Abstract
We revisit polarization rotation due to gravity, known as the gravitational Faraday effect, with a view on its role in quantum communications with Earth-orbiting satellites. In a static spherically symmetric gravitational field Faraday rotation is purely a reference frame (gauge) effect. This is so also in the leading post-Newtonian expansion of the Earth's gravitational field. However, establishing the local reference frame with respect to distant stars leads to the nonzero Faraday phase. In communications between a ground station and an Earth-orbiting spacecraft this phase is of the order of 10-10. Under the same conditions the Wigner phase of special relativity is typically of the order 10-4-10-5. These phases lead to the physical lower bound on communication errors. However, both types of errors can be simultaneously mitigated. Moreover, they are countered by a fully reference frame independent scheme that also handles arbitrary misalignments between the reference frames of sender and receiver.
Original language | English |
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Article number | 042610 |
Pages (from-to) | 042610-1- 042610-9 |
Number of pages | 9 |
Journal | Physical Review A: covering atomic, molecular, and optical physics and quantum information |
Volume | 104 |
Issue number | 4 |
DOIs | |
Publication status | Published - 28 Oct 2021 |
Bibliographical note
Copyright ©2021 American Physical Society. Firstly published in Physical Review A, 104(4), 042610. The original publication is available at https://doi.org/10.1103/PhysRevA.104.042610. Version archived for private and non-commercial use with the permission of the author/s and according to publisher conditions. For further rights please contact the publisher.Keywords
- Black-Hole