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- W2889708550 abstract "We consider a neutrino-free hot neutron star that contains antikaon condensates in its core and is at finite entropy per baryon. We find the equation of state for a range of entropies and antikaon optical potentials and generate the mass profile of static as well as rotating stars. Rotation induces many changes in the stellar equilibrium, and hence its structural properties evolve. In this work, we report the effect of rotation on the mass and shape of a hot neutron star for different equations of state and thermodynamic conditions. Temperature profile of hot, static neutron star is also explored. We also make a crude estimate of the amplitude of gravitational waves emitted by an axisymmetric rotating NS with high magnetic field." @default.
- W2889708550 created "2018-09-27" @default.
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- W2889708550 date "2018-09-04" @default.
- W2889708550 modified "2023-10-10" @default.
- W2889708550 title "Properties of rapidly rotating hot neutron stars with antikaon condensates at constant entropy per baryon" @default.
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- W2889708550 doi "https://doi.org/10.1103/physrevc.98.035801" @default.
- W2889708550 hasPublicationYear "2018" @default.
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