Liquid Helium and Liquid Neon-Sensitive, Low Background Scintillation Media for the Detection of Low Energy Neutrinos
Abstract The use of liquid helium and neon as scintillators for neutrino detection is investigated. Several unique properties of these cryogens make them promising candidates for real-time solar neutrino spectroscopy: large ultraviolet scintillation yields from ionizing radiation, transparency to th...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
McKinsey, D. N. [verfasserIn] |
|---|
| Format: |
Artikel |
|---|---|
| Sprache: |
Englisch |
| Erschienen: |
2000 |
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| Schlagwörter: |
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| Anmerkung: |
© Plenum Publishing Corporation 2000 |
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| Übergeordnetes Werk: |
Enthalten in: Journal of low temperature physics - Kluwer Academic Publishers-Plenum Publishers, 1969, 118(2000), 3-4 vom: Feb., Seite 153-165 |
|---|---|
| Übergeordnetes Werk: |
volume:118 ; year:2000 ; number:3-4 ; month:02 ; pages:153-165 |
| Links: |
|---|
| DOI / URN: |
10.1023/A:1004690906370 |
|---|
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OLC2036787851 |
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| 520 | |a Abstract The use of liquid helium and neon as scintillators for neutrino detection is investigated. Several unique properties of these cryogens make them promising candidates for real-time solar neutrino spectroscopy: large ultraviolet scintillation yields from ionizing radiation, transparency to their own scintillation light, and low levels of radioactive impurities. When neutrinos scatter from electrons in liquid helium or neon, ultraviolet light is emitted. The ultraviolet scintillation light can be efficiently converted to the visible with wavelength shifting films. In this way the neutrino-electron scattering events can be detected by photomultiplier tubes at room temperature. We conclude that the solar neutrino flux from the p+p→$ e^{+} $+d+νe reaction could be characterized and monitored versus time using a 10 ton mass of liquid helium or neon as a scintillation target. | ||
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10.1023/A:1004690906370 doi (DE-627)OLC2036787851 (DE-He213)A:1004690906370-p DE-627 ger DE-627 rakwb eng 530 VZ McKinsey, D. N. verfasserin aut Liquid Helium and Liquid Neon-Sensitive, Low Background Scintillation Media for the Detection of Low Energy Neutrinos 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Plenum Publishing Corporation 2000 Abstract The use of liquid helium and neon as scintillators for neutrino detection is investigated. Several unique properties of these cryogens make them promising candidates for real-time solar neutrino spectroscopy: large ultraviolet scintillation yields from ionizing radiation, transparency to their own scintillation light, and low levels of radioactive impurities. When neutrinos scatter from electrons in liquid helium or neon, ultraviolet light is emitted. The ultraviolet scintillation light can be efficiently converted to the visible with wavelength shifting films. In this way the neutrino-electron scattering events can be detected by photomultiplier tubes at room temperature. We conclude that the solar neutrino flux from the p+p→$ e^{+} $+d+νe reaction could be characterized and monitored versus time using a 10 ton mass of liquid helium or neon as a scintillation target. Neon Ultraviolet Light Liquid Helium Photomultiplier Tube Solar Neutrino Doyle, J. M. aut Enthalten in Journal of low temperature physics Kluwer Academic Publishers-Plenum Publishers, 1969 118(2000), 3-4 vom: Feb., Seite 153-165 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:118 year:2000 number:3-4 month:02 pages:153-165 https://doi.org/10.1023/A:1004690906370 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_20 GBV_ILN_22 GBV_ILN_32 GBV_ILN_40 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2005 GBV_ILN_2185 GBV_ILN_4082 GBV_ILN_4126 GBV_ILN_4306 GBV_ILN_4323 GBV_ILN_4700 AR 118 2000 3-4 02 153-165 |
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10.1023/A:1004690906370 doi (DE-627)OLC2036787851 (DE-He213)A:1004690906370-p DE-627 ger DE-627 rakwb eng 530 VZ McKinsey, D. N. verfasserin aut Liquid Helium and Liquid Neon-Sensitive, Low Background Scintillation Media for the Detection of Low Energy Neutrinos 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Plenum Publishing Corporation 2000 Abstract The use of liquid helium and neon as scintillators for neutrino detection is investigated. Several unique properties of these cryogens make them promising candidates for real-time solar neutrino spectroscopy: large ultraviolet scintillation yields from ionizing radiation, transparency to their own scintillation light, and low levels of radioactive impurities. When neutrinos scatter from electrons in liquid helium or neon, ultraviolet light is emitted. The ultraviolet scintillation light can be efficiently converted to the visible with wavelength shifting films. In this way the neutrino-electron scattering events can be detected by photomultiplier tubes at room temperature. We conclude that the solar neutrino flux from the p+p→$ e^{+} $+d+νe reaction could be characterized and monitored versus time using a 10 ton mass of liquid helium or neon as a scintillation target. Neon Ultraviolet Light Liquid Helium Photomultiplier Tube Solar Neutrino Doyle, J. M. aut Enthalten in Journal of low temperature physics Kluwer Academic Publishers-Plenum Publishers, 1969 118(2000), 3-4 vom: Feb., Seite 153-165 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:118 year:2000 number:3-4 month:02 pages:153-165 https://doi.org/10.1023/A:1004690906370 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_20 GBV_ILN_22 GBV_ILN_32 GBV_ILN_40 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2005 GBV_ILN_2185 GBV_ILN_4082 GBV_ILN_4126 GBV_ILN_4306 GBV_ILN_4323 GBV_ILN_4700 AR 118 2000 3-4 02 153-165 |
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10.1023/A:1004690906370 doi (DE-627)OLC2036787851 (DE-He213)A:1004690906370-p DE-627 ger DE-627 rakwb eng 530 VZ McKinsey, D. N. verfasserin aut Liquid Helium and Liquid Neon-Sensitive, Low Background Scintillation Media for the Detection of Low Energy Neutrinos 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Plenum Publishing Corporation 2000 Abstract The use of liquid helium and neon as scintillators for neutrino detection is investigated. Several unique properties of these cryogens make them promising candidates for real-time solar neutrino spectroscopy: large ultraviolet scintillation yields from ionizing radiation, transparency to their own scintillation light, and low levels of radioactive impurities. When neutrinos scatter from electrons in liquid helium or neon, ultraviolet light is emitted. The ultraviolet scintillation light can be efficiently converted to the visible with wavelength shifting films. In this way the neutrino-electron scattering events can be detected by photomultiplier tubes at room temperature. We conclude that the solar neutrino flux from the p+p→$ e^{+} $+d+νe reaction could be characterized and monitored versus time using a 10 ton mass of liquid helium or neon as a scintillation target. Neon Ultraviolet Light Liquid Helium Photomultiplier Tube Solar Neutrino Doyle, J. M. aut Enthalten in Journal of low temperature physics Kluwer Academic Publishers-Plenum Publishers, 1969 118(2000), 3-4 vom: Feb., Seite 153-165 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:118 year:2000 number:3-4 month:02 pages:153-165 https://doi.org/10.1023/A:1004690906370 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_20 GBV_ILN_22 GBV_ILN_32 GBV_ILN_40 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2005 GBV_ILN_2185 GBV_ILN_4082 GBV_ILN_4126 GBV_ILN_4306 GBV_ILN_4323 GBV_ILN_4700 AR 118 2000 3-4 02 153-165 |
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10.1023/A:1004690906370 doi (DE-627)OLC2036787851 (DE-He213)A:1004690906370-p DE-627 ger DE-627 rakwb eng 530 VZ McKinsey, D. N. verfasserin aut Liquid Helium and Liquid Neon-Sensitive, Low Background Scintillation Media for the Detection of Low Energy Neutrinos 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Plenum Publishing Corporation 2000 Abstract The use of liquid helium and neon as scintillators for neutrino detection is investigated. Several unique properties of these cryogens make them promising candidates for real-time solar neutrino spectroscopy: large ultraviolet scintillation yields from ionizing radiation, transparency to their own scintillation light, and low levels of radioactive impurities. When neutrinos scatter from electrons in liquid helium or neon, ultraviolet light is emitted. The ultraviolet scintillation light can be efficiently converted to the visible with wavelength shifting films. In this way the neutrino-electron scattering events can be detected by photomultiplier tubes at room temperature. We conclude that the solar neutrino flux from the p+p→$ e^{+} $+d+νe reaction could be characterized and monitored versus time using a 10 ton mass of liquid helium or neon as a scintillation target. Neon Ultraviolet Light Liquid Helium Photomultiplier Tube Solar Neutrino Doyle, J. M. aut Enthalten in Journal of low temperature physics Kluwer Academic Publishers-Plenum Publishers, 1969 118(2000), 3-4 vom: Feb., Seite 153-165 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:118 year:2000 number:3-4 month:02 pages:153-165 https://doi.org/10.1023/A:1004690906370 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_20 GBV_ILN_22 GBV_ILN_32 GBV_ILN_40 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2005 GBV_ILN_2185 GBV_ILN_4082 GBV_ILN_4126 GBV_ILN_4306 GBV_ILN_4323 GBV_ILN_4700 AR 118 2000 3-4 02 153-165 |
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10.1023/A:1004690906370 doi (DE-627)OLC2036787851 (DE-He213)A:1004690906370-p DE-627 ger DE-627 rakwb eng 530 VZ McKinsey, D. N. verfasserin aut Liquid Helium and Liquid Neon-Sensitive, Low Background Scintillation Media for the Detection of Low Energy Neutrinos 2000 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Plenum Publishing Corporation 2000 Abstract The use of liquid helium and neon as scintillators for neutrino detection is investigated. Several unique properties of these cryogens make them promising candidates for real-time solar neutrino spectroscopy: large ultraviolet scintillation yields from ionizing radiation, transparency to their own scintillation light, and low levels of radioactive impurities. When neutrinos scatter from electrons in liquid helium or neon, ultraviolet light is emitted. The ultraviolet scintillation light can be efficiently converted to the visible with wavelength shifting films. In this way the neutrino-electron scattering events can be detected by photomultiplier tubes at room temperature. We conclude that the solar neutrino flux from the p+p→$ e^{+} $+d+νe reaction could be characterized and monitored versus time using a 10 ton mass of liquid helium or neon as a scintillation target. Neon Ultraviolet Light Liquid Helium Photomultiplier Tube Solar Neutrino Doyle, J. M. aut Enthalten in Journal of low temperature physics Kluwer Academic Publishers-Plenum Publishers, 1969 118(2000), 3-4 vom: Feb., Seite 153-165 (DE-627)129546267 (DE-600)218311-0 (DE-576)014996642 0022-2291 nnns volume:118 year:2000 number:3-4 month:02 pages:153-165 https://doi.org/10.1023/A:1004690906370 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_20 GBV_ILN_22 GBV_ILN_32 GBV_ILN_40 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2005 GBV_ILN_2185 GBV_ILN_4082 GBV_ILN_4126 GBV_ILN_4306 GBV_ILN_4323 GBV_ILN_4700 AR 118 2000 3-4 02 153-165 |
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Liquid Helium and Liquid Neon-Sensitive, Low Background Scintillation Media for the Detection of Low Energy Neutrinos |
| abstract |
Abstract The use of liquid helium and neon as scintillators for neutrino detection is investigated. Several unique properties of these cryogens make them promising candidates for real-time solar neutrino spectroscopy: large ultraviolet scintillation yields from ionizing radiation, transparency to their own scintillation light, and low levels of radioactive impurities. When neutrinos scatter from electrons in liquid helium or neon, ultraviolet light is emitted. The ultraviolet scintillation light can be efficiently converted to the visible with wavelength shifting films. In this way the neutrino-electron scattering events can be detected by photomultiplier tubes at room temperature. We conclude that the solar neutrino flux from the p+p→$ e^{+} $+d+νe reaction could be characterized and monitored versus time using a 10 ton mass of liquid helium or neon as a scintillation target. © Plenum Publishing Corporation 2000 |
| abstractGer |
Abstract The use of liquid helium and neon as scintillators for neutrino detection is investigated. Several unique properties of these cryogens make them promising candidates for real-time solar neutrino spectroscopy: large ultraviolet scintillation yields from ionizing radiation, transparency to their own scintillation light, and low levels of radioactive impurities. When neutrinos scatter from electrons in liquid helium or neon, ultraviolet light is emitted. The ultraviolet scintillation light can be efficiently converted to the visible with wavelength shifting films. In this way the neutrino-electron scattering events can be detected by photomultiplier tubes at room temperature. We conclude that the solar neutrino flux from the p+p→$ e^{+} $+d+νe reaction could be characterized and monitored versus time using a 10 ton mass of liquid helium or neon as a scintillation target. © Plenum Publishing Corporation 2000 |
| abstract_unstemmed |
Abstract The use of liquid helium and neon as scintillators for neutrino detection is investigated. Several unique properties of these cryogens make them promising candidates for real-time solar neutrino spectroscopy: large ultraviolet scintillation yields from ionizing radiation, transparency to their own scintillation light, and low levels of radioactive impurities. When neutrinos scatter from electrons in liquid helium or neon, ultraviolet light is emitted. The ultraviolet scintillation light can be efficiently converted to the visible with wavelength shifting films. In this way the neutrino-electron scattering events can be detected by photomultiplier tubes at room temperature. We conclude that the solar neutrino flux from the p+p→$ e^{+} $+d+νe reaction could be characterized and monitored versus time using a 10 ton mass of liquid helium or neon as a scintillation target. © Plenum Publishing Corporation 2000 |
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GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_20 GBV_ILN_22 GBV_ILN_32 GBV_ILN_40 GBV_ILN_70 GBV_ILN_170 GBV_ILN_2005 GBV_ILN_2185 GBV_ILN_4082 GBV_ILN_4126 GBV_ILN_4306 GBV_ILN_4323 GBV_ILN_4700 |
| container_issue |
3-4 |
| title_short |
Liquid Helium and Liquid Neon-Sensitive, Low Background Scintillation Media for the Detection of Low Energy Neutrinos |
| url |
https://doi.org/10.1023/A:1004690906370 |
| remote_bool |
false |
| author2 |
Doyle, J. M. |
| author2Str |
Doyle, J. M. |
| ppnlink |
129546267 |
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| hochschulschrift_bool |
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| doi_str |
10.1023/A:1004690906370 |
| up_date |
2024-07-04T04:11:23.617Z |
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7.402173 |