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.
Faraoni, Cosmology in scalar tensor gravity(2004)
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Neutron Stars in Causal Scalar-Tensor Theories
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.