pyseobnr.eob.dynamics.initial_conditions_aligned_precessing

Computes the quasi-precessing initial conditions in polar coordinates.

These have the same equations as the aligned-spin, however: - the Hamiltonian is different because it depends on several spin degrees of freedom - appropriate spin projections (and spins themselves) are passed to the Hamiltonian and the RR forces

Functions

IC_cons_augm(u, omega, H, chi1_v, chi2_v, ...)	The equations defining the 'conservative' part of the QC initial conditions, namely for r and pphi.
IC_diss_augm(u, r, pphi, H, RR, chi1_v, ...)	Initial conditions for the "dissipative" part, namely pr
computeIC_augm(omega, H, RR, chi1_v, chi2_v, ...)	Compute the initial conditions for an aligned-spin BBH binary