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dc.contributor.authorCirelli, Marco
dc.contributor.authorFornengo, Nicolao
dc.contributor.authorKavanagh, Bradley James
dc.contributor.authorPinettia, Elena
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2024-02-07T10:36:20Z
dc.date.available2024-02-07T10:36:20Z
dc.date.issued2022
dc.identifier.issn1824-8039
dc.identifier.urihttps://hdl.handle.net/10902/31501
dc.description.abstractWe present bounds on Dark Matter (DM) in the MeV to GeV mass range, obtained by using X-ray measurements from the Integral telescope. A crucial element, that allows us to derived bounds competitive or stronger than existing ones from other techniques, resides in the inclusion of the contribution from inverse Compton scattering on galactic radiation fields and on the CMB. This contribution is based on [1], to which we refer for additional detailses_ES
dc.description.sponsorshipFunding and research infrastructure acknowledgements. The original work [1] on which this proceeding is based had benefitted from the following funding: ∗ European Research Council (Erc) under the EU Seventh Framework Programme (FP7/2007-2013)/Erc Starting Grant (agreement n. 278234 — ‘NewDark’ project) [work of M.C.]. ∗ Cnrs 80|Prime grant (‘DaMeFer’ project) [work of M.C.]. ∗ Departments of Excellence grant awarded by the Italian Ministry of Education, University and Research (Miur) [work of N.F. and E.P.]. ∗ Research grant of the Università Italo-Francese, under Bando Vinci 2020 [work of E.P.]. ∗ Research grant The Dark Universe: A Synergic Multimessenger Approach, No. 2017X7X85K funded by the Italian Ministry of Education, University and Research (Miur) [work of N.F. and E.P.]. ∗ Research grant The Anisotropic Dark Universe, No. CSTO161409, funded by Compagnia di Sanpaolo and University of Torino [work of N.F. and E.P.]. ∗ Research grant TAsP (Theoretical Astroparticle Physics) funded by Istituto Nazionale di Fisica Nucleare (Infn) [work of N.F. and E.P.]. ∗ Spanish Agencia Estatal de Investigación (Aei, Miciu) for the support to the Unidad de Excelencia María de Maeztu Instituto de Física de Cantabria, ref. MDM-2017-0765 [work of B.J.K.].es_ES
dc.format.extent8 p.es_ES
dc.language.isoenges_ES
dc.publisherSissa Medialabes_ES
dc.rightsAttribution-NonCommercial-NoDerivatives 4.0 International © Los autoreses_ES
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/*
dc.sourcePoS - Proceedings of Science, 2022, 406, 096es_ES
dc.titleSub-GeV dark matter and X-rayses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://pos.sissa.it/406/096/es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.22323/1.406.0096
dc.type.versionpublishedVersiones_ES


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Attribution-NonCommercial-NoDerivatives 4.0 International © Los autoresExcepto si se señala otra cosa, la licencia del ítem se describe como Attribution-NonCommercial-NoDerivatives 4.0 International © Los autores