Nuclear matter within the relativistic-mean-field model involving free-space nucleon-nucleon forces

Journal Article · Wed Jul 15 00:00:00 EDT 2009 · Physics of Atomic Nuclei

DOI:https://doi.org/10.1134/S1063778809070072· OSTI ID:21405875

Kryshen, E L ^[1]

---

1. Russian Academy of Sciences, Petersburg Nuclear Physics Institute (Russian Federation)

Masses and radii of neutron stars were calculated within the relativistic-mean-field model by using free-space nucleon-nucleon forces. Multiparticle forces and correlations were taken into account phenomenologically by introducing a nonlinearity in isoscalar channels and three-particle forces in the scalar-isovector channel.

• OSTI ID: 21405875
• Journal Information: Physics of Atomic Nuclei, Vol. 72, Issue 7; Other Information: DOI: 10.1134/S1063778809070072; Copyright (c) 2009 Pleiades Publishing, Ltd.; ISSN 1063-7788
• Country of Publication: United States
• Language: English

Related Subjects

73 NUCLEAR PHYSICS AND RADIATION PHYSICS
CORRELATIONS
ISOVECTORS
MASS
MEAN-FIELD THEORY
NEUTRON STARS
NONLINEAR PROBLEMS
NUCLEAR MATTER
NUCLEON-NUCLEON INTERACTIONS
PARTICLES
RELATIVISTIC RANGE
SCALARS
SPACE
BARYON-BARYON INTERACTIONS
ENERGY RANGE
HADRON-HADRON INTERACTIONS
INTERACTIONS
MATTER
PARTICLE INTERACTIONS
STARS
TENSORS
VECTORS