Ab initio response functions for Cherenkov-based neutron detectors
Neutron time-of-flight diagnostics at the NIF were recently outfitted with Cherenkov detectors. A fused silica radiator delivers sub-nanosecond response time and is optically coupled to a microchannel plate photomultiplier tube with gain from ∼1 to 104. Capitalizing on fast time response and gamma-r...
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Veröffentlicht in: | Review of scientific instruments 2018-10, Vol.89 (10), p.10I136-10I136 |
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creator | Schlossberg, D. J. Moore, A. S. Beeman, B. V. Eckart, M. J. Grim, G. P. Hartouni, E. P. Hatarik, R. Rubery, M. S. Sayre, D. B. Waltz, C. |
description | Neutron time-of-flight diagnostics at the NIF were recently outfitted with Cherenkov detectors. A fused silica radiator delivers sub-nanosecond response time and is optically coupled to a microchannel plate photomultiplier tube with gain from ∼1 to 104. Capitalizing on fast time response and gamma-ray sensitivity, these systems can provide better than 30 ps precision for measuring first moments of neutron distributions. Generation of ab initio instrument response functions (IRFs) is critical to meet the |
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J. ; Moore, A. S. ; Beeman, B. V. ; Eckart, M. J. ; Grim, G. P. ; Hartouni, E. P. ; Hatarik, R. ; Rubery, M. S. ; Sayre, D. B. ; Waltz, C.</creator><creatorcontrib>Schlossberg, D. J. ; Moore, A. S. ; Beeman, B. V. ; Eckart, M. J. ; Grim, G. P. ; Hartouni, E. P. ; Hatarik, R. ; Rubery, M. S. ; Sayre, D. B. ; Waltz, C.</creatorcontrib><description>Neutron time-of-flight diagnostics at the NIF were recently outfitted with Cherenkov detectors. A fused silica radiator delivers sub-nanosecond response time and is optically coupled to a microchannel plate photomultiplier tube with gain from ∼1 to 104. Capitalizing on fast time response and gamma-ray sensitivity, these systems can provide better than 30 ps precision for measuring first moments of neutron distributions. Generation of ab initio instrument response functions (IRFs) is critical to meet the <1% uncertainty needed. A combination of Monte Carlo modeling, benchtop characterization, and in situ comparison is employed. Close agreement is shown between the modeled IRFs and in situ measurements using the NIF’s short-pulse advanced radiographic capability beams. First and second moments of neutron spectra calculated using ab initio IRFs agree well with established scintillator measurements. Next-step designs offer increased sensitivity and time-response.</description><identifier>ISSN: 0034-6748</identifier><identifier>EISSN: 1089-7623</identifier><identifier>DOI: 10.1063/1.5039399</identifier><identifier>PMID: 30399741</identifier><identifier>CODEN: RSINAK</identifier><language>eng</language><publisher>United States: American Institute of Physics</publisher><subject>Beams (radiation) ; Cerenkov counters ; Computer simulation ; Detectors ; Fused silica ; Gamma rays ; In situ measurement ; Mathematical models ; Microchannel plates ; Microchannels ; Nanosecond response ; Neutron counters ; Neutron spectra ; Photomultiplier tubes ; Radiators ; Response functions ; Response time ; Scientific apparatus & instruments ; Scintillation counters ; Sensitivity ; Silicon dioxide ; Time response</subject><ispartof>Review of scientific instruments, 2018-10, Vol.89 (10), p.10I136-10I136</ispartof><rights>Author(s)</rights><rights>2018 Author(s). Published by AIP Publishing.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c445t-9b68d9b6612eb554d7abbe963af915f73d5d25f105bc9da17f751fe4e2c942203</citedby><cites>FETCH-LOGICAL-c445t-9b68d9b6612eb554d7abbe963af915f73d5d25f105bc9da17f751fe4e2c942203</cites><orcidid>0000-0002-8713-9448 ; 0000-0001-9869-4351 ; 0000000287139448 ; 0000000198694351</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://pubs.aip.org/rsi/article-lookup/doi/10.1063/1.5039399$$EHTML$$P50$$Gscitation$$H</linktohtml><link.rule.ids>230,314,777,781,791,882,4499,27906,27907,76134</link.rule.ids><backlink>$$Uhttps://www.ncbi.nlm.nih.gov/pubmed/30399741$$D View this record in MEDLINE/PubMed$$Hfree_for_read</backlink><backlink>$$Uhttps://www.osti.gov/biblio/1477812$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Schlossberg, D. J.</creatorcontrib><creatorcontrib>Moore, A. S.</creatorcontrib><creatorcontrib>Beeman, B. V.</creatorcontrib><creatorcontrib>Eckart, M. J.</creatorcontrib><creatorcontrib>Grim, G. P.</creatorcontrib><creatorcontrib>Hartouni, E. P.</creatorcontrib><creatorcontrib>Hatarik, R.</creatorcontrib><creatorcontrib>Rubery, M. S.</creatorcontrib><creatorcontrib>Sayre, D. B.</creatorcontrib><creatorcontrib>Waltz, C.</creatorcontrib><title>Ab initio response functions for Cherenkov-based neutron detectors</title><title>Review of scientific instruments</title><addtitle>Rev Sci Instrum</addtitle><description>Neutron time-of-flight diagnostics at the NIF were recently outfitted with Cherenkov detectors. A fused silica radiator delivers sub-nanosecond response time and is optically coupled to a microchannel plate photomultiplier tube with gain from ∼1 to 104. Capitalizing on fast time response and gamma-ray sensitivity, these systems can provide better than 30 ps precision for measuring first moments of neutron distributions. Generation of ab initio instrument response functions (IRFs) is critical to meet the <1% uncertainty needed. A combination of Monte Carlo modeling, benchtop characterization, and in situ comparison is employed. Close agreement is shown between the modeled IRFs and in situ measurements using the NIF’s short-pulse advanced radiographic capability beams. First and second moments of neutron spectra calculated using ab initio IRFs agree well with established scintillator measurements. Next-step designs offer increased sensitivity and time-response.</description><subject>Beams (radiation)</subject><subject>Cerenkov counters</subject><subject>Computer simulation</subject><subject>Detectors</subject><subject>Fused silica</subject><subject>Gamma rays</subject><subject>In situ measurement</subject><subject>Mathematical models</subject><subject>Microchannel plates</subject><subject>Microchannels</subject><subject>Nanosecond response</subject><subject>Neutron counters</subject><subject>Neutron spectra</subject><subject>Photomultiplier tubes</subject><subject>Radiators</subject><subject>Response functions</subject><subject>Response time</subject><subject>Scientific apparatus & instruments</subject><subject>Scintillation counters</subject><subject>Sensitivity</subject><subject>Silicon dioxide</subject><subject>Time response</subject><issn>0034-6748</issn><issn>1089-7623</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNp90E9LHDEYBvBQlLpqD_0CZdCLLcyaN38mk6Mu1goLXvQcZpI3OHY32SYzgt_eLLttoVBzSCD8ePLmIeQz0DnQhl_CXFKuudYfyAxoq2vVMH5AZpRyUTdKtEfkOOdnWpYE-EiOeOFaCZiR66u-GsIwDrFKmDcxZKz8FGy5CLnyMVWLJ0wYfsaXuu8yuirgNKYYKocj2jGmfEoOfbfK-Gl_npDH7zcPix_18v72bnG1rK0Qcqx137SubA0w7KUUTnV9j7rhndcgveJOOiY9UNlb7TpQXknwKJBZLRij_ISc7XJjHgeT7VDef7IxhDKGAaFUC6ygix3apPhrwjya9ZAtrlZdwDhlw4DTdtsLFHr-D32OUwrlC0UxKlrOpCrq607ZFHNO6M0mDesuvRqgZtu-AbNvv9gv-8SpX6P7I3_XXcC3HdhO3207fjftv_glpr_QbJznb28dmV4</recordid><startdate>201810</startdate><enddate>201810</enddate><creator>Schlossberg, D. 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J.</creatorcontrib><creatorcontrib>Moore, A. S.</creatorcontrib><creatorcontrib>Beeman, B. V.</creatorcontrib><creatorcontrib>Eckart, M. J.</creatorcontrib><creatorcontrib>Grim, G. P.</creatorcontrib><creatorcontrib>Hartouni, E. P.</creatorcontrib><creatorcontrib>Hatarik, R.</creatorcontrib><creatorcontrib>Rubery, M. S.</creatorcontrib><creatorcontrib>Sayre, D. B.</creatorcontrib><creatorcontrib>Waltz, C.</creatorcontrib><collection>PubMed</collection><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>MEDLINE - Academic</collection><collection>OSTI.GOV</collection><jtitle>Review of scientific instruments</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Schlossberg, D. J.</au><au>Moore, A. S.</au><au>Beeman, B. V.</au><au>Eckart, M. J.</au><au>Grim, G. P.</au><au>Hartouni, E. P.</au><au>Hatarik, R.</au><au>Rubery, M. S.</au><au>Sayre, D. B.</au><au>Waltz, C.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Ab initio response functions for Cherenkov-based neutron detectors</atitle><jtitle>Review of scientific instruments</jtitle><addtitle>Rev Sci Instrum</addtitle><date>2018-10</date><risdate>2018</risdate><volume>89</volume><issue>10</issue><spage>10I136</spage><epage>10I136</epage><pages>10I136-10I136</pages><issn>0034-6748</issn><eissn>1089-7623</eissn><coden>RSINAK</coden><abstract>Neutron time-of-flight diagnostics at the NIF were recently outfitted with Cherenkov detectors. A fused silica radiator delivers sub-nanosecond response time and is optically coupled to a microchannel plate photomultiplier tube with gain from ∼1 to 104. 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subjects | Beams (radiation) Cerenkov counters Computer simulation Detectors Fused silica Gamma rays In situ measurement Mathematical models Microchannel plates Microchannels Nanosecond response Neutron counters Neutron spectra Photomultiplier tubes Radiators Response functions Response time Scientific apparatus & instruments Scintillation counters Sensitivity Silicon dioxide Time response |
title | Ab initio response functions for Cherenkov-based neutron detectors |
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