For two-dimensionally correlated quantum states, the quasiclassical geodesic proper time becomes non-quadratic in a correlation momentum, so the effective spacetime geometry is Finsler and time dilation depends on entropy and purity.
Quantum interferometric visibility as a witness of general relativistic proper time
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abstract
Current attempts to probe general relativistic effects in quantum mechanics focus on precision measurements of phase shifts in matter-wave interferometry. Yet, phase shifts can always be explained as arising due to an Aharonov-Bohm effect, where a particle in a flat space-time is subject to an effective potential. Here we propose a novel quantum effect that cannot be explained without the general relativistic notion of proper time. We consider interference of a "clock" - a particle with evolving internal degrees of freedom - that will not only display a phase shift, but also reduce the visibility of the interference pattern. According to general relativity proper time flows at different rates in different regions of space-time. Therefore, due to quantum complementarity the visibility will drop to the extent to which the path information becomes available from reading out the proper time from the "clock". Such a gravitationally induced decoherence would provide the first test of the genuine general relativistic notion of proper time in quantum mechanics.
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Relativistic implications of entropy and purity
For two-dimensionally correlated quantum states, the quasiclassical geodesic proper time becomes non-quadratic in a correlation momentum, so the effective spacetime geometry is Finsler and time dilation depends on entropy and purity.