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- W2358967692 abstract "In the framework of the relativistic mean field theory,the influence of the strong hyperon-hyperon(YY) interaction on the neutron star at finite temperature is studied.Results show that the inclusion of the strong YY interaction makes,(1) star matter is further hyperonized and(2) the maximum mass decreases while the corresponding radius increases.On the other hand,with the increase of temperature,the influence of the strong YY interaction is highly suppressed.When temperature is higher than 46MeV,the strong YY interaction has nearly no influence on neutron star matter." @default.
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- W2358967692 date "2009-01-01" @default.
- W2358967692 modified "2023-09-23" @default.
- W2358967692 title "The Influence of the Strong Hyperon-hyperon Interaction on the Neutron Star at Finite Temperature" @default.
- W2358967692 hasPublicationYear "2009" @default.
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