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Please use this identifier to cite or link to this item: https://dspace.iiti.ac.in/handle/123456789/7710
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dc.contributor.authorPandey, Sujataen_US
dc.date.accessioned2022-03-17T01:00:00Z-
dc.date.accessioned2022-03-21T11:13:48Z-
dc.date.available2022-03-17T01:00:00Z-
dc.date.available2022-03-21T11:13:48Z-
dc.date.issued2021-
dc.identifier.citationPandey, S. (2021). Can new interactions with dark matter lead to flux change of astrophysical neutrinos at icecube? Paper presented at the Springer Proceedings in Physics, , 261 977-980. doi:10.1007/978-981-33-4408-2_141en_US
dc.identifier.isbn9.78981E+12-
dc.identifier.issn0930-8989-
dc.identifier.otherEID(2-s2.0-85111078431)-
dc.identifier.urihttps://doi.org/10.1007/978-981-33-4408-2_141-
dc.identifier.urihttps://dspace.iiti.ac.in/handle/123456789/7710-
dc.description.abstractNeutrinos can scatter off the dark matter as they travel through the cosmos and reach the Earth. These interactions can alter the neutrino spectrum at IceCube. Here, we explore the possibility of changes in the neutrino spectrum as neutrino interacts with the dark matter by considering neutrino–dark matter interaction. In this context, interactions via light Z′ mediators are particularly interesting as they can lead to dip and cut-off like features in the neutrino spectrum at IceCube. We illustrate that various models of AGN, which predict more flux than the observed at IceCube, can be resolved through this mechanism. © 2021, Springer Nature Singapore Pte Ltd.en_US
dc.language.isoenen_US
dc.publisherSpringer Science and Business Media Deutschland GmbHen_US
dc.sourceSpringer Proceedings in Physicsen_US
dc.subjectDark Matteren_US
dc.subjectGalaxiesen_US
dc.subjectIce cubesen_US
dc.subjectNeutrino spectrumen_US
dc.subjectNeutronsen_US
dc.titleCan New Interactions with Dark Matter Lead to Flux Change of Astrophysical Neutrinos at Icecube?en_US
dc.typeConference Paperen_US
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