Decoupling and non-decoupling dynamics of large D black holes
A bstract The limit of large number of dimensions localizes the gravitational field of a black hole in a well-defined region near the horizon. The perturbative dynamics of the black hole can then be characterized in terms of states in the near-horizon geometry. We investigate this by computing the s...
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| Veröffentlicht in: | The journal of high energy physics 2014-07, Vol.2014 (7), p.1, Article 113 |
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| container_title | The journal of high energy physics |
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| creator | Emparan, Roberto Suzuki, Ryotaku Tanabe, Kentaro |
| description | A
bstract
The limit of large number of dimensions localizes the gravitational field of a black hole in a well-defined region near the horizon. The perturbative dynamics of the black hole can then be characterized in terms of states in the near-horizon geometry. We investigate this by computing the spectrum of quasinormal modes of the Schwarzschild black hole in the 1
/D
expansion, which we find splits into two classes. Most modes are
non-decoupled modes
: non-normalizable states of the near-horizon geometry that straddle between the near-horizon zone and the asymptotic zone. They have frequency of order
D/r
0
(with
r
0
the horizon radius), and are also present in a large class of other black holes. There also exist a much smaller number of
decoupled modes
: normalizable states of the near-horizon geometry that are strongly suppressed in the asymptotic region. They have frequency of order 1
/r
0
, and are specific of each black hole. Our results for their frequencies are in excellent agreement with numerical calculations, in some cases even in
D
= 4. |
| doi_str_mv | 10.1007/JHEP07(2014)113 |
| format | Article |
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bstract
The limit of large number of dimensions localizes the gravitational field of a black hole in a well-defined region near the horizon. The perturbative dynamics of the black hole can then be characterized in terms of states in the near-horizon geometry. We investigate this by computing the spectrum of quasinormal modes of the Schwarzschild black hole in the 1
/D
expansion, which we find splits into two classes. Most modes are
non-decoupled modes
: non-normalizable states of the near-horizon geometry that straddle between the near-horizon zone and the asymptotic zone. They have frequency of order
D/r
0
(with
r
0
the horizon radius), and are also present in a large class of other black holes. There also exist a much smaller number of
decoupled modes
: normalizable states of the near-horizon geometry that are strongly suppressed in the asymptotic region. They have frequency of order 1
/r
0
, and are specific of each black hole. Our results for their frequencies are in excellent agreement with numerical calculations, in some cases even in
D
= 4.</description><identifier>ISSN: 1029-8479</identifier><identifier>EISSN: 1029-8479</identifier><identifier>DOI: 10.1007/JHEP07(2014)113</identifier><language>eng</language><publisher>Berlin/Heidelberg: Springer Berlin Heidelberg</publisher><subject>Black holes ; Classical and Quantum Gravitation ; Elementary Particles ; High energy physics ; Physics ; Physics and Astronomy ; Quantum Field Theories ; Quantum Field Theory ; Quantum Physics ; Relativity Theory ; String Theory</subject><ispartof>The journal of high energy physics, 2014-07, Vol.2014 (7), p.1, Article 113</ispartof><rights>The Author(s) 2014</rights><rights>SISSA, Trieste, Italy 2014</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c417t-4511269ca22e0fa2e77e32e8af8052141ebd265d43ee6fdf607ebf59228ea2bb3</citedby><cites>FETCH-LOGICAL-c417t-4511269ca22e0fa2e77e32e8af8052141ebd265d43ee6fdf607ebf59228ea2bb3</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/JHEP07(2014)113$$EPDF$$P50$$Gspringer$$Hfree_for_read</linktopdf><linktohtml>$$Uhttps://doi.org/10.1007/JHEP07(2014)113$$EHTML$$P50$$Gspringer$$Hfree_for_read</linktohtml><link.rule.ids>314,780,784,864,27924,27925,41120,42189,51576</link.rule.ids></links><search><creatorcontrib>Emparan, Roberto</creatorcontrib><creatorcontrib>Suzuki, Ryotaku</creatorcontrib><creatorcontrib>Tanabe, Kentaro</creatorcontrib><title>Decoupling and non-decoupling dynamics of large D black holes</title><title>The journal of high energy physics</title><addtitle>J. High Energ. Phys</addtitle><description>A
bstract
The limit of large number of dimensions localizes the gravitational field of a black hole in a well-defined region near the horizon. The perturbative dynamics of the black hole can then be characterized in terms of states in the near-horizon geometry. We investigate this by computing the spectrum of quasinormal modes of the Schwarzschild black hole in the 1
/D
expansion, which we find splits into two classes. Most modes are
non-decoupled modes
: non-normalizable states of the near-horizon geometry that straddle between the near-horizon zone and the asymptotic zone. They have frequency of order
D/r
0
(with
r
0
the horizon radius), and are also present in a large class of other black holes. There also exist a much smaller number of
decoupled modes
: normalizable states of the near-horizon geometry that are strongly suppressed in the asymptotic region. They have frequency of order 1
/r
0
, and are specific of each black hole. Our results for their frequencies are in excellent agreement with numerical calculations, in some cases even in
D
= 4.</description><subject>Black holes</subject><subject>Classical and Quantum Gravitation</subject><subject>Elementary Particles</subject><subject>High energy physics</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Field Theories</subject><subject>Quantum Field Theory</subject><subject>Quantum Physics</subject><subject>Relativity Theory</subject><subject>String Theory</subject><issn>1029-8479</issn><issn>1029-8479</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2014</creationdate><recordtype>article</recordtype><sourceid>C6C</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNp1kL1PwzAQxS0EEqUws1pigSH0znHiZGBAbflSJRhgtpzkXFpSu9jt0P-eVEGiC9OdTu-90_sxdolwiwBq9PI0fQN1LQDlDWJ6xAYIokwKqcrjg_2UncW4BMAMSxiwuwnVfrtuF27OjWu48y5p_k7NzpnVoo7cW96aMCc-4VVr6i_-6VuK5-zEmjbSxe8cso-H6fv4KZm9Pj6P72dJLVFtEpkhirysjRAE1ghSilJBhbEFZAIlUtWIPGtkSpTbxuagqLJZKURBRlRVOmRXfe46-O8txY1e-m1w3UuNCoqujMplpxr1qjr4GANZvQ6LlQk7jaD3jHTPSO8Z6Y5R54DeETulm1M4yP3H8gO6z2ew</recordid><startdate>20140701</startdate><enddate>20140701</enddate><creator>Emparan, Roberto</creator><creator>Suzuki, Ryotaku</creator><creator>Tanabe, Kentaro</creator><general>Springer Berlin Heidelberg</general><general>Springer Nature B.V</general><scope>C6C</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FE</scope><scope>8FG</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>P5Z</scope><scope>P62</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope></search><sort><creationdate>20140701</creationdate><title>Decoupling and non-decoupling dynamics of large D black holes</title><author>Emparan, Roberto ; Suzuki, Ryotaku ; Tanabe, Kentaro</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c417t-4511269ca22e0fa2e77e32e8af8052141ebd265d43ee6fdf607ebf59228ea2bb3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2014</creationdate><topic>Black holes</topic><topic>Classical and Quantum Gravitation</topic><topic>Elementary Particles</topic><topic>High energy physics</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum Field Theories</topic><topic>Quantum Field Theory</topic><topic>Quantum Physics</topic><topic>Relativity Theory</topic><topic>String Theory</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Emparan, Roberto</creatorcontrib><creatorcontrib>Suzuki, Ryotaku</creatorcontrib><creatorcontrib>Tanabe, Kentaro</creatorcontrib><collection>Springer_OA刊</collection><collection>CrossRef</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies & Aerospace Collection</collection><collection>ProQuest Central Essentials</collection><collection>AUTh Library subscriptions: ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest advanced technologies & aerospace journals</collection><collection>ProQuest Advanced Technologies & Aerospace Collection</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><jtitle>The journal of high energy physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Emparan, Roberto</au><au>Suzuki, Ryotaku</au><au>Tanabe, Kentaro</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Decoupling and non-decoupling dynamics of large D black holes</atitle><jtitle>The journal of high energy physics</jtitle><stitle>J. High Energ. Phys</stitle><date>2014-07-01</date><risdate>2014</risdate><volume>2014</volume><issue>7</issue><spage>1</spage><pages>1-</pages><artnum>113</artnum><issn>1029-8479</issn><eissn>1029-8479</eissn><abstract>A
bstract
The limit of large number of dimensions localizes the gravitational field of a black hole in a well-defined region near the horizon. The perturbative dynamics of the black hole can then be characterized in terms of states in the near-horizon geometry. We investigate this by computing the spectrum of quasinormal modes of the Schwarzschild black hole in the 1
/D
expansion, which we find splits into two classes. Most modes are
non-decoupled modes
: non-normalizable states of the near-horizon geometry that straddle between the near-horizon zone and the asymptotic zone. They have frequency of order
D/r
0
(with
r
0
the horizon radius), and are also present in a large class of other black holes. There also exist a much smaller number of
decoupled modes
: normalizable states of the near-horizon geometry that are strongly suppressed in the asymptotic region. They have frequency of order 1
/r
0
, and are specific of each black hole. Our results for their frequencies are in excellent agreement with numerical calculations, in some cases even in
D
= 4.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1007/JHEP07(2014)113</doi><oa>free_for_read</oa></addata></record> |
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| source | Springer_OA刊; DOAJ Directory of Open Access Journals; Free E-Journal (出版社公開部分のみ）; Alma/SFX Local Collection |
| subjects | Black holes Classical and Quantum Gravitation Elementary Particles High energy physics Physics Physics and Astronomy Quantum Field Theories Quantum Field Theory Quantum Physics Relativity Theory String Theory |
| title | Decoupling and non-decoupling dynamics of large D black holes |
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