High-Energy Neutrino Flavor State Transition Probabilities

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dc.citation.articleNumber10666en_US
dc.citation.issueNumber22en_US
dc.citation.journalTitleApplied Sciencesen_US
dc.citation.volumeNumber14en_US
dc.contributor.authorHarrison, Johnen_US
dc.contributor.authorAnantua, Richarden_US
dc.date.accessioned2025-01-09T20:16:59Zen_US
dc.date.available2025-01-09T20:16:59Zen_US
dc.date.issued2024en_US
dc.description.abstractWe analytically determine neutrino transitional probabilities and abundance ratios at various distances from the source of creation in several astrophysical contexts, including the Sun, supernovae and cosmic rays. In doing so, we determine the probability of a higher-order transition state from ντ→νλ, where νλ represents a more massive generation than Standard Model neutrinos. We first calculate an approximate cross-section for high-energy neutrinos which allows us to formulate comparisons for the oscillation distances of solar, supernova and higher-energy cosmic ray neutrinos. The flavor distributions of the resulting neutrino populations from each source detected on Earth are then compared via fractional density charts.en_US
dc.identifier.citationHarrison, J., & Anantua, R. (2024). High-Energy Neutrino Flavor State Transition Probabilities. Applied Sciences, 14(22), Article 22. https://doi.org/10.3390/app142210666en_US
dc.identifier.digitalapplsci-14-10666-v2en_US
dc.identifier.doihttps://doi.org/10.3390/app142210666en_US
dc.identifier.urihttps://hdl.handle.net/1911/118120en_US
dc.language.isoengen_US
dc.publisherMDPIen_US
dc.rightsExcept where otherwise noted, this work is licensed under a Creative Commons Attribution (CC BY) license. Permission to reuse, publish, or reproduce the work beyond the terms of the license or beyond the bounds of fair use or other exemptions to copyright law must be obtained from the copyright holder.en_US
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/en_US
dc.subject.keywordneutrinosen_US
dc.subject.keywordneutrino oscillationen_US
dc.subject.keyworddetectionen_US
dc.titleHigh-Energy Neutrino Flavor State Transition Probabilitiesen_US
dc.typeJournal articleen_US
dc.type.dcmiTexten_US
dc.type.publicationpublisher versionen_US
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