Data of transport and thermodynamics of nuclear matter with muons

Data reported in arXiv:2603.23904v1. Transport and thermodynamics information using a metamodel to describe neutron star matter (nuclear matter with electrons and muons), transport is studied as a function of temperature and density, thermodynamics as a function of density and density thresholds of direct Urca processes with electrons and muons as a function of the symmetry slope and incompressibility of assymetric matter. Names of the files specified the parameters used. Consider the following examples: A file like transport_varying_temperature_nuclear_matter_J32MeV_L70MeV_K240MeV_nB3n0_omg1kHz_200326.txt contains 13 columns with the temperature and the transport coefficients mentioned in our first draft and the transitions rates lambda1 and lambda2 for every value of the temperature. In this file we set the symmetry energy J=32 MeV, the slope L=70 MeV, the incompressibility (symmetric part of the energy density) K=240 MeV, the baryon number density nB=3n0 with n0 the saturation density, the angular frequency omega/2\pi=1 kHz. A file like transport_varying_density_nuclear_matter_J32MeV_L50MeV_K240MeV_T5MeV_200326.txt contains 12 columns with the baryon number density (normalized by the saturation density) and the transport coefficients mentioned in our first draft and the transitions rates lambda1 and lambda2 for every value of the baryon number density (normalized by the saturation density). In this file we set the symmetry energy J=32 MeV, the slope L=50 MeV, the incompressibility (symmetric part of the energy density) K=240 MeV and temperature T=5 MeV (in these files we set omega/2\pi=1 kHz). A file like thermodynamics_varying_density_nuclear_matter_J32MeV_L50MeV_K240MeV_200326.txt contains 11 columns with the baryon number density (normalized by the saturation density) and particle fractions, inverse susceptibilities and the incompressibility of nuclear matter (eq. 49 v1) for every value of the baryon number density (normalized by the saturation density). In this file we set the symmetry energy J=32 MeV, the slope L=50 MeV and the incompressibility (symmetric part of the energy density) K=240 MeV.A file like thresholddUrcae_varying_slope_nuclear_matter_J32MeV_K240MeV_Ksym0MeV_230326.txt contains two columns with the slope L and its corresponding density threshold of direct Urca processes. The name of the file indicates if the processes consider electrons or muons: dUrcae (for electrons) and dUrcamu (for muons) and we set the symmetry energy J=32 MeV, the incompressibility (symmetric part of the energy density) K=240 MeV and Ksym=0 MeV.A file like thrdUe_with_curvature_nuclear_matter_J32_K240_L110_180326.txt contains two columns with the Ksym and its corresponding density threshold of direct Urca processes. The name of the file indicates if the processes consider electrons or muons: dUe (for electrons) and dUmu (for muons) and we set the symmetry energy J=32 MeV, the incompressibility (symmetric part of the energy density) K=240 MeV and L=110 MeV.