Published November 16, 2001 | Version v1
Journal article Metadata-only

Nuclear equation of state

Creators

  • 1. Gesellschaft fuer Schwerionenforschung mbH, D-64291 Darmstadt (Germany)
  • 2. National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy, Michigan State University, East Lansing, Michigan 48824 (United States)

Description

Nuclear equation of state plays an important role in the evolution of the Universe, in supernova explosions and, thus, in the production of heavy elements, and in stability of neutron stars. The equation constrains the two- and three-nucleon interactions and the quantum chromodynamics in nonperturbative regime. Despite the importance of the equation, though, its features had remained fairly obscure. The talk reviews new results on the equation of state from measurements of giant nuclear oscillations and from studies of particle emission in central collisions of heavy nuclei

Additional details

Identifiers

DOI
10.1063/1.1427443;
arXiv
arXiv:nucl-th/0112006v1;

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
597
Journal Issue
1
Journal Page Range
p. 24-42
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
International conference on nonequilibrium and nonlinear dynamics in nuclear and other finite systems
Dates
21-25 May 2001
Place
Beijing (China)

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
35076552
Subject category
S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ALPHA PARTICLES; EQUATIONS OF STATE; GALACTIC EVOLUTION; HEAVY NUCLEI; NEUTRON STARS; NUCLEAR MATTER; NUCLEAR STRUCTURE; NUCLEOSYNTHESIS; QUANTUM CHROMODYNAMICS; SUPERNOVAE; THREE-BODY PROBLEM; TWO-BODY PROBLEM; UNIVERSE; VIBRATIONAL STATES
Descriptors DEC
BINARY STARS; CHARGED PARTICLES; ENERGY LEVELS; EQUATIONS; ERUPTIVE VARIABLE STARS; EVOLUTION; EXCITED STATES; FIELD THEORIES; IONIZING RADIATIONS; MANY-BODY PROBLEM; MATTER; NUCLEI; QUANTUM FIELD THEORY; RADIATIONS; STARS; SYNTHESIS; VARIABLE STARS

Optional Information

Notes
(c) 2001 American Institute of Physics.