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gr-qc 1

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2025 1

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Neutron Stars in Causal Scalar-Tensor Theories

gr-qc · 2025-05-29 · conditional · novelty 6.0

Solving modified TOV equations in an anti-screened K-essence scalar-tensor theory, the authors find two solution branches per central density and a critical density cutoff, producing mass-radius predictions that can match neutron star observations.

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  • Neutron Stars in Causal Scalar-Tensor Theories gr-qc · 2025-05-29 · conditional · none · ref 2

    Solving modified TOV equations in an anti-screened K-essence scalar-tensor theory, the authors find two solution branches per central density and a critical density cutoff, producing mass-radius predictions that can match neutron star observations.