Cosmology and stellar equilibrium using Newtonian hydrodynamics with general relativistic pressure
P. O. Baqui, J. C. Fabris, and O. F. Piattella

TL;DR
This paper derives Newtonian equations incorporating relativistic pressure effects, analyzing their impact on cosmology and stellar equilibrium, revealing significant differences from standard theories and potential for improved simulations.
Contribution
The authors explicitly derive and analyze Newtonian equations with relativistic pressure effects, comparing their predictions with General Relativity and other theories in cosmology and stellar physics.
Findings
Universe acceleration with positive pressure predicted
Small-scale perturbations match relativistic results
Neutron star mass limits are significantly higher
Abstract
We revisit the analysis made by Hwang and Noh [JCAP 1310 (2013)] aiming the construction of a Newtonian set of equations incorporating pressure effects typical of the General Relativity theory. We explicitly derive the Hwang-Noh equations, comparing them with similar computations found in the literature. Then, we investigate the cosmological expansion, linear cosmological perturbations theory and stellar equilibrium by using the new set of equations and comparing the results with those coming from the usual Newtonian theory, from the Neo-Newtonian theory and from the General Relativity theory. We show that the predictions for the background evolution of the Universe are deeply changed with respect to the General Relativity theory: the acceleration of the Universe is achieved with positive pressure. On the other hand, the behaviour of small cosmological perturbations…
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