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Neutron Stars in Aether Scalar-Tensor Theory
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Aether Scalar-Tensor theory is a modification of general relativity proposed to explain galactic and cosmological mass discrepancies conventionally attributed to dark matter.~The theory is able to fit the cosmic microwave background and the linear matter power spectrum.~In this work, we derive the Tolman-Oppenheimer-Volkoff equation in this theory and solve it for realistic nuclear equations of state to predict the mass-radius relation of neutron stars.~We find solutions that are compatible with all current observations of neutron stars.
Forward citations
Cited by 2 Pith papers
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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.
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How black hole mimickers and Shapiro-free lenses signal effective dark matter
Two new exact solutions in aether-scalar-tensor gravity describe a black-hole-mimicking wormhole and a massless lens with negative Shapiro time delay.
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