! File: submodule_bns_lorene_io.f90 ! Authors: Francesco Torsello (FT) !************************************************************************ ! Copyright (C) 2020-2023 Francesco Torsello * ! * ! This file is part of SPHINCS_ID * ! * ! SPHINCS_ID is free software: you can redistribute it and/or modify * ! it under the terms of the GNU General Public License as published by * ! the Free Software Foundation, either version 3 of the License, or * ! (at your option) any later version. * ! * ! SPHINCS_ID is distributed in the hope that it will be useful, * ! but WITHOUT ANY WARRANTY; without even the implied warranty of * ! MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the * ! GNU General Public License for more details. * ! * ! You should have received a copy of the GNU General Public License * ! along with SPHINCS_ID. If not, see . * ! The copy of the GNU General Public License should be in the file * ! 'COPYING'. * !************************************************************************ SUBMODULE (bns_lorene) io !******************************************** ! !# This submodule contains the implementation of the ! methods of TYPE [[bnslorene]] that handle I/O (input/output) ! ! FT 05.11.2021 ! !******************************************** IMPLICIT NONE CONTAINS !-------------------! !-- SUBROUTINES --! !-------------------! MODULE PROCEDURE print_summary_bnslorene !************************************************ ! !# Prints a summary of the physical properties the |bns| system ! produced by | lorene to the standard output and, optionally, ! to a formatted file whose name is given as the optional ! argument `filename` ! ! FT 4.02.2022 ! !************************************************ IMPLICIT NONE PRINT *, " * Binary system of neutron stars produced by LORENE:" PRINT * PRINT *, " x coordinate of the center of mass of the system= ", & !"weighted with the baryonic mass= ", & (this% barycenter1_x*this% mass1 + this% barycenter2_x*this% mass2) & /(this% mass1 + this% mass2) !PRINT *, " Center of mass of the system, weighted with the ", & ! "gravitational mass= ", (this% barycenter1_x*this% mass_grav1 & ! + this% barycenter2_x*this% mass_grav2) & ! /(this% mass_grav1 + this% mass_grav2) PRINT * PRINT *, " ADM mass of the system= ", this% adm_mass, "MSun" PRINT * PRINT *, " ADM linear momentum of the system=(", & this% linear_momentum_x, ", " PRINT *, " ", & this% linear_momentum_y, ", " PRINT *, " ", & this% linear_momentum_z, ") Msun*c" PRINT * PRINT *, " Velocity of the center of mass of the system=" PRINT *, " ADM linear momentum / ADM mass =(", & this% linear_momentum_x/this% adm_mass, ", " PRINT *, " ", & this% linear_momentum_y/this% adm_mass, ", " PRINT *, " ", & this% linear_momentum_z/this% adm_mass, ") c" PRINT * PRINT *, " Bowen-York angular momentum of the system= (", & this% angular_momentum_x, ", " PRINT *, " ", & this% angular_momentum_y, ", " PRINT *, " ", & this% angular_momentum_z, ") G*Msun^2/c" PRINT * END PROCEDURE print_summary_bnslorene MODULE PROCEDURE print_bns_properties !**************************************************** ! !# Print the parameters of the binary neutron ! stars' initial data computed by |lorene| ! ! FT 8.10.2020 ! !**************************************************** USE constants, ONLY: c_light, cm2km, m2cm, kg2g USE utility, ONLY: k_lorene2cu, k_lorene2cu_pwp, Msun_geo, km2m, & density_si2cu, zero, one, two, four, five, ten, & use_eos_from_id, eos$poly, eos$pwpoly, eos$tabu$compose IMPLICIT NONE IF( this% angular_momentum_z == zero )THEN PRINT * PRINT *, " ** The parameters have not been read yet. ", & "Call the SUBROUTINE read_id_params to read them." PRINT * STOP ELSE PRINT * PRINT *, " ** The parameters of the binary system are:" PRINT * PRINT *, " Distance between the points of highest density = ",& this% distance, " M_sun^geo = ", this% distance*Msun_geo, " km" PRINT *, " Distance between the barycenters = ", & this% distance_com, " M_sun^geo", this% distance_com*Msun_geo, & " km" PRINT * PRINT *, " Baryonic mass of NS 1 = ", this% mass1, " M_sun" PRINT *, " Baryonic mass of NS 2 = ", this% mass2, " M_sun" PRINT *, " Gravitational mass of NS 1 in the binary system = ", & this% mass_grav1, " M_sun" PRINT *, " Gravitational mass of NS 2 in the binary system = ", & this% mass_grav2, " M_sun" PRINT *, " ADM mass = ", this% adm_mass, " M_sun" PRINT * PRINT *, " Stellar center of NS 1 = ", this% center1_x, " M_sun^geo" PRINT *, " Stellar center of NS 2 = ", this% center2_x, " M_sun^geo" PRINT *, " Barycenter of NS 1 = ", this% barycenter1_x, " M_sun^geo" PRINT *, " Barycenter of NS 2 = ", this% barycenter2_x, " M_sun^geo" PRINT *, " Orbital angular velocity Omega_0 = ", & this% angular_vel, " rad/s = ", & this% angular_vel/(c_light*cm2km), "km^{-1}" PRINT *, " mOmega = ", & "Omega_0[km^{-1}]*(mass_grav1[km] + mass_grav2[km]) = ",& this% mOmega, "[pure number]" PRINT *, " Bowen-York angular momentum of the system, x component = ", & this% angular_momentum_x, " G M_sun^2 /c" PRINT *, " Bowen-York angular momentum of the system, y component = ", & this% angular_momentum_y, " G M_sun^2 /c" PRINT *, " Bowen-York angular momentum of the system, z component = ", & this% angular_momentum_z, " G M_sun^2 /c" PRINT *, " Estimated time of the merger t_merger = ", this% t_merger, & " M_sun^geo = ", this% t_merger*MSun_geo/(c_light*cm2km) & *ten*ten*ten, " ms, from Peters_PR_136_B1224_1964, eq. (5.10)" PRINT * PRINT *, " Estimated separation to have the merger at t_merger = 2000", & " Msun_geo = ", two*ten*ten*ten*MSun_geo/(c_light*cm2km) & *ten*ten*ten, " ms :", & ( two*ten*ten*ten*( this% mass_grav1*this% mass_grav2* & ( this% mass_grav1 + this% mass_grav2 ) ) & /(five/(two**(two*four))) )**(one/four), "M_sun^geo = ", & ( two*ten*ten*ten*( this% mass_grav1*this% mass_grav2* & ( this% mass_grav1 + this% mass_grav2 ) ) & /(five/(two**(two*four))) ) & **(one/four)*Msun_geo, & "km, from Peters_PR_136_B1224_1964, eq. (5.10)" PRINT * PRINT *, " Radii of star 1: " PRINT *, " Areal (or circumferential) radius for the star in the", & " binary system [the one used in the", & " (gravitational)mass-(areal)radius diagrams",& " is for a TOV star], x direction:", & this% area_radius1, " M_sun^geo = ", & this% area_radius1*Msun_geo, " km" PRINT *, " x direction, towards companion = ", & this% radius1_x_comp, " M_sun^geo" PRINT *, " x direction, opposite to companion = ", & this% radius1_x_opp, " M_sun^geo" PRINT *, " y direction = ", this% radius1_y, " M_sun^geo" PRINT *, " z direction = ", this% radius1_z, " M_sun^geo" PRINT *, " Radii of star 2 :" PRINT *, " Areal (or circumferential) radius for the star in the", & " binary system [the one used in the", & " (gravitational)mass-(areal)radius diagrams",& " is for a TOV star], x direction:", & this% area_radius2, " M_sun^geo", & this% area_radius2*Msun_geo, " km" PRINT *, " x direction, towards companion = ", & this% radius2_x_comp, " M_sun^geo" PRINT *, " x direction, opposite to companion = ", & this% radius2_x_opp, " M_sun^geo" PRINT *, " y direction = ", this% radius2_y, " M_sun^geo" PRINT *, " z direction = ", this% radius2_z, " M_sun^geo" PRINT * PRINT *, " Hydro quantities at the center of star 1: " PRINT *, " Central enthalpy = ", this% ent_center1, " c^2" PRINT *, " Central baryon number density = ", this% nbar_center1, & " (M_sun^geo)^{-3} =", & this% nbar_center1/(MSun_geo*km2m*m2cm)**3, "cm^{-3}" PRINT *, " Central baryon mass density = ", this% rho_center1, & " M_sun^geo (M_sun^geo)^{-3} =", & this% rho_center1/density_si2cu*kg2g/(m2cm**3), "g cm^{-3}" PRINT *, " Central energy density = ", this% energy_density_center1, & " M_sun^geo c^2 (M_sun^geo)^{-3}", & this% energy_density_center1/density_si2cu*kg2g/(m2cm**3), & "g c^2 cm^{-3}" PRINT *, " Central specific energy = ", this% specific_energy_center1, & " c^2" PRINT *, " Central pressure = ", this% pressure_center1, & " M_sun^geo c^2 (M_sun^geo)^{-3}", & this% pressure_center1/density_si2cu*kg2g/(m2cm**3), & "g c^2 cm^{-3}" PRINT *, " Hydro quantities at the center of star 2: " PRINT *, " Central enthalpy = ", this% ent_center2, " c^2" PRINT *, " Central baryon number density = ", this% nbar_center2, & " (M_sun^geo)^{-3} =", & this% nbar_center2/(MSun_geo*km2m*m2cm)**3, "cm^{-3}" PRINT *, " Central baryon mass density = ", this% rho_center2, & " M_sun^geo (M_sun^geo)^{-3} =", & this% rho_center2/density_si2cu*kg2g/(m2cm**3), "g cm^{-3}" PRINT *, " Central energy density = ", this% energy_density_center2, & " M_sun^geo c^2 (M_sun^geo)^{-3}", & this% energy_density_center2/density_si2cu*kg2g/(m2cm**3), & "g c^2 cm^{-3}" PRINT *, " Central specific energy = ", this% specific_energy_center2, & " c^2" PRINT *, " Central pressure = ", this% pressure_center2, & " M_sun^geo c^2 (M_sun^geo)^{-3}", & this% pressure_center2/density_si2cu*kg2g/(m2cm**3), & "g c^2 cm^{-3}" PRINT * !IF( show_progress ) & PRINT *, " Equations of state for star 1 (EOS1) = ", this% eos1 !IF( show_progress ) & PRINT *, " Equations of state for star 2 (EOS2) = ", this% eos2 !IF( show_progress ) PRINT * IF( this% eos1_id == eos$poly )THEN ! If the EOS is polytropic PRINT *, " Parameters for EOS1: " PRINT *, " Polytopic index gamma_1 = ", this% gamma_1 PRINT *, " Pressure coefficient = ",& this% kappa_1/k_lorene2cu( this% gamma_1 ), & "rho_nuc c^2 / n_nuc^gamma_1 = ", this% kappa_1, & "[pure number]" PRINT *, " Parameters for EOS2: " PRINT *, " Polytopic index gamma_2 = ", this% gamma_2 PRINT *, " Pressure coefficient = ",& this% kappa_2/k_lorene2cu( this% gamma_2 ), & "rho_nuc c^2 / n_nuc^gamma_2 = ", this% kappa_2, & "[pure number]" PRINT * ELSEIF( this% eos1_id == eos$pwpoly )THEN ! If the EOS is piecewise polytropic PRINT *, " Parameters for EOS1: " PRINT *, " Number of polytropic indexes = ", this% npeos_1 PRINT *, " Polytopic index gamma0_1 = ", this% gamma0_1 PRINT *, " Polytopic index gamma1_1 = ", this% gamma1_1 PRINT *, " Polytopic index gamma2_1 = ", this% gamma2_1 PRINT *, " Polytopic index gamma3_1 = ", this% gamma3_1 PRINT *, " Pressure coefficient for the crust (here from SLy) = ",& this% kappa0_1/k_lorene2cu_pwp( this% gamma0_1 ), & "rho_nuc c^2 / n_nuc^gamma0_1 = ", this% kappa0_1, & "[pure number]" PRINT *, " Pressure coefficient for the first polytrope = ",& this% kappa1_1/k_lorene2cu_pwp( this% gamma1_1 ), & "rho_nuc c^2 / n_nuc^gamma1_1", this% kappa1_1, & "[pure number]" PRINT *, " Pressure coefficient for the second polytrope = ",& this% kappa2_1/k_lorene2cu_pwp( this% gamma2_1 ), & "rho_nuc c^2 / n_nuc^gamma2_1", this% kappa2_1, & "[pure number]" PRINT *, " Pressure coefficient for the third polytrope = ",& this% kappa3_1/k_lorene2cu_pwp( this% gamma3_1 ), & "rho_nuc c^2 / n_nuc^gamma3_1", this% kappa3_1, & "[pure number]" PRINT *, " Base 10 exponent of the pressure at the first fiducial " & // "density (between gamma_0 and gamma_1) (dyne/cm^2)= ", & this% logP1_1 PRINT *, " Base 10 exponent of first fiducial density (g/cm^3) = ", & this% logRho0_1 PRINT *, " Base 10 exponent of second fiducial density (g/cm^3) = ",& this% logRho1_1 PRINT *, " Base 10 exponent of third fiducial density (g/cm^3) = ", & this% logRho2_1 PRINT * PRINT *, " Parameters for EOS2: " PRINT *, " Number of polytropic indexes = ", this% npeos_2 PRINT *, " Polytopic index gamma0_2 = ", this% gamma0_2 PRINT *, " Polytopic index gamma1_2 = ", this% gamma1_2 PRINT *, " Polytopic index gamma2_2 = ", this% gamma2_2 PRINT *, " Polytopic index gamma3_2 = ", this% gamma3_2 PRINT *, " Pressure coefficient for the crust (here from SLy) = ",& this% kappa0_2/k_lorene2cu_pwp( this% gamma0_2 ), & "rho_nuc c^2 / n_nuc^gamma0_2 = ", this% kappa0_2, & "[pure number]" PRINT *, " Pressure coefficient for the first polytrope = ",& this% kappa1_2/k_lorene2cu_pwp( this% gamma1_2 ), & "rho_nuc c^2 / n_nuc^gamma1_2", this% kappa1_2, & "[pure number]" PRINT *, " Pressure coefficient for the second polytrope = ",& this% kappa2_2/k_lorene2cu_pwp( this% gamma2_2 ), & "rho_nuc c^2 / n_nuc^gamma2_2", this% kappa2_2, & "[pure number]" PRINT *, " Pressure coefficient for the third polytrope = ",& this% kappa3_2/k_lorene2cu_pwp( this% gamma3_2 ), & "rho_nuc c^2 / n_nuc^gamma3_2", this% kappa3_2, & "[pure number]" PRINT *, " Base 10 exponent of the pressure at the first fiducial " & // "density (between gamma_0 and gamma_1) (dyne/cm^2)= ", & this% logP1_2 PRINT *, " Base 10 exponent of first fiducial density (g/cm^3) = ", & this% logRho0_2 PRINT *, " Base 10 exponent of second fiducial density (g/cm^3) = ",& this% logRho1_2 PRINT *, " Base 10 exponent of third fiducial density (g/cm^3) = ", & this% logRho2_2 PRINT * ELSEIF( this% eos1_id == eos$tabu$compose )THEN ! If the EOS is tabulated PRINT * PRINT *, " ** Using tabulated CompOSE EOS" PRINT * IF(.NOT.use_eos_from_id)THEN PRINT *, " Equations of state for star 1 (EOS1) = ", & TRIM(this% eos_filenames(1)) PRINT *, " Table located at: ", TRIM(this% eos_table1) PRINT * PRINT *, " Equations of state for star 2 (EOS2) = ", & TRIM(this% eos_filenames(2)) PRINT *, " Table located at: ", TRIM(this% eos_table2) PRINT * ENDIF ELSE PRINT *, "** ERROR in SUBROUTINE read_bns_properties in SUBMODULE ", & "bns_lorene@properties!", & " The equation of state is unknown!" STOP ENDIF ENDIF END PROCEDURE print_bns_properties END SUBMODULE io