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Peres metric : ウィキペディア英語版 | Peres metric In mathematical physics, the Peres metric is defined by the proper time : for any arbitrary function ''f''. If ''f'' is a harmonic function with respect to ''x'' and ''y'', then the corresponding Peres metric satisfies the Einstein field equations in vacuum. Such a metric is often studied in the context of gravitational waves. The metric is named for Israeli physicist Asher Peres, who first defined the metric in 1959. ==See also==
*Introduction to the mathematics of general relativity *Stress–energy tensor *Metric tensor (general relativity)
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