In Aether Scalar-Tensor theory, slowly rotating neutron stars obey approximate universal moment-of-inertia versus compactness relations that deviate from general relativity and are fit with parameter-dependent formulae.
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Slowly Rotating Neutron Stars in Aether Scalar-Tensor Theory
In Aether Scalar-Tensor theory, slowly rotating neutron stars obey approximate universal moment-of-inertia versus compactness relations that deviate from general relativity and are fit with parameter-dependent formulae.