The properties of spin polarized neutron matter are studied both at zero and finite temperature using the D1 and the D1P parameterizations of the Gogny interaction. The results show two different behaviors: whereas the D1P force exhibits a ferromagnetic transition at a density of $\rho_c \sim 1.31$ fm$^{-3}$ whose onset increases with temperature, no sign of such a transition is found for D1 at any density and temperature, in agreement with recent microscopic calculations
We study some properties of spin-polarized neutron matter in the presence of a strong magnetic field...
The Thomas-Fermi (TF) model is used to calculate the equation of state of thermal polarized neutron ...
The Brueckner-Hartree-Fock formalism is applied to study spin polarized neutron matter properties. R...
The properties of spin polarized neutron matter are studied both at zero and finite temperature usin...
The properties of spin polarized neutron matter are studied both at zero and finite temperature usin...
The properties of spin polarized neutron matter are studied both at zero and finite temperature usin...
The properties of spin-polarized neutron matter are studied at both zero and finite temperature usin...
AbstractThe properties of spin polarized neutron matter are studied both at zero and finite temperat...
The properties of spin polarized neutron matter are studied both at zero and finite temperature with...
The possibility of ferromagnetic and antiferromagnetic phase transitions in symmetric nuclear matter...
The properties of spin polarized neutron matter are studied both at zero and finite temperature usin...
We study some properties of spin-polarized neutron matter in the presence of a strong magnetic field...
The properties of spin-polarized neutron matter are studied at both zero and finite temperature usin...
Magnetars are neutron stars possessing a magnetic field of about 1014-1015 G at the surface. Ther-mo...
We study some properties of spin-polarized neutron matter in the presence of a strong magnetic field...
We study some properties of spin-polarized neutron matter in the presence of a strong magnetic field...
The Thomas-Fermi (TF) model is used to calculate the equation of state of thermal polarized neutron ...
The Brueckner-Hartree-Fock formalism is applied to study spin polarized neutron matter properties. R...
The properties of spin polarized neutron matter are studied both at zero and finite temperature usin...
The properties of spin polarized neutron matter are studied both at zero and finite temperature usin...
The properties of spin polarized neutron matter are studied both at zero and finite temperature usin...
The properties of spin-polarized neutron matter are studied at both zero and finite temperature usin...
AbstractThe properties of spin polarized neutron matter are studied both at zero and finite temperat...
The properties of spin polarized neutron matter are studied both at zero and finite temperature with...
The possibility of ferromagnetic and antiferromagnetic phase transitions in symmetric nuclear matter...
The properties of spin polarized neutron matter are studied both at zero and finite temperature usin...
We study some properties of spin-polarized neutron matter in the presence of a strong magnetic field...
The properties of spin-polarized neutron matter are studied at both zero and finite temperature usin...
Magnetars are neutron stars possessing a magnetic field of about 1014-1015 G at the surface. Ther-mo...
We study some properties of spin-polarized neutron matter in the presence of a strong magnetic field...
We study some properties of spin-polarized neutron matter in the presence of a strong magnetic field...
The Thomas-Fermi (TF) model is used to calculate the equation of state of thermal polarized neutron ...
The Brueckner-Hartree-Fock formalism is applied to study spin polarized neutron matter properties. R...