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The Physics of Massive Star Death

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dc.contributor.advisor Thompson, Todd
dc.creator Pejcha, Ondrej
dc.date.accessioned 2011-04-04T11:36:09Z
dc.date.available 2011-04-04T11:36:09Z
dc.date.issued 2011-03
dc.identifier.uri http://hdl.handle.net/1811/48355
dc.description Mathematical and Physical Sciences: 1st Place (The Ohio State University Edward F. Hayes Graduate Research Forum) en_US
dc.description.abstract Neutrino heating may drive explosions of massive stars (core-collapse supernovae). Although it is known that the stalled accretion shock turns into explosion when the neutrino luminosity reaches critical value (L_crit), the reason for existence of L_crit as well as its dependence on parameters of the problem are unknown. We find that there is a direct correspondence between the isothermal accretion flow bounded by a shock and L_crit. We provide an accurate condition for explosion. We find that the luminosity from the cooling of the flow is sub-dominant to the core luminosity for driving the explosion. We suggest that the reduction in L_crit as a function of dimension is due to less efficient cooling in higher dimensions. en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries 2011 Edward F. Hayes Graduate Research Forum. 25th en_US
dc.subject supernova en_US
dc.subject shock wave en_US
dc.subject star en_US
dc.subject accretion en_US
dc.subject hydrodynamics en_US
dc.title The Physics of Massive Star Death en_US
dc.type Article en_US
dc.description.embargo No embargo en_US