Analytic black-hole solutions are reconstructed via conservation laws from variational symmetries in symmetric teleparallel scalar-tensor gravity, and the theory is shown to support viable compact-star interiors matched to extremal Reissner-Nordström exteriors.
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A minimally decoupled anisotropic strange star model with MIT bag EOS and g(r)=sin(Psi r^2) reproduces observed pulsar masses up to 2.28 solar masses with radii 11.3-12.9 km while satisfying stability.
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Compact Stars in Symmetric Teleparallel Scalar-Tensor Gravity
Analytic black-hole solutions are reconstructed via conservation laws from variational symmetries in symmetric teleparallel scalar-tensor gravity, and the theory is shown to support viable compact-star interiors matched to extremal Reissner-Nordström exteriors.
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Probing geometrically perturbed strange stars with minimal decoupling using millisecond pulsar timing observations
A minimally decoupled anisotropic strange star model with MIT bag EOS and g(r)=sin(Psi r^2) reproduces observed pulsar masses up to 2.28 solar masses with radii 11.3-12.9 km while satisfying stability.