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3
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85038927640
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C. R. Evans in Proceedings of 13th Texas Symposium on Relativistic Astrophysics, edited by M. P. Ulmer (World Scientific, Singapore, 1987), p. 152.
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C. R. Evans in Proceedings of 13th Texas Symposium on Relativistic Astrophysics, edited by M. P. Ulmer (World Scientific, Singapore, 1987), p. 152.
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4
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85038932076
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The initial recoil shocks alone may generate nearly constant entropy when the equation of state is sufficiently stiff, in which case the progenitor stars are nearly homogeneous and the pre-shock gas parameters nearly uniform. Neutrino diffusion and convection may further reduce the entropy gradient.
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The initial recoil shocks alone may generate nearly constant entropy when the equation of state is sufficiently stiff, in which case the progenitor stars are nearly homogeneous and the pre-shock gas parameters nearly uniform. Neutrino diffusion and convection may further reduce the entropy gradient.
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5
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85038924602
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A. M. Abrahams and C. R. Evans in Proceedings of the 6th Marcel Grossman Meeting on General Relativity, edited by F. Sato and T. Nakamura (World Scientific, Singapore, 1992), p. 1331.
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A. M. Abrahams and C. R. Evans in Proceedings of the 6th Marcel Grossman Meeting on General Relativity, edited by F. Sato and T. Nakamura (World Scientific, Singapore, 1992), p. 1331.
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6
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85038927575
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One must be especially careful to obey constraint (18) when setting up a numerical simulation, where it is not possible to start the stars off at infinite separation.
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One must be especially careful to obey constraint (18) when setting up a numerical simulation, where it is not possible to start the stars off at infinite separation.
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7
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85038932969
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L. L. Smarr and J. R. Wilson as reported by J. Wilson in Sources of Gravitational Radiation, edited by L. L. Smarr (Cambridge University Press, Cambridge, England, 1979), p. 423.
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L. L. Smarr and J. R. Wilson as reported by J. Wilson in Sources of Gravitational Radiation, edited by L. L. Smarr (Cambridge University Press, Cambridge, England, 1979), p. 423.
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8
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85038936757
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The gravitational waveform for the relativistic simulation reported in Refs.
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The gravitational waveform for the relativistic simulation reported in Refs. 5 matches well with the Newtonian result reported in Ref. 2; see Fig. 8 of Ref. 2. The waveform probes the bulk motion of the coalescing matter and therefore attests to the similarity of the behavior.
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