Horizon complementarity in elliptic de Sitter space

Lucas Hackl and Yasha Neiman
Phys. Rev. D 91, 044016 – Published 11 February 2015

Abstract

We study a quantum field in elliptic de Sitter space dS4/Z2—the spacetime obtained from identifying antipodal points in dS4. We find that the operator algebra and Hilbert space cannot be defined for the entire space, but only for observable causal patches. This makes the system into an explicit realization of the horizon complementarity principle. In the absence of a global quantum theory, we propose a recipe for translating operators and states between observers. This translation involves information loss, in accordance with the fact that two observers see different patches of the spacetime. As a check, we recover the thermal state at the de Sitter temperature as a state that appears the same to all observers. This thermal state arises from the same functional that, in ordinary dS4, describes the Bunch-Davies vacuum.

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  • Received 23 September 2014

DOI:https://doi.org/10.1103/PhysRevD.91.044016

© 2015 American Physical Society

Authors & Affiliations

Lucas Hackl1,* and Yasha Neiman2,†

  • 1Institute for Gravitation and the Cosmos and Physics Department, Penn State, University Park, Pennsylvania 16802, USA
  • 2Perimeter Institute for Theoretical Physics, 31 Caroline Street N, Waterloo, Ontario N2L 2Y5, Canada

  • *lucas.hackl@psu.edu
  • yashula@gmail.com

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Vol. 91, Iss. 4 — 15 February 2015

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