Helium bubble bursting in tungsten
Molecular dynamics simulations have been used to systematically study the pressure evolution and bursting behavior of sub-surface helium bubbles and the resulting tungsten surface morphology. This study specifically investigates how bubble shape and size, temperature, tungsten surface orientation, a...
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Veröffentlicht in: | Journal of applied physics 2013-12, Vol.114 (24) |
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creator | Sefta, Faiza Juslin, Niklas Wirth, Brian D. |
description | Molecular dynamics simulations have been used to systematically study the pressure evolution and bursting behavior of sub-surface helium bubbles and the resulting tungsten surface morphology. This study specifically investigates how bubble shape and size, temperature, tungsten surface orientation, and ligament thickness above the bubble influence bubble stability and surface evolution. The tungsten surface is roughened by a combination of adatom “islands,” craters, and pinholes. The present study provides insight into the mechanisms and conditions leading to various tungsten topology changes, which we believe are the initial stages of surface evolution leading to the formation of nanoscale fuzz. |
doi_str_mv | 10.1063/1.4860315 |
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This study specifically investigates how bubble shape and size, temperature, tungsten surface orientation, and ligament thickness above the bubble influence bubble stability and surface evolution. The tungsten surface is roughened by a combination of adatom “islands,” craters, and pinholes. The present study provides insight into the mechanisms and conditions leading to various tungsten topology changes, which we believe are the initial stages of surface evolution leading to the formation of nanoscale fuzz.</description><identifier>ISSN: 0021-8979</identifier><identifier>EISSN: 1089-7550</identifier><identifier>DOI: 10.1063/1.4860315</identifier><language>eng</language><publisher>Melville: American Institute of Physics</publisher><subject>Adatoms ; Applied physics ; BUBBLES ; Bursting ; CRATERS ; Evolution ; HELIUM ; Molecular dynamics ; MOLECULAR DYNAMICS METHOD ; MORPHOLOGY ; NANOSCIENCE AND NANOTECHNOLOGY ; NANOSTRUCTURES ; ORIENTATION ; Pinholes ; Surface stability ; THICKNESS ; TUNGSTEN</subject><ispartof>Journal of applied physics, 2013-12, Vol.114 (24)</ispartof><rights>2013 AIP Publishing LLC.</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c384t-c1096cfb5c60b6e0bd9dcaff7f4d21fda46908a76fa1153fde16c3a7a6194e53</citedby><cites>FETCH-LOGICAL-c384t-c1096cfb5c60b6e0bd9dcaff7f4d21fda46908a76fa1153fde16c3a7a6194e53</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,315,782,786,887,27933,27934</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/22267761$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Sefta, Faiza</creatorcontrib><creatorcontrib>Juslin, Niklas</creatorcontrib><creatorcontrib>Wirth, Brian D.</creatorcontrib><title>Helium bubble bursting in tungsten</title><title>Journal of applied physics</title><description>Molecular dynamics simulations have been used to systematically study the pressure evolution and bursting behavior of sub-surface helium bubbles and the resulting tungsten surface morphology. This study specifically investigates how bubble shape and size, temperature, tungsten surface orientation, and ligament thickness above the bubble influence bubble stability and surface evolution. The tungsten surface is roughened by a combination of adatom “islands,” craters, and pinholes. The present study provides insight into the mechanisms and conditions leading to various tungsten topology changes, which we believe are the initial stages of surface evolution leading to the formation of nanoscale fuzz.</description><subject>Adatoms</subject><subject>Applied physics</subject><subject>BUBBLES</subject><subject>Bursting</subject><subject>CRATERS</subject><subject>Evolution</subject><subject>HELIUM</subject><subject>Molecular dynamics</subject><subject>MOLECULAR DYNAMICS METHOD</subject><subject>MORPHOLOGY</subject><subject>NANOSCIENCE AND NANOTECHNOLOGY</subject><subject>NANOSTRUCTURES</subject><subject>ORIENTATION</subject><subject>Pinholes</subject><subject>Surface stability</subject><subject>THICKNESS</subject><subject>TUNGSTEN</subject><issn>0021-8979</issn><issn>1089-7550</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2013</creationdate><recordtype>article</recordtype><recordid>eNpFkL1OwzAYRS0EEqUw8AYRLDCk-PO_R1QBRarE0t1yHLukSp1iOwNvT1ArmO5ydHXvQegW8AKwoE-wYEpgCvwMzQArXUvO8TmaYUygVlrqS3SV8w5jAEX1DN2tfN-N-6oZm6b3U6RcurituliVMW5z8fEaXQTbZ39zyjnavL5slqt6_fH2vnxe144qVmoHWAsXGu4EboTHTatbZ0OQgbUEQmuZ0FhZKYIF4DS0HoSjVloBmnlO5-j-WDtMC0x2XfHu0w0xelcMIURIKWCiHo7UIQ1fo8_F7LvsfN_b6IcxG-CTBcEUk_-Ff-huGFOcLhgCRArJpVIT9XikXBpyTj6YQ-r2Nn0bwOZXqQFzUkp_AIgEZe4</recordid><startdate>20131228</startdate><enddate>20131228</enddate><creator>Sefta, Faiza</creator><creator>Juslin, Niklas</creator><creator>Wirth, Brian D.</creator><general>American Institute of Physics</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>7U5</scope><scope>OTOTI</scope></search><sort><creationdate>20131228</creationdate><title>Helium bubble bursting in tungsten</title><author>Sefta, Faiza ; Juslin, Niklas ; Wirth, Brian D.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c384t-c1096cfb5c60b6e0bd9dcaff7f4d21fda46908a76fa1153fde16c3a7a6194e53</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2013</creationdate><topic>Adatoms</topic><topic>Applied physics</topic><topic>BUBBLES</topic><topic>Bursting</topic><topic>CRATERS</topic><topic>Evolution</topic><topic>HELIUM</topic><topic>Molecular dynamics</topic><topic>MOLECULAR DYNAMICS METHOD</topic><topic>MORPHOLOGY</topic><topic>NANOSCIENCE AND NANOTECHNOLOGY</topic><topic>NANOSTRUCTURES</topic><topic>ORIENTATION</topic><topic>Pinholes</topic><topic>Surface stability</topic><topic>THICKNESS</topic><topic>TUNGSTEN</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Sefta, Faiza</creatorcontrib><creatorcontrib>Juslin, Niklas</creatorcontrib><creatorcontrib>Wirth, Brian D.</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>OSTI.GOV</collection><jtitle>Journal of applied physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Sefta, Faiza</au><au>Juslin, Niklas</au><au>Wirth, Brian D.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Helium bubble bursting in tungsten</atitle><jtitle>Journal of applied physics</jtitle><date>2013-12-28</date><risdate>2013</risdate><volume>114</volume><issue>24</issue><issn>0021-8979</issn><eissn>1089-7550</eissn><abstract>Molecular dynamics simulations have been used to systematically study the pressure evolution and bursting behavior of sub-surface helium bubbles and the resulting tungsten surface morphology. This study specifically investigates how bubble shape and size, temperature, tungsten surface orientation, and ligament thickness above the bubble influence bubble stability and surface evolution. The tungsten surface is roughened by a combination of adatom “islands,” craters, and pinholes. The present study provides insight into the mechanisms and conditions leading to various tungsten topology changes, which we believe are the initial stages of surface evolution leading to the formation of nanoscale fuzz.</abstract><cop>Melville</cop><pub>American Institute of Physics</pub><doi>10.1063/1.4860315</doi></addata></record> |
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subjects | Adatoms Applied physics BUBBLES Bursting CRATERS Evolution HELIUM Molecular dynamics MOLECULAR DYNAMICS METHOD MORPHOLOGY NANOSCIENCE AND NANOTECHNOLOGY NANOSTRUCTURES ORIENTATION Pinholes Surface stability THICKNESS TUNGSTEN |
title | Helium bubble bursting in tungsten |
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