Fitting formulae for photon spectra from WIMP annihilation

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 p...

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Detalles Bibliográficos
Autores: Ruiz Cembranos, José Alberto, Cruz Dombriz, Álvaro de la, Dobado González, Antonio, Lineros, R., López Maroto, Antonio
Tipo de recurso: artículo
Fecha de publicación:2011
País:España
Institución:Universidad Complutense de Madrid (UCM)
Repositorio:Docta Complutense
Idioma:inglés
OAI Identifier:oai:docta.ucm.es:20.500.14352/43732
Acceso en línea:https://hdl.handle.net/20.500.14352/43732
Access Level:acceso abierto
Palabra clave:53
Física (Física)
22 Física
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spelling Fitting formulae for photon spectra from WIMP annihilationRuiz Cembranos, José AlbertoCruz Dombriz, Álvaro de laDobado González, AntonioLineros, R.López Maroto, Antonio53Física (Física)22 FísicaAnnihilation 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.Iop Publishing LtdUniversidad Complutense de Madrid20112011-01-0120112011-01-01journal articlehttp://purl.org/coar/resource_type/c_6501info:eu-repo/semantics/articleapplication/pdfhttps://hdl.handle.net/20.500.14352/43732reponame:Docta Complutenseinstname:Universidad Complutense de Madrid (UCM)Inglésengopen accesshttp://purl.org/coar/access_right/c_abf2Atribución 3.0 Españahttps://creativecommons.org/licenses/by/3.0/es/info:eu-repo/semantics/openAccessoai:docta.ucm.es:20.500.14352/437322026-06-02T12:44:21Z
dc.title.none.fl_str_mv Fitting formulae for photon spectra from WIMP annihilation
title Fitting formulae for photon spectra from WIMP annihilation
spellingShingle Fitting formulae for photon spectra from WIMP annihilation
Ruiz Cembranos, José Alberto
53
Física (Física)
22 Física
title_short Fitting formulae for photon spectra from WIMP annihilation
title_full Fitting formulae for photon spectra from WIMP annihilation
title_fullStr Fitting formulae for photon spectra from WIMP annihilation
title_full_unstemmed Fitting formulae for photon spectra from WIMP annihilation
title_sort Fitting formulae for photon spectra from WIMP annihilation
dc.creator.none.fl_str_mv Ruiz Cembranos, José Alberto
Cruz Dombriz, Álvaro de la
Dobado González, Antonio
Lineros, R.
López Maroto, Antonio
author Ruiz Cembranos, José Alberto
author_facet Ruiz Cembranos, José Alberto
Cruz Dombriz, Álvaro de la
Dobado González, Antonio
Lineros, R.
López Maroto, Antonio
author_role author
author2 Cruz Dombriz, Álvaro de la
Dobado González, Antonio
Lineros, R.
López Maroto, Antonio
author2_role author
author
author
author
dc.contributor.none.fl_str_mv Universidad Complutense de Madrid
dc.subject.none.fl_str_mv 53
Física (Física)
22 Física
topic 53
Física (Física)
22 Física
description 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.
publishDate 2011
dc.date.none.fl_str_mv 2011
2011-01-01
2011
2011-01-01
dc.type.none.fl_str_mv journal article
http://purl.org/coar/resource_type/c_6501
dc.type.openaire.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.none.fl_str_mv https://hdl.handle.net/20.500.14352/43732
url https://hdl.handle.net/20.500.14352/43732
dc.language.none.fl_str_mv Inglés
eng
language_invalid_str_mv Inglés
language eng
dc.rights.none.fl_str_mv open access
http://purl.org/coar/access_right/c_abf2
Atribución 3.0 España
https://creativecommons.org/licenses/by/3.0/es/
dc.rights.openaire.fl_str_mv info:eu-repo/semantics/openAccess
rights_invalid_str_mv open access
http://purl.org/coar/access_right/c_abf2
Atribución 3.0 España
https://creativecommons.org/licenses/by/3.0/es/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv Iop Publishing Ltd
publisher.none.fl_str_mv Iop Publishing Ltd
dc.source.none.fl_str_mv reponame:Docta Complutense
instname:Universidad Complutense de Madrid (UCM)
instname_str Universidad Complutense de Madrid (UCM)
reponame_str Docta Complutense
collection Docta Complutense
repository.name.fl_str_mv
repository.mail.fl_str_mv
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score 15.300719

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