High Efficiency Detection of Argon Scintillation Light of 128nm Using LAAPDs
The possibility of efficient collection and detection of vacuum ultraviolet light as emitted by argon, krypton, and xenon gas is studied. Absolute quantum efficiencies of large area avalanche photodiodes (LAAPDs) are derived at these wavelengths. VUV light of wavelengths down to the 128nm of Ar emis...
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description | The possibility of efficient collection and detection of vacuum ultraviolet light as emitted by argon, krypton, and xenon gas is studied. Absolute quantum efficiencies of large area avalanche photodiodes (LAAPDs) are derived at these wavelengths. VUV light of wavelengths down to the 128nm of Ar emission is shown to be detectable with silicon avalanche photodiodes at quantum efficiencies above 42%. Flexible Mylar foil overcoated with Al+MgF\(_2\) is measured to have a specular reflectivity of \(\sim\)91% at argon emission wavelength. Low-pressure argon gas is shown to emit significant amounts of non-UV radiation. The average energy expenditure for the creation of non-UV photons in argon gas at this pressure is measured to be below 378 eV. |
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Absolute quantum efficiencies of large area avalanche photodiodes (LAAPDs) are derived at these wavelengths. VUV light of wavelengths down to the 128nm of Ar emission is shown to be detectable with silicon avalanche photodiodes at quantum efficiencies above 42%. Flexible Mylar foil overcoated with Al+MgF\(_2\) is measured to have a specular reflectivity of \(\sim\)91% at argon emission wavelength. Low-pressure argon gas is shown to emit significant amounts of non-UV radiation. 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Absolute quantum efficiencies of large area avalanche photodiodes (LAAPDs) are derived at these wavelengths. VUV light of wavelengths down to the 128nm of Ar emission is shown to be detectable with silicon avalanche photodiodes at quantum efficiencies above 42%. Flexible Mylar foil overcoated with Al+MgF\(_2\) is measured to have a specular reflectivity of \(\sim\)91% at argon emission wavelength. Low-pressure argon gas is shown to emit significant amounts of non-UV radiation. The average energy expenditure for the creation of non-UV photons in argon gas at this pressure is measured to be below 378 eV.</description><subject>Argon</subject><subject>Avalanche diodes</subject><subject>Emission</subject><subject>Foils</subject><subject>Krypton</subject><subject>Low pressure</subject><subject>Mylar</subject><subject>Photodiodes</subject><subject>Photons</subject><subject>Ultraviolet radiation</subject><subject>Wavelengths</subject><subject>Xenon</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2005</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNqNi08LgjAAxUcQJOW186Cztj9O11HS6OAhqM4istnEtnIz6ttn0Qfo9H6833sALDEKI84YWlf9Uz1CxDBGGzoBHqEUBzwiZAZ8a1uEEIkTwhj1QLFXzQXmUqpaCV2_YCacqJ0yGhoJ074Z4Vgr7VTXVd-6GA_uIzHh-grPVukGFml6yOwCTGXVWeH_cg5Wu_y03Qe33twHYV3ZmqHXoyoJ4hjHSRwR-t_qDSA8QUs</recordid><startdate>20051110</startdate><enddate>20051110</enddate><creator>Chandrasekharan, R</creator><creator>Knecht, A</creator><creator>Messina, M</creator><creator>Regenfus, C</creator><creator>Rubbia, A</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20051110</creationdate><title>High Efficiency Detection of Argon Scintillation Light of 128nm Using LAAPDs</title><author>Chandrasekharan, R ; Knecht, A ; Messina, M ; Regenfus, C ; Rubbia, A</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_20811676423</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2005</creationdate><topic>Argon</topic><topic>Avalanche diodes</topic><topic>Emission</topic><topic>Foils</topic><topic>Krypton</topic><topic>Low pressure</topic><topic>Mylar</topic><topic>Photodiodes</topic><topic>Photons</topic><topic>Ultraviolet radiation</topic><topic>Wavelengths</topic><topic>Xenon</topic><toplevel>online_resources</toplevel><creatorcontrib>Chandrasekharan, R</creatorcontrib><creatorcontrib>Knecht, A</creatorcontrib><creatorcontrib>Messina, M</creatorcontrib><creatorcontrib>Regenfus, C</creatorcontrib><creatorcontrib>Rubbia, A</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>Proquest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Access via ProQuest (Open Access)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Chandrasekharan, R</au><au>Knecht, A</au><au>Messina, M</au><au>Regenfus, C</au><au>Rubbia, A</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>High Efficiency Detection of Argon Scintillation Light of 128nm Using LAAPDs</atitle><jtitle>arXiv.org</jtitle><date>2005-11-10</date><risdate>2005</risdate><eissn>2331-8422</eissn><abstract>The possibility of efficient collection and detection of vacuum ultraviolet light as emitted by argon, krypton, and xenon gas is studied. Absolute quantum efficiencies of large area avalanche photodiodes (LAAPDs) are derived at these wavelengths. VUV light of wavelengths down to the 128nm of Ar emission is shown to be detectable with silicon avalanche photodiodes at quantum efficiencies above 42%. Flexible Mylar foil overcoated with Al+MgF\(_2\) is measured to have a specular reflectivity of \(\sim\)91% at argon emission wavelength. Low-pressure argon gas is shown to emit significant amounts of non-UV radiation. The average energy expenditure for the creation of non-UV photons in argon gas at this pressure is measured to be below 378 eV.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.0511093</doi><oa>free_for_read</oa></addata></record> |
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subjects | Argon Avalanche diodes Emission Foils Krypton Low pressure Mylar Photodiodes Photons Ultraviolet radiation Wavelengths Xenon |
title | High Efficiency Detection of Argon Scintillation Light of 128nm Using LAAPDs |
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