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This paper advances the Gravitational Poissonian Spontaneous Localization (GPSL) model by demonstrating how distinct spatial smearings for collapse and gravitational feedback components can drastically reduce spontaneous heating rates in hybrid quantum-classical gravity frameworks. By applying these refined theoretical bounds to neutron star thermodynamics, the authors establish new constraints on the model's parameters using existing astronomical data. This work represents a significant step toward reconciling stochastic collapse mechanisms with macroscopic gravitational phenomena.
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Gravitational Poissonian Spontaneous Localization Model of Hybrid Quantum-Classical Newtonian Gravity: Energy Increase and Experimental Bounds

arXiv3 min de cititArticolul și perspectiva sunt în engleză.

arXiv:2602.19377v2 Announce Type: replace Abstract: The Gravitational Poissonian Spontaneous Localization (GPSL) model is a hybrid classical-quantum framework in which Newtonian gravity emerges from stochastic collapses of a smeared mass-density operator. Consistency of the hybrid dynamics entails momentum diffusion and, hence, spontaneous heating. Without smearing, which enters both the collapse (measurement) and gravitational-feedback components of the dynamics, the heating rate would be divergent. Previous work assumed identical smearings for both components. Here, we treat the general case of distinct spatial smearings $g_{r_C} (\mathbf x)$ and $g_{r_G} (\mathbf x)$, characterized, respectively, by length scales $r_C$ and $r_G$. We characterize the spontaneous heating rate for arbitrary $g_{r_C} (\mathbf x)$ and $g_{r_G} (\mathbf x)$, and then discuss which smearing profiles minimize the spontaneous heating rate in relevant physical situations. Remarkably, there are situations in which, while the measurement noise remains the same, allowing $g_{r_G} (\mathbf x)\neq g_{r_C} (\mathbf x)$ may reduce the feedback-induced spontaneous heating by more than 60 orders of magnitude already for $r_G = 10 r_C$. Finally, we use our results to estimate the spontaneous heating rate of neutron stars and to set new lower bounds on the model's parameters by comparing the theoretical predictions with astronomical data on temperature, radius, and mass of neutron stars.

Abstract:The Gravitational Poissonian Spontaneous Localization (GPSL) model is a hybrid classical-quantum framework in which Newtonian gravity emerges from stochastic collapses of a smeared mass-density operator. Consistency of the hybrid dynamics entails momentum diffusion and, hence, spontaneous heating. Without smearing, which enters both the collapse (measurement) and gravitational-feedback components of the dynamics, the heating rate would be divergent. Previous work assumed identical smearings for both components. Here, we treat the general case of distinct spatial smearings $g_{r_C} (\mathbf x)$ and $g_{r_G} (\mathbf x)$, characterized, respectively, by length scales $r_C$ and $r_G$. We characterize the spontaneous heating rate for arbitrary $g_{r_C} (\mathbf x)$ and $g_{r_G} (\mathbf x)$, and then discuss which smearing profiles minimize the spontaneous heating rate in relevant physical situations. Remarkably, there are situations in which, while the measurement noise remains the same, allowing $g_{r_G} (\mathbf x)\neq g_{r_C} (\mathbf x)$ may reduce the feedback-induced spontaneous heating by more than 60 orders of magnitude already for $r_G = 10 r_C$. Finally, we use our results to estimate the spontaneous heating rate of neutron stars and to set new lower bounds on the model's parameters by comparing the theoretical predictions with astronomical data on temperature, radius, and mass of neutron stars.

13 pages plus appendices, 8 figures. Close to published version

arXiv:2602.19377 [quant-ph]

(or arXiv:2602.19377v2 [quant-ph] for this version)

https://doi.org/10.48550/arXiv.2602.19377 Focus to learn more arXiv-issued DOI via DataCite

Class. Quantum Grav. 43, 165005 (2026)

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