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Equation of state of nucleon matter and neutron star structure
Properties of dense nucleon matter and the structure of neutron stars are studied using variational chain summation methods and the new Argonne ${v}_{18}$ two-nucleon interaction, which provides an
Solar fusion cross sections
We review and analyze the available information on the nuclear-fusion cross sections that are most important for solar energy generation and solar neutrino production. We provide best values for the
Hot Nuclear Matter
The theory of hot nuclear matter has been developed primarily to help understand some aspects of highly excited nuclei, heavy-ion reactions, supernova and neutron stars. In the next two sections we
Realistic models of pion-exchange three-nucleon interactions
We present realistic models of pion-exchange three-nucleon interactions obtained by fitting the energies of all the 17 bound or narrow states of 3{<=}A{<=}8 nucleons, calculated with less than 2%
Superfluid Fermi gases with large scattering length.
TLDR
Calculated quantum Monte Carlo calculations of superfluid Fermi gases with short-range two-body attractive interactions with infinite scattering length show that their pairing gap is approximately twice the energy per particle.
Spin-isospin structure and pion condensation in nucleon matter
We report variational calculations of symmetric nuclear matter and pure neutron matter, using the new Argonne v{sub 18} two-nucleon and Urbana IX three-nucleon interactions. At the equilibrium
Quantum Monte Carlo calculations of nuclei with A 7
We report quantum Monte Carlo calculations of ground and low-lying excited states for nuclei with A{le}7 using a realistic Hamiltonian containing the Argonne v{sub 18} two-nucleon and Urbana IX
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