Superdense nuclei in degenerate nuclear plasma
Journal Article
·
· Sov. Astron. (Engl. Transl.); (United States)
OSTI ID:5577492
The properties of compressed matter consisting of superdense nuclei are examined, with allowance for the presence of a pion condensate. Calculations are performed for two alternative sets of nuclear interaction constants, one giving superdense, superbound nuclei, while the other gives metastable superdense nuclei. The analysis is carried out for collapse occurring in both complete and partial equilibrium. Configurations are calculated for white dwarfs composed of superdense, superbound nuclei.
- Research Organization:
- Erevanskii Gosudarstvennyi Universitet, Yerevan, Armenian SSR
- OSTI ID:
- 5577492
- Journal Information:
- Sov. Astron. (Engl. Transl.); (United States), Journal Name: Sov. Astron. (Engl. Transl.); (United States) Vol. 24; ISSN SAAJA
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BARYONS
BOSONS
DWARF STARS
ELEMENTARY PARTICLES
EQUATIONS
EQUATIONS OF STATE
EQUILIBRIUM
FERMIONS
FLUIDS
HADRONS
INSTABILITY
LIQUIDS
MESONS
NEUTRON STARS
NUCLEI
NUCLEONS
PIONS
PLASMA DENSITY
PLASMA INSTABILITY
PSEUDOSCALAR MESONS
STARS
THERMAL EQUILIBRIUM
THERMODYNAMICS
WHITE DWARF STARS
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BARYONS
BOSONS
DWARF STARS
ELEMENTARY PARTICLES
EQUATIONS
EQUATIONS OF STATE
EQUILIBRIUM
FERMIONS
FLUIDS
HADRONS
INSTABILITY
LIQUIDS
MESONS
NEUTRON STARS
NUCLEI
NUCLEONS
PIONS
PLASMA DENSITY
PLASMA INSTABILITY
PSEUDOSCALAR MESONS
STARS
THERMAL EQUILIBRIUM
THERMODYNAMICS
WHITE DWARF STARS