Core-collapse supernovae and the equation of state
Core-collapse supernovae (CCSN) mark the end of the life of massive stars and are cosmic laboratories for physics at the extremes. Numerical simulations of these explosions are essential to understanding the complex mechanisms that are involved. All four fundamental interactions have to be taken i...
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Format: | Others |
Language: | en |
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2019
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Online Access: | https://tuprints.ulb.tu-darmstadt.de/8840/1/Dissertation_hannahyasin_final.pdf Yasin, Hannah <http://tuprints.ulb.tu-darmstadt.de/view/person/Yasin=3AHannah=3A=3A.html> (2019): Core-collapse supernovae and the equation of state.Darmstadt, Technische Universität, DOI: 10.25534/tuprints-00008840 <https://doi.org/10.25534/tuprints-00008840>, [Ph.D. Thesis] |
Internet
https://tuprints.ulb.tu-darmstadt.de/8840/1/Dissertation_hannahyasin_final.pdfYasin, Hannah <http://tuprints.ulb.tu-darmstadt.de/view/person/Yasin=3AHannah=3A=3A.html> (2019): Core-collapse supernovae and the equation of state.Darmstadt, Technische Universität, DOI: 10.25534/tuprints-00008840 <https://doi.org/10.25534/tuprints-00008840>, [Ph.D. Thesis]