A microscopic equation of state for neutron-rich matter and its effect on neutron star properties
arXiv:1111.0695
Abstract
Chapter prepared for the book "Astrophysics", ISBN 979-953-307-389-6, INTECH Publishers (in press).
34 pages, 20 figures
References in corpus (11)
- Shapiro delay measurement of a two solar mass neutron star
- Neutron Star Observations: Prognosis for Equation of State Constraints
- Constraints on the high-density nuclear equation of state from the phenomenology of compact stars and heavy-ion collisions
- An Eccentric Binary Millisecond Pulsar in the Galactic Plane
- Nuclear symmetry energy and its density slope at normal density extracted from global nucleon optical potentials
- Evidence for 1122 Hz X-Ray Burst Oscillations from the Neutron-Star X-Ray Transient XTE J1739-285
- Isotopic Dependence of the Nuclear Caloric Curve
- Fusion process studied with preequilibrium giant dipole resonance in time dependent Hartree-Fock theory
- The neutron skin of Pb and the density dependence of the symmetry energy
- Spin- and isospin-polarized states of nuclear matter in the Dirac-Brueckner-Hartree-Fock model
- Neutron-proton elliptic flow in Au + Au