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This repository has been archived by the owner on Jun 3, 2022. It is now read-only.
At the moment, the disc velocities for a disc in the equatorial plane are assumed to have circular photon orbits in the Kerr metric. This should be made generic for any arbitrary metric, so that redshifts for thin accretion discs may be calculated beyond Kerr.
The text was updated successfully, but these errors were encountered:
At the moment, the disc velocities for a disc in the equatorial plane are assumed to have circular photon orbits in the Kerr metric. This should be made generic for any arbitrary metric, so that redshifts for thin accretion discs may be calculated beyond Kerr.
The text was updated successfully, but these errors were encountered: