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- W1504202136 abstract "We present results from the first generation of multi-dimensional general relativistic neutrino hydrodynamics simulations of core-collapse supernovae. A comparison with models computed using either the purely Newtonian approximation or the effective gravitational potential approach reveals appreciable quantitative differences in the heating conditions and the gravitational wave spectra. Our results underscore the important role of general relativity in the supernova problem (which appears to be on par with other important factors such as the dimensionality and the equation of state) both for our understanding of the explosion dynamics as well as for predictions of observable signatures." @default.
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- W1504202136 date "2011-12-08" @default.
- W1504202136 modified "2023-09-27" @default.
- W1504202136 title "General Relativistic Explosion Models of Core-Collapse Supernovae" @default.
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