Information conservation in de Sitter tunneling

Abstract In this paper, we consider the three most general cases of progressive de Sitter spacetime. The charged and magnetic particles tunnel into the magnetically charged Reissner–Nordström de Sitter black hole (the most general case of a static black hole), the Kerr–Newman–Kasuya de Sitter black...

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Main Author: Baoyu Tan
Format: Article
Language:English
Published: SpringerOpen 2025-04-01
Series:European Physical Journal C: Particles and Fields
Online Access:https://doi.org/10.1140/epjc/s10052-025-14101-4
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author Baoyu Tan
author_facet Baoyu Tan
author_sort Baoyu Tan
collection DOAJ
description Abstract In this paper, we consider the three most general cases of progressive de Sitter spacetime. The charged and magnetic particles tunnel into the magnetically charged Reissner–Nordström de Sitter black hole (the most general case of a static black hole), the Kerr–Newman–Kasuya de Sitter black hole (the most general case of a rotating black hole), and Bardeen de Sitter black hole (black hole without singularities). We use Parikh–Wilczek method to calculate the radiation spectra of these black holes respectively, and find that they deviate from the pure thermal spectra, satisfying the unitary principle. Our results support the conservation of information and are generally true for all asymptotic de Sitter space-times.
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issn 1434-6052
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publishDate 2025-04-01
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series European Physical Journal C: Particles and Fields
spelling doaj-art-a0187dff86644a52bde07a57978385112025-08-20T03:04:53ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60522025-04-0185411910.1140/epjc/s10052-025-14101-4Information conservation in de Sitter tunnelingBaoyu Tan0College of Mathematics and Physics, Beijing University of Chemical TechnologyAbstract In this paper, we consider the three most general cases of progressive de Sitter spacetime. The charged and magnetic particles tunnel into the magnetically charged Reissner–Nordström de Sitter black hole (the most general case of a static black hole), the Kerr–Newman–Kasuya de Sitter black hole (the most general case of a rotating black hole), and Bardeen de Sitter black hole (black hole without singularities). We use Parikh–Wilczek method to calculate the radiation spectra of these black holes respectively, and find that they deviate from the pure thermal spectra, satisfying the unitary principle. Our results support the conservation of information and are generally true for all asymptotic de Sitter space-times.https://doi.org/10.1140/epjc/s10052-025-14101-4
spellingShingle Baoyu Tan
Information conservation in de Sitter tunneling
European Physical Journal C: Particles and Fields
title Information conservation in de Sitter tunneling
title_full Information conservation in de Sitter tunneling
title_fullStr Information conservation in de Sitter tunneling
title_full_unstemmed Information conservation in de Sitter tunneling
title_short Information conservation in de Sitter tunneling
title_sort information conservation in de sitter tunneling
url https://doi.org/10.1140/epjc/s10052-025-14101-4
work_keys_str_mv AT baoyutan informationconservationindesittertunneling