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- W1927821502 abstract ". Gravitational radiation from the first phase of the gravitational collapse of a stellar core, i.e. the dynamical phase which precedes the formation of a shock and a bounce, is studied by means of a 3-D pseudo-spectral self-gravitating hydro code. It is shown that the efficiency of this process is very low (of the order of a few percent) and insensitive to the equation of state and to whether the initial configuration is axisymmetric, with an initial quadrupole of rotational or tidal origin, or fully asymmetric. An attempt to treat shock waves in asymmetric situations is described and preliminary results obtained from stellar core bounce are presented." @default.
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- W1927821502 date "1992-12-10" @default.
- W1927821502 modified "2023-09-27" @default.
- W1927821502 title "Gravitational radiation from 3D gravitational stellar core collapse" @default.
- W1927821502 doi "https://doi.org/10.1017/cbo9780511524639.022" @default.
- W1927821502 hasPublicationYear "1992" @default.
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