Impact of the Equation of State in Core-Collapse Supernovae
One of the key ingredients to the core collapse supernova mechanism is the physics of matter at or near nuclear density. Included in simulations as part of the Equation of State (EoS), nuclear repulsion experienced at high densities is responsible for the bounce shock, which initially causes the out...
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Trace: Tennessee Research and Creative Exchange
2007
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| Online Access: | http://trace.tennessee.edu/utk_gradthes/109 |