Thermonuclear Supernovae: Simulations of the Deflagration Stage and Their Implications
Large-scale, three-dimensional numerical simulations of the deflagration stage of a thermonuclear supernova explosion show the formation and evolution of a highly convoluted turbulent flame in the gravitational field of an expanding carbon-oxygen white dwarf. The flame dynamics are dominated by the...
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| Veröffentlicht in: | Science (American Association for the Advancement of Science) 2003-01, Vol.299 (5603), p.77-81 |
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| container_title | Science (American Association for the Advancement of Science) |
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| creator | Gamezo, Vadim N. Khokhlov, Alexei M. Oran, Elaine S. Chtchelkanova, Almadena Y. Rosenberg, Robert O. |
| description | Large-scale, three-dimensional numerical simulations of the deflagration stage of a thermonuclear supernova explosion show the formation and evolution of a highly convoluted turbulent flame in the gravitational field of an expanding carbon-oxygen white dwarf. The flame dynamics are dominated by the gravity-induced Rayleigh-Taylor instability that controls the burning rate. The thermonuclear deflagration releases enough energy to produce a healthy explosion. The turbulent flame, however, leaves large amounts of unbumed and partially burned material near the star center, whereas observations that imply these materials are present only in outer layers. This disagreement could be resolved if the deflagration triggers a detonation. |
| doi_str_mv | 10.1126/science.1078129 |
| format | Article |
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The flame dynamics are dominated by the gravity-induced Rayleigh-Taylor instability that controls the burning rate. The thermonuclear deflagration releases enough energy to produce a healthy explosion. The turbulent flame, however, leaves large amounts of unbumed and partially burned material near the star center, whereas observations that imply these materials are present only in outer layers. This disagreement could be resolved if the deflagration triggers a detonation.</description><identifier>ISSN: 0036-8075</identifier><identifier>EISSN: 1095-9203</identifier><identifier>DOI: 10.1126/science.1078129</identifier><identifier>PMID: 12446871</identifier><identifier>CODEN: SCIEAS</identifier><language>eng</language><publisher>Washington, DC: American Association for the Advancement of Science</publisher><subject>Astronomy ; Astrophysics ; Climate ; Deflagration ; Earth, ocean, space ; Elementary particle and nuclear processes ; Energy ; Exact sciences and technology ; Flame propagation ; Flames ; Fundamental aspects of astrophysics ; Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations ; Kinetics ; Late stages of stellar evolution (including black holes) ; Observations ; Physics ; Plumes ; Runaways ; Stars ; Stellar characteristics and properties ; Stellar structure, interiors, evolution, nucleosynthesis, ages ; Supernovae ; Supernovas ; Three dimensional modeling ; Turbulence ; Turbulent flames</subject><ispartof>Science (American Association for the Advancement of Science), 2003-01, Vol.299 (5603), p.77-81</ispartof><rights>Copyright 2003 American Association for the Advancement of Science</rights><rights>2003 INIST-CNRS</rights><rights>COPYRIGHT 2003 American Association for the Advancement of Science</rights><rights>COPYRIGHT 2003 American Association for the Advancement of Science</rights><rights>Copyright American Association for the Advancement of Science Jan 3, 2003</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c737t-5f2f8f774dc30adca2d11e4a97ac82d03b886d3a495be93f21a9f1ce3ee584833</citedby><cites>FETCH-LOGICAL-c737t-5f2f8f774dc30adca2d11e4a97ac82d03b886d3a495be93f21a9f1ce3ee584833</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://www.jstor.org/stable/pdf/3833228$$EPDF$$P50$$Gjstor$$H</linktopdf><linktohtml>$$Uhttps://www.jstor.org/stable/3833228$$EHTML$$P50$$Gjstor$$H</linktohtml><link.rule.ids>314,776,780,799,2871,2872,27901,27902,57992,58225</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=14468097$$DView record in Pascal Francis$$Hfree_for_read</backlink><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/12446871$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink></links><search><creatorcontrib>Gamezo, Vadim N.</creatorcontrib><creatorcontrib>Khokhlov, Alexei M.</creatorcontrib><creatorcontrib>Oran, Elaine S.</creatorcontrib><creatorcontrib>Chtchelkanova, Almadena Y.</creatorcontrib><creatorcontrib>Rosenberg, Robert O.</creatorcontrib><title>Thermonuclear Supernovae: Simulations of the Deflagration Stage and Their Implications</title><title>Science (American Association for the Advancement of Science)</title><addtitle>Science</addtitle><description>Large-scale, three-dimensional numerical simulations of the deflagration stage of a thermonuclear supernova explosion show the formation and evolution of a highly convoluted turbulent flame in the gravitational field of an expanding carbon-oxygen white dwarf. The flame dynamics are dominated by the gravity-induced Rayleigh-Taylor instability that controls the burning rate. The thermonuclear deflagration releases enough energy to produce a healthy explosion. The turbulent flame, however, leaves large amounts of unbumed and partially burned material near the star center, whereas observations that imply these materials are present only in outer layers. This disagreement could be resolved if the deflagration triggers a detonation.</description><subject>Astronomy</subject><subject>Astrophysics</subject><subject>Climate</subject><subject>Deflagration</subject><subject>Earth, ocean, space</subject><subject>Elementary particle and nuclear processes</subject><subject>Energy</subject><subject>Exact sciences and technology</subject><subject>Flame propagation</subject><subject>Flames</subject><subject>Fundamental aspects of astrophysics</subject><subject>Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations</subject><subject>Kinetics</subject><subject>Late stages of stellar evolution (including black holes)</subject><subject>Observations</subject><subject>Physics</subject><subject>Plumes</subject><subject>Runaways</subject><subject>Stars</subject><subject>Stellar characteristics and properties</subject><subject>Stellar structure, interiors, evolution, nucleosynthesis, ages</subject><subject>Supernovae</subject><subject>Supernovas</subject><subject>Three dimensional modeling</subject><subject>Turbulence</subject><subject>Turbulent flames</subject><issn>0036-8075</issn><issn>1095-9203</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2003</creationdate><recordtype>article</recordtype><sourceid>8G5</sourceid><sourceid>BEC</sourceid><sourceid>BENPR</sourceid><sourceid>GUQSH</sourceid><sourceid>M2O</sourceid><recordid>eNqN082LEzEUAPBBFLeunr2IDILiYWc3H_OReFur1kKxh657DWnmZTYlM6nJjOh_b2oHl0phSw6BvN97h7z3kuQlRpcYk_IqKAOdgkuMKoYJf5RMMOJFxgmij5MJQrTMGKqKs-RZCBuEYozTp8kZJnlesgpPktubO_Ct6wZlQfp0NWzBd-6nhA_pyrSDlb1xXUidTvs7SD-BtrLxfx_TVS8bSGVXp7GG8em83Vqj9gnPkyda2gAvxvs8-f7l8830a7ZYzubT60WmKlr1WaGJZrqq8lpRJGslSY0x5JJXUjFSI7pmrKypzHmxBk41wZJrrIACFCxnlJ4n7_Z1t979GCD0ojVBgbWyAzcEURGe4xI_DAlDOeGEnQRRjvmDELOyYAUrI3zzH9y4wXfxWwTBtOCEl1VEF3vUSAvCdNr1XqoGOvDSug60ic_XvCx5WWAUeXaEx1NDa9Qx__7AR9LDr76RQwhivvp2Ml3enkw_zk6lbLY4oBfHqHLWQgMizs90ecCv9lx5F4IHLbbetNL_FhiJ3ZKIcUnEuCQx4_XYkGHdQn3vx62I4O0IZFDSai87ZcK92zHEd017tXeb0Dv_L07jYJI4Sn8AAA4fcA</recordid><startdate>20030103</startdate><enddate>20030103</enddate><creator>Gamezo, Vadim N.</creator><creator>Khokhlov, Alexei M.</creator><creator>Oran, Elaine S.</creator><creator>Chtchelkanova, Almadena Y.</creator><creator>Rosenberg, Robert O.</creator><general>American Association for the Advancement of Science</general><general>The American Association for the Advancement of Science</general><scope>IQODW</scope><scope>NPM</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>8GL</scope><scope>IBG</scope><scope>IOV</scope><scope>ISN</scope><scope>0-V</scope><scope>3V.</scope><scope>7QF</scope><scope>7QG</scope><scope>7QL</scope><scope>7QP</scope><scope>7QQ</scope><scope>7QR</scope><scope>7SC</scope><scope>7SE</scope><scope>7SN</scope><scope>7SP</scope><scope>7SR</scope><scope>7SS</scope><scope>7T7</scope><scope>7TA</scope><scope>7TB</scope><scope>7TK</scope><scope>7TM</scope><scope>7U5</scope><scope>7U9</scope><scope>7X2</scope><scope>7X7</scope><scope>7XB</scope><scope>88A</scope><scope>88B</scope><scope>88E</scope><scope>88I</scope><scope>8AF</scope><scope>8BQ</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FH</scope><scope>8FI</scope><scope>8FJ</scope><scope>8FK</scope><scope>8G5</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>ALSLI</scope><scope>ARAPS</scope><scope>ATCPS</scope><scope>AZQEC</scope><scope>BBNVY</scope><scope>BEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>C1K</scope><scope>CCPQU</scope><scope>CJNVE</scope><scope>D1I</scope><scope>DWQXO</scope><scope>F28</scope><scope>FR3</scope><scope>FYUFA</scope><scope>GHDGH</scope><scope>GNUQQ</scope><scope>GUQSH</scope><scope>H8D</scope><scope>H8G</scope><scope>H94</scope><scope>HCIFZ</scope><scope>JG9</scope><scope>JQ2</scope><scope>K9-</scope><scope>K9.</scope><scope>KB.</scope><scope>KR7</scope><scope>L6V</scope><scope>L7M</scope><scope>LK8</scope><scope>L~C</scope><scope>L~D</scope><scope>M0K</scope><scope>M0P</scope><scope>M0R</scope><scope>M0S</scope><scope>M1P</scope><scope>M2O</scope><scope>M2P</scope><scope>M7N</scope><scope>M7P</scope><scope>M7S</scope><scope>MBDVC</scope><scope>P5Z</scope><scope>P62</scope><scope>P64</scope><scope>PATMY</scope><scope>PCBAR</scope><scope>PDBOC</scope><scope>PQEDU</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>PYCSY</scope><scope>Q9U</scope><scope>R05</scope><scope>RC3</scope><scope>7TG</scope><scope>KL.</scope><scope>7X8</scope></search><sort><creationdate>20030103</creationdate><title>Thermonuclear Supernovae: Simulations of the Deflagration Stage and Their Implications</title><author>Gamezo, Vadim N. ; 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| ispartof | Science (American Association for the Advancement of Science), 2003-01, Vol.299 (5603), p.77-81 |
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| source | American Association for the Advancement of Science; Jstor Complete Legacy |
| subjects | Astronomy Astrophysics Climate Deflagration Earth, ocean, space Elementary particle and nuclear processes Energy Exact sciences and technology Flame propagation Flames Fundamental aspects of astrophysics Fundamental astronomy and astrophysics. Instrumentation, techniques, and astronomical observations Kinetics Late stages of stellar evolution (including black holes) Observations Physics Plumes Runaways Stars Stellar characteristics and properties Stellar structure, interiors, evolution, nucleosynthesis, ages Supernovae Supernovas Three dimensional modeling Turbulence Turbulent flames |
| title | Thermonuclear Supernovae: Simulations of the Deflagration Stage and Their Implications |
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