Nuclear reaction rates and opacity in massive star evolution calculations

dc.contributor.authorBahena, David
dc.contributor.authorKlapp, Jaime
dc.contributor.authorDehnen, Heinz
dc.date.accessioned2021-03-29T07:30:24Z
dc.date.available2021-03-29T07:30:24Z
dc.date.issued2010-08-02eng
dc.description.abstractNuclear reaction rates and opacity are important parameters in stellar evolution. The input physics in a stellar evolution code determines the main theoretical characteristics of the stellar structure, evolution and nucleosynthesis of a star. For different input physics, in this work we calculate stellar evolution models of very massive first stars during the hydrogen and helium burning phases. We have considered 100 and 200M galactic and pregalactic stars with metallicity Z = 10−6 and 109, respectively. The results show important differences from old to new formulations for the opacity and nuclear reaction rates, in particular the evolutionary tracks are significantly affected, that indicates the importance of using up to date and reliable input physics. The triple alpha reaction activates sooner for pregalactic than for galactic stars.eng
dc.description.versionpublishedde
dc.identifier.doi10.1088/1742-6596/239/1/012004eng
dc.identifier.urihttps://kops.uni-konstanz.de/handle/123456789/53282
dc.language.isoengeng
dc.subject.ddc530eng
dc.titleNuclear reaction rates and opacity in massive star evolution calculationseng
dc.typeJOURNAL_ARTICLEde
dspace.entity.typePublication
kops.citation.bibtex
@article{Bahena2010-08-02Nucle-53282,
  year={2010},
  doi={10.1088/1742-6596/239/1/012004},
  title={Nuclear reaction rates and opacity in massive star evolution calculations},
  volume={239},
  issn={1742-6588},
  journal={Journal of Physics: Conference Series},
  author={Bahena, David and Klapp, Jaime and Dehnen, Heinz},
  note={Article Number: 012004}
}
kops.citation.iso690BAHENA, David, Jaime KLAPP, Heinz DEHNEN, 2010. Nuclear reaction rates and opacity in massive star evolution calculations. In: Journal of Physics: Conference Series. Institute of Physics Publishing (IOP). 2010, 239, 012004. ISSN 1742-6588. eISSN 1742-6596. Available under: doi: 10.1088/1742-6596/239/1/012004deu
kops.citation.iso690BAHENA, David, Jaime KLAPP, Heinz DEHNEN, 2010. Nuclear reaction rates and opacity in massive star evolution calculations. In: Journal of Physics: Conference Series. Institute of Physics Publishing (IOP). 2010, 239, 012004. ISSN 1742-6588. eISSN 1742-6596. Available under: doi: 10.1088/1742-6596/239/1/012004eng
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kops.sourcefieldJournal of Physics: Conference Series. Institute of Physics Publishing (IOP). 2010, <b>239</b>, 012004. ISSN 1742-6588. eISSN 1742-6596. Available under: doi: 10.1088/1742-6596/239/1/012004deu
kops.sourcefield.plainJournal of Physics: Conference Series. Institute of Physics Publishing (IOP). 2010, 239, 012004. ISSN 1742-6588. eISSN 1742-6596. Available under: doi: 10.1088/1742-6596/239/1/012004deu
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source.publisherInstitute of Physics Publishing (IOP)eng

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