Absence of gravitationally induced entanglement in certain semi-classical theories of gravity
- URL: http://arxiv.org/abs/2510.20991v1
- Date: Thu, 23 Oct 2025 20:39:07 GMT
- Title: Absence of gravitationally induced entanglement in certain semi-classical theories of gravity
- Authors: Ward Struyve,
- Abstract summary: A class of semi-classical models is examined that treat gravity classically, through some potential in the Schr"odinger equation.<n>It is shown that these models do not generate entanglement.
- Score: 0.0
- License: http://creativecommons.org/licenses/by/4.0/
- Abstract: Bose et al. and Marletto and Vedral proposed an experiment to test whether gravity can induce entanglement between massive systems, arguing that the capacity to do so would imply the quantum nature of gravity. In this work, a class of semi-classical models is examined that treat gravity classically, through some potential in the Schr\"odinger equation, and it is shown that these models do not generate entanglement. This class includes the Newton-Schr\"odinger model, where gravity is sourced by the wave function, the Bohmian analogue, where gravity is sourced by actual point-particles, and an interpolating model proposed by D\"oner and Grossardt. These models are analyzed in the context of the proposed experiment and contrasted with the standard Newtonian potential, which does generate entanglement.
Related papers
- Collapse-based models for gravity do not violate the Entanglement-Based Witness of non-classicality [0.0]
An entanglement-based witness of non-classicality can be applied to testing quantum effects in gravity.<n>Recent claims have been made that collapse-based models of classical gravity can predict gravitationally induced entanglement.
arXiv Detail & Related papers (2025-03-25T15:44:59Z) - The Role of Quantum Measurements when Testing the Quantum Nature of Gravity [12.091555830963683]
We argue that the Causal Conditional Formulation of Schroedinger-Newton (CCSN) theory is a minimum model within this framework.<n>Since CCSN can be viewed as a quantum feedback control scheme, it can be made causal and free from pathologies that previously plagued SN theories.<n>We show that the mass-concentration effect of self classical gravity still makes CCSN much easier to test than testing the mutual entanglement.
arXiv Detail & Related papers (2025-03-14T21:09:17Z) - Hybrid Classical-Quantum Newtonian Gravity with stable vacuum [0.0]
We investigate a hybrid classical-quantum model in which classical Newtonian gravity emerges from collapses of the mass density operator.<n>We show that GPSL ensures vacuum stability; this, together with its applicability to identical particles and fields, makes it a promising candidate for a relativistic generalization.<n>We provide explicit examples, including the dynamics of a single particle and a rigid sphere, to illustrate the distinctive phenomenology of the model.
arXiv Detail & Related papers (2025-02-07T15:19:13Z) - Positivity and Entanglement in Markovian Open Quantum Systems and Hybrid Classical-Quantum Theories of Gravity [0.0]
We identify a class of continuous variable Markovian master equations for which positivity and complete positivity become equivalent.<n>We investigate the entangling properties of models of classical gravity interacting with quantum matter.<n>We prove that entanglement generation can indeed take place within these models.
arXiv Detail & Related papers (2025-01-27T17:53:50Z) - Semiclassical gravity phenomenology under the causal-conditional quantum measurement prescription II: Heisenberg picture and apparent optical entanglement [13.04737397490371]
In quantum gravity theory, a state-dependent gravitational potential introduces nonlinearity into the state evolution.
The formalism for understanding the continuous quantum measurement process on the quantum state has been previously discussed using the Schr"odinger picture.
In this work, an equivalent formalism using the Heisenberg picture is developed and applied to the analysis of two optomechanical experiment protocols.
arXiv Detail & Related papers (2024-11-08T14:07:18Z) - 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) - Testing Quantum Gravity using Pulsed Optomechanical Systems [13.650870855008112]
We consider the Schr"odinger-Newton (SN) theory and the Correlated Worldline (CWL) theory, and show that they can be distinguished from conventional quantum mechanics.
We find that discriminating between the theories will be very difficult until experimental control over low frequency quantum optomechanical systems is pushed further.
arXiv Detail & Related papers (2023-11-03T17:06:57Z) - Testing the nonclassicality of gravity with the field of a single
delocalized mass [55.2480439325792]
A setup is proposed that is based on a single delocalized mass coupled to a harmonically trapped test mass.
We investigate the in-principle feasibility of such an experiment, which turns out to crucially depend on the ability to tame Casimir-Polder forces.
arXiv Detail & Related papers (2023-07-18T15:40:16Z) - Strongly incoherent gravity [0.0]
A non-entangling version of an arbitrary two-body potential $V(r)$ arises from local measurements and feedback forces.
This produces a non-relativistic model of gravity with fundamental loss of unitarity.
As an alternative to testing entanglement properties, we show that the entire remaining parameter space can be tested by looking for loss of quantum coherence in small systems.
arXiv Detail & Related papers (2023-01-20T01:09:12Z) - Machine Learning for Discovering Effective Interaction Kernels between
Celestial Bodies from Ephemerides [10.77689830299308]
We use a data-driven learning approach to derive a stable and accurate model for the motion of celestial bodies in our Solar System.
By modeling the major astronomical bodies in the Solar System as pairwise interacting agents, our learned model generate extremely accurate dynamics.
Our model can provide a unified explanation to the observation data, especially in terms of reproducing the perihelion precession of Mars, Mercury, and the Moon.
arXiv Detail & Related papers (2021-08-26T16:30:59Z) - A no-go theorem on the nature of the gravitational field beyond quantum
theory [0.0]
Table-top experiments involving massive quantum systems have been proposed to test the interface of quantum theory and gravity.
In particular, the crucial point of the debate is whether it is possible to conclude anything on the quantum nature of the gravitational field.
We introduce the framework of Generalised Probabilistic Theories (GPTs) to study the nature of the gravitational field.
arXiv Detail & Related papers (2020-12-02T19:00:03Z)
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.