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Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/7755
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dc.contributor.authorSahdev, Vandana-
dc.contributor.authorMaharana, Suvam-
dc.contributor.authorSACHDEVA, DIVYA-
dc.contributor.editorMohanty, Bedangadas-
dc.contributor.editorSwain, Sanjay Kumar-
dc.contributor.editorSingh, Ranbir-
dc.contributor.editorKashyap, Varchaswi K. S.-
dc.date.accessioned2023-04-26T09:28:11Z-
dc.date.available2023-04-26T09:28:11Z-
dc.date.issued2022-10-
dc.identifier.citationProceedings of the XXIV DAE-BRNS High Energy Physics Symposium, Jatni, India, 287–291.en_US
dc.identifier.isbn9789811923531-
dc.identifier.isbn9789811923548-
dc.identifier.urihttps://doi.org/10.1007/978-981-19-2354-8_52en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/7755-
dc.description.abstractWe discuss how the recent observation of an excess in the electron recoil events at the XENON1T detector, coupled with the requirement to explain the issue of dark matter relic density and muon anomalous magnetic moment, can be addressed using a scalar sector extension of the standard model.en_US
dc.language.isoenen_US
dc.publisherSpringer Natureen_US
dc.subjectInelastic scatteringen_US
dc.subjectXENON1Ten_US
dc.subjectMuon g-2en_US
dc.subjectDark matteren_US
dc.subject2022en_US
dc.titleExplaining the XENON1T Excess and Dark Matter with Three Scalarsen_US
dc.typeBook chapteren_US
dc.contributor.departmentDept. of Physicsen_US
dc.title.bookProceedings of the XXIV DAE-BRNS High Energy Physics Symposium, Jatni, Indiaen_US
dc.identifier.sourcetitleProceedings of the XXIV DAE-BRNS High Energy Physics Symposium, Jatni, Indiaen_US
dc.publication.originofpublisherForeignen_US
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