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    | LALSIM-NS-MASS-RADIUS(1) | User Commands | LALSIM-NS-MASS-RADIUS(1) | 
NAME¶
lalsim-ns-mass-radius - manual page for lalsim-ns-mass-radius 6.0.0
DESCRIPTION¶
usage: /home/abuild/rpmbuild/BUILD/lalsimulation-6.0.0-build/python3.13/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"]
 
format string conversions:¶
- %c
 - is replaced by the dimensionless compactness M/R
 - %l
 - is replaced by the dimensionless tidal parameter
 - %k
 - is replaced by the tidal love number k2
 - %m
 - is replaced by the mass in solar masses
 - %r
 - is replaced by the radius in kilometers
 
recognized tabulated equations of state:¶
- ALF1, ALF2, ALF3, ALF4, AP1, AP2, AP3, AP4, APR4_EPP BBB2, BGN1H1, BPAL12, BSK19, BSK20, BSK21, ENG, FPS GNH3, GS1, GS2, H1, H2, H3, H4, H5, H6, H7, MPA1, MS1B MS1B_PP, MS1_PP, MS1, MS2, PAL6, PCL2, PS, QMC700 SLY4, SLY, SQM1, SQM2, SQM3, WFF1, WFF2, WFF3, APR BHF_BBB2, KDE0V, KDE0V1, RS, SK255, SK272, SKA, SKB SKI2, SKI3, SKI4, SKI5, SKI6, SKMP, SKOP, SLY2, SLY230A SLY9, HQC18, GMSR_BSK14_BSK24, GMSR_DHSL59_BSK24, GMSR_DHSL69_BSK24 GMSR_F0_BSK24, GMSR_H1_BSK24, GMSR_H2_BSK24, GMSR_H3_BSK24 GMSR_H4_BSK24, GMSR_H5_BSK24, GMSR_LN55_BSK24, GMSR_SLY5_BSK24 GPPVA_DD2_BSK24, GPPVA_DDME2_BSK24, GPPVA_FSU2_BSK24 GPPVA_FSU2H_BSK24, GPPVA_NL3WRL55_BSK24, KDE0V_BSK24 KDE0V1_BSK24, PCP_BSK24_BSK24, RG_SLY4_BSK24, RS_BSK24 SK255_BSK24, SKA_BSK24, SKB_BSK24, SKI2_BSK24, SKI3_BSK24 SKI4_BSK24, SKI6_BSK24, SKOP_BSK24, SLY2_BSK24, SLY9_BSK24 SLY230A_BSK24, XMLSLZ_DDLZ1_BSK24, XMLSLZ_DDME2_BSK24 XMLSLZ_DDMEX_BSK24, XMLSLZ_GM1_BSK24, XMLSLZ_MTVTC_BSK24 XMLSLZ_NL3_BSK24, XMLSLZ_PKDD_BSK24, XMLSLZ_TM1_BSK24 XMLSLZ_TW99_BSK24, ABHT_QMC_RMF1_META, ABHT_QMC_RMF2_META ABHT_QMC_RMF3_META, ABHT_QMC_RMF4_META, BL_CHIRAL_META
 
| December 2024 | LALSimulation |