Published December 2004 | Version v1
Journal article Metadata-only

Equation of state of nuclear matter, neutron rich nuclei in laboratories and pasta nuclei in neutron star crusts

Creators

  • 1. Aichi Shukutoku Univ., Dept. of Media Theories and Production, Aichi (Japan)
  • 2. The Inst. of Physical and Chemical Research, Wako, Saitama (Japan)

Description

Macroscopic properties of neutron rich nuclei in laboratories and nuclei in neutron star crusts are supposed to be dominated by the equation of state (EOS) of asymmetric nuclear matter. In this study, we attempt to identify the most important EOS parameter that governs these properties. (author)

Additional details

Publishing Information

Journal Title
Progress of Theoretical Physics, Supplement
Journal Issue
no.156
Journal Page Range
p. 137-138
ISSN
0375-9687

Conference

Title
YITP workshop on nuclear matter under extreme conditions
Dates
1-3 Dec 2003
Place
Kyoto (Japan)

INIS

Country of Publication
Japan
Country of Input or Organization
Japan
INIS RN
36039696
Subject category
S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ENERGY DENSITY; EQUATIONS OF STATE; MASS DISTRIBUTION; NEUTRON STARS; NEUTRON-RICH ISOTOPES; NUCLEAR MATTER; PARAMETRIC ANALYSIS; PARTICLE RADII; SURFACES; THICKNESS; THOMAS-FERMI MODEL
Descriptors DEC
ATOMIC MODELS; BETA DECAY RADIOISOTOPES; BETA-MINUS DECAY RADIOISOTOPES; DIMENSIONS; DISTRIBUTION; EQUATIONS; ISOTOPES; MATHEMATICAL MODELS; MATTER; PARTICLE PROPERTIES; RADIOISOTOPES; SPATIAL DISTRIBUTION; STARS

Optional Information

Notes
3 refs., 3 figs.