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Radiation-balanced simulations for binary inspiral

By John Whelan and others
The late stage of the inspiral of two black holes may have important non-Newtonian effects that are unrelated to radiation reaction. To understand these effects we approximate a slowly inspiralling binary by a stationary solution to Einstein's equations in which the holes orbit eternally. Radiation reaction is nullified by specifying... Show more
October 1, 2001
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Radiation-balanced simulations for binary inspiral
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