Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/8190
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dc.contributor.authorPandey, Sujataen_US
dc.contributor.authorKarmakar, Siddharthaen_US
dc.contributor.authorRakshit, Subhenduen_US
dc.date.accessioned2022-03-17T01:00:00Z-
dc.date.accessioned2022-03-21T11:15:29Z-
dc.date.available2022-03-17T01:00:00Z-
dc.date.available2022-03-21T11:15:29Z-
dc.date.issued2019-
dc.identifier.citationPandey, S., Karmakar, S., & Rakshit, S. (2019). Interactions of astrophysical neutrinos with dark matter: A model building perspective. Journal of High Energy Physics, 2019(1) doi:10.1007/JHEP01(2019)095en_US
dc.identifier.issn1029-8479-
dc.identifier.otherEID(2-s2.0-85060162038)-
dc.identifier.urihttps://doi.org/10.1007/JHEP01(2019)095-
dc.identifier.urihttps://dspace.iiti.ac.in/handle/123456789/8190-
dc.description.abstractWe explore the possibility that high energy astrophysical neutrinos can interact with the dark matter on their way to Earth. Keeping in mind that new physics might leave its signature at such energies, we have considered all possible topologies for effective interactions between neutrino and dark matter. Building models, that give rise to a significant flux suppression of astrophysical neutrinos at Earth, is rather difficult. We present a Z′-mediated model in this context. Encompassing a large variety of models, a wide range of dark matter masses from 10−21 eV up to a TeV, this study aims at highlighting the challenges one encounters in such a model building endeavour after satisfying various cosmological constraints, collider search limits and electroweak precision measurements. © 2019, The Author(s).en_US
dc.language.isoenen_US
dc.publisherSpringer Verlagen_US
dc.sourceJournal of High Energy Physicsen_US
dc.titleInteractions of astrophysical neutrinos with dark matter: a model building perspectiveen_US
dc.typeJournal Articleen_US
dc.rights.licenseAll Open Access, Gold, Green-
Appears in Collections:Department of Physics

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