The Density-Dependent Correlations among Observables in Nuclear Matter and Hyperon-Rich Neutron Stars
Joint Authors
Source
Advances in High Energy Physics
Issue
Vol. 2009, Issue 2009 (31 Dec. 2009), pp.1-15, 15 p.
Publisher
Hindawi Publishing Corporation
Publication Date
2009-05-18
Country of Publication
Egypt
No. of Pages
15
Main Subjects
Abstract EN
The conserving σ-ω-ρ mean-field approximation with nonlinear interactions of hadrons has been applied to examine properties of nuclear matter and hyperonic neutron stars.
The nonlinear interactions that will produce density-dependent effective masses and coupling constants of hadrons are included in order to examine density correlations among properties of nuclear matter and neutron stars such as binding energy, incompressibility, K, symmetry energy, a4, hyperon-onset density, and maximum masses of neutron stars.
The conditions of conserving approximations in order to maintain thermodynamic consistency to an approximation are essential for the analysis of density-dependent correlations.
American Psychological Association (APA)
Uechi, Schun T.& Uechi, Hiroshi. 2009. The Density-Dependent Correlations among Observables in Nuclear Matter and Hyperon-Rich Neutron Stars. Advances in High Energy Physics،Vol. 2009, no. 2009, pp.1-15.
https://search.emarefa.net/detail/BIM-487468
Modern Language Association (MLA)
Uechi, Schun T.& Uechi, Hiroshi. The Density-Dependent Correlations among Observables in Nuclear Matter and Hyperon-Rich Neutron Stars. Advances in High Energy Physics No. 2009 (2009), pp.1-15.
https://search.emarefa.net/detail/BIM-487468
American Medical Association (AMA)
Uechi, Schun T.& Uechi, Hiroshi. The Density-Dependent Correlations among Observables in Nuclear Matter and Hyperon-Rich Neutron Stars. Advances in High Energy Physics. 2009. Vol. 2009, no. 2009, pp.1-15.
https://search.emarefa.net/detail/BIM-487468
Data Type
Journal Articles
Language
English
Notes
Includes bibliographical references
Record ID
BIM-487468