The Gravity of the Classical Klein-Gordon field
Piero Chiarelli

TL;DR
This paper derives a covariant gravity theory from the Klein-Gordon equation using a hydrodynamic approach, revealing a quantum-induced cosmological pressure tensor that could explain cosmic acceleration without a classical cosmological constant.
Contribution
It introduces a novel Einstein-like gravity model based on the Klein-Gordon field, incorporating a quantum pressure tensor that emerges naturally and affects cosmological dynamics.
Findings
Derives Einstein-like gravity equations from the Klein-Gordon field.
Introduces a quantum cosmological pressure tensor density (CPTD) that can mimic dark energy.
Shows the CPTD's expectation value is independent of vacuum energy and aligns with astronomical observations.
Abstract
The work shows that the evolution of the field of the free Klein-Gordon equation (KGE), in the hydrodynamic representation, can be represented by the motion of a mass density subject to the Bohm-type quantum potential, whose equation can be derived by a minimum action principle. Once the quantum hydrodynamic motion equations have been covariantly extended to the curved space-time, the gravity equation (GE), determining the geometry of the space-time, is obtained by minimizing the overall action comprehending the gravitational field. The derived Einstein-like gravity for the KGE field shows an energy-impulse tensor density (EITD) that is a function of the field with the spontaneous emergence of the cosmological pressure tensor density (CPTD) that in the classical limit leads to the cosmological constant(CC). The energy-impulse tensor of the theory shows analogies with the modified…
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.
