doi.org/10.1088/1742-6596/314/1/012063 http://iopscience.iop.org http://arxiv.org/abs/1012.4473 Fitting formulae for photon spectra from WIMP annihilation