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nrutils.py File Reference

Prototypes

def lalinference.imrtgr.nrutils.bbh_final_mass_non_spinning_Panetal (m1, m2)
 Calculate the mass of the final BH resulting from the merger of two non-spinning black holes using eqn. More...
 
def lalinference.imrtgr.nrutils.bbh_final_spin_non_spinning_Panetal (m1, m2)
 Calculate the spin of the final BH resulting from the merger of two non-spinning black holes using eqn. More...
 
def lalinference.imrtgr.nrutils.calc_isco_radius (a)
 Calculate the ISCO radius of a Kerr BH as a function of the Kerr parameter using eqns. More...
 
def lalinference.imrtgr.nrutils.bbh_final_spin_non_precessing_Healyetal (m1, m2, chi1, chi2, version="2014")
 Calculate the spin of the final BH resulting from the merger of two black holes with non-precessing spins using fit from Healy et al Phys Rev D 90, 104004 (2014) (version == "2014") or the small update from Healy and Lousto arXiv:1610.09713 (version == "2016") More...
 
def lalinference.imrtgr.nrutils.bbh_final_mass_non_precessing_Healyetal (m1, m2, chi1, chi2, version="2014", chif=None)
 Calculate the mass of the final BH resulting from the merger of two black holes with non-precessing spins using fit from Healy et al Phys Rev D 90, 104004 (2014) (version == "2014") or the small update from Healy and Lousto arXiv:1610.09713 (version == "2016") More...
 
def lalinference.imrtgr.nrutils.bbh_final_spin_projected_spin_Healyetal (m1, m2, chi1, chi2, tilt1, tilt2)
 wrapper to bbh_final_spin_projected_spins() for backwards compatibility More...
 
def lalinference.imrtgr.nrutils.bbh_final_mass_projected_spin_Healyetal (m1, m2, chi1, chi2, tilt1, tilt2, chif=None)
 wrapper to bbh_final_mass_projected_spins() for backwards compatibility More...
 
def lalinference.imrtgr.nrutils.bbh_final_spin_precessing_Healyetal_extension_Minit (m1, m2, chi1, chi2, tilt1, tilt2, phi12)
 wrapper to bbh_final_spin_precessing() for backwards compatibility More...
 
def lalinference.imrtgr.nrutils.bbh_final_mass_projected_spins (m1, m2, chi1, chi2, tilt1, tilt2, fitname, chif=None)
 Calculate the mass of the final BH resulting from the merger of two black holes, only using the projected spins along the total angular momentum and some aligned-spin fit from the literature. More...
 
def lalinference.imrtgr.nrutils.bbh_final_spin_projected_spins (m1, m2, chi1, chi2, tilt1, tilt2, fitname, truncate=bbh_Kerr_trunc_opts.trunc)
 Calculate the (signed) dimensionless spin parameter of the final BH resulting from the merger of two black holes, only using the projected spins along the total angular momentum and some aligned-spin fit from the literature. More...
 
def lalinference.imrtgr.nrutils.bbh_final_spin_precessing (m1, m2, chi1, chi2, tilt1, tilt2, phi12, fitname, truncate=bbh_Kerr_trunc_opts.trunc)
 Calculate the magnitude of the dimensionless spin parameter of the final BH resulting from the merger of two black holes, including the in-plane spin components; by either using a precessing fit from the literature; or by first projecting the spins along the angular momentum and using an aligned-spin fit from the literature, then adding in quadrature the in-plane dimensionful spin scaled by the initial mass squared. More...
 
def lalinference.imrtgr.nrutils.bbh_final_mass_non_precessing_Husaetal (m1, m2, chi1, chi2)
 Calculate the mass of the final BH resulting from the merger of two black holes with non-precessing spins using the fits used by IMRPhenomD, given in Eqs. More...
 
def lalinference.imrtgr.nrutils.bbh_final_spin_non_precessing_Husaetal (m1, m2, chi1, chi2)
 Calculate the spin of the final BH resulting from the merger of two black holes with non-precessing spins using the fits used by IMRPhenomD, given in Eqs. More...
 
def lalinference.imrtgr.nrutils.bbh_UIBfits_setup (m1, m2, chi1, chi2)
 common setup function for UIB final-state and luminosity fit functions More...
 
def lalinference.imrtgr.nrutils.bbh_final_mass_non_precessing_UIB2016 (m1, m2, chi1, chi2, version="v2")
 Calculate the final mass with the aligned-spin NR fit by Xisco Jimenez Forteza, David Keitel, Sascha Husa et al. More...
 
def lalinference.imrtgr.nrutils.bbh_final_spin_non_precessing_UIB2016 (m1, m2, chi1, chi2, version="v2")
 Calculate the final spin with the aligned-spin NR fit by Xisco Jimenez Forteza, David Keitel, Sascha Husa et al. More...
 
def lalinference.imrtgr.nrutils.bbh_final_spin_non_precessing_HBR2016 (m1, m2, chi1z, chi2z, version="M3J3")
 Calculate the (signed) dimensionless spin of the final BH resulting from the merger of two black holes with aligned spins using the fit from Hofmann, Barausse, and Rezzolla ApJL 825, L19 (2016), henceforth HBR. More...
 
def lalinference.imrtgr.nrutils.bbh_final_spin_precessing_HBR2016 (m1, m2, chi1, chi2, tilt1, tilt2, phi12, version="M3J3")
 Calculate the dimensionless spin of the final BH resulting from the merger of two black holes with precessing spins using the fit from Hofmann, Barausse, and Rezzolla ApJL 825, L19 (2016), henceforth HBR. More...
 
def lalinference.imrtgr.nrutils.bbh_aligned_Lpeak_6mode_SHXJDK (q, chi1, chi2)
 wrapper to bbh_peak_luminosity_non_precessing_T1600018() for backwards compatibility More...
 
def lalinference.imrtgr.nrutils.bbh_peak_luminosity_non_precessing_T1600018 (m1, m2, chi1, chi2)
 Calculate the peak luminosity (using modes 22, 21, 33, 32, 44, and 43) of a binary black hole with aligned spins using the fit made by Sascha Husa, Xisco Jimenez Forteza, David Keitel [LIGO-T1500598] using 5th order in chieff and return results in units of 10^56 ergs/s. More...
 
def lalinference.imrtgr.nrutils.bbh_peak_luminosity_non_precessing_UIB2016 (m1, m2, chi1, chi2)
 Calculate the peak luminosity with the aligned-spin NR fit by David Keitel, Xisco Jimenez Forteza, Sascha Husa, Lionel London et al. More...
 
def lalinference.imrtgr.nrutils.bbh_peak_luminosity_non_precessing_Healyetal (m1, m2, chi1z, chi2z)
 Calculate the peak luminosity of an aligned-spin binary black hole coalescence using the fit from Healy and Lousto arXiv:1610.09713 (henceforth HL) More...
 
def lalinference.imrtgr.nrutils.bbh_peak_luminosity_projected_spins (m1, m2, chi1, chi2, tilt1, tilt2, fitname)
 Calculate the peak luminosity of the merger of two black holes, only using the projected spins along the total angular momentum and some aligned-spin fit from the literature. More...
 
def lalinference.imrtgr.nrutils.bbh_average_fits_precessing (m1, m2, chi1, chi2, tilt1, tilt2, phi12, quantity, fits)
 Convenience functions. More...
 

Go to the source code of this file.

Data Structures

class  lalinference.imrtgr.nrutils.bbh_final_state_fits
 Final mass and spin fits. More...
 
class  lalinference.imrtgr.nrutils.bbh_Kerr_trunc_opts
 
class  lalinference.imrtgr.nrutils.bbh_Lpeak_fits
 Peak luminosity fits. More...
 

Namespaces

namespace  lalinference
 
namespace  lalinference.imrtgr
 
namespace  lalinference.imrtgr.nrutils