Ultra High Energy Neutrinos and Gamma Rays in Astrophysics: A Multi-messenger Study

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dc.contributor.authorSarmah, Prantik
dc.date.accessioned2024-04-25T06:53:01Z
dc.date.available2024-04-25T06:53:01Z
dc.date.issued2024
dc.descriptionSupervisor: Chakraborty, Sovanen_US
dc.description.abstractThe advancement of diverse high-energy neutrino and gamma-ray observatories has recently introduced a fresh perspective in multi-messenger astrophysics, enabling us to delve into the high-energy realms of our universe. This thesis embarks on a comprehensive examination of ultra-high energy (UHE) neutrinos and gamma-rays emitted by a variety of astrophysical sources, encompassing both Galactic and Extra-galactic entities such as young supernovae, supernova remnants, etc., spanning energy ranges from Giga-electronvolts to Zeta electronvolts. These particles emerge as secondary products resulting from the interactions of UHE cosmic rays with various targets such as protons and photons. The thesis investigates the propagation of these UHE secondary particles through space, while also scrutinizing their detectability, a crucial aspect for unraveling the origins and mechanisms behind high-energy cosmic ray production.en_US
dc.identifier.otherROLL NO.186121018
dc.identifier.urihttps://gyan.iitg.ac.in/handle/123456789/2602
dc.language.isoenen_US
dc.relation.ispartofseriesTH-3334;
dc.subjectUltra High Energyen_US
dc.subjectCosmic Raysen_US
dc.subjectCosmic Raysen_US
dc.subjectNeutrinosen_US
dc.subjectGamma Raysen_US
dc.subjectSupernovaeen_US
dc.titleUltra High Energy Neutrinos and Gamma Rays in Astrophysics: A Multi-messenger Studyen_US
dc.typeThesisen_US
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