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Neutrino fluxes from dark matter in the HESS J1745-290 source at the Galactic center

dc.contributor.authorRuiz Cembranos, José Alberto
dc.contributor.authorGammaldi, Viviana
dc.contributor.authorLópez Maroto, Antonio
dc.date.accessioned2023-06-19T13:26:27Z
dc.date.available2023-06-19T13:26:27Z
dc.date.issued2014-08-07
dc.description© 2014 American Physical Society. We would like to thank Juande Zornoza and Carlos de los Heros for useful comments. This work has been supported by UCM predoctoral grant, MICINN (Spain) project numbers FIS 2008-01323, FIS2011-23000, FPA2011-27853-01, Consolider-Ingenio MULTIDARK CSD2009-00064, and the Department of Energy, Contract DE-AC02-76SF00515. J. A. R. C. thanks the support of the Becas Complutense del Amo program.
dc.description.abstractThe spectral study of the HESS J1745-290 high-energy gamma-ray cutoff from the Galactic center is compatible with a signal of dark matter (DM) annihilation or decay. If this is the case, a neutrino flux from that source is also expected. We analyze the neutrino flux predicted by DM particles able to create the HESS J1745-290 gamma-rays observations. We focus on the electroweak and hadronic channels, which are favored by present measurements. In particular, we study DM annihilating into W+W- and u (u) over bar with DM masses of 48.8 and 27.9 TeV, respectively. We estimate the resolution angle and exposition time necessary to test the DM hypothesis as the origin of the gamma-ray signal.
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.sponsorshipDepartment of Energy
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/27392
dc.identifier.doi10.1103/PhysRevD.90.043004
dc.identifier.issn1550-7998
dc.identifier.officialurlhttp://dx.doi.org/10.1103/PhysRevD.90.043004
dc.identifier.relatedurlhttp://journals.aps.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/33700
dc.issue.number4
dc.journal.titlePhysical Review D
dc.language.isoeng
dc.publisherAmerican Physical Society
dc.relation.projectIDFIS2008-01323
dc.relation.projectIDFIS2011-23000
dc.relation.projectIDFPA2011-27853-01
dc.relation.projectIDCSD2009-00064
dc.relation.projectIDDE-AC02-76SF00515
dc.rights.accessRightsopen access
dc.subject.cdu53
dc.subject.keywordGamma-ray source
dc.subject.keywordCenter black-hole
dc.subject.keywordHigh-energy
dc.subject.keywordHalos
dc.subject.keywordContraction
dc.subject.keywordSimulations
dc.subject.keywordTelescope
dc.subject.keywordDirection
dc.subject.keywordEmission
dc.subject.keywordBaryons
dc.subject.ucmFísica (Física)
dc.subject.unesco22 Física
dc.titleNeutrino fluxes from dark matter in the HESS J1745-290 source at the Galactic center
dc.typejournal article
dc.volume.number90
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