MÖBIUS MIRRORS

dc.contributor.author	Good, Michael R R
dc.contributor.author	Linder, Eric V
dc.date.accessioned	2023-03-28T09:37:34Z
dc.date.available	2023-03-28T09:37:34Z
dc.date.issued	2022
dc.description.abstract	An accelerating boundary (mirror) acts as a horizon and black hole analog, radiating energy with some particle spectrum. We demonstrate that a Möbius transformation on the null coordinate advanced time mirror trajectory uniquely keeps invariant not only the energy flux but the particle spectrum. We clarify how the geometric entanglement entropy is also invariant. The transform allows generation of families of dynamically distinct trajectories, including $\mathcal{PT}$-symmetric ones, mapping from the eternally thermal mirror to the de Sitter horizon, and different boundary motions corresponding to Kerr or Schwarzschild black holes.	en_US
dc.identifier.citation	Good, M. F., & Linder, E. V. (2022). Möbius mirrors. Classical and Quantum Gravity, 39(10), 105003. https://doi.org/10.1088/1361-6382/ac60c3	en_US
dc.identifier.uri	http://nur.nu.edu.kz/handle/123456789/6987
dc.language.iso	en	en_US
dc.publisher	Classical and Quantum Gravity	en_US
dc.rights	Attribution-NonCommercial-ShareAlike 3.0 United States	*
dc.rights.uri	http://creativecommons.org/licenses/by-nc-sa/3.0/us/	*
dc.subject	Type of access: Open Access	en_US
dc.subject	moving mirrors	en_US
dc.subject	Hawking radiation	en_US
dc.subject	dynamical Casimir effect	en_US
dc.title	MÖBIUS MIRRORS	en_US
dc.type	Article	en_US
workflow.import.source	science

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