Impact of a Finite-Temperature Equation of State on Neutron Stars
In this research, we study how a finite-temperature nuclear equation of state suitable for astrophysical simulations impacts the oscillation modes of neutron stars. We chose the Shen equation of state (EOS) because it accurately describes both stable and unstable nuclei as well as nuclear incompress...
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| Format: | Others |
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BYU ScholarsArchive
2011
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| Online Access: | https://scholarsarchive.byu.edu/etd/2603 https://scholarsarchive.byu.edu/cgi/viewcontent.cgi?article=3602&context=etd |