  We describe the first numerical Tolman-Oppenheimer-Volkoff solutions of
compact objects in entangled relativity, which is an alternative to the
framework of general relativity that does not have any additional free
parameter. Assuming a simple polytropic equation of state and the conservation
of the rest-mass density, we notably show that, for any given density, compact
objects are always heavier (up to $\sim 8\%$) in entangled relativity than in
general relativity -- for any given central density within the usual range of
neutron stars' central densities, or for a given radius of the resulting
compact object.
