Published September 2011
| Version v1
Journal article
Nuclear Matter Equation Of State And Incompressibility In The Relativistic Density Dependent Hadron Field Theory
Description
Nuclear matter equation of state and incompressibility are determined utilizing the relativistic density dependent Hadron field theory. Nuclear matter is studied at symmetric ground-state and at supernova collapse conditions, and pressure density of isentropic nuclear matter is determined as a function of the density at supernova collapse conditions. The value of the ground-state nuclear matter incompressibility is within the interval determined by isoscalar giant monopole resonance measurements and relativistic calculations. And the dependency of the coupling parameters on density leads to results closer to the results of calculations used in the study of supernova explosion than the results of other relativistic calculations.(author)
Additional details
Publishing Information
- Journal Title
- Aalam Al-Zarra
- Journal Issue
- 135
- Journal Page Range
- p. 60
- ISSN
- 1607-985X
- CODEN
- AAALE5
INIS
- Country of Publication
- Syrian Arab Republic
- Country of Input or Organization
- Syrian Arab Republic
- INIS RN
- 42103050
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS; S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- BRUECKNER METHOD; DENSITY; EQUATIONS OF STATE; HADRONS; HARTREE-FOCK METHOD; INCOMPRESSIBLE FLOW; NUCLEAR MATTER; RELATIVISTIC RANGE; SUPERNOVAE
- Descriptors DEC
- APPROXIMATIONS; BINARY STARS; CALCULATION METHODS; ELEMENTARY PARTICLES; ENERGY RANGE; EQUATIONS; ERUPTIVE VARIABLE STARS; FLUID FLOW; MATTER; PHYSICAL PROPERTIES; STARS; VARIABLE STARS
Optional Information
- Notes
- Abstract of paper published in Acta Physica Polonica, v. B42(6), 2011