An implementation of the deflection angle in the equitorial plane as a function of the black hole mass, spin, and asymptotic impact parameters, as detailed in Iyer and Hansen (2009).
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Updated
Jul 19, 2023 - Julia
An implementation of the deflection angle in the equitorial plane as a function of the black hole mass, spin, and asymptotic impact parameters, as detailed in Iyer and Hansen (2009).
Fast analytic Kerr raytracing
An implementation of realistic, finite-temperature nuclear-matter models in neutron-star seismology.
Maurer-Cartan-Lie frame connections ∇ Grassmann.jl TensorField derivations
Extensible spacetime agnostic general relativistic ray-tracing (GRRT).
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