On the role of pressure in generating the gravitational field
A.I. Nikishov

TL;DR
This paper explores how pressure influences gravitational fields in Einstein's equations, questioning why classical solutions depend only on mass despite linearized theories indicating pressure's role.
Contribution
It highlights the discrepancy between classical and linearized solutions regarding pressure's role, suggesting a potential need for alternative gravitational theories.
Findings
Schwarzschild solution depends only on mass parameter
Linearized Einstein equations include pressure analogue
Implication for phenomenological gravity models
Abstract
The Einstein equations for static gravitational field depend on energy density and pressure. So one may expect that solutions should depend on two parameters: mass and its analogue originated from pressure. Yet the Schwarzschild solution have only mass parameter. So does its linear approximation. On the other hand the solutions of linearized Einstein equations, obtained using graviton propagator, contain mass and its pressure analogue. This suggests that a phenomenological approach to gravity, using propagators and many graviton vertices, should lead to a theory different from general relativity.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsRelativity and Gravitational Theory · Cosmology and Gravitation Theories · Geophysics and Gravity Measurements
