Two-Mode Harmonic Oscillator Model of Reissner-Nordström Black Hole
In this paper, we will assume that the Reissner-Nordström black hole can be dynamically expressed, at the classical level, in terms of a reduced phase space consisting of the physical observables and their canonical conjugates. More specifically, we propose that the phase space can be described by t...
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| Veröffentlicht in: | International journal of theoretical physics 2009-04, Vol.48 (4), p.994-1002 |
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| container_title | International journal of theoretical physics |
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| creator | Li, Chuan’an |
| description | In this paper, we will assume that the Reissner-Nordström black hole can be dynamically expressed, at the classical level, in terms of a reduced phase space consisting of the physical observables and their canonical conjugates. More specifically, we propose that the phase space can be described by the black hole’s mass and charge along with their respective conjugates. In this four-dimensional phase space we perform a couple of canonical transformations to obtain a two-mode harmonic oscillator model of Reissner-Nordström black hole. By adopting this model, the quantum spectrum and wave function of horizon area are presented. |
| doi_str_mv | 10.1007/s10773-008-9873-0 |
| format | Article |
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More specifically, we propose that the phase space can be described by the black hole’s mass and charge along with their respective conjugates. In this four-dimensional phase space we perform a couple of canonical transformations to obtain a two-mode harmonic oscillator model of Reissner-Nordström black hole. By adopting this model, the quantum spectrum and wave function of horizon area are presented.</description><identifier>ISSN: 0020-7748</identifier><identifier>EISSN: 1572-9575</identifier><identifier>DOI: 10.1007/s10773-008-9873-0</identifier><language>eng</language><publisher>Boston: Springer US</publisher><subject>Black holes ; Elementary Particles ; Mathematical and Computational Physics ; Physics ; Physics and Astronomy ; Quantum Field Theory ; Quantum Physics ; Theoretical</subject><ispartof>International journal of theoretical physics, 2009-04, Vol.48 (4), p.994-1002</ispartof><rights>Springer Science+Business Media, LLC 2008</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c321t-1fd3617d362087ae31d6dd228283c5959a1d581aa307c02fefb8583cd21e00c33</citedby><cites>FETCH-LOGICAL-c321t-1fd3617d362087ae31d6dd228283c5959a1d581aa307c02fefb8583cd21e00c33</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s10773-008-9873-0$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s10773-008-9873-0$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>314,777,781,27905,27906,41469,42538,51300</link.rule.ids></links><search><creatorcontrib>Li, Chuan’an</creatorcontrib><title>Two-Mode Harmonic Oscillator Model of Reissner-Nordström Black Hole</title><title>International journal of theoretical physics</title><addtitle>Int J Theor Phys</addtitle><description>In this paper, we will assume that the Reissner-Nordström black hole can be dynamically expressed, at the classical level, in terms of a reduced phase space consisting of the physical observables and their canonical conjugates. 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By adopting this model, the quantum spectrum and wave function of horizon area are presented.</description><subject>Black holes</subject><subject>Elementary Particles</subject><subject>Mathematical and Computational Physics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Field Theory</subject><subject>Quantum Physics</subject><subject>Theoretical</subject><issn>0020-7748</issn><issn>1572-9575</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2009</creationdate><recordtype>article</recordtype><recordid>eNp9kE1OwzAQhS0EEqVwAHZZsjGM7bp2llABRSpUQmVtGdtBKUlcPKkQt-EUHAAuhqOyZjE_0rw3mvkIOWVwzgDUBTJQSlAATUs9NHtkxKTitJRK7pMRAAeq1EQfkiPENQCUMNEjcr16j_Q--lDMbWpjV7tiia5uGtvHVAyDpojV9-djqBG7kOhDTB779PPVFleNda_FPDbhmBxUtsFw8lfH5OnmejWb08Xy9m52uaBOcNZTVnkxZSonDlrZIJifes-55lo4WcrSMi81s1aAcsCrUD1rmUeeswDghBiTs93eTYpv24C9aWt0IV_bhbhFw7jQQ0xklrKd1KWImEJlNqlubfowDMyAzOyQmYzMDMgMZA_feTBru5eQzDpuU5c_-sf0C0XMbs4</recordid><startdate>20090401</startdate><enddate>20090401</enddate><creator>Li, Chuan’an</creator><general>Springer US</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>20090401</creationdate><title>Two-Mode Harmonic Oscillator Model of Reissner-Nordström Black Hole</title><author>Li, Chuan’an</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c321t-1fd3617d362087ae31d6dd228283c5959a1d581aa307c02fefb8583cd21e00c33</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2009</creationdate><topic>Black holes</topic><topic>Elementary Particles</topic><topic>Mathematical and Computational Physics</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum Field Theory</topic><topic>Quantum Physics</topic><topic>Theoretical</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Li, Chuan’an</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><jtitle>International journal of theoretical physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Li, Chuan’an</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Two-Mode Harmonic Oscillator Model of Reissner-Nordström Black Hole</atitle><jtitle>International journal of theoretical physics</jtitle><stitle>Int J Theor Phys</stitle><date>2009-04-01</date><risdate>2009</risdate><volume>48</volume><issue>4</issue><spage>994</spage><epage>1002</epage><pages>994-1002</pages><issn>0020-7748</issn><eissn>1572-9575</eissn><abstract>In this paper, we will assume that the Reissner-Nordström black hole can be dynamically expressed, at the classical level, in terms of a reduced phase space consisting of the physical observables and their canonical conjugates. 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| subjects | Black holes Elementary Particles Mathematical and Computational Physics Physics Physics and Astronomy Quantum Field Theory Quantum Physics Theoretical |
| title | Two-Mode Harmonic Oscillator Model of Reissner-Nordström Black Hole |
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