Anisotropic quark stars in Einstein-Gauss-Bonnet theory
Recent progress in the determination of both masses and radii of neutron stars has put strong constraints on the equation of state (EoS) above the nuclear saturation density. Within a confining quark matter model, we propose an anisotropic star consisting of a homogeneous and unpaired charge-neutral...
Main Authors: | , , , |
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Format: | Article |
Language: | English |
Published: |
Elsevier
2021-08-01
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Series: | Physics Letters B |
Online Access: | http://www.sciencedirect.com/science/article/pii/S0370269321003634 |