OSU Navigation Bar

The Ohio State University University Libraries Knowledge Bank

The Physics of Massive Star Death

Please use this identifier to cite or link to this item: http://hdl.handle.net/1811/48355

Show full item record

Files Size Format View
pejcha_proceedings.pdf 204.4Kb PDF View/Open

Title: The Physics of Massive Star Death
Creators: Pejcha, Ondrej
Advisor: Thompson, Todd
Issue Date: 2011-03
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.
Embargo: No embargo
Series/Report no.: 2011 Edward F. Hayes Graduate Research Forum. 25th
Keywords: supernova
shock wave
star
accretion
hydrodynamics
Description: Mathematical and Physical Sciences: 1st Place (The Ohio State University Edward F. Hayes Graduate Research Forum)
URI: http://hdl.handle.net/1811/48355
Bookmark and Share