A method of determining apparent horizons in three-dimensional numerical relativity

Details A method of determining apparent horizons in three-dimensional numerical relativity A method of determining apparent horizons in three-dimensional numerical relativity

Dec 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984phla..106..235n&link_type=abstract

Physics Letters A, Volume 106, Issue 5-6, p. 235-238.

Physics

37

Scientific paper

Using the (3 + 1)-formalism of the Einstein equations, we give a method
of determining apparent horizons in general space-times. We have
determined them numerically for four examples. The method will enable us
to know whether or not a black hole is formed for numerically generated
space-times in three-dimensional numerical relativity.

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