Non-relativistic limit of scalar and Dirac fields in curved spacetime
arXiv:2210.02405 · doi:10.1103/PhysRevD.107.045012
Abstract
We give from first principles the non-relativistic limit of scalar and Dirac fields in curved spacetime. We aim to find general relativistic corrections to the quantum theory of particles affected by Newtonian gravity, a regime nowadays experimentally accessible. We believe that the ever-improving measurement accuracy and the theoretical interest in finding general relativistic effects in quantum systems require the introduction of corrections to the Schrödinger-Newtonian theory. We rigorously determine these corrections by the non-relativistic limit of fully relativistic quantum theories in curved spacetime. For curved static spacetimes, we show how a non-inertial observer (equivalently, an observer in the presence of a gravitational field) can distinguish a scalar field from a Dirac field by particle-gravity interaction. We study the Rindler spacetime and discuss the difference between the resulting non-relativistic Hamiltonians. We find that for sufficiently large acceleration, the gravity-spin coupling dominates over the corrections for scalar fields, promoting Dirac particles as the best candidates for observing non-Newtonian gravity in quantum particle phenomenology.
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Cited by in corpus (5)
- Minkowski vacuum in Rindler spacetime and Unruh thermal state for Dirac fields
- Frame-dependence of the non-relativistic limit of quantum fields
- Limits to the observation of the Unruh radiation via first-quantized hydrogen-like atoms
- Bound-state solutions for the charged Dirac oscillator in a rotating frame in the Bonnor-Melvin-Lambda spacetime
- Localization in Quantum Field Theory for inertial and accelerated observers