A simple gravitational self-decoherence model
Gabriel H. S. Aguiar, George E. A. Matsas
TL;DR
The paper introduces a gravitational self-decoherence mechanism that invokes a Heisenberg cut at $M_C \sim M_P$ to separate quantum and classical behavior, positing a gravitational interaction between a particle and a nonphysical virtual clone with a cutoff length $L_C$ that models information transfer to spacetime degrees of freedom. Decoherence is shown to be negligible for $m \ll M_C$ but significant as $m$ approaches the cut, quantified by a purity measure $\eta(t)$ and, in Stern-Gerlach scenarios, by a spin-coherence measure $\xi(t)$; the two-body evolution plus tracing over the clone yields observable mass-dependent deviations from standard QM. The authors connect their model to current experimental capabilities and propose a double Stern-Gerlach-like experiment as a concrete test to distinguish their predictions from QM and Schrödinger-Newton-type models. Overall, the framework provides a falsifiable route to explain the quantum-to-classical transition via gravitational degrees of freedom at the Planck scale, with limited (and fixed) parameter freedom around $M_C \sim M_P$.
Abstract
One of the most significant debates of our time is whether our macroscopic world (i) naturally emerges from quantum mechanics or (ii) requires new physics. We argue for the latter and propose a simple gravitational self-decoherence mechanism. For this purpose, we postulate the existence of a Heisenberg cut such that particles with masses $m$ much smaller and larger than a critical mass $M_{\rm C}$ (of the order of the Planck mass $M_{\rm P}$) would be necessarily treated according to quantum and classical rules, respectively. Our effective model is designed to capture the new physics that free quantum particles would experience as their masses approach $M_{\rm C}$. The purity loss for free quantum particles is evaluated and shown to be highly inefficient for quantum particles with $m \ll M_{\rm C}$ but very effective for those with $m \sim M_{\rm C}$. The physical picture behind it is that coherence would (easily) leak from heavy enough particles to (non-observable) spacetime quantum degrees of freedom. Finally, we contextualize our proposal with state-of-the-art experiments and show how it can be tested in a future Stern-Gerlach-like experiment.
