Please use this identifier to cite or link to this item:
http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5398
Full metadata record
DC Field | Value | Language |
---|---|---|
dc.contributor.author | GHOSH, DIPTIMOY | en_US |
dc.contributor.author | SACHDEVA, DIVYA | en_US |
dc.date.accessioned | 2020-12-04T11:39:56Z | - |
dc.date.available | 2020-12-04T11:39:56Z | - |
dc.date.issued | 2020-10 | en_US |
dc.identifier.citation | Journal of Cosmology and Astroparticle Physics, 2020. | en_US |
dc.identifier.issn | 1475-7516 | en_US |
dc.identifier.uri | http://dr.iiserpune.ac.in:8080/xmlui/handle/123456789/5398 | - |
dc.identifier.uri | https://doi.org/10.1088/1475-7516/2020/10/060 | en_US |
dc.description.abstract | In 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.iso | en | en_US |
dc.publisher | IOP Publishing | en_US |
dc.subject | Axions | en_US |
dc.subject | Big bang nucleosynthesis | en_US |
dc.subject | 2020 | en_US |
dc.subject | 2020-DEC-WEEK1 | en_US |
dc.subject | TOC-DEC-2020 | en_US |
dc.title | Constraints on Axion-Lepton coupling from Big Bang Nucleosynthesis | en_US |
dc.type | Article | en_US |
dc.contributor.department | Dept. of Physics | en_US |
dc.identifier.sourcetitle | Journal of Cosmology and Astroparticle Physics | en_US |
dc.publication.originofpublisher | Foreign | en_US |
Appears in Collections: | JOURNAL ARTICLES |
Files in This Item:
There are no files associated with this item.
Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.