2014
DOI: 10.48550/arxiv.1412.0802
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n-partite information in Hawking radiation

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“…We remark that this regularized term is now finite at the limit ǫ → 0 or β → ∞. The regularized one-partite information I [1] = −∆S ′ div also becomes finite at limit M → ω. We compare the behavior of ( 2) and ( 14) in the Fig.…”
Section: Btz Black Hole and Finite Entanglement Entropymentioning
confidence: 81%
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“…We remark that this regularized term is now finite at the limit ǫ → 0 or β → ∞. The regularized one-partite information I [1] = −∆S ′ div also becomes finite at limit M → ω. We compare the behavior of ( 2) and ( 14) in the Fig.…”
Section: Btz Black Hole and Finite Entanglement Entropymentioning
confidence: 81%
“…The central charge c encodes the degrees of freedom in the field theory, while the constant of proportionality α could depend on species and spins of radiated particles [10]. These similarities between (2) and (4) as summarized in the Table I, have made us propose a (0 + 1)−dimensional quench model such that a massive radiated particle comes in sudden entangled with a black hole of mass M would carry the entanglement entropy S E ∼ ln(M/m p ) at late time [1]. In fact, the entropy difference (3) agrees with the definition of one-partite information in our quench model and the two-partite information are closely related to the definition of mutual information in the Parikh-Wilczek tunneling model [11][12][13].…”
Section: Introductionmentioning
confidence: 88%
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