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Numerical solver for the modified Teukolsky equation for non-Kerr geometries
The numerical solver is used to solve the modified Teukolsky equation for studying gravitational wave propagation in non-Kerr geometries. Non-Kerr geometries include black holes, wormholes, etc., which are of great significance in the universe. The modified Teukolsky equation can more accurately describe gravitational waves in these geometries. To verify the accuracy, stability, and efficiency of the numerical solver, a series of tests are conducted.
Edited at 2025-01-13 08:31:36
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Numerical solver for the modified Teukolsky equation for non-Kerr geometries
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