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DC Field | Value | Language |
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dc.contributor.author | Primulando R. | |
dc.contributor.author | Uttayarat P. | |
dc.date.accessioned | 2021-04-05T03:22:57Z | - |
dc.date.available | 2021-04-05T03:22:57Z | - |
dc.date.issued | 2018 | |
dc.identifier.issn | 11266708 | |
dc.identifier.other | 2-s2.0-85048278940 | |
dc.identifier.uri | https://ir.swu.ac.th/jspui/handle/123456789/13266 | - |
dc.identifier.uri | https://www.scopus.com/inward/record.uri?eid=2-s2.0-85048278940&doi=10.1007%2fJHEP06%282018%29026&partnerID=40&md5=9bc9e46ee9a8760026a84dcbbcc3ae24 | |
dc.description.abstract | We 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.title | Dark matter-neutrino interaction in light of collider and neutrino telescope data | |
dc.type | Article | |
dc.rights.holder | Scopus | |
dc.identifier.bibliograpycitation | Journal of High Energy Physics. Vol 2018, No.6 (2018) | |
dc.identifier.doi | 10.1007/JHEP06(2018)026 | |
Appears in Collections: | Scopus 1983-2021 |
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