Information conservation in de Sitter tunneling
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-Nordstr\"{o}m de Sitter black hole (the most general case of a static black hole), the Kerr-Newman-Kasuya de Sitter black...
Gespeichert in:
| 1. Verfasser: | |
|---|---|
| Format: | Artikel |
| Sprache: | eng |
| Schlagworte: | |
| Online-Zugang: | Volltext bestellen |
| Tags: |
Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
|
| container_end_page | |
|---|---|
| container_issue | |
| container_start_page | |
| container_title | |
| container_volume | |
| creator | Tan, Baoyu |
| description | 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-Nordstr\"{o}m 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. |
| doi_str_mv | 10.48550/arxiv.2409.03653 |
| format | Article |
| fullrecord | <record><control><sourceid>arxiv_GOX</sourceid><recordid>TN_cdi_arxiv_primary_2409_03653</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2409_03653</sourcerecordid><originalsourceid>FETCH-arxiv_primary_2409_036533</originalsourceid><addsrcrecordid>eNpjYJA0NNAzsTA1NdBPLKrILNMzMjGw1DMwNjM15mTQ98xLyy_KTSzJzM9TSM7PK04tKoNwMvMUUlIVgjNLSlKLFEpK8_JSczLz0nkYWNMSc4pTeaE0N4O8m2uIs4cu2Oj4gqLM3MSiyniQFfFgK4wJqwAATvEw8w</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype></control><display><type>article</type><title>Information conservation in de Sitter tunneling</title><source>arXiv.org</source><creator>Tan, Baoyu</creator><creatorcontrib>Tan, Baoyu</creatorcontrib><description>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-Nordstr\"{o}m 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.</description><identifier>DOI: 10.48550/arxiv.2409.03653</identifier><language>eng</language><subject>Physics - General Relativity and Quantum Cosmology</subject><creationdate>2024-09</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,776,881</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2409.03653$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2409.03653$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Tan, Baoyu</creatorcontrib><title>Information conservation in de Sitter tunneling</title><description>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-Nordstr\"{o}m 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.</description><subject>Physics - General Relativity and Quantum Cosmology</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNpjYJA0NNAzsTA1NdBPLKrILNMzMjGw1DMwNjM15mTQ98xLyy_KTSzJzM9TSM7PK04tKoNwMvMUUlIVgjNLSlKLFEpK8_JSczLz0nkYWNMSc4pTeaE0N4O8m2uIs4cu2Oj4gqLM3MSiyniQFfFgK4wJqwAATvEw8w</recordid><startdate>20240905</startdate><enddate>20240905</enddate><creator>Tan, Baoyu</creator><scope>GOX</scope></search><sort><creationdate>20240905</creationdate><title>Information conservation in de Sitter tunneling</title><author>Tan, Baoyu</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-arxiv_primary_2409_036533</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Physics - General Relativity and Quantum Cosmology</topic><toplevel>online_resources</toplevel><creatorcontrib>Tan, Baoyu</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Tan, Baoyu</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Information conservation in de Sitter tunneling</atitle><date>2024-09-05</date><risdate>2024</risdate><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-Nordstr\"{o}m 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.</abstract><doi>10.48550/arxiv.2409.03653</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | DOI: 10.48550/arxiv.2409.03653 |
| ispartof | |
| issn | |
| language | eng |
| recordid | cdi_arxiv_primary_2409_03653 |
| source | arXiv.org |
| subjects | Physics - General Relativity and Quantum Cosmology |
| title | Information conservation in de Sitter tunneling |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-25T11%3A30%3A33IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-arxiv_GOX&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Information%20conservation%20in%20de%20Sitter%20tunneling&rft.au=Tan,%20Baoyu&rft.date=2024-09-05&rft_id=info:doi/10.48550/arxiv.2409.03653&rft_dat=%3Carxiv_GOX%3E2409_03653%3C/arxiv_GOX%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |