Diffusion in the stochastic Klein-Gordon equation
- URL: http://arxiv.org/abs/2511.10738v1
- Date: Thu, 13 Nov 2025 19:00:07 GMT
- Title: Diffusion in the stochastic Klein-Gordon equation
- Authors: Jonathan Oppenheim, Emanuele Panella,
- Abstract summary: We study the phenomenology of linearised classical-quantum hybrid gravity.<n>In particular, we describe how to compute the non-equilibrium two point function of the scalar field.<n>We conclude by discussing possible implications of anomalous diffusion for hybrid theories of gravity.
- Score: 0.0
- License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
- Abstract: Theories of gravity in which the metric is fundamentally classical predict stochastic fluctuations in the gravitational field. In this article, we study the stochastic Klein-Gordon equation as a starting point to understand the phenomenology of linearised classical-quantum hybrid gravity. In particular, we describe how to compute the non-equilibrium two point function of the scalar field, showing explicitly the role of the initial state in regulating divergences. To do so, we use a "mod-squared-retarded" pole-prescription and find that the covariance in the field is non-zero only outside the lightcone, scales inversely with the spatial distance of the spacetime points and grows linearly in time. The energy has a contact divergence similar to that found in the quantum case. We conclude by discussing possible implications of anomalous diffusion for hybrid theories of gravity, especially looking at the energy density in the predicted gravitational waves background, which can be inferred from the scalar covariances.
Related papers
- Testing classicality of gravity by gravitation decoherence [0.0]
We discuss an influence of an external weak gravitational field on the gravitational self-decoherence effect with help of the extension of regularized Shr"odinger-Newton equation in a curved background.<n>We demonstrate that it leads to the experimentally verifiable conclusions about applicability of the classical description of the weak gravitation field.
arXiv Detail & Related papers (2025-03-07T11:48:45Z) - Dynamics of Topological Defects in a Rashba Spin-Orbit Coupled Bose-Einstein Condensate [14.50864620620941]
We investigate the quench dynamics of a two-dimensional Rashba spin-orbit coupled Bose-Einstein condensate.<n>During this quench, topological defects emerge in the form of vortices.
arXiv Detail & Related papers (2024-12-25T09:31:42Z) - Ultracold Neutrons in the Low Curvature Limit: Remarks on the
post-Newtonian effects [49.1574468325115]
We apply a perturbative scheme to derive the non-relativistic Schr"odinger equation in curved spacetime.
We calculate the next-to-leading order corrections to the neutron's energy spectrum.
While the current precision for observations of ultracold neutrons may not yet enable to probe them, they could still be relevant in the future or in alternative circumstances.
arXiv Detail & Related papers (2023-12-30T16:45:56Z) - Real-time dynamics of false vacuum decay [49.1574468325115]
We investigate false vacuum decay of a relativistic scalar field in the metastable minimum of an asymmetric double-well potential.
We employ the non-perturbative framework of the two-particle irreducible (2PI) quantum effective action at next-to-leading order in a large-N expansion.
arXiv Detail & Related papers (2023-10-06T12:44:48Z) - From locality to irregularity: Introducing local quenches in massive
scalar field theory [68.8204255655161]
We consider the dynamics of excited local states in massive scalar field theory in an arbitrary spacetime dimension.
We identify different regimes of their evolution depending on the values of the field mass and the quench regularization parameter.
We also investigate the local quenches in massive scalar field theory on a cylinder and show that they cause an erratic and chaotic-like evolution of observables.
arXiv Detail & Related papers (2022-05-24T18:00:07Z) - Quantum dynamics corresponding to chaotic BKL scenario [62.997667081978825]
Quantization smears the gravitational singularity avoiding its localization in the configuration space.
Results suggest that the generic singularity of general relativity can be avoided at quantum level.
arXiv Detail & Related papers (2022-04-24T13:32:45Z) - Gravitationally induced decoherence vs space-time diffusion: testing the
quantum nature of gravity [0.0]
We consider two interacting systems when one is treated classically while the other system remains quantum.
We prove that such hybrid dynamics necessarily results in decoherence of the quantum system, and a breakdown in predictability in the classical phase space.
Applying the trade-off relation to gravity, we find a relationship between the strength of gravitationally-induced decoherence versus diffusion of the metric and its conjugate momenta.
arXiv Detail & Related papers (2022-03-03T19:52:11Z) - Locally mediated entanglement in linearised quantum gravity [0.0]
An information-theoretic argument: entanglement mediated by a local field certifies that the field is not classical.
Previous derivations of the effect modelled gravity as instantaneous.
In this framework, entanglement is clearly mediated by a quantum feature of the field.
arXiv Detail & Related papers (2022-02-07T17:29:33Z) - Gravitational decoherence: a non relativistic spin 1/2 fermionic model [0.0]
We derive a non relativistic model for the gravitational decoherence of spin 1/2 particles.
We discuss the differences with the scalar bosonic model and we describe the regimes in which they become negligible.
arXiv Detail & Related papers (2020-12-02T16:54:00Z) - Topological Quantum Gravity of the Ricci Flow [62.997667081978825]
We present a family of topological quantum gravity theories associated with the geometric theory of the Ricci flow.
First, we use BRST quantization to construct a "primitive" topological Lifshitz-type theory for only the spatial metric.
We extend the primitive theory by gauging foliation-preserving spacetime symmetries.
arXiv Detail & Related papers (2020-10-29T06:15:30Z) - On the decoherence effect of a stochastic gravitational perturbation on
scalar matter and the possibility of its interferometric detection [0.0]
We show how the master equation reproduces the results present in the literature by taking appropriate limits.
We apply our model to a matter wave experiment, providing a formula for determining the magnitude of gravitational decoherence.
arXiv Detail & Related papers (2019-12-29T21:08:44Z)
This list is automatically generated from the titles and abstracts of the papers in this site.
This site does not guarantee the quality of this site (including all information) and is not responsible for any consequences.