V. P. Stefanov, D. S. Mogilevtsev, I. Yu. Rybak, A. Stefanov
Abstract
Here, we discuss an influence of an external weak gravitational field on the gravitational self-decoherence effect with help of the stochastic extension of regularized Shrödinger-Newton equation in a curved background. We derive the master equation and demonstrate that it leads to the experimentally verifiable conclusions about applicability of the classical description of the weak gravitation field. Namely, a presence of oscillating terms in the otherwise purely exponential decay of the coherence would indicate classicality of gravity for the case.
Keywords
Formal aspects of field theory / field theory in curved space
Physical Review D
Volume 111, Issue 065026, Page 11
2025 March
