Gravitationally decoupled strange star models can reach maximum masses of 2.87 to 2.95 solar masses and predict radii of 10.6 to 12.1 km for known massive compact objects.
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Role of gravitational decoupling on theoretical insights of relativistic massive compact stars in the mass gap
Gravitationally decoupled strange star models can reach maximum masses of 2.87 to 2.95 solar masses and predict radii of 10.6 to 12.1 km for known massive compact objects.