Enhancing the light yield of He:CF4 based gaseous detector

The CYGNO experiment aims to build a large ( O ( 10 ) m 3 ) directional detector for rare event searches, such as nuclear recoils (NRs) induced by dark matter (DM), such as weakly interactive massive particles (WIMPs). The detector concept comprises a time projection chamber (TPC), filled with a He:...

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Veröffentlicht in:The European physical journal. C, Particles and fields Particles and fields, 2024-10, Vol.84 (10), p.1122
Hauptverfasser: Amaro, Fernando Domingues, Antonietti, Rita, Baracchini, Elisabetta, Benussi, Luigi, Bianco, Stefano, Campagnola, Roberto, Capoccia, Cesidio, Caponero, Michele, Cardoso, Danilo Santos, de Carvalho, Luan Gomes Mattosinhos, Cavoto, Gianluca, Costa, Igor Abritta, Croce, Antonio, Dané, Emiliano, Dho, Giorgio, Di Giambattista, Flaminia, Di Marco, Emanuele, D’Astolfo, Melba, D’Imperio, Giulia, Fiorina, Davide, Iacoangeli, Francesco, Islam, Zahoor ul, Lima Jùnior, Herman Pessoa, Kemp, Ernesto, Maccarrone, Giovanni, Mano, Rui Daniel Passos, Marcelo Gregorio, Robert Renz, Marques, David José Gaspar, Mazzitelli, Giovanni, McLean, Alasdair Gregor, Messina, Andrea, Meloni, Pietro, Monteiro, Cristina Maria Bernardes, Nobrega, Rafael Antunes, Pains, Igor Fonseca, Paoletti, Emiliano, Passamonti, Luciano, Petrucci, Fabrizio, Piacentini, Stefano, Piccolo, Davide, Pierluigi, Daniele, Pinci, Davide, Prajapati, Atul, Renga, Francesco, Roque, Rita Joana da Cruz, Rosatelli, Filippo, Russo, Alessandro, dos Santos, Joaquim Marques Ferreira, Saviano, Giovanna, Silva, Pedro Alberto Oliveira Costa, Spooner, Neil John Curwen, Tesauro, Roberto, Tomassini, Sandro, Torelli, Samuele
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container_title The European physical journal. C, Particles and fields
container_volume 84
creator Amaro, Fernando Domingues
Antonietti, Rita
Baracchini, Elisabetta
Benussi, Luigi
Bianco, Stefano
Campagnola, Roberto
Capoccia, Cesidio
Caponero, Michele
Cardoso, Danilo Santos
de Carvalho, Luan Gomes Mattosinhos
Cavoto, Gianluca
Costa, Igor Abritta
Croce, Antonio
Dané, Emiliano
Dho, Giorgio
Di Giambattista, Flaminia
Di Marco, Emanuele
D’Astolfo, Melba
D’Imperio, Giulia
Fiorina, Davide
Iacoangeli, Francesco
Islam, Zahoor ul
Lima Jùnior, Herman Pessoa
Kemp, Ernesto
Maccarrone, Giovanni
Mano, Rui Daniel Passos
Marcelo Gregorio, Robert Renz
Marques, David José Gaspar
Mazzitelli, Giovanni
McLean, Alasdair Gregor
Messina, Andrea
Meloni, Pietro
Monteiro, Cristina Maria Bernardes
Nobrega, Rafael Antunes
Pains, Igor Fonseca
Paoletti, Emiliano
Passamonti, Luciano
Petrucci, Fabrizio
Piacentini, Stefano
Piccolo, Davide
Pierluigi, Daniele
Pinci, Davide
Prajapati, Atul
Renga, Francesco
Roque, Rita Joana da Cruz
Rosatelli, Filippo
Russo, Alessandro
dos Santos, Joaquim Marques Ferreira
Saviano, Giovanna
Silva, Pedro Alberto Oliveira Costa
Spooner, Neil John Curwen
Tesauro, Roberto
Tomassini, Sandro
Torelli, Samuele
description The CYGNO experiment aims to build a large ( O ( 10 ) m 3 ) directional detector for rare event searches, such as nuclear recoils (NRs) induced by dark matter (DM), such as weakly interactive massive particles (WIMPs). The detector concept comprises a time projection chamber (TPC), filled with a He:CF 4 60/40 scintillating gas mixture at room temperature and atmospheric pressure, equipped with an amplification stage made of a stack of three gas electron multipliers (GEMs) which are coupled to an optical readout. The latter consists in scientific CMOS (sCMOS) cameras and photomultipliers tubes (PMTs). The maximisation of the light yield of the amplification stage plays a major role in the determination of the energy threshold of the experiment. In this paper, we simulate the effect of the addition of a strong electric field below the last GEM plane on the GEM field structure and we experimentally test it by means of a 10 × 10 cm 2 readout area prototype. The experimental measurements analyse stacks of different GEMs and helium concentrations in the gas mixture combined with this extra electric field, studying their performances in terms of light yield, energy resolution and intrinsic diffusion. It is found that the use of this additional electric field permits large light yield increases without degrading intrinsic characteristics of the amplification stage with respect to the regular use of GEMs.
doi_str_mv 10.1140/epjc/s10052-024-13471-5
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C, Particles and fields</title><addtitle>Eur. Phys. J. C</addtitle><description>The CYGNO experiment aims to build a large ( O ( 10 ) m 3 ) directional detector for rare event searches, such as nuclear recoils (NRs) induced by dark matter (DM), such as weakly interactive massive particles (WIMPs). The detector concept comprises a time projection chamber (TPC), filled with a He:CF 4 60/40 scintillating gas mixture at room temperature and atmospheric pressure, equipped with an amplification stage made of a stack of three gas electron multipliers (GEMs) which are coupled to an optical readout. The latter consists in scientific CMOS (sCMOS) cameras and photomultipliers tubes (PMTs). The maximisation of the light yield of the amplification stage plays a major role in the determination of the energy threshold of the experiment. 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It is found that the use of this additional electric field permits large light yield increases without degrading intrinsic characteristics of the amplification stage with respect to the regular use of GEMs.</description><subject>Astronomy</subject><subject>Astrophysics and Cosmology</subject><subject>Dark matter</subject><subject>Electric fields</subject><subject>Elementary Particles</subject><subject>Energy resolution</subject><subject>Gas detectors</subject><subject>Gas mixtures</subject><subject>Hadrons</subject><subject>Heavy Ions</subject><subject>Measurement Science and Instrumentation</subject><subject>Nuclear Energy</subject><subject>Nuclear Physics</subject><subject>Photodegradation</subject><subject>Photomultiplier tubes</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Quantum Field Theories</subject><subject>Quantum Field Theory</subject><subject>Radiation counters</subject><subject>Regular Article - Experimental Physics</subject><subject>Room temperature</subject><subject>Sensors</subject><subject>String Theory</subject><subject>Weakly interacting massive particles</subject><issn>1434-6044</issn><issn>1434-6052</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2024</creationdate><recordtype>article</recordtype><sourceid>C6C</sourceid><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNpFkE1LxDAQhoMouK7-BgOe684kaZPuTZb9EBa86DmkTfpFaWvTHvz3Zq3oZd5heJmZ9yHkEeEZUcDGDU2-8QgQswiYiJALiVF8RVYouIiSML_-64W4JXfeNwDBCmpFtvuuMl1edyWdKkfbuqwm-lW71tK-oCe33R0EzYx3lpah9rOn1k0un_rxntwUpvXu4VfX5OOwf9-dovPb8XX3co4GRB4-wTyzzBgOQTOTSpScJQiusJjGSlkVMwWQ5amR0ijGUqGcBMYs4wqt5GvytOwdxv5zdn7STT-PXTipOTLkqYghCS61uPwwhjRu_Hch6AspfSGlF1I6xNc_pHTMvwFCtVr8</recordid><startdate>20241029</startdate><enddate>20241029</enddate><creator>Amaro, Fernando Domingues</creator><creator>Antonietti, Rita</creator><creator>Baracchini, Elisabetta</creator><creator>Benussi, Luigi</creator><creator>Bianco, Stefano</creator><creator>Campagnola, Roberto</creator><creator>Capoccia, Cesidio</creator><creator>Caponero, Michele</creator><creator>Cardoso, Danilo Santos</creator><creator>de Carvalho, Luan Gomes Mattosinhos</creator><creator>Cavoto, Gianluca</creator><creator>Costa, Igor Abritta</creator><creator>Croce, Antonio</creator><creator>Dané, Emiliano</creator><creator>Dho, Giorgio</creator><creator>Di Giambattista, Flaminia</creator><creator>Di Marco, Emanuele</creator><creator>D’Astolfo, Melba</creator><creator>D’Imperio, Giulia</creator><creator>Fiorina, Davide</creator><creator>Iacoangeli, Francesco</creator><creator>Islam, Zahoor ul</creator><creator>Lima Jùnior, Herman Pessoa</creator><creator>Kemp, Ernesto</creator><creator>Maccarrone, Giovanni</creator><creator>Mano, Rui Daniel Passos</creator><creator>Marcelo Gregorio, Robert Renz</creator><creator>Marques, David José Gaspar</creator><creator>Mazzitelli, Giovanni</creator><creator>McLean, Alasdair Gregor</creator><creator>Messina, Andrea</creator><creator>Meloni, Pietro</creator><creator>Monteiro, Cristina Maria Bernardes</creator><creator>Nobrega, Rafael Antunes</creator><creator>Pains, Igor Fonseca</creator><creator>Paoletti, Emiliano</creator><creator>Passamonti, Luciano</creator><creator>Petrucci, Fabrizio</creator><creator>Piacentini, Stefano</creator><creator>Piccolo, Davide</creator><creator>Pierluigi, Daniele</creator><creator>Pinci, Davide</creator><creator>Prajapati, Atul</creator><creator>Renga, Francesco</creator><creator>Roque, Rita Joana da Cruz</creator><creator>Rosatelli, Filippo</creator><creator>Russo, Alessandro</creator><creator>dos Santos, Joaquim Marques Ferreira</creator><creator>Saviano, Giovanna</creator><creator>Silva, Pedro Alberto Oliveira Costa</creator><creator>Spooner, Neil John Curwen</creator><creator>Tesauro, Roberto</creator><creator>Tomassini, Sandro</creator><creator>Torelli, Samuele</creator><general>Springer Berlin Heidelberg</general><general>Springer Nature B.V</general><scope>C6C</scope><scope>7U5</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>H8D</scope><scope>HCIFZ</scope><scope>L7M</scope><scope>P5Z</scope><scope>P62</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><orcidid>https://orcid.org/0000-0001-9454-9894</orcidid></search><sort><creationdate>20241029</creationdate><title>Enhancing the light yield of He:CF4 based gaseous detector</title><author>Amaro, Fernando Domingues ; Antonietti, Rita ; Baracchini, Elisabetta ; Benussi, Luigi ; Bianco, Stefano ; Campagnola, Roberto ; Capoccia, Cesidio ; Caponero, Michele ; Cardoso, Danilo Santos ; de Carvalho, Luan Gomes Mattosinhos ; Cavoto, Gianluca ; Costa, Igor Abritta ; Croce, Antonio ; Dané, Emiliano ; Dho, Giorgio ; Di Giambattista, Flaminia ; Di Marco, Emanuele ; D’Astolfo, Melba ; D’Imperio, Giulia ; Fiorina, Davide ; Iacoangeli, Francesco ; Islam, Zahoor ul ; Lima Jùnior, Herman Pessoa ; Kemp, Ernesto ; Maccarrone, Giovanni ; Mano, Rui Daniel Passos ; Marcelo Gregorio, Robert Renz ; Marques, David José Gaspar ; Mazzitelli, Giovanni ; McLean, Alasdair Gregor ; Messina, Andrea ; Meloni, Pietro ; Monteiro, Cristina Maria Bernardes ; Nobrega, Rafael Antunes ; Pains, Igor Fonseca ; Paoletti, Emiliano ; Passamonti, Luciano ; Petrucci, Fabrizio ; Piacentini, Stefano ; Piccolo, Davide ; Pierluigi, Daniele ; Pinci, Davide ; Prajapati, Atul ; Renga, Francesco ; Roque, Rita Joana da Cruz ; Rosatelli, Filippo ; Russo, Alessandro ; dos Santos, Joaquim Marques Ferreira ; Saviano, Giovanna ; Silva, Pedro Alberto Oliveira Costa ; Spooner, Neil John Curwen ; Tesauro, Roberto ; Tomassini, Sandro ; Torelli, Samuele</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-p1131-51cbd2aa30cbdba971732610efd19588d852800bc9a77a822948e7022d2381d73</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2024</creationdate><topic>Astronomy</topic><topic>Astrophysics and Cosmology</topic><topic>Dark matter</topic><topic>Electric fields</topic><topic>Elementary Particles</topic><topic>Energy resolution</topic><topic>Gas detectors</topic><topic>Gas mixtures</topic><topic>Hadrons</topic><topic>Heavy Ions</topic><topic>Measurement Science and Instrumentation</topic><topic>Nuclear Energy</topic><topic>Nuclear Physics</topic><topic>Photodegradation</topic><topic>Photomultiplier tubes</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Quantum Field Theories</topic><topic>Quantum Field Theory</topic><topic>Radiation counters</topic><topic>Regular Article - Experimental Physics</topic><topic>Room temperature</topic><topic>Sensors</topic><topic>String Theory</topic><topic>Weakly interacting massive particles</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Amaro, Fernando Domingues</creatorcontrib><creatorcontrib>Antonietti, Rita</creatorcontrib><creatorcontrib>Baracchini, Elisabetta</creatorcontrib><creatorcontrib>Benussi, Luigi</creatorcontrib><creatorcontrib>Bianco, Stefano</creatorcontrib><creatorcontrib>Campagnola, Roberto</creatorcontrib><creatorcontrib>Capoccia, Cesidio</creatorcontrib><creatorcontrib>Caponero, Michele</creatorcontrib><creatorcontrib>Cardoso, Danilo Santos</creatorcontrib><creatorcontrib>de Carvalho, Luan Gomes Mattosinhos</creatorcontrib><creatorcontrib>Cavoto, Gianluca</creatorcontrib><creatorcontrib>Costa, Igor Abritta</creatorcontrib><creatorcontrib>Croce, Antonio</creatorcontrib><creatorcontrib>Dané, Emiliano</creatorcontrib><creatorcontrib>Dho, Giorgio</creatorcontrib><creatorcontrib>Di Giambattista, Flaminia</creatorcontrib><creatorcontrib>Di Marco, Emanuele</creatorcontrib><creatorcontrib>D’Astolfo, Melba</creatorcontrib><creatorcontrib>D’Imperio, Giulia</creatorcontrib><creatorcontrib>Fiorina, Davide</creatorcontrib><creatorcontrib>Iacoangeli, Francesco</creatorcontrib><creatorcontrib>Islam, Zahoor ul</creatorcontrib><creatorcontrib>Lima Jùnior, Herman Pessoa</creatorcontrib><creatorcontrib>Kemp, Ernesto</creatorcontrib><creatorcontrib>Maccarrone, Giovanni</creatorcontrib><creatorcontrib>Mano, Rui Daniel Passos</creatorcontrib><creatorcontrib>Marcelo Gregorio, Robert Renz</creatorcontrib><creatorcontrib>Marques, David José Gaspar</creatorcontrib><creatorcontrib>Mazzitelli, Giovanni</creatorcontrib><creatorcontrib>McLean, Alasdair Gregor</creatorcontrib><creatorcontrib>Messina, Andrea</creatorcontrib><creatorcontrib>Meloni, Pietro</creatorcontrib><creatorcontrib>Monteiro, Cristina Maria Bernardes</creatorcontrib><creatorcontrib>Nobrega, Rafael Antunes</creatorcontrib><creatorcontrib>Pains, Igor Fonseca</creatorcontrib><creatorcontrib>Paoletti, Emiliano</creatorcontrib><creatorcontrib>Passamonti, Luciano</creatorcontrib><creatorcontrib>Petrucci, Fabrizio</creatorcontrib><creatorcontrib>Piacentini, Stefano</creatorcontrib><creatorcontrib>Piccolo, Davide</creatorcontrib><creatorcontrib>Pierluigi, Daniele</creatorcontrib><creatorcontrib>Pinci, Davide</creatorcontrib><creatorcontrib>Prajapati, Atul</creatorcontrib><creatorcontrib>Renga, Francesco</creatorcontrib><creatorcontrib>Roque, Rita Joana da Cruz</creatorcontrib><creatorcontrib>Rosatelli, Filippo</creatorcontrib><creatorcontrib>Russo, Alessandro</creatorcontrib><creatorcontrib>dos Santos, Joaquim Marques Ferreira</creatorcontrib><creatorcontrib>Saviano, Giovanna</creatorcontrib><creatorcontrib>Silva, Pedro Alberto Oliveira Costa</creatorcontrib><creatorcontrib>Spooner, Neil John Curwen</creatorcontrib><creatorcontrib>Tesauro, Roberto</creatorcontrib><creatorcontrib>Tomassini, Sandro</creatorcontrib><creatorcontrib>Torelli, Samuele</creatorcontrib><collection>Springer Nature OA/Free Journals</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>Advanced Technologies &amp; 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C, Particles and fields</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Amaro, Fernando Domingues</au><au>Antonietti, Rita</au><au>Baracchini, Elisabetta</au><au>Benussi, Luigi</au><au>Bianco, Stefano</au><au>Campagnola, Roberto</au><au>Capoccia, Cesidio</au><au>Caponero, Michele</au><au>Cardoso, Danilo Santos</au><au>de Carvalho, Luan Gomes Mattosinhos</au><au>Cavoto, Gianluca</au><au>Costa, Igor Abritta</au><au>Croce, Antonio</au><au>Dané, Emiliano</au><au>Dho, Giorgio</au><au>Di Giambattista, Flaminia</au><au>Di Marco, Emanuele</au><au>D’Astolfo, Melba</au><au>D’Imperio, Giulia</au><au>Fiorina, Davide</au><au>Iacoangeli, Francesco</au><au>Islam, Zahoor ul</au><au>Lima Jùnior, Herman Pessoa</au><au>Kemp, Ernesto</au><au>Maccarrone, Giovanni</au><au>Mano, Rui Daniel Passos</au><au>Marcelo Gregorio, Robert Renz</au><au>Marques, David José Gaspar</au><au>Mazzitelli, Giovanni</au><au>McLean, Alasdair Gregor</au><au>Messina, Andrea</au><au>Meloni, Pietro</au><au>Monteiro, Cristina Maria Bernardes</au><au>Nobrega, Rafael Antunes</au><au>Pains, Igor Fonseca</au><au>Paoletti, Emiliano</au><au>Passamonti, Luciano</au><au>Petrucci, Fabrizio</au><au>Piacentini, Stefano</au><au>Piccolo, Davide</au><au>Pierluigi, Daniele</au><au>Pinci, Davide</au><au>Prajapati, Atul</au><au>Renga, Francesco</au><au>Roque, Rita Joana da Cruz</au><au>Rosatelli, Filippo</au><au>Russo, Alessandro</au><au>dos Santos, Joaquim Marques Ferreira</au><au>Saviano, Giovanna</au><au>Silva, Pedro Alberto Oliveira Costa</au><au>Spooner, Neil John Curwen</au><au>Tesauro, Roberto</au><au>Tomassini, Sandro</au><au>Torelli, Samuele</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Enhancing the light yield of He:CF4 based gaseous detector</atitle><jtitle>The European physical journal. C, Particles and fields</jtitle><stitle>Eur. Phys. J. C</stitle><date>2024-10-29</date><risdate>2024</risdate><volume>84</volume><issue>10</issue><spage>1122</spage><pages>1122-</pages><issn>1434-6044</issn><eissn>1434-6052</eissn><abstract>The CYGNO experiment aims to build a large ( O ( 10 ) m 3 ) directional detector for rare event searches, such as nuclear recoils (NRs) induced by dark matter (DM), such as weakly interactive massive particles (WIMPs). The detector concept comprises a time projection chamber (TPC), filled with a He:CF 4 60/40 scintillating gas mixture at room temperature and atmospheric pressure, equipped with an amplification stage made of a stack of three gas electron multipliers (GEMs) which are coupled to an optical readout. The latter consists in scientific CMOS (sCMOS) cameras and photomultipliers tubes (PMTs). The maximisation of the light yield of the amplification stage plays a major role in the determination of the energy threshold of the experiment. In this paper, we simulate the effect of the addition of a strong electric field below the last GEM plane on the GEM field structure and we experimentally test it by means of a 10 × 10 cm 2 readout area prototype. The experimental measurements analyse stacks of different GEMs and helium concentrations in the gas mixture combined with this extra electric field, studying their performances in terms of light yield, energy resolution and intrinsic diffusion. It is found that the use of this additional electric field permits large light yield increases without degrading intrinsic characteristics of the amplification stage with respect to the regular use of GEMs.</abstract><cop>Berlin/Heidelberg</cop><pub>Springer Berlin Heidelberg</pub><doi>10.1140/epjc/s10052-024-13471-5</doi><orcidid>https://orcid.org/0000-0001-9454-9894</orcidid><oa>free_for_read</oa></addata></record>
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subjects Astronomy
Astrophysics and Cosmology
Dark matter
Electric fields
Elementary Particles
Energy resolution
Gas detectors
Gas mixtures
Hadrons
Heavy Ions
Measurement Science and Instrumentation
Nuclear Energy
Nuclear Physics
Photodegradation
Photomultiplier tubes
Physics
Physics and Astronomy
Quantum Field Theories
Quantum Field Theory
Radiation counters
Regular Article - Experimental Physics
Room temperature
Sensors
String Theory
Weakly interacting massive particles
title Enhancing the light yield of He:CF4 based gaseous detector
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