25–28 May 2026
Albano Building 3
Europe/Stockholm timezone

Gravitational self-interaction mitigates superluminal signalling

28 May 2026, 10:20
20m
Albano 3: 4204 - SU Conference Room (56 seats) (Albano Building 3)

Albano 3: 4204 - SU Conference Room (56 seats)

Albano Building 3

Hannes Alfvéns väg 12, 114 19 Stockholm
56

Speaker

Mrs Julia Osęka-Lenart (Astronomical Observatory, Jagiellonian University)

Description

The Schrödinger–Newton equation aims at describing the dynamics of massive quantum systems subject to the gravitational self-interaction. As a deterministic nonlinear quantum wave equation, it is generally believed to conflict with the relativistic no-signalling principle. Here I challenge this viewpoint and show that it is of a key importance to study the quantitative and operational character of the superluminal effects. To this end, a rigorous formalism of probability measures on spacetime was employed to quantify the probability of a successful superluminal bit transfer via the single-particle Schrödinger–Newton equation. Here it is demonstrated that such a quantity decreases with the increasing size and mass of the system. Furthermore, I prove that the Einstein–Dirac system, which yields the Schrödinger–Newton equation in the non-relativistic limit, is perfectly compatible with the relativistic causal structure. The presented study demonstrates that the Schrödinger–Newton equation, which is by construction non-relativistic, is in fact ‘more compatible’ with the no-signalling principle than the ordinary free Schrödinger equation.

Author

Mrs Julia Osęka-Lenart (Astronomical Observatory, Jagiellonian University)

Presentation materials

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