How and when will a neutron star become a hyperon star?

Chinese Physics Letters

Volumn 18, Issue 12, 2001, Pages 1571-1574

  Jia, Huan Yu ^a   Sun, Bao Xi ^b   Meng, Jie ^a,b,c   Zhao, En Guang ^b  

^a PEKING UNIVERSITY   (China)

^b INSTITUTE OF THEORETICAL PHYSICS   (China)

^c CENTER OF THEORETICAL NUCLEAR PHYSICS   (China)

Author keywords

[No Author keywords available]

Indexed keywords

HADRONS; MEAN FIELD THEORY; NEUTRONS;

BARYON DENSITY; COUPLING CONSTANTS; COUPLING RATIOS; HYPERON STARS; NEUTRON STARS; NUCLEAR MATTERS; PARAMETER SET; PROPERTY; RELATIVISTIC MEAN-FIELD THEORIES; SATURATION DENSITY;

STARS;

EID: 0035731969     PISSN: 0256307X     EISSN: None     Source Type: Journal    
DOI: 10.1088/0256-307X/18/12/309     Document Type: Article

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