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
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Compute the PN formula for the dimensionless orbit-averaged orbital frequency 'x' from the eccentricity 'e', relativistic anomaly 'z', and angular velocity 'omega'. |
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Compute the RHS of the EOB evolution equations including the evolution of the Keplerian elements for eccentric models as described in [Gamboa2024a] . |
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Compute the RHS of the secular evolution equations for eccentricity, relativistic anomaly and dimensionless orbit-averaged orbital frequency x = (M omega_avg)^{2/3}. |