2026-06-27T23:04:58Zhttps://docta.ucm.es/rest/oai/requestoai:docta.ucm.es:20.500.14352/437322023-08-26T19:31:50Zcom_20.500.14352_14col_20.500.14352_15
Docta Complutense
author
Ruiz Cembranos, José Alberto
author
Cruz Dombriz, Álvaro de la
author
Dobado González, Antonio
author
Lineros, R.
author
López Maroto, Antonio
2023-06-20T03:31:47Z
2023-06-20T03:31:47Z
2011
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.orghttp://arxiv.org/abs/1012.4473
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.
eng
Atribución 3.0 España
Fitting formulae for photon spectra from WIMP annihilation
journal article
URL
https://docta.ucm.es/bitstreams/d262cbc0-a7fd-4960-9c2d-7118d6ce8aad/download
File
MD5
4c34896b7ad8824f41139461276967cb
607652
application/pdf
DobadoAntonio09libre.pdf
URL
https://docta.ucm.es/bitstreams/615ae82f-50dc-4c4b-ab3d-789fe7cb4beb/download
File
MD5
477d0152985f9ff8af7b0aeecfd43203
13773
text/plain
DobadoAntonio09libre.pdf.txt