Please use this identifier to cite or link to this item: https://ir.swu.ac.th/jspui/handle/123456789/13266
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dc.contributor.authorPrimulando R.
dc.contributor.authorUttayarat P.
dc.date.accessioned2021-04-05T03:22:57Z-
dc.date.available2021-04-05T03:22:57Z-
dc.date.issued2018
dc.identifier.issn11266708
dc.identifier.other2-s2.0-85048278940
dc.identifier.urihttps://ir.swu.ac.th/jspui/handle/123456789/13266-
dc.identifier.urihttps://www.scopus.com/inward/record.uri?eid=2-s2.0-85048278940&doi=10.1007%2fJHEP06%282018%29026&partnerID=40&md5=9bc9e46ee9a8760026a84dcbbcc3ae24
dc.description.abstractWe study the DM-neutrino interaction in the framework of simplified model. The phenomenology of such an interaction are derived. We also investigate the bound on DM-neutrino interaction from the LHC and neutrino telescopes. We find that for the case of a scalar dark matter, the LHC gives a stronger bound on dark matter annihilation cross-section than the neutrino telescopes. However, for the fermionic dark matter case the neutrino telescopes bounds are more stringent for dark matter mass, ≳ 200 MeV. In the case of lower DM mass, the neutrino telescopes provide better bounds for a light mediator, while the collider bounds are better for a heavy mediator. Possible UV completions of the simplified model are briefly discussed. © 2018, The Author(s).
dc.titleDark matter-neutrino interaction in light of collider and neutrino telescope data
dc.typeArticle
dc.rights.holderScopus
dc.identifier.bibliograpycitationJournal of High Energy Physics. Vol 2018, No.6 (2018)
dc.identifier.doi10.1007/JHEP06(2018)026
Appears in Collections:Scopus 1983-2021

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