Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/8536
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dc.contributor.authorBHOWMICK, SUPRITHAen_US
dc.contributor.authorGHOSH, DIPTIMOYen_US
dc.contributor.authorSachdeva, Divyaen_US
dc.date.accessioned2024-02-12T11:51:00Z-
dc.date.available2024-02-12T11:51:00Z-
dc.date.issued2023-07en_US
dc.identifier.citationJournal of Cosmology and Astroparticle Physics, 2023(07).en_US
dc.identifier.issn1475-7516en_US
dc.identifier.urihttps://doi.org/10.1088/1475-7516/2023/07/039en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/8536-
dc.description.abstractElastic collisions with relativistic electrons from the blazar's jet can accelerate dark matter (DM) particles in the DM spike surrounding the supermassive black hole at its center. This can allow one to set stringent limits on the DM-electron scattering cross section (σ̅eχ) for DM masses less than 100 MeV. We consider DM particles boosted by energetic electrons in the jets of the blazars TXS 0506+056 and BL Lacertae. Both vector and scalar mediators for the scattering of electron and electrophilic fermionic DM are studied. We highlight that the ensuing energy dependence of the S-matrix for the corresponding Lorentz structure of the vertex significantly modifies the constraints. We find that the revised exclusion limits are orders of magnitude stronger than the equivalent results for the simple constant cross section assumption. Our limits are also assessed for the less cuspy spike.en_US
dc.language.isoenen_US
dc.publisherIOP Publishingen_US
dc.subjectDark matter experimentsen_US
dc.subjectDark matter theoryen_US
dc.subject2023en_US
dc.titleBlazar boosted dark matter direct detection constraints on aex: role of energy dependent cross sectionen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitleJournal of Cosmology and Astroparticle Physicsen_US
dc.publication.originofpublisherForeignen_US
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