Localized qubits in curved spacetimes
Matthew C. Palmer, Maki Takahashi, Hans F. Westman

TL;DR
This paper develops a formalism for analyzing localized qubits, such as spin and polarization, in curved spacetimes, incorporating gravitational effects and quantum information concepts for potential precision measurements.
Contribution
It introduces a WKB-based approach to describe the unitary evolution of localized qubits in curved spacetime, including gravitational phases and multipartite quantum states.
Findings
Derived a relativistic description of gravitationally induced phases.
Modeled the gravitational shift in the COW experiment.
Extended the formalism to quantum information processes like entanglement.
Abstract
We provide a systematic and self-contained exposition of the subject of localized qubits in curved spacetimes. This research was motivated by a simple experimental question: if we move a spatially localized qubit, initially in a state |\psi_1>, along some spacetime path \Gamma from a spacetime point x_1 to another point x_2, what will the final quantum state |\psi_2> be at point x_2? This paper addresses this question for two physical realizations of the qubit: spin of a massive fermion and polarization of a photon. Our starting point is the Dirac and Maxwell equations that describe respectively the one-particle states of localized massive fermions and photons. In the WKB limit we show how one can isolate a two-dimensional quantum state which evolves unitarily along \Gamma. The quantum states for these two realizations are represented by a left-handed 2-spinor in the case of massive…
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