pyseobnr.eob.dynamics.rhs_aligned_ecc

Contains the actual RHS of the EOM, wrapped in cython. This allows some of the cython functions used in the RHS to be called more efficiently.

Functions

compute_x(e, z, omega, RR)

Compute the PN formula for the dimensionless orbit-averaged orbital frequency 'x' from the eccentricity 'e', relativistic anomaly 'z', and angular velocity 'omega'.

get_rhs_ecc(t, z, H, RR, chi_1, chi_2, m_1, ...)

Compute the RHS of the EOB evolution equations including the evolution of the Keplerian elements for eccentric models as described in [Gamboa2024a] .

get_rhs_ecc_secular(t, Kep, RR)

Compute the RHS of the secular evolution equations for eccentricity, relativistic anomaly and dimensionless orbit-averaged orbital frequency x = (M omega_avg)^{2/3}.