Abstract
We study unilateral coherence and coherence distribution in the background of a Schwarzschild black hole. We find that, comparing to the flat spacetime, two types of unilateral coherence corresponding to the measurements on system A and system B, respectively, are asymmetric for any Hawking temperature, and the accessible coherence of system B is bigger than the accessible coherence of system A in curved spacetime. We also find that the local coherence of system B reduces with the increase of Hawking temperature, while the local coherence of system A remains unchanged. Unlike behavior of quantum entanglement in curved spacetime, the remaining coherence (correlated coherence) increases with the increase of finitevalued Hawking temperature.
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This work is supported by the Key projects of science research in University of Anhui Province(GrantKJ2020A0695 and the Innovation Project of Excellent Talents Training in Anhui Province(2020zyrc153).
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Bao, R., Wang, Y. & Wu, SM. Unilateral Coherence and Coherence Distribution in Curved Spacetime. Int J Theor Phys 60, 3426–3434 (2021). https://doi.org/10.1007/s10773-021-04918-6
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DOI: https://doi.org/10.1007/s10773-021-04918-6