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- W3104824419 endingPage "1550007" @default.
- W3104824419 startingPage "1550007" @default.
- W3104824419 abstract "We study the effects of anisotropic pressure (AI-P) on properties of the neutron stars (NSs) with hyperons inside its core within the framework of extended relativistic mean field. It is found that the main effects of AI-P on NS matter is to increase the stiffness of the equation of state EOS, which compensates for the softening of the EOS due to the hyperons. The maximum mass and redshift predictions of anisotropic neutron star with hyperonic core are quite compatible with the result of recent observational constraints if we use the parameter of AI-P model h ≤ 0.8 [L. Herrera and W. Barreto, Phys. Rev. D 88 (2013) 084022.] and Λ ≤ -1.15 [D. D. Doneva and S. S. Yazadjiev, Phys. Rev. D 85 (2012) 124023.]. The radius of the corresponding NS at M = 1.4 M ⊙ is more than 13 km, while the effect of AI-P on the minimum mass of NS is insignificant. Furthermore, due to the AI-P in the NS, the maximum mass limit of higher than 2.1 M ⊙ cannot rule out the presence of hyperons in the NS core." @default.
- W3104824419 created "2020-11-23" @default.
- W3104824419 creator A5027614946 @default.
- W3104824419 date "2015-01-01" @default.
- W3104824419 modified "2023-10-01" @default.
- W3104824419 title "Anisotropic pressure and hyperons in neutron stars" @default.
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- W3104824419 doi "https://doi.org/10.1142/s021830131550007x" @default.
- W3104824419 hasPublicationYear "2015" @default.
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