Strange Quark Stars in 4D Einstein-Gauss-Bonnet Gravity

Understand

The existence of strange matter in compact stars may pose striking sequels of the various physical phenomena.

• As an alternative to neutron stars, a new class of compact stars called strange stars should exist if the strange matter hypothesis is true.
• In the present article, we investigate the possible construction of the strange stars in quark matter phases based on the MIT bag model.
• We consider scenarios in which strange stars have no crusts.