96a3319·Author: Samuel Cupp·Closed by: Samuel Cupp·2022-10-11
Description
Adds capability for simulations of the gravitational self-force in the Regge-Wheeler-Zerilli gauge, as well as observers for the metric perturbation, strain, and fluxes. Currently only circular orbits are fully implemented.
Adds capability for simulations of the gravitational self-force in the Regge-Wheeler-Zerilli gauge, as well as observers for the metric perturbation, strain, and fluxes. Currently only circular orbits are fully implemented.