Secondary scintillation yield of xenon with sub-percent levels of CO2 additive for rare-event detection
Xe–CO2 mixtures are important alternatives to pure xenon in Time Projection Chambers (TPC) based on secondary scintillation (electroluminescence) signal amplification with applications in the important field of rare event detection such as directional dark matter, double electron capture and double...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
C.A.O. Henriques [verfasserIn] E.D.C. Freitas [verfasserIn] C.D.R. Azevedo [verfasserIn] D. González-Díaz [verfasserIn] R.D.P. Mano [verfasserIn] M.R. Jorge [verfasserIn] L.M.P. Fernandes [verfasserIn] C.M.B. Monteiro [verfasserIn] J.J. Gómez-Cadenas [verfasserIn] V. Álvarez [verfasserIn] J.M. Benlloch-Rodríguez [verfasserIn] F.I.G.M. Borges [verfasserIn] A. Botas [verfasserIn] S. Cárcel [verfasserIn] J.V. Carríon [verfasserIn] S. Cebrían [verfasserIn] C.A.N. Conde [verfasserIn] J. Díaz [verfasserIn] M. Diesburg [verfasserIn] R. Esteve [verfasserIn] R. Felkai [verfasserIn] P. Ferrario [verfasserIn] A.L. Ferreira [verfasserIn] A. Goldschmidt [verfasserIn] R.M. Gutiérrez [verfasserIn] J. Hauptman [verfasserIn] A.I. Hernandez [verfasserIn] J.A. Hernando Morata [verfasserIn] V. Herrero [verfasserIn] B.J.P. Jones [verfasserIn] L. Labarga [verfasserIn] A. Laing [verfasserIn] P. Lebrun [verfasserIn] I. Liubarsky [verfasserIn] N. López-March [verfasserIn] M. Losada [verfasserIn] J. Martín-Albo [verfasserIn] G. Martínez-Lema [verfasserIn] A. Martínez [verfasserIn] A.D. McDonald [verfasserIn] F. Monrabal [verfasserIn] F.J. Mora [verfasserIn] L.M. Moutinho [verfasserIn] J. Muñoz Vidal [verfasserIn] M. Musti [verfasserIn] M. Nebot-Guinot [verfasserIn] P. Novella [verfasserIn] D.R. Nygren [verfasserIn] B. Palmeiro [verfasserIn] A. Para [verfasserIn] J. Pérez [verfasserIn] M. Querol [verfasserIn] J. Renner [verfasserIn] L. Ripoll [verfasserIn] J. Rodríguez [verfasserIn] L. Rogers [verfasserIn] F.P. Santos [verfasserIn] J.M.F. dos Santos [verfasserIn] A. Simón [verfasserIn] C. Sofka [verfasserIn] M. Sorel [verfasserIn] T. Stiegler [verfasserIn] J.F. Toledo [verfasserIn] J. Torrent [verfasserIn] Z. Tsamalaidze [verfasserIn] J.F.C.A. Veloso [verfasserIn] R. Webb [verfasserIn] J.T. White [verfasserIn] N. Yahlali [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2017 |
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| Übergeordnetes Werk: |
In: Physics Letters B - Elsevier, 2015, 773(2017), Seite 663-671 |
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| Übergeordnetes Werk: |
volume:773 ; year:2017 ; pages:663-671 |
| Links: |
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| DOI / URN: |
10.1016/j.physletb.2017.09.017 |
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| Katalog-ID: |
DOAJ052426661 |
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| 100 | 0 | |a C.A.O. Henriques |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Secondary scintillation yield of xenon with sub-percent levels of CO2 additive for rare-event detection |
| 264 | 1 | |c 2017 | |
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| 520 | |a Xe–CO2 mixtures are important alternatives to pure xenon in Time Projection Chambers (TPC) based on secondary scintillation (electroluminescence) signal amplification with applications in the important field of rare event detection such as directional dark matter, double electron capture and double beta decay detection. The addition of CO2 to pure xenon at the level of 0.05–0.1% can reduce significantly the scale of electron diffusion from 10 mm/m to 2.5 mm/m, with high impact on the discrimination efficiency of the events through pattern recognition of the topology of primary ionization trails. We have measured the electroluminescence (EL) yield of Xe–CO2 mixtures, with sub-percent CO2 concentrations. We demonstrate that the EL production is still high in these mixtures, 70% and 35% relative to that produced in pure xenon, for CO2 concentrations around 0.05% and 0.1%, respectively. The contribution of the statistical fluctuations in EL production to the energy resolution increases with increasing CO2 concentration, being smaller than the contribution of the Fano factor for concentrations below 0.1% CO2. Keywords: Double beta decay, Neutrino, Rare event detection, Electroluminescence, Secondary scintillation, Xenon | ||
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10.1016/j.physletb.2017.09.017 doi (DE-627)DOAJ052426661 (DE-599)DOAJ0457251c164a4ed0b8935d393646dea9 DE-627 ger DE-627 rakwb eng QC1-999 C.A.O. Henriques verfasserin aut Secondary scintillation yield of xenon with sub-percent levels of CO2 additive for rare-event detection 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Xe–CO2 mixtures are important alternatives to pure xenon in Time Projection Chambers (TPC) based on secondary scintillation (electroluminescence) signal amplification with applications in the important field of rare event detection such as directional dark matter, double electron capture and double beta decay detection. The addition of CO2 to pure xenon at the level of 0.05–0.1% can reduce significantly the scale of electron diffusion from 10 mm/m to 2.5 mm/m, with high impact on the discrimination efficiency of the events through pattern recognition of the topology of primary ionization trails. We have measured the electroluminescence (EL) yield of Xe–CO2 mixtures, with sub-percent CO2 concentrations. We demonstrate that the EL production is still high in these mixtures, 70% and 35% relative to that produced in pure xenon, for CO2 concentrations around 0.05% and 0.1%, respectively. The contribution of the statistical fluctuations in EL production to the energy resolution increases with increasing CO2 concentration, being smaller than the contribution of the Fano factor for concentrations below 0.1% CO2. Keywords: Double beta decay, Neutrino, Rare event detection, Electroluminescence, Secondary scintillation, Xenon Physics E.D.C. Freitas verfasserin aut C.D.R. Azevedo verfasserin aut D. González-Díaz verfasserin aut R.D.P. Mano verfasserin aut M.R. Jorge verfasserin aut L.M.P. Fernandes verfasserin aut C.M.B. Monteiro verfasserin aut J.J. Gómez-Cadenas verfasserin aut V. Álvarez verfasserin aut J.M. Benlloch-Rodríguez verfasserin aut F.I.G.M. Borges verfasserin aut A. Botas verfasserin aut S. Cárcel verfasserin aut J.V. Carríon verfasserin aut S. Cebrían verfasserin aut C.A.N. Conde verfasserin aut J. Díaz verfasserin aut M. Diesburg verfasserin aut R. Esteve verfasserin aut R. Felkai verfasserin aut P. Ferrario verfasserin aut A.L. Ferreira verfasserin aut A. Goldschmidt verfasserin aut R.M. Gutiérrez verfasserin aut J. Hauptman verfasserin aut A.I. Hernandez verfasserin aut J.A. Hernando Morata verfasserin aut V. Herrero verfasserin aut B.J.P. Jones verfasserin aut L. Labarga verfasserin aut A. Laing verfasserin aut P. Lebrun verfasserin aut I. Liubarsky verfasserin aut N. López-March verfasserin aut M. Losada verfasserin aut J. Martín-Albo verfasserin aut G. Martínez-Lema verfasserin aut A. Martínez verfasserin aut A.D. McDonald verfasserin aut F. Monrabal verfasserin aut F.J. Mora verfasserin aut L.M. Moutinho verfasserin aut J. Muñoz Vidal verfasserin aut M. Musti verfasserin aut M. Nebot-Guinot verfasserin aut P. Novella verfasserin aut D.R. Nygren verfasserin aut B. Palmeiro verfasserin aut A. Para verfasserin aut J. Pérez verfasserin aut M. Querol verfasserin aut J. Renner verfasserin aut L. Ripoll verfasserin aut J. Rodríguez verfasserin aut L. Rogers verfasserin aut F.P. Santos verfasserin aut J.M.F. dos Santos verfasserin aut A. Simón verfasserin aut C. Sofka verfasserin aut M. Sorel verfasserin aut T. Stiegler verfasserin aut J.F. Toledo verfasserin aut J. Torrent verfasserin aut Z. Tsamalaidze verfasserin aut J.F.C.A. Veloso verfasserin aut R. Webb verfasserin aut J.T. White verfasserin aut N. Yahlali verfasserin aut In Physics Letters B Elsevier, 2015 773(2017), Seite 663-671 (DE-627)266015360 (DE-600)1466612-1 18732445 nnns volume:773 year:2017 pages:663-671 https://doi.org/10.1016/j.physletb.2017.09.017 kostenfrei https://doaj.org/article/0457251c164a4ed0b8935d393646dea9 kostenfrei http://www.sciencedirect.com/science/article/pii/S0370269317307153 kostenfrei https://doaj.org/toc/0370-2693 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 773 2017 663-671 |
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10.1016/j.physletb.2017.09.017 doi (DE-627)DOAJ052426661 (DE-599)DOAJ0457251c164a4ed0b8935d393646dea9 DE-627 ger DE-627 rakwb eng QC1-999 C.A.O. Henriques verfasserin aut Secondary scintillation yield of xenon with sub-percent levels of CO2 additive for rare-event detection 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Xe–CO2 mixtures are important alternatives to pure xenon in Time Projection Chambers (TPC) based on secondary scintillation (electroluminescence) signal amplification with applications in the important field of rare event detection such as directional dark matter, double electron capture and double beta decay detection. The addition of CO2 to pure xenon at the level of 0.05–0.1% can reduce significantly the scale of electron diffusion from 10 mm/m to 2.5 mm/m, with high impact on the discrimination efficiency of the events through pattern recognition of the topology of primary ionization trails. We have measured the electroluminescence (EL) yield of Xe–CO2 mixtures, with sub-percent CO2 concentrations. We demonstrate that the EL production is still high in these mixtures, 70% and 35% relative to that produced in pure xenon, for CO2 concentrations around 0.05% and 0.1%, respectively. The contribution of the statistical fluctuations in EL production to the energy resolution increases with increasing CO2 concentration, being smaller than the contribution of the Fano factor for concentrations below 0.1% CO2. Keywords: Double beta decay, Neutrino, Rare event detection, Electroluminescence, Secondary scintillation, Xenon Physics E.D.C. Freitas verfasserin aut C.D.R. Azevedo verfasserin aut D. González-Díaz verfasserin aut R.D.P. Mano verfasserin aut M.R. Jorge verfasserin aut L.M.P. Fernandes verfasserin aut C.M.B. Monteiro verfasserin aut J.J. Gómez-Cadenas verfasserin aut V. Álvarez verfasserin aut J.M. Benlloch-Rodríguez verfasserin aut F.I.G.M. Borges verfasserin aut A. Botas verfasserin aut S. Cárcel verfasserin aut J.V. Carríon verfasserin aut S. Cebrían verfasserin aut C.A.N. Conde verfasserin aut J. Díaz verfasserin aut M. Diesburg verfasserin aut R. Esteve verfasserin aut R. Felkai verfasserin aut P. Ferrario verfasserin aut A.L. Ferreira verfasserin aut A. Goldschmidt verfasserin aut R.M. Gutiérrez verfasserin aut J. Hauptman verfasserin aut A.I. Hernandez verfasserin aut J.A. Hernando Morata verfasserin aut V. Herrero verfasserin aut B.J.P. Jones verfasserin aut L. Labarga verfasserin aut A. Laing verfasserin aut P. Lebrun verfasserin aut I. Liubarsky verfasserin aut N. López-March verfasserin aut M. Losada verfasserin aut J. Martín-Albo verfasserin aut G. Martínez-Lema verfasserin aut A. Martínez verfasserin aut A.D. McDonald verfasserin aut F. Monrabal verfasserin aut F.J. Mora verfasserin aut L.M. Moutinho verfasserin aut J. Muñoz Vidal verfasserin aut M. Musti verfasserin aut M. Nebot-Guinot verfasserin aut P. Novella verfasserin aut D.R. Nygren verfasserin aut B. Palmeiro verfasserin aut A. Para verfasserin aut J. Pérez verfasserin aut M. Querol verfasserin aut J. Renner verfasserin aut L. Ripoll verfasserin aut J. Rodríguez verfasserin aut L. Rogers verfasserin aut F.P. Santos verfasserin aut J.M.F. dos Santos verfasserin aut A. Simón verfasserin aut C. Sofka verfasserin aut M. Sorel verfasserin aut T. Stiegler verfasserin aut J.F. Toledo verfasserin aut J. Torrent verfasserin aut Z. Tsamalaidze verfasserin aut J.F.C.A. Veloso verfasserin aut R. Webb verfasserin aut J.T. White verfasserin aut N. Yahlali verfasserin aut In Physics Letters B Elsevier, 2015 773(2017), Seite 663-671 (DE-627)266015360 (DE-600)1466612-1 18732445 nnns volume:773 year:2017 pages:663-671 https://doi.org/10.1016/j.physletb.2017.09.017 kostenfrei https://doaj.org/article/0457251c164a4ed0b8935d393646dea9 kostenfrei http://www.sciencedirect.com/science/article/pii/S0370269317307153 kostenfrei https://doaj.org/toc/0370-2693 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 773 2017 663-671 |
| allfields_unstemmed |
10.1016/j.physletb.2017.09.017 doi (DE-627)DOAJ052426661 (DE-599)DOAJ0457251c164a4ed0b8935d393646dea9 DE-627 ger DE-627 rakwb eng QC1-999 C.A.O. Henriques verfasserin aut Secondary scintillation yield of xenon with sub-percent levels of CO2 additive for rare-event detection 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Xe–CO2 mixtures are important alternatives to pure xenon in Time Projection Chambers (TPC) based on secondary scintillation (electroluminescence) signal amplification with applications in the important field of rare event detection such as directional dark matter, double electron capture and double beta decay detection. The addition of CO2 to pure xenon at the level of 0.05–0.1% can reduce significantly the scale of electron diffusion from 10 mm/m to 2.5 mm/m, with high impact on the discrimination efficiency of the events through pattern recognition of the topology of primary ionization trails. We have measured the electroluminescence (EL) yield of Xe–CO2 mixtures, with sub-percent CO2 concentrations. We demonstrate that the EL production is still high in these mixtures, 70% and 35% relative to that produced in pure xenon, for CO2 concentrations around 0.05% and 0.1%, respectively. The contribution of the statistical fluctuations in EL production to the energy resolution increases with increasing CO2 concentration, being smaller than the contribution of the Fano factor for concentrations below 0.1% CO2. Keywords: Double beta decay, Neutrino, Rare event detection, Electroluminescence, Secondary scintillation, Xenon Physics E.D.C. Freitas verfasserin aut C.D.R. Azevedo verfasserin aut D. González-Díaz verfasserin aut R.D.P. Mano verfasserin aut M.R. Jorge verfasserin aut L.M.P. Fernandes verfasserin aut C.M.B. Monteiro verfasserin aut J.J. Gómez-Cadenas verfasserin aut V. Álvarez verfasserin aut J.M. Benlloch-Rodríguez verfasserin aut F.I.G.M. Borges verfasserin aut A. Botas verfasserin aut S. Cárcel verfasserin aut J.V. Carríon verfasserin aut S. Cebrían verfasserin aut C.A.N. Conde verfasserin aut J. Díaz verfasserin aut M. Diesburg verfasserin aut R. Esteve verfasserin aut R. Felkai verfasserin aut P. Ferrario verfasserin aut A.L. Ferreira verfasserin aut A. Goldschmidt verfasserin aut R.M. Gutiérrez verfasserin aut J. Hauptman verfasserin aut A.I. Hernandez verfasserin aut J.A. Hernando Morata verfasserin aut V. Herrero verfasserin aut B.J.P. Jones verfasserin aut L. Labarga verfasserin aut A. Laing verfasserin aut P. Lebrun verfasserin aut I. Liubarsky verfasserin aut N. López-March verfasserin aut M. Losada verfasserin aut J. Martín-Albo verfasserin aut G. Martínez-Lema verfasserin aut A. Martínez verfasserin aut A.D. McDonald verfasserin aut F. Monrabal verfasserin aut F.J. Mora verfasserin aut L.M. Moutinho verfasserin aut J. Muñoz Vidal verfasserin aut M. Musti verfasserin aut M. Nebot-Guinot verfasserin aut P. Novella verfasserin aut D.R. Nygren verfasserin aut B. Palmeiro verfasserin aut A. Para verfasserin aut J. Pérez verfasserin aut M. Querol verfasserin aut J. Renner verfasserin aut L. Ripoll verfasserin aut J. Rodríguez verfasserin aut L. Rogers verfasserin aut F.P. Santos verfasserin aut J.M.F. dos Santos verfasserin aut A. Simón verfasserin aut C. Sofka verfasserin aut M. Sorel verfasserin aut T. Stiegler verfasserin aut J.F. Toledo verfasserin aut J. Torrent verfasserin aut Z. Tsamalaidze verfasserin aut J.F.C.A. Veloso verfasserin aut R. Webb verfasserin aut J.T. White verfasserin aut N. Yahlali verfasserin aut In Physics Letters B Elsevier, 2015 773(2017), Seite 663-671 (DE-627)266015360 (DE-600)1466612-1 18732445 nnns volume:773 year:2017 pages:663-671 https://doi.org/10.1016/j.physletb.2017.09.017 kostenfrei https://doaj.org/article/0457251c164a4ed0b8935d393646dea9 kostenfrei http://www.sciencedirect.com/science/article/pii/S0370269317307153 kostenfrei https://doaj.org/toc/0370-2693 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 773 2017 663-671 |
| allfieldsGer |
10.1016/j.physletb.2017.09.017 doi (DE-627)DOAJ052426661 (DE-599)DOAJ0457251c164a4ed0b8935d393646dea9 DE-627 ger DE-627 rakwb eng QC1-999 C.A.O. Henriques verfasserin aut Secondary scintillation yield of xenon with sub-percent levels of CO2 additive for rare-event detection 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Xe–CO2 mixtures are important alternatives to pure xenon in Time Projection Chambers (TPC) based on secondary scintillation (electroluminescence) signal amplification with applications in the important field of rare event detection such as directional dark matter, double electron capture and double beta decay detection. The addition of CO2 to pure xenon at the level of 0.05–0.1% can reduce significantly the scale of electron diffusion from 10 mm/m to 2.5 mm/m, with high impact on the discrimination efficiency of the events through pattern recognition of the topology of primary ionization trails. We have measured the electroluminescence (EL) yield of Xe–CO2 mixtures, with sub-percent CO2 concentrations. We demonstrate that the EL production is still high in these mixtures, 70% and 35% relative to that produced in pure xenon, for CO2 concentrations around 0.05% and 0.1%, respectively. The contribution of the statistical fluctuations in EL production to the energy resolution increases with increasing CO2 concentration, being smaller than the contribution of the Fano factor for concentrations below 0.1% CO2. Keywords: Double beta decay, Neutrino, Rare event detection, Electroluminescence, Secondary scintillation, Xenon Physics E.D.C. Freitas verfasserin aut C.D.R. Azevedo verfasserin aut D. González-Díaz verfasserin aut R.D.P. Mano verfasserin aut M.R. Jorge verfasserin aut L.M.P. Fernandes verfasserin aut C.M.B. Monteiro verfasserin aut J.J. Gómez-Cadenas verfasserin aut V. Álvarez verfasserin aut J.M. Benlloch-Rodríguez verfasserin aut F.I.G.M. Borges verfasserin aut A. Botas verfasserin aut S. Cárcel verfasserin aut J.V. Carríon verfasserin aut S. Cebrían verfasserin aut C.A.N. Conde verfasserin aut J. Díaz verfasserin aut M. Diesburg verfasserin aut R. Esteve verfasserin aut R. Felkai verfasserin aut P. Ferrario verfasserin aut A.L. Ferreira verfasserin aut A. Goldschmidt verfasserin aut R.M. Gutiérrez verfasserin aut J. Hauptman verfasserin aut A.I. Hernandez verfasserin aut J.A. Hernando Morata verfasserin aut V. Herrero verfasserin aut B.J.P. Jones verfasserin aut L. Labarga verfasserin aut A. Laing verfasserin aut P. Lebrun verfasserin aut I. Liubarsky verfasserin aut N. López-March verfasserin aut M. Losada verfasserin aut J. Martín-Albo verfasserin aut G. Martínez-Lema verfasserin aut A. Martínez verfasserin aut A.D. McDonald verfasserin aut F. Monrabal verfasserin aut F.J. Mora verfasserin aut L.M. Moutinho verfasserin aut J. Muñoz Vidal verfasserin aut M. Musti verfasserin aut M. Nebot-Guinot verfasserin aut P. Novella verfasserin aut D.R. Nygren verfasserin aut B. Palmeiro verfasserin aut A. Para verfasserin aut J. Pérez verfasserin aut M. Querol verfasserin aut J. Renner verfasserin aut L. Ripoll verfasserin aut J. Rodríguez verfasserin aut L. Rogers verfasserin aut F.P. Santos verfasserin aut J.M.F. dos Santos verfasserin aut A. Simón verfasserin aut C. Sofka verfasserin aut M. Sorel verfasserin aut T. Stiegler verfasserin aut J.F. Toledo verfasserin aut J. Torrent verfasserin aut Z. Tsamalaidze verfasserin aut J.F.C.A. Veloso verfasserin aut R. Webb verfasserin aut J.T. White verfasserin aut N. Yahlali verfasserin aut In Physics Letters B Elsevier, 2015 773(2017), Seite 663-671 (DE-627)266015360 (DE-600)1466612-1 18732445 nnns volume:773 year:2017 pages:663-671 https://doi.org/10.1016/j.physletb.2017.09.017 kostenfrei https://doaj.org/article/0457251c164a4ed0b8935d393646dea9 kostenfrei http://www.sciencedirect.com/science/article/pii/S0370269317307153 kostenfrei https://doaj.org/toc/0370-2693 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 773 2017 663-671 |
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10.1016/j.physletb.2017.09.017 doi (DE-627)DOAJ052426661 (DE-599)DOAJ0457251c164a4ed0b8935d393646dea9 DE-627 ger DE-627 rakwb eng QC1-999 C.A.O. Henriques verfasserin aut Secondary scintillation yield of xenon with sub-percent levels of CO2 additive for rare-event detection 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Xe–CO2 mixtures are important alternatives to pure xenon in Time Projection Chambers (TPC) based on secondary scintillation (electroluminescence) signal amplification with applications in the important field of rare event detection such as directional dark matter, double electron capture and double beta decay detection. The addition of CO2 to pure xenon at the level of 0.05–0.1% can reduce significantly the scale of electron diffusion from 10 mm/m to 2.5 mm/m, with high impact on the discrimination efficiency of the events through pattern recognition of the topology of primary ionization trails. We have measured the electroluminescence (EL) yield of Xe–CO2 mixtures, with sub-percent CO2 concentrations. We demonstrate that the EL production is still high in these mixtures, 70% and 35% relative to that produced in pure xenon, for CO2 concentrations around 0.05% and 0.1%, respectively. The contribution of the statistical fluctuations in EL production to the energy resolution increases with increasing CO2 concentration, being smaller than the contribution of the Fano factor for concentrations below 0.1% CO2. Keywords: Double beta decay, Neutrino, Rare event detection, Electroluminescence, Secondary scintillation, Xenon Physics E.D.C. Freitas verfasserin aut C.D.R. Azevedo verfasserin aut D. González-Díaz verfasserin aut R.D.P. Mano verfasserin aut M.R. Jorge verfasserin aut L.M.P. Fernandes verfasserin aut C.M.B. Monteiro verfasserin aut J.J. Gómez-Cadenas verfasserin aut V. Álvarez verfasserin aut J.M. Benlloch-Rodríguez verfasserin aut F.I.G.M. Borges verfasserin aut A. Botas verfasserin aut S. Cárcel verfasserin aut J.V. Carríon verfasserin aut S. Cebrían verfasserin aut C.A.N. Conde verfasserin aut J. Díaz verfasserin aut M. Diesburg verfasserin aut R. Esteve verfasserin aut R. Felkai verfasserin aut P. Ferrario verfasserin aut A.L. Ferreira verfasserin aut A. Goldschmidt verfasserin aut R.M. Gutiérrez verfasserin aut J. Hauptman verfasserin aut A.I. Hernandez verfasserin aut J.A. Hernando Morata verfasserin aut V. Herrero verfasserin aut B.J.P. Jones verfasserin aut L. Labarga verfasserin aut A. Laing verfasserin aut P. Lebrun verfasserin aut I. Liubarsky verfasserin aut N. López-March verfasserin aut M. Losada verfasserin aut J. Martín-Albo verfasserin aut G. Martínez-Lema verfasserin aut A. Martínez verfasserin aut A.D. McDonald verfasserin aut F. Monrabal verfasserin aut F.J. Mora verfasserin aut L.M. Moutinho verfasserin aut J. Muñoz Vidal verfasserin aut M. Musti verfasserin aut M. Nebot-Guinot verfasserin aut P. Novella verfasserin aut D.R. Nygren verfasserin aut B. Palmeiro verfasserin aut A. Para verfasserin aut J. Pérez verfasserin aut M. Querol verfasserin aut J. Renner verfasserin aut L. Ripoll verfasserin aut J. Rodríguez verfasserin aut L. Rogers verfasserin aut F.P. Santos verfasserin aut J.M.F. dos Santos verfasserin aut A. Simón verfasserin aut C. Sofka verfasserin aut M. Sorel verfasserin aut T. Stiegler verfasserin aut J.F. Toledo verfasserin aut J. Torrent verfasserin aut Z. Tsamalaidze verfasserin aut J.F.C.A. Veloso verfasserin aut R. Webb verfasserin aut J.T. White verfasserin aut N. Yahlali verfasserin aut In Physics Letters B Elsevier, 2015 773(2017), Seite 663-671 (DE-627)266015360 (DE-600)1466612-1 18732445 nnns volume:773 year:2017 pages:663-671 https://doi.org/10.1016/j.physletb.2017.09.017 kostenfrei https://doaj.org/article/0457251c164a4ed0b8935d393646dea9 kostenfrei http://www.sciencedirect.com/science/article/pii/S0370269317307153 kostenfrei https://doaj.org/toc/0370-2693 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_150 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_187 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2014 GBV_ILN_2025 GBV_ILN_2034 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2064 GBV_ILN_2111 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4367 GBV_ILN_4700 AR 773 2017 663-671 |
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C.A.O. Henriques @@aut@@ E.D.C. Freitas @@aut@@ C.D.R. Azevedo @@aut@@ D. González-Díaz @@aut@@ R.D.P. Mano @@aut@@ M.R. Jorge @@aut@@ L.M.P. Fernandes @@aut@@ C.M.B. Monteiro @@aut@@ J.J. Gómez-Cadenas @@aut@@ V. Álvarez @@aut@@ J.M. Benlloch-Rodríguez @@aut@@ F.I.G.M. Borges @@aut@@ A. Botas @@aut@@ S. Cárcel @@aut@@ J.V. Carríon @@aut@@ S. Cebrían @@aut@@ C.A.N. Conde @@aut@@ J. Díaz @@aut@@ M. Diesburg @@aut@@ R. Esteve @@aut@@ R. Felkai @@aut@@ P. Ferrario @@aut@@ A.L. Ferreira @@aut@@ A. Goldschmidt @@aut@@ R.M. Gutiérrez @@aut@@ J. Hauptman @@aut@@ A.I. Hernandez @@aut@@ J.A. Hernando Morata @@aut@@ V. Herrero @@aut@@ B.J.P. Jones @@aut@@ L. Labarga @@aut@@ A. Laing @@aut@@ P. Lebrun @@aut@@ I. Liubarsky @@aut@@ N. López-March @@aut@@ M. Losada @@aut@@ J. Martín-Albo @@aut@@ G. Martínez-Lema @@aut@@ A. Martínez @@aut@@ A.D. McDonald @@aut@@ F. Monrabal @@aut@@ F.J. Mora @@aut@@ L.M. Moutinho @@aut@@ J. Muñoz Vidal @@aut@@ M. Musti @@aut@@ M. Nebot-Guinot @@aut@@ P. Novella @@aut@@ D.R. Nygren @@aut@@ B. Palmeiro @@aut@@ A. Para @@aut@@ J. Pérez @@aut@@ M. Querol @@aut@@ J. Renner @@aut@@ L. Ripoll @@aut@@ J. Rodríguez @@aut@@ L. Rogers @@aut@@ F.P. Santos @@aut@@ J.M.F. dos Santos @@aut@@ A. Simón @@aut@@ C. Sofka @@aut@@ M. Sorel @@aut@@ T. Stiegler @@aut@@ J.F. Toledo @@aut@@ J. Torrent @@aut@@ Z. Tsamalaidze @@aut@@ J.F.C.A. Veloso @@aut@@ R. Webb @@aut@@ J.T. White @@aut@@ N. Yahlali @@aut@@ |
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C.A.O. Henriques E.D.C. Freitas C.D.R. Azevedo D. González-Díaz R.D.P. Mano M.R. Jorge L.M.P. Fernandes C.M.B. Monteiro J.J. Gómez-Cadenas V. Álvarez J.M. Benlloch-Rodríguez F.I.G.M. Borges A. Botas S. Cárcel J.V. Carríon S. Cebrían C.A.N. Conde J. Díaz M. Diesburg R. Esteve R. Felkai P. Ferrario A.L. Ferreira A. Goldschmidt R.M. Gutiérrez J. Hauptman A.I. Hernandez J.A. Hernando Morata V. Herrero B.J.P. Jones L. Labarga A. Laing P. Lebrun I. Liubarsky N. López-March M. Losada J. Martín-Albo G. Martínez-Lema A. Martínez A.D. McDonald F. Monrabal F.J. Mora L.M. Moutinho J. Muñoz Vidal M. Musti M. Nebot-Guinot P. Novella D.R. Nygren B. Palmeiro A. Para J. Pérez M. Querol J. Renner L. Ripoll J. Rodríguez L. Rogers F.P. Santos J.M.F. dos Santos A. Simón C. Sofka M. Sorel T. Stiegler J.F. Toledo J. Torrent Z. Tsamalaidze J.F.C.A. Veloso R. Webb J.T. White N. Yahlali |
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| title_sort |
secondary scintillation yield of xenon with sub-percent levels of co2 additive for rare-event detection |
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Secondary scintillation yield of xenon with sub-percent levels of CO2 additive for rare-event detection |
| abstract |
Xe–CO2 mixtures are important alternatives to pure xenon in Time Projection Chambers (TPC) based on secondary scintillation (electroluminescence) signal amplification with applications in the important field of rare event detection such as directional dark matter, double electron capture and double beta decay detection. The addition of CO2 to pure xenon at the level of 0.05–0.1% can reduce significantly the scale of electron diffusion from 10 mm/m to 2.5 mm/m, with high impact on the discrimination efficiency of the events through pattern recognition of the topology of primary ionization trails. We have measured the electroluminescence (EL) yield of Xe–CO2 mixtures, with sub-percent CO2 concentrations. We demonstrate that the EL production is still high in these mixtures, 70% and 35% relative to that produced in pure xenon, for CO2 concentrations around 0.05% and 0.1%, respectively. The contribution of the statistical fluctuations in EL production to the energy resolution increases with increasing CO2 concentration, being smaller than the contribution of the Fano factor for concentrations below 0.1% CO2. Keywords: Double beta decay, Neutrino, Rare event detection, Electroluminescence, Secondary scintillation, Xenon |
| abstractGer |
Xe–CO2 mixtures are important alternatives to pure xenon in Time Projection Chambers (TPC) based on secondary scintillation (electroluminescence) signal amplification with applications in the important field of rare event detection such as directional dark matter, double electron capture and double beta decay detection. The addition of CO2 to pure xenon at the level of 0.05–0.1% can reduce significantly the scale of electron diffusion from 10 mm/m to 2.5 mm/m, with high impact on the discrimination efficiency of the events through pattern recognition of the topology of primary ionization trails. We have measured the electroluminescence (EL) yield of Xe–CO2 mixtures, with sub-percent CO2 concentrations. We demonstrate that the EL production is still high in these mixtures, 70% and 35% relative to that produced in pure xenon, for CO2 concentrations around 0.05% and 0.1%, respectively. The contribution of the statistical fluctuations in EL production to the energy resolution increases with increasing CO2 concentration, being smaller than the contribution of the Fano factor for concentrations below 0.1% CO2. Keywords: Double beta decay, Neutrino, Rare event detection, Electroluminescence, Secondary scintillation, Xenon |
| abstract_unstemmed |
Xe–CO2 mixtures are important alternatives to pure xenon in Time Projection Chambers (TPC) based on secondary scintillation (electroluminescence) signal amplification with applications in the important field of rare event detection such as directional dark matter, double electron capture and double beta decay detection. The addition of CO2 to pure xenon at the level of 0.05–0.1% can reduce significantly the scale of electron diffusion from 10 mm/m to 2.5 mm/m, with high impact on the discrimination efficiency of the events through pattern recognition of the topology of primary ionization trails. We have measured the electroluminescence (EL) yield of Xe–CO2 mixtures, with sub-percent CO2 concentrations. We demonstrate that the EL production is still high in these mixtures, 70% and 35% relative to that produced in pure xenon, for CO2 concentrations around 0.05% and 0.1%, respectively. The contribution of the statistical fluctuations in EL production to the energy resolution increases with increasing CO2 concentration, being smaller than the contribution of the Fano factor for concentrations below 0.1% CO2. Keywords: Double beta decay, Neutrino, Rare event detection, Electroluminescence, Secondary scintillation, Xenon |
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Secondary scintillation yield of xenon with sub-percent levels of CO2 additive for rare-event detection |
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E.D.C. Freitas C.D.R. Azevedo D. González-Díaz R.D.P. Mano M.R. Jorge L.M.P. Fernandes C.M.B. Monteiro J.J. Gómez-Cadenas V. Álvarez J.M. Benlloch-Rodríguez F.I.G.M. Borges A. Botas S. Cárcel J.V. Carríon S. Cebrían C.A.N. Conde J. Díaz M. Diesburg R. Esteve R. Felkai P. Ferrario A.L. Ferreira A. Goldschmidt R.M. Gutiérrez J. Hauptman A.I. Hernandez J.A. Hernando Morata V. Herrero B.J.P. Jones L. Labarga A. Laing P. Lebrun I. Liubarsky N. López-March M. Losada J. Martín-Albo G. Martínez-Lema A. Martínez A.D. McDonald F. Monrabal F.J. Mora L.M. Moutinho J. Muñoz Vidal M. Musti M. Nebot-Guinot P. Novella D.R. Nygren B. Palmeiro A. Para J. Pérez M. Querol J. Renner L. Ripoll J. Rodríguez L. Rogers F.P. Santos J.M.F. dos Santos A. Simón C. Sofka M. Sorel T. Stiegler J.F. Toledo J. Torrent Z. Tsamalaidze J.F.C.A. Veloso R. Webb J.T. White N. Yahlali |
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E.D.C. Freitas C.D.R. Azevedo D. González-Díaz R.D.P. Mano M.R. Jorge L.M.P. Fernandes C.M.B. Monteiro J.J. Gómez-Cadenas V. Álvarez J.M. Benlloch-Rodríguez F.I.G.M. Borges A. Botas S. Cárcel J.V. Carríon S. Cebrían C.A.N. Conde J. Díaz M. Diesburg R. Esteve R. Felkai P. Ferrario A.L. Ferreira A. Goldschmidt R.M. Gutiérrez J. Hauptman A.I. Hernandez J.A. Hernando Morata V. Herrero B.J.P. Jones L. Labarga A. Laing P. Lebrun I. Liubarsky N. López-March M. Losada J. Martín-Albo G. Martínez-Lema A. Martínez A.D. McDonald F. Monrabal F.J. Mora L.M. Moutinho J. Muñoz Vidal M. Musti M. Nebot-Guinot P. Novella D.R. Nygren B. Palmeiro A. Para J. Pérez M. Querol J. Renner L. Ripoll J. Rodríguez L. Rogers F.P. Santos J.M.F. dos Santos A. Simón C. Sofka M. Sorel T. Stiegler J.F. Toledo J. Torrent Z. Tsamalaidze J.F.C.A. Veloso R. Webb J.T. White N. Yahlali |
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Henriques</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Secondary scintillation yield of xenon with sub-percent levels of CO2 additive for rare-event detection</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2017</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">Computermedien</subfield><subfield code="b">c</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Online-Ressource</subfield><subfield code="b">cr</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Xe–CO2 mixtures are important alternatives to pure xenon in Time Projection Chambers (TPC) based on secondary scintillation (electroluminescence) signal amplification with applications in the important field of rare event detection such as directional dark matter, double electron capture and double beta decay detection. 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|
| score |
7.39956 |