pint.derived_quantities

Functions to compute various derived quantities from pulsar spin parameters, masses, etc.

Functions

a1sini(mp, mc, pb[, i])	Pulsar's semi-major axis.
companion_mass(pb, x[, i, mp])	Commpute the companion mass from the orbital parameters
dispersion_slope(dm)	Compute the dispersion slope.
dr(mp, mc, pb)	Post-Keplerian Roemer delay term
dth(mp, mc, pb)	Post-Keplerian Roemer delay term
f_to_p(p, pd[, pdd])	Converts P, Pdot to F, Fdot (or vice versa)
gamma(mp, mc, pb, e)	Post-Keplerian time dilation and gravitational redshift gamma, assuming general relativity.
mass_funct(pb, x)	Compute binary mass function from period and semi-major axis
mass_funct2(mp, mc, i)	Compute binary mass function from masses and inclination
omdot(mp, mc, pb, e)	Post-Keplerian longitude of periastron precession rate omdot, assuming general relativity.
omdot_to_mtot(omdot, pb, e)	Determine total mass from Post-Keplerian longitude of periastron precession rate omdot, assuming general relativity.
p_to_f(p, pd[, pdd])	Converts P, Pdot to F, Fdot (or vice versa)
pbdot(mp, mc, pb, e)	Post-Keplerian orbital decay pbdot, assuming general relativity.
pferrs(porf, porferr[, pdorfd, pdorfderr])	Convert P, Pdot to F, Fdot with uncertainties (or vice versa).
pulsar_B(f, fdot[, I, R])	Compute pulsar surface magnetic field
pulsar_B_lightcyl(f, fdot[, I, R])	Compute pulsar magnetic field at the light cylinder
pulsar_age(f, fdot[, n, fo])	Compute pulsar characteristic age
pulsar_edot(f, fdot[, I])	Compute pulsar spindown energy loss rate
pulsar_mass(pb, x, mc, i)	Compute pulsar mass from orbital parameters
shklovskii_factor(pmtot, D)	Compute magnitude of Shklovskii correction factor.
sini(mp, mc, pb, x)	Post-Keplerian sine of inclination, assuming general relativity.