NAME¶

lalsim-ns-mass-radius - manual page for lalsim-ns-mass-radius 5.3.1

DESCRIPTION¶

usage: /home/abuild/rpmbuild/BUILD/python3.11/bin/.libs/lalsim-ns-mass-radius [options]

-h, --help

print this message and exit

-f FILE, --eos-file=FILE

use EOS with from data filename FILE

-n NAME, --eos-name=NAME

use EOS with name NAME

-U, --calculate-virial-theorem

calculate and print Virial theorem besides M, R

-E, --choose-relative-error

choose a value for the TOV solver routine relative error (default epsrel=1e-6)

You may choose a central value for the rest-mass density (in kg/m^3) or the energy density (in J/m^3) as follows -d, --central-rest-mass-density central rest-mass density -e, --central-energy-density central energy density If none are chosen the the program will use a standard fixed value

-P, --polytrope

use single polytrope

-G GAMMA, --gamma=GAMMA

adiabatic index

-p PRESSURE, --pressure=PRESSURE

pressure at reference density

-r DENSITY, --density=DENSITY

reference density

-Q, --piecewisepolytrope

use 4-parameter piecewise polytrope (PRD 79, 124032 (2009))

-q log(p_1), --logp1=log(p_1)

log of pressure at rho_1=10^17.7 kg/m^3

-1 Gamma_1, --gamma1=Gamma_1

adiabatic index <10^17.7 kg/m^3

-2 Gamma_2, --gamma2=Gamma_2

adiabatic index 10^17.7--10^18 kg/m^3

-3 Gamma_3, --gamma3=Gamma_3

adiabatic index >10^18.0 kg/m^3

-S --4paramspectraldecomp

use 4-parameter spectral decomposition (PRD 82, 103011 (2010))

-w SDgamma0, --SDgamma0=SDgamma0

adiabatic index spectral decomposition coefficient 1 0.2--2.0

-x SDgamma1, --SDgamma1=SDgamma1

adiabatic index spectral decomposition coefficient 2 -1.6--1.7

-y SDgamma2, --SDgamma2=SDgamma2

adiabatic index spectral decomposition coefficient 3 -0.8--0.6

-z SDgamma3, --SDgamma3=SDgamma3

adiabatic index spectral decomposition coefficient 4 -0.2--0.2

-N NPTS, --npts=NPTS

output NPTS points [100]

-F FORMAT, --format=FORMAT

output format FORMAT ["%r\t%m\n"]