For neutron stars near the critical compactness, scalar-tensor gravity can change computed X-ray pulse fluxes by up to 80% and inferred radii by about 10%.
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X-ray pulsed light curves of highly compact neutron stars as probes of scalar-tensor theories of gravity
For neutron stars near the critical compactness, scalar-tensor gravity can change computed X-ray pulse fluxes by up to 80% and inferred radii by about 10%.