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Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5642
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dc.contributor.authorChoudhury, Debajyotien_US
dc.contributor.authorMaharana, Suvamen_US
dc.contributor.authorSahdev, Vandanaen_US
dc.contributor.authorSACHDEVA, DIVYAen_US
dc.date.accessioned2021-02-23T08:40:19Z
dc.date.available2021-02-23T08:40:19Z
dc.date.issued2021-01en_US
dc.identifier.citationPhysical Review D, 103(1), 015006.en_US
dc.identifier.issn2470-0010en_US
dc.identifier.issn2470-0029en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5642
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.103.015006en_US
dc.description.abstractA very economic scenario with just three extra scalar fields beyond the Standard Model is invoked to explain the muon anomalous magnetic moment, the requisite relic abundance of dark matter as well as the XENON1T excess through the inelastic down-scattering of the dark scalar.en_US
dc.language.isoenen_US
dc.publisherAmerican Physical Societyen_US
dc.subjectVector Gauge Bosonen_US
dc.subjectPHI-Meson Decaysen_US
dc.subjectSearchen_US
dc.subjectConstraintsen_US
dc.subjectE(+)E(-)en_US
dc.subjectLimiten_US
dc.subject2021-FEB-WEEK2en_US
dc.subjectTOC-FEB-2021en_US
dc.subject2021en_US
dc.titleDark matter, muon anomalous magnetic moment, and the XENON1T excessen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitlePhysical Review Den_US
dc.publication.originofpublisherForeignen_US
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