Please use this identifier to cite or link to this item: http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5398
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dc.contributor.authorGHOSH, DIPTIMOYen_US
dc.contributor.authorSACHDEVA, DIVYAen_US
dc.date.accessioned2020-12-04T11:39:56Z-
dc.date.available2020-12-04T11:39:56Z-
dc.date.issued2020-10en_US
dc.identifier.citationJournal of Cosmology and Astroparticle Physics, 2020.en_US
dc.identifier.issn1475-7516en_US
dc.identifier.urihttp://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5398-
dc.identifier.urihttps://doi.org/10.1088/1475-7516/2020/10/060en_US
dc.description.abstractIn this article, we study the implications of the coupling between Axion-Like-Particles (ALPs) and Leptons to cosmology in particular, the Big Bang Nucleosynthesis (BBN) . We show that the BBN, through the constraint on the effective number of relativistic neutrino species, provides the most stringent bound on the ALP-electron interaction strength for the mass of axion between 20 keV and 1 MeV . For other values of the mass, the BBN bound complements the stellar-evolution and laboratory bounds.en_US
dc.language.isoenen_US
dc.publisherIOP Publishingen_US
dc.subjectAxionsen_US
dc.subjectBig bang nucleosynthesisen_US
dc.subject2020en_US
dc.subject2020-DEC-WEEK1en_US
dc.subjectTOC-DEC-2020en_US
dc.titleConstraints on Axion-Lepton coupling from Big Bang Nucleosynthesisen_US
dc.typeArticleen_US
dc.contributor.departmentDept. of Physicsen_US
dc.identifier.sourcetitleJournal of Cosmology and Astroparticle Physicsen_US
dc.publication.originofpublisherForeignen_US
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