AbstractThe properties of spin polarized neutron matter are studied both at zero and finite temperature within the framework of the Brueckner–Hartree–Fock formalism, using the Argonne v18 nucleon–nucleon interaction. The free energy, energy and entropy per particle are calculated for several values of the spin polarization, densities and temperatures together with the magnetic susceptibility of the system. The results show no indication of a ferromagnetic transition at any density and temperature
The equation of state of neutron matter is affected by the presence of a magnetic field due to the i...
Background: The possible existence of a phase transition to a ferromagnetic state in neutron matter ...
Background: The possible existence of a phase transition to a ferromagnetic state in neutron matter ...
The properties of spin polarized neutron matter are studied both at zero and finite temperature with...
The Brueckner-Hartree-Fock formalism is applied to study spin polarized neutron matter properties. R...
In this work, the Static Fluctuation Approximation (SFA) is used to investigate the thermodynamics p...
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...
Magnetars are neutron stars possessing a magnetic field of about 1014-1015 G at the surface. Ther-mo...
The properties of spin-polarized neutron matter are studied at both zero and finite temperature usin...
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 Brueckner--Hartree--Fock formalism is applied to study spin polarized neutron matter properties....
The equation of state of neutron matter is affected by the presence of a magnetic field due to the i...
Background: The possible existence of a phase transition to a ferromagnetic state in neutron matter ...
Background: The possible existence of a phase transition to a ferromagnetic state in neutron matter ...
The properties of spin polarized neutron matter are studied both at zero and finite temperature with...
The Brueckner-Hartree-Fock formalism is applied to study spin polarized neutron matter properties. R...
In this work, the Static Fluctuation Approximation (SFA) is used to investigate the thermodynamics p...
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...
Magnetars are neutron stars possessing a magnetic field of about 1014-1015 G at the surface. Ther-mo...
The properties of spin-polarized neutron matter are studied at both zero and finite temperature usin...
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 Brueckner--Hartree--Fock formalism is applied to study spin polarized neutron matter properties....
The equation of state of neutron matter is affected by the presence of a magnetic field due to the i...
Background: The possible existence of a phase transition to a ferromagnetic state in neutron matter ...
Background: The possible existence of a phase transition to a ferromagnetic state in neutron matter ...