Quasi-normal oscillations of a schwarzschild black hole
The modes of oscillation of a Schwarzschild black hole are determined within an analytic framework. These quasi-normal modes are related to the bound states of the inverted black hole potential which is approximated by the inverted Eckart potential. For a given angular momentum parameter j, the real...
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Veröffentlicht in: | Physics letters. A 1984-01, Vol.100 (5), p.231-234 |
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creator | Blome, Hans-Joachim Mashhoon, Bahram |
description | The modes of oscillation of a Schwarzschild black hole are determined within an analytic framework. These quasi-normal modes are related to the bound states of the inverted black hole potential which is approximated by the inverted Eckart potential. For a given angular momentum parameter
j, the real part of the quasi-normal frequency decreases as the mode number
n (or, equivalently, the damping factor) increases, in agreement with the results of numerical studies. |
doi_str_mv | 10.1016/0375-9601(84)90769-2 |
format | Article |
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j, the real part of the quasi-normal frequency decreases as the mode number
n (or, equivalently, the damping factor) increases, in agreement with the results of numerical studies.</description><identifier>ISSN: 0375-9601</identifier><identifier>EISSN: 1873-2429</identifier><identifier>DOI: 10.1016/0375-9601(84)90769-2</identifier><identifier>CODEN: PYLAAG</identifier><language>eng</language><publisher>Amsterdam: Elsevier B.V</publisher><subject>Classical general relativity ; Exact sciences and technology ; General relativity and gravitation ; Physics</subject><ispartof>Physics letters. A, 1984-01, Vol.100 (5), p.231-234</ispartof><rights>1984</rights><rights>1984 INIST-CNRS</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c364t-c27db40cc94749e559ed0699092412aca9f5e67d7cc695d04e01282fb77ddaf63</citedby><cites>FETCH-LOGICAL-c364t-c27db40cc94749e559ed0699092412aca9f5e67d7cc695d04e01282fb77ddaf63</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.sciencedirect.com/science/article/pii/0375960184907692$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>314,776,780,3537,27901,27902,65306</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=9600983$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>Blome, Hans-Joachim</creatorcontrib><creatorcontrib>Mashhoon, Bahram</creatorcontrib><title>Quasi-normal oscillations of a schwarzschild black hole</title><title>Physics letters. A</title><description>The modes of oscillation of a Schwarzschild black hole are determined within an analytic framework. These quasi-normal modes are related to the bound states of the inverted black hole potential which is approximated by the inverted Eckart potential. For a given angular momentum parameter
j, the real part of the quasi-normal frequency decreases as the mode number
n (or, equivalently, the damping factor) increases, in agreement with the results of numerical studies.</description><subject>Classical general relativity</subject><subject>Exact sciences and technology</subject><subject>General relativity and gravitation</subject><subject>Physics</subject><issn>0375-9601</issn><issn>1873-2429</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1984</creationdate><recordtype>article</recordtype><recordid>eNp9kE1LAzEQhoMoWKv_wMMeRPSwmmSzyc5FkOIXFETQc0gnWRrdbmqyVfTXm9ri0dNcnvedmYeQY0YvGGXyklaqLkFSdtaIc6BKQsl3yIg1qiq54LBLRn_IPjlI6ZXSnKMwIuppZZIv-xAXpitCQt91ZvChT0VoC1MknH-a-J2H72wx6wy-FfPQuUOy15ouuaPtHJOX25vnyX05fbx7mFxPS6ykGErkys4ERQShBLi6BmepBKDABeMGDbS1k8oqRAm1pcJRxhvezpSy1rSyGpPTTe8yhveVS4Ne-IQuH9m7sEqai0oCqyGDYgNiDClF1-pl9AsTvzSjem1JrxXotQLdCP1rSfMcO9n2m4Sma6Pp0ae_bMYpNFXGrjaYy79-eBd1NuV6dNZHh4O2wf-_5wfTr3qK</recordid><startdate>19840101</startdate><enddate>19840101</enddate><creator>Blome, Hans-Joachim</creator><creator>Mashhoon, Bahram</creator><general>Elsevier B.V</general><general>Elsevier Science</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>19840101</creationdate><title>Quasi-normal oscillations of a schwarzschild black hole</title><author>Blome, Hans-Joachim ; Mashhoon, Bahram</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c364t-c27db40cc94749e559ed0699092412aca9f5e67d7cc695d04e01282fb77ddaf63</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1984</creationdate><topic>Classical general relativity</topic><topic>Exact sciences and technology</topic><topic>General relativity and gravitation</topic><topic>Physics</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Blome, Hans-Joachim</creatorcontrib><creatorcontrib>Mashhoon, Bahram</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Physics letters. A</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Blome, Hans-Joachim</au><au>Mashhoon, Bahram</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Quasi-normal oscillations of a schwarzschild black hole</atitle><jtitle>Physics letters. A</jtitle><date>1984-01-01</date><risdate>1984</risdate><volume>100</volume><issue>5</issue><spage>231</spage><epage>234</epage><pages>231-234</pages><issn>0375-9601</issn><eissn>1873-2429</eissn><coden>PYLAAG</coden><abstract>The modes of oscillation of a Schwarzschild black hole are determined within an analytic framework. These quasi-normal modes are related to the bound states of the inverted black hole potential which is approximated by the inverted Eckart potential. For a given angular momentum parameter
j, the real part of the quasi-normal frequency decreases as the mode number
n (or, equivalently, the damping factor) increases, in agreement with the results of numerical studies.</abstract><cop>Amsterdam</cop><pub>Elsevier B.V</pub><doi>10.1016/0375-9601(84)90769-2</doi><tpages>4</tpages></addata></record> |
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subjects | Classical general relativity Exact sciences and technology General relativity and gravitation Physics |
title | Quasi-normal oscillations of a schwarzschild black hole |
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