Pairing gaps in neutron stars

Nucleonic {sup 1}S{sub 0} and {sup 3}PF{sub 2} pairing gaps in neutron stars are determined and their sensitivity to medium effects realized through nucleonic three-body forces, and the presence of hyperons is explored.

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Bibliographic Details
Published in:Physical review. C, Nuclear physics Nuclear physics, 2004-10, Vol.70 (4), Article 048802
Main Authors: Zhou, Xian-Rong, Schulze, H.-J., Zhao, En-Guang, Pan, Feng, Draayer, J. P.
Format: Article
Language:English
Subjects:
ENERGY LEVELS
HYPERONS
NEUTRON STARS
NUCLEAR FORCES
NUCLEAR MATTER
NUCLEAR MODELS
NUCLEAR PHYSICS AND RADIATION PHYSICS
SENSITIVITY
THREE-BODY PROBLEM
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Description
Summary:Nucleonic {sup 1}S{sub 0} and {sup 3}PF{sub 2} pairing gaps in neutron stars are determined and their sensitivity to medium effects realized through nucleonic three-body forces, and the presence of hyperons is explored.
ISSN:0556-2813
1089-490X
DOI:10.1103/PhysRevC.70.048802