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Fitting formulae for photon spectra from WIMP annihilation

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dc.contributor.authorRuiz Cembranos, José Alberto
dc.contributor.authorCruz Dombriz, Álvaro de la
dc.contributor.authorDobado González, Antonio
dc.contributor.authorLineros, R.
dc.contributor.authorLópez Maroto, Antonio
dc.date.accessioned2023-06-20T03:31:47Z
dc.date.available2023-06-20T03:31:47Z
dc.date.issued2011
dc.description© IOP Publishing. Spanish Relativity Meeting on Gravity as a Crossroad in Physics (2010. Granada,España). This work was supported by MICINN (Spain) project numbers FIS 2008-01323 and FPA 2008- 00592, FPA2008-00319, CAM/UCM 910309, and Consolider-Ingenio MULTIDARK CSD2009- 00064. AdlCD was also supported by the National Research Foundation (South Africa). RL was also supported by the EC contract UNILHC PITN-GA-2009-237920 and PROMETEO/2009/091 (Generalitat Valenciana).
dc.description.abstractAnnihilation 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.
dc.description.departmentDepto. de Física Teórica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipMICINN (Spain)
dc.description.sponsorshipConsolider-Ingenio MULTIDARK
dc.description.sponsorshipNational Research Foundation (South Africa)
dc.description.sponsorshipEC contract
dc.description.sponsorshipGeneralitat Valenciana
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/20682
dc.identifier.doi10.1088/1742-6596/314/1/012063
dc.identifier.issn1742-6588
dc.identifier.officialurlhttp://dx.doi.org/10.1088/1742-6596/314/1/012063
dc.identifier.relatedurlhttp://iopscience.iop.org
dc.identifier.relatedurlhttp://arxiv.org/abs/1012.4473
dc.identifier.urihttps://hdl.handle.net/20.500.14352/43732
dc.journal.titleJournal of Physics: Conference Series
dc.language.isoeng
dc.publisherIop Publishing Ltd
dc.relation.projectIDFIS 2008-01323
dc.relation.projectIDFPA 2008- 00592
dc.relation.projectIDFPA 2008-00319
dc.relation.projectIDCAM/UCM 910309
dc.relation.projectIDCSD2009- 00064
dc.relation.projectIDUNILHC PITN-GA-2009-237920
dc.relation.projectIDPROMETEO/2009/091
dc.rightsAtribución 3.0 España
dc.rights.accessRightsopen access
dc.rights.urihttps://creativecommons.org/licenses/by/3.0/es/
dc.subject.cdu53
dc.subject.ucmFísica (Física)
dc.subject.unesco22 Física
dc.titleFitting formulae for photon spectra from WIMP annihilation
dc.typejournal article
dc.volume.number314
dcterms.references[1] K. Sigurdson and M. Kamionkowski, PRL 92, 171302 (2004); J. A. R. Cembranos et al. , PRL 90, 241301 (2003); J. A. R. Cembranos and L. E. Strigari, PRD 77, 123519 (2008); J. A. R. Cembranos, PRL 102, 141301 (2009). [2] J. A. R. Cembranos, A. de la Cruz-Dombriz, A. Dobado, R. A. Lineros, A. L. Maroto, arXiv(hep-ph): http://arxiv.org/abs/1009.4936. [3] T. Sjostrand, S. Mrenna and P. Skands, JHEP05 (2006) 026 (LUTP 06-13, FERMILAB-PUB-06-052-CD-T).
dspace.entity.typePublication
relation.isAuthorOfPublicationc5a4cc87-ceba-494d-95ab-d54b9b1a35e3
relation.isAuthorOfPublication16523fad-99a9-422c-9a8e-c949ccffadec
relation.isAuthorOfPublicatione14691a1-d3b0-47b7-96d5-24d645534471
relation.isAuthorOfPublication.latestForDiscoveryc5a4cc87-ceba-494d-95ab-d54b9b1a35e3

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