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곽규진

Kwak, Kyujin
Computational Astrophysics Lab.
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dc.citation.conferencePlace KO -
dc.citation.title 14th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG2017 -
dc.citation.volume 1947 -
dc.contributor.author Ko. Heamin -
dc.contributor.author Kusakabe, Motohiko -
dc.contributor.author Cheoun, Myung-Ki -
dc.contributor.author Kwak, Kyujin -
dc.contributor.author Kim, Kyungsik -
dc.date.accessioned 2023-12-19T18:39:24Z -
dc.date.available 2023-12-19T18:39:24Z -
dc.date.created 2018-11-01 -
dc.date.issued 2017-06-27 -
dc.description.abstract Stars ending with core collapse supernovae (SNe) emit a tremendous number of neutrinos during their explosions. While these neutrinos pass through each layer of the stars, they react with the nuclides in the progenitor. Although the neutrino cross sections are very small, its huge flux is high enough to react with nuclides to change their abundances. We consider this ν-process, by which abundances of some elements may be explained exclusively by this neutrino process. One of the candidates is 98Tc. In this study, we check the ν-process contributions due to the neutrino reactions. In this calculation we also include the neutrino oscillation effect in the matter with varying density, so called MSW effect, not only for 98Tc production but also 4He and 12C destruction, which occurs at first in the He/C layer in the present model. -
dc.identifier.bibliographicCitation 14th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG2017, v.1947 -
dc.identifier.doi 10.1063/1.5030831 -
dc.identifier.isbn 978-073541642-0 -
dc.identifier.issn 0094-243X -
dc.identifier.scopusid 2-s2.0-85047476609 -
dc.identifier.uri https://scholarworks.unist.ac.kr/handle/201301/37531 -
dc.identifier.url https://aip.scitation.org/doi/abs/10.1063/1.5030831 -
dc.language 영어 -
dc.publisher 14th International Symposium on Origin of Matter and Evolution of Galaxies, OMEG2017 -
dc.title Production of light elements and 98Tc through the ν -process with the neutrino oscillation in supernova explosion -
dc.type Conference Paper -
dc.date.conferenceDate 2017-06-27 -

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