
arXiv: 2011.14629
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.
9 pages, 7 figures
density, star: compact, Tolman-Oppenheimer-Volkoff equation, [PHYS.GRQC] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], alternative theories of gravity, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), 530, General Relativity and Quantum Cosmology, General relativity, relativity theory, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], general relativity, conservation law, entanglement, neutron star, numerical calculations, equation of state
density, star: compact, Tolman-Oppenheimer-Volkoff equation, [PHYS.GRQC] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], alternative theories of gravity, FOS: Physical sciences, General Relativity and Quantum Cosmology (gr-qc), 530, General Relativity and Quantum Cosmology, General relativity, relativity theory, [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc], general relativity, conservation law, entanglement, neutron star, numerical calculations, equation of state
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