Impact of spatiotemporal smoothing on the two-plasmon–decay instability
Higher levels of hot electrons from the two-plasmon–decay instability are observed when smoothing by spectral dispersion (SSD) is turned off in directly driven inertial confinement fusion experiments at the Omega Laser Facility. This finding is explained using a hot-spot model based on speckle stati...
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creator | Turnbull, D. Maximov, A. V. Cao, D. Christopherson, A. R. Edgell, D. H. Follett, R. K. Gopalaswamy, V. Knauer, J. P. Palastro, J. P. Shvydky, A. Stoeckl, C. Wen, H. Froula, D. H. |
description | Higher levels of hot electrons from the two-plasmon–decay instability are observed when smoothing by spectral dispersion (SSD) is turned off in directly driven inertial confinement fusion experiments at the Omega Laser Facility. This finding is explained using a hot-spot model based on speckle statistics and simulation results from the laser–plasma simulation environment. The model accurately reproduces the relative increase in hot-electron activity at two different drive intensities although it slightly overestimates the absolute number of hot electrons in all cases. Extrapolating from the current
≈
360-GHz system while adhering to the logic of the hot-spot model suggests that a larger SSD bandwidth should significantly mitigate hot-electron generation, and legacy 1-THz OMEGA experiments appear to support this conclusion. These results demonstrate that it is essential to account for laser speckles and spatiotemporal smoothing to obtain quantitative agreement with experiments. A compilation of hot-electron data from the past two decades reveals several other important points: (1) many prior experiments are more easily understood using recent results from multibeam absolute instability theory and (2) experiments with ignition-scale conditions produce less hot electrons compared to OMEGA spherical experiments for a given vacuum overlapped intensity, which is a promising result for validating performance predictions based on hydrodynamic scaling relations. |
doi_str_mv | 10.1063/5.0019080 |
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≈
360-GHz system while adhering to the logic of the hot-spot model suggests that a larger SSD bandwidth should significantly mitigate hot-electron generation, and legacy 1-THz OMEGA experiments appear to support this conclusion. These results demonstrate that it is essential to account for laser speckles and spatiotemporal smoothing to obtain quantitative agreement with experiments. A compilation of hot-electron data from the past two decades reveals several other important points: (1) many prior experiments are more easily understood using recent results from multibeam absolute instability theory and (2) experiments with ignition-scale conditions produce less hot electrons compared to OMEGA spherical experiments for a given vacuum overlapped intensity, which is a promising result for validating performance predictions based on hydrodynamic scaling relations.</description><identifier>ISSN: 1070-664X</identifier><identifier>EISSN: 1089-7674</identifier><identifier>DOI: 10.1063/5.0019080</identifier><identifier>CODEN: PHPAEN</identifier><language>eng</language><publisher>Melville: American Institute of Physics</publisher><subject>Decay ; Experiments ; Hot electrons ; Inertial confinement fusion ; Lasers ; Plasma physics ; Smoothing ; Stability</subject><ispartof>Physics of plasmas, 2020-10, Vol.27 (10)</ispartof><rights>Author(s)</rights><rights>2020 Author(s). Published under license by AIP Publishing.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c389t-1c17236069c5dd4af720cb33fd6c6ac47791e03f7f8dc72c9e45f5789e5d542e3</citedby><cites>FETCH-LOGICAL-c389t-1c17236069c5dd4af720cb33fd6c6ac47791e03f7f8dc72c9e45f5789e5d542e3</cites><orcidid>0000-0002-6721-1924 ; 0000-0002-8013-9314 ; 0000-0002-9887-1028 ; 0000-0001-6981-3956 ; 0000-0001-5375-5800 ; 0000-0001-8567-380X ; 0000000298871028 ; 0000000280139314 ; 000000018567380X ; 0000000153755800 ; 0000000169813956 ; 0000000267211924</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://pubs.aip.org/pop/article-lookup/doi/10.1063/5.0019080$$EHTML$$P50$$Gscitation$$H</linktohtml><link.rule.ids>230,314,776,780,790,881,4498,27901,27902,76353</link.rule.ids><backlink>$$Uhttps://www.osti.gov/biblio/1681063$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Turnbull, D.</creatorcontrib><creatorcontrib>Maximov, A. V.</creatorcontrib><creatorcontrib>Cao, D.</creatorcontrib><creatorcontrib>Christopherson, A. R.</creatorcontrib><creatorcontrib>Edgell, D. H.</creatorcontrib><creatorcontrib>Follett, R. K.</creatorcontrib><creatorcontrib>Gopalaswamy, V.</creatorcontrib><creatorcontrib>Knauer, J. P.</creatorcontrib><creatorcontrib>Palastro, J. P.</creatorcontrib><creatorcontrib>Shvydky, A.</creatorcontrib><creatorcontrib>Stoeckl, C.</creatorcontrib><creatorcontrib>Wen, H.</creatorcontrib><creatorcontrib>Froula, D. H.</creatorcontrib><title>Impact of spatiotemporal smoothing on the two-plasmon–decay instability</title><title>Physics of plasmas</title><description>Higher levels of hot electrons from the two-plasmon–decay instability are observed when smoothing by spectral dispersion (SSD) is turned off in directly driven inertial confinement fusion experiments at the Omega Laser Facility. This finding is explained using a hot-spot model based on speckle statistics and simulation results from the laser–plasma simulation environment. The model accurately reproduces the relative increase in hot-electron activity at two different drive intensities although it slightly overestimates the absolute number of hot electrons in all cases. Extrapolating from the current
≈
360-GHz system while adhering to the logic of the hot-spot model suggests that a larger SSD bandwidth should significantly mitigate hot-electron generation, and legacy 1-THz OMEGA experiments appear to support this conclusion. These results demonstrate that it is essential to account for laser speckles and spatiotemporal smoothing to obtain quantitative agreement with experiments. A compilation of hot-electron data from the past two decades reveals several other important points: (1) many prior experiments are more easily understood using recent results from multibeam absolute instability theory and (2) experiments with ignition-scale conditions produce less hot electrons compared to OMEGA spherical experiments for a given vacuum overlapped intensity, which is a promising result for validating performance predictions based on hydrodynamic scaling relations.</description><subject>Decay</subject><subject>Experiments</subject><subject>Hot electrons</subject><subject>Inertial confinement fusion</subject><subject>Lasers</subject><subject>Plasma physics</subject><subject>Smoothing</subject><subject>Stability</subject><issn>1070-664X</issn><issn>1089-7674</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNqd0M1KxDAQB_AgCq6rB9-g6Emha9J8tUdZ_FhY8KLgLWTTxM3SJjXJKnvzHXxDn8SWLnj3NMPwY2b4A3CO4AxBhm_oDEJUwRIegAmCZZVzxsnh0HOYM0Zej8FJjBsIIWG0nIDFou2kSpk3Wexksj7ptvNBNllsvU9r694y77K01ln69HnXyH7ufr6-a63kLrMuJrmyjU27U3BkZBP12b5Owcv93fP8MV8-PSzmt8tc4bJKOVKIF5hBVila10QaXkC1wtjUTDGpCOcV0hAbbspa8UJVmlBDeVlpWlNSaDwFF-NeH5MVUdmk1Vp557RKArFyiKFHlyPqgn_f6pjExm-D6_8SBaEFo4RC1KurUangYwzaiC7YVoadQFAMewQV-zh7ez3a4eIQlPsf_vDhD4quNvgXJzeD5Q</recordid><startdate>202010</startdate><enddate>202010</enddate><creator>Turnbull, D.</creator><creator>Maximov, A. 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V. ; Cao, D. ; Christopherson, A. R. ; Edgell, D. H. ; Follett, R. K. ; Gopalaswamy, V. ; Knauer, J. P. ; Palastro, J. P. ; Shvydky, A. ; Stoeckl, C. ; Wen, H. ; Froula, D. H.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c389t-1c17236069c5dd4af720cb33fd6c6ac47791e03f7f8dc72c9e45f5789e5d542e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Decay</topic><topic>Experiments</topic><topic>Hot electrons</topic><topic>Inertial confinement fusion</topic><topic>Lasers</topic><topic>Plasma physics</topic><topic>Smoothing</topic><topic>Stability</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Turnbull, D.</creatorcontrib><creatorcontrib>Maximov, A. V.</creatorcontrib><creatorcontrib>Cao, D.</creatorcontrib><creatorcontrib>Christopherson, A. R.</creatorcontrib><creatorcontrib>Edgell, D. H.</creatorcontrib><creatorcontrib>Follett, R. 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H.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Impact of spatiotemporal smoothing on the two-plasmon–decay instability</atitle><jtitle>Physics of plasmas</jtitle><date>2020-10</date><risdate>2020</risdate><volume>27</volume><issue>10</issue><issn>1070-664X</issn><eissn>1089-7674</eissn><coden>PHPAEN</coden><abstract>Higher levels of hot electrons from the two-plasmon–decay instability are observed when smoothing by spectral dispersion (SSD) is turned off in directly driven inertial confinement fusion experiments at the Omega Laser Facility. This finding is explained using a hot-spot model based on speckle statistics and simulation results from the laser–plasma simulation environment. The model accurately reproduces the relative increase in hot-electron activity at two different drive intensities although it slightly overestimates the absolute number of hot electrons in all cases. Extrapolating from the current
≈
360-GHz system while adhering to the logic of the hot-spot model suggests that a larger SSD bandwidth should significantly mitigate hot-electron generation, and legacy 1-THz OMEGA experiments appear to support this conclusion. These results demonstrate that it is essential to account for laser speckles and spatiotemporal smoothing to obtain quantitative agreement with experiments. A compilation of hot-electron data from the past two decades reveals several other important points: (1) many prior experiments are more easily understood using recent results from multibeam absolute instability theory and (2) experiments with ignition-scale conditions produce less hot electrons compared to OMEGA spherical experiments for a given vacuum overlapped intensity, which is a promising result for validating performance predictions based on hydrodynamic scaling relations.</abstract><cop>Melville</cop><pub>American Institute of Physics</pub><doi>10.1063/5.0019080</doi><tpages>11</tpages><orcidid>https://orcid.org/0000-0002-6721-1924</orcidid><orcidid>https://orcid.org/0000-0002-8013-9314</orcidid><orcidid>https://orcid.org/0000-0002-9887-1028</orcidid><orcidid>https://orcid.org/0000-0001-6981-3956</orcidid><orcidid>https://orcid.org/0000-0001-5375-5800</orcidid><orcidid>https://orcid.org/0000-0001-8567-380X</orcidid><orcidid>https://orcid.org/0000000298871028</orcidid><orcidid>https://orcid.org/0000000280139314</orcidid><orcidid>https://orcid.org/000000018567380X</orcidid><orcidid>https://orcid.org/0000000153755800</orcidid><orcidid>https://orcid.org/0000000169813956</orcidid><orcidid>https://orcid.org/0000000267211924</orcidid><oa>free_for_read</oa></addata></record> |
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source | 美国小型学会期刊集(AIP Scitation平台); Alma/SFX Local Collection |
subjects | Decay Experiments Hot electrons Inertial confinement fusion Lasers Plasma physics Smoothing Stability |
title | Impact of spatiotemporal smoothing on the two-plasmon–decay instability |
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