Please use this identifier to cite or link to this item: http://hdl.handle.net/123456789/2748
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dc.contributor.authorJha, Ashish Kumar-
dc.date.accessioned2026-02-18T10:42:01Z-
dc.date.available2026-02-18T10:42:01Z-
dc.date.issued2024-04-01-
dc.identifier.urihttp://hdl.handle.net/123456789/2748-
dc.description.abstractIn recent years, we have seen significant advances in observational astrophysics. These observations allow us to probe our fundamental physics theories, i.e., to test our standard model. In this thesis, we will explore a case using relics from the early universe, specifically Big Bang Nucleosynthesis, to investigate an existing tension in neutron lifetime measurements. We will introduce new states carrying baryon numbers(darkbaryons)toaddress theneutronlifetime issue. In particular, we examine a model of dark baryons that give rise to purely invisible dark decay channels of neutrons and, hence, are difficult to detect in terrestrial experiments. We can show that this model, nonetheless, impacts primordial nucleosynthesis, particularly altering the abundanceofDand4He. Thisgivesrisetonewconstraints, which we derive considering this dark baryon as a dark matter candidate.en_US
dc.language.isoenen_US
dc.publisherIISER- Mohalien_US
dc.subjectThermal History of the Universeen_US
dc.subjectBig Bang Nucleosynthesisen_US
dc.subjectDark Neutron Modelsen_US
dc.subjectNeutron Dark Decayen_US
dc.titleDark Neutron Models in Big Bang Nucleosynthesisen_US
dc.typeThesisen_US
dc.guideProf. Harvinder Kaur Jassal and Prof. Nirmal Rajen_US
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