Results from the OPERA Experiment in the CNGS Beam

The OPERA experiment was designed to observe <inline-formula< <math display="inline"< <semantics< <mrow< <msub< <mi<ν</mi< <mi<μ</mi< </msub< <mo<→</mo< <msub< <mi<ν</mi< <mi<τ</mi< </m...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Alessandro Paoloni [verfasserIn] on Behalf of OPERA Collaboration [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2018

Schlagwörter:	neutrino oscillations OPERA experiment Tau neutrino cross section cosmic ray physics

Übergeordnetes Werk:	In: Universe - MDPI AG, 2015, 4(2018), 12, p 143
Übergeordnetes Werk:	volume:4 ; year:2018 ; number:12, p 143

Links:	Link aufrufen Link aufrufen Link aufrufen Journal toc

DOI / URN:	10.3390/universe4120143

Katalog-ID:	DOAJ084743778

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spelling	10.3390/universe4120143 doi (DE-627)DOAJ084743778 (DE-599)DOAJ8b7b2f00c36142d0a0ade5e09b6d638e DE-627 ger DE-627 rakwb eng QC793-793.5 Alessandro Paoloni verfasserin aut Results from the OPERA Experiment in the CNGS Beam 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The OPERA experiment was designed to observe <inline-formula< <math display="inline"< <semantics< <mrow< <msub< <mi<ν</mi< <mi<μ</mi< </msub< <mo<→</mo< <msub< <mi<ν</mi< <mi<τ</mi< </msub< </mrow< </semantics< </math< </inline-formula< oscillations through <inline-formula< <math display="inline"< <semantics< <mi<τ</mi< </semantics< </math< </inline-formula< appearance on the CERN Neutrino to Gran Sasso (CNGS) beam over a baseline of 730 km. OPERA was a hybrid experiment composed of lead plates and emulsion layers acting as a target for neutrino interactions. The experiment was complemented with electronic detectors: scintillator strips used as Target Trackers and muon spectrometers. A review of the OPERA final results is presented in this paper. neutrino oscillations OPERA experiment Tau neutrino cross section cosmic ray physics Elementary particle physics on Behalf of OPERA Collaboration verfasserin aut In Universe MDPI AG, 2015 4(2018), 12, p 143 (DE-627)820684236 (DE-600)2813994-X 22181997 nnns volume:4 year:2018 number:12, p 143 https://doi.org/10.3390/universe4120143 kostenfrei https://doaj.org/article/8b7b2f00c36142d0a0ade5e09b6d638e kostenfrei https://www.mdpi.com/2218-1997/4/12/143 kostenfrei https://doaj.org/toc/2218-1997 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 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 4 2018 12, p 143
allfields_unstemmed	10.3390/universe4120143 doi (DE-627)DOAJ084743778 (DE-599)DOAJ8b7b2f00c36142d0a0ade5e09b6d638e DE-627 ger DE-627 rakwb eng QC793-793.5 Alessandro Paoloni verfasserin aut Results from the OPERA Experiment in the CNGS Beam 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The OPERA experiment was designed to observe <inline-formula< <math display="inline"< <semantics< <mrow< <msub< <mi<ν</mi< <mi<μ</mi< </msub< <mo<→</mo< <msub< <mi<ν</mi< <mi<τ</mi< </msub< </mrow< </semantics< </math< </inline-formula< oscillations through <inline-formula< <math display="inline"< <semantics< <mi<τ</mi< </semantics< </math< </inline-formula< appearance on the CERN Neutrino to Gran Sasso (CNGS) beam over a baseline of 730 km. OPERA was a hybrid experiment composed of lead plates and emulsion layers acting as a target for neutrino interactions. The experiment was complemented with electronic detectors: scintillator strips used as Target Trackers and muon spectrometers. A review of the OPERA final results is presented in this paper. neutrino oscillations OPERA experiment Tau neutrino cross section cosmic ray physics Elementary particle physics on Behalf of OPERA Collaboration verfasserin aut In Universe MDPI AG, 2015 4(2018), 12, p 143 (DE-627)820684236 (DE-600)2813994-X 22181997 nnns volume:4 year:2018 number:12, p 143 https://doi.org/10.3390/universe4120143 kostenfrei https://doaj.org/article/8b7b2f00c36142d0a0ade5e09b6d638e kostenfrei https://www.mdpi.com/2218-1997/4/12/143 kostenfrei https://doaj.org/toc/2218-1997 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 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 4 2018 12, p 143
allfieldsGer	10.3390/universe4120143 doi (DE-627)DOAJ084743778 (DE-599)DOAJ8b7b2f00c36142d0a0ade5e09b6d638e DE-627 ger DE-627 rakwb eng QC793-793.5 Alessandro Paoloni verfasserin aut Results from the OPERA Experiment in the CNGS Beam 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The OPERA experiment was designed to observe <inline-formula< <math display="inline"< <semantics< <mrow< <msub< <mi<ν</mi< <mi<μ</mi< </msub< <mo<→</mo< <msub< <mi<ν</mi< <mi<τ</mi< </msub< </mrow< </semantics< </math< </inline-formula< oscillations through <inline-formula< <math display="inline"< <semantics< <mi<τ</mi< </semantics< </math< </inline-formula< appearance on the CERN Neutrino to Gran Sasso (CNGS) beam over a baseline of 730 km. OPERA was a hybrid experiment composed of lead plates and emulsion layers acting as a target for neutrino interactions. The experiment was complemented with electronic detectors: scintillator strips used as Target Trackers and muon spectrometers. A review of the OPERA final results is presented in this paper. neutrino oscillations OPERA experiment Tau neutrino cross section cosmic ray physics Elementary particle physics on Behalf of OPERA Collaboration verfasserin aut In Universe MDPI AG, 2015 4(2018), 12, p 143 (DE-627)820684236 (DE-600)2813994-X 22181997 nnns volume:4 year:2018 number:12, p 143 https://doi.org/10.3390/universe4120143 kostenfrei https://doaj.org/article/8b7b2f00c36142d0a0ade5e09b6d638e kostenfrei https://www.mdpi.com/2218-1997/4/12/143 kostenfrei https://doaj.org/toc/2218-1997 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 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 4 2018 12, p 143
allfieldsSound	10.3390/universe4120143 doi (DE-627)DOAJ084743778 (DE-599)DOAJ8b7b2f00c36142d0a0ade5e09b6d638e DE-627 ger DE-627 rakwb eng QC793-793.5 Alessandro Paoloni verfasserin aut Results from the OPERA Experiment in the CNGS Beam 2018 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier The OPERA experiment was designed to observe <inline-formula< <math display="inline"< <semantics< <mrow< <msub< <mi<ν</mi< <mi<μ</mi< </msub< <mo<→</mo< <msub< <mi<ν</mi< <mi<τ</mi< </msub< </mrow< </semantics< </math< </inline-formula< oscillations through <inline-formula< <math display="inline"< <semantics< <mi<τ</mi< </semantics< </math< </inline-formula< appearance on the CERN Neutrino to Gran Sasso (CNGS) beam over a baseline of 730 km. OPERA was a hybrid experiment composed of lead plates and emulsion layers acting as a target for neutrino interactions. The experiment was complemented with electronic detectors: scintillator strips used as Target Trackers and muon spectrometers. A review of the OPERA final results is presented in this paper. neutrino oscillations OPERA experiment Tau neutrino cross section cosmic ray physics Elementary particle physics on Behalf of OPERA Collaboration verfasserin aut In Universe MDPI AG, 2015 4(2018), 12, p 143 (DE-627)820684236 (DE-600)2813994-X 22181997 nnns volume:4 year:2018 number:12, p 143 https://doi.org/10.3390/universe4120143 kostenfrei https://doaj.org/article/8b7b2f00c36142d0a0ade5e09b6d638e kostenfrei https://www.mdpi.com/2218-1997/4/12/143 kostenfrei https://doaj.org/toc/2218-1997 Journal toc kostenfrei GBV_USEFLAG_A SYSFLAG_A GBV_DOAJ GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 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_95 GBV_ILN_105 GBV_ILN_110 GBV_ILN_151 GBV_ILN_161 GBV_ILN_170 GBV_ILN_213 GBV_ILN_230 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_2014 GBV_ILN_4012 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4249 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 4 2018 12, p 143
language	English
source	In Universe 4(2018), 12, p 143 volume:4 year:2018 number:12, p 143
sourceStr	In Universe 4(2018), 12, p 143 volume:4 year:2018 number:12, p 143
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institution	findex.gbv.de
topic_facet	neutrino oscillations OPERA experiment Tau neutrino cross section cosmic ray physics Elementary particle physics
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container_title	Universe
authorswithroles_txt_mv	Alessandro Paoloni @@aut@@ on Behalf of OPERA Collaboration @@aut@@
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callnumber-first	Q - Science
author	Alessandro Paoloni
spellingShingle	Alessandro Paoloni misc QC793-793.5 misc neutrino oscillations misc OPERA experiment misc Tau neutrino cross section misc cosmic ray physics misc Elementary particle physics Results from the OPERA Experiment in the CNGS Beam
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topic_title	QC793-793.5 Results from the OPERA Experiment in the CNGS Beam neutrino oscillations OPERA experiment Tau neutrino cross section cosmic ray physics
topic	misc QC793-793.5 misc neutrino oscillations misc OPERA experiment misc Tau neutrino cross section misc cosmic ray physics misc Elementary particle physics
topic_unstemmed	misc QC793-793.5 misc neutrino oscillations misc OPERA experiment misc Tau neutrino cross section misc cosmic ray physics misc Elementary particle physics
topic_browse	misc QC793-793.5 misc neutrino oscillations misc OPERA experiment misc Tau neutrino cross section misc cosmic ray physics misc Elementary particle physics
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title	Results from the OPERA Experiment in the CNGS Beam
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title_full	Results from the OPERA Experiment in the CNGS Beam
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title_sort	results from the opera experiment in the cngs beam
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title_auth	Results from the OPERA Experiment in the CNGS Beam
abstract	The OPERA experiment was designed to observe <inline-formula< <math display="inline"< <semantics< <mrow< <msub< <mi<ν</mi< <mi<μ</mi< </msub< <mo<→</mo< <msub< <mi<ν</mi< <mi<τ</mi< </msub< </mrow< </semantics< </math< </inline-formula< oscillations through <inline-formula< <math display="inline"< <semantics< <mi<τ</mi< </semantics< </math< </inline-formula< appearance on the CERN Neutrino to Gran Sasso (CNGS) beam over a baseline of 730 km. OPERA was a hybrid experiment composed of lead plates and emulsion layers acting as a target for neutrino interactions. The experiment was complemented with electronic detectors: scintillator strips used as Target Trackers and muon spectrometers. A review of the OPERA final results is presented in this paper.
abstractGer	The OPERA experiment was designed to observe <inline-formula< <math display="inline"< <semantics< <mrow< <msub< <mi<ν</mi< <mi<μ</mi< </msub< <mo<→</mo< <msub< <mi<ν</mi< <mi<τ</mi< </msub< </mrow< </semantics< </math< </inline-formula< oscillations through <inline-formula< <math display="inline"< <semantics< <mi<τ</mi< </semantics< </math< </inline-formula< appearance on the CERN Neutrino to Gran Sasso (CNGS) beam over a baseline of 730 km. OPERA was a hybrid experiment composed of lead plates and emulsion layers acting as a target for neutrino interactions. The experiment was complemented with electronic detectors: scintillator strips used as Target Trackers and muon spectrometers. A review of the OPERA final results is presented in this paper.
abstract_unstemmed	The OPERA experiment was designed to observe <inline-formula< <math display="inline"< <semantics< <mrow< <msub< <mi<ν</mi< <mi<μ</mi< </msub< <mo<→</mo< <msub< <mi<ν</mi< <mi<τ</mi< </msub< </mrow< </semantics< </math< </inline-formula< oscillations through <inline-formula< <math display="inline"< <semantics< <mi<τ</mi< </semantics< </math< </inline-formula< appearance on the CERN Neutrino to Gran Sasso (CNGS) beam over a baseline of 730 km. OPERA was a hybrid experiment composed of lead plates and emulsion layers acting as a target for neutrino interactions. The experiment was complemented with electronic detectors: scintillator strips used as Target Trackers and muon spectrometers. A review of the OPERA final results is presented in this paper.
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