Fully Self-Consistent Semiclassical Gravity

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Main Authors: Muciño, R., Okon, E., Sudarsky, D., Wiedemann, M.
Format: Preprint
Published: 2025
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author Muciño, R.
Okon, E.
Sudarsky, D.
Wiedemann, M.
author_facet Muciño, R.
Okon, E.
Sudarsky, D.
Wiedemann, M.
contents A theory of quantum gravity consists of a gravitational framework which, unlike general relativity, takes into account the quantum character of matter. In spite of impressive advances, no fully satisfactory, self-consistent and empirically viable theory with those characteristics has ever been constructed. A successful semiclassical gravity model, in which the classical Einstein tensor couples to the expectation value of the energy-momentum tensor of quantum matter fields, would, at the very least, constitute a useful stepping stone towards quantum gravity. However, not only no empirically viable semiclassical theory has ever been proposed, but the self-consistency of semiclassical gravity itself has been called into question repeatedly over the years. Here, we put forward a fully self-consistent, empirically viable semiclassical gravity framework, in which the expectation value of the energy-momentum tensor of a quantum field, evolving via a relativistic objective collapse dynamics, couples to a fully classical Einstein tensor. We present the general framework, a concrete example, and briefly explore possible empirical consequences of our model.
format Preprint
id arxiv_https___arxiv_org_abs_2506_17149
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Fully Self-Consistent Semiclassical Gravity
Muciño, R.
Okon, E.
Sudarsky, D.
Wiedemann, M.
General Relativity and Quantum Cosmology
History and Philosophy of Physics
Quantum Physics
A theory of quantum gravity consists of a gravitational framework which, unlike general relativity, takes into account the quantum character of matter. In spite of impressive advances, no fully satisfactory, self-consistent and empirically viable theory with those characteristics has ever been constructed. A successful semiclassical gravity model, in which the classical Einstein tensor couples to the expectation value of the energy-momentum tensor of quantum matter fields, would, at the very least, constitute a useful stepping stone towards quantum gravity. However, not only no empirically viable semiclassical theory has ever been proposed, but the self-consistency of semiclassical gravity itself has been called into question repeatedly over the years. Here, we put forward a fully self-consistent, empirically viable semiclassical gravity framework, in which the expectation value of the energy-momentum tensor of a quantum field, evolving via a relativistic objective collapse dynamics, couples to a fully classical Einstein tensor. We present the general framework, a concrete example, and briefly explore possible empirical consequences of our model.
title Fully Self-Consistent Semiclassical Gravity
topic General Relativity and Quantum Cosmology
History and Philosophy of Physics
Quantum Physics
url https://arxiv.org/abs/2506.17149