Results 251 to 260 of about 202,682 (289)
Some of the next articles are maybe not open access.
Nuclear Physics A, 1971
Abstract The matter in neutron stars is essentially in its ground state and ranges in density up to and beyond 3 × 10 14 g/cm 3 , the density of nuclear matter. Here we determine the constitution of the ground state of matter and its equation of state in the regime from 4.3 × 10 11 g/cm 3 where free neutrons begin to “drip” out of the nuclei, up ...
GORDON BAYM +2 more
openaire +3 more sources
Abstract The matter in neutron stars is essentially in its ground state and ranges in density up to and beyond 3 × 10 14 g/cm 3 , the density of nuclear matter. Here we determine the constitution of the ground state of matter and its equation of state in the regime from 4.3 × 10 11 g/cm 3 where free neutrons begin to “drip” out of the nuclei, up ...
GORDON BAYM +2 more
openaire +3 more sources
Physical Review D, 1975
The ground state of solid neutron matter is investigated using the $t$-matrix formalism developed for the quantum crystal problem. Studies of neutrons interacting through the repulsive part of the Reid $^{1}S_{0}$ interaction, the Reid $^{1}S_{0}$ interaction, and the full Reid potentials are made in the Hartree, Hartree $t$-matrix, Hartree-Fock, and ...
M. T. Takemori, R. A. Guyer
openaire +1 more source
The ground state of solid neutron matter is investigated using the $t$-matrix formalism developed for the quantum crystal problem. Studies of neutrons interacting through the repulsive part of the Reid $^{1}S_{0}$ interaction, the Reid $^{1}S_{0}$ interaction, and the full Reid potentials are made in the Hartree, Hartree $t$-matrix, Hartree-Fock, and ...
M. T. Takemori, R. A. Guyer
openaire +1 more source
Kinetic Magnetohydrodynamics of Neutron Matter
Theoretical and Mathematical Physics, 2000zbMATH Open Web Interface contents unavailable due to conflicting licenses.
Akhiezer, A. I. +2 more
openaire +1 more source
EOS of neutron-rich matter and pure neutron matter
Science China Physics, Mechanics and Astronomy, 2012We report the equation of state (EOS) of pure neutron matter (PNM) and neutron-rich matter (NRM) for the realistic Urbana V14 two nucleon interaction, obtained by using a Variational Monte Carlo (VMC) method. Also, many body interactions are included as a phenomenological density dependent term in the potential.
openaire +2 more sources
Physical Review C, 1999
The Bertsch, nonparametric model of neutron matter is analyzed and strong indications are found that, in the infinite system limit, the ground state is a Fermi liquid with an effective mass, except for a set of measure zero.
openaire +1 more source
The Bertsch, nonparametric model of neutron matter is analyzed and strong indications are found that, in the infinite system limit, the ground state is a Fermi liquid with an effective mass, except for a set of measure zero.
openaire +1 more source