Search for "anomalies" from neutrino and anti-neutrino oscillations at Delta_m^2 ~ 1eV^2 with muon spectrometers and large LAr-TPC imaging detectors

Antonello, M.; Bagliani, D.; Baibussinov, B.; Bilokon, H.; Boffelli, F.; Bonesini, M.; Calligarich, E.; Canci, N.; Centro, S.; Cesana, A.; Cieślik, K.; Cline, D.; Cocco, A. G.; Dequal, Daniele; Dermenev, A.; Dolfini, R.; Gerone, M. De; Dussoni, S.; Farnese, C.; Fava, A.; Ferrari, A.; Fiorillo, G.; Garvey, G. T.; Gatti, F.; Gibin, D.; Gninenko, S.; Guber, F.F.; Guglielmi, A.; Haranczyk, M.; Holeczek, J.; Ivashkin, A.; Kirsanov, M.; Kisiel, J.; Kochanek, I.; Kurepin, A.; Łagoda, J.; Lucchini, G.; Louis, W.C.; Mania, S.; Mannocchi, G.; Marchini, S.; Матвеев, В.А.; Menegolli, A.; Meng, G.; Mills, G. B.; Montanari, C.; Nicoletto, M.; Otwinowski, S.; Palczewski, T.; Passardi, G.; Perfetto, F.; Picchi, P.; Pietropaolo, F.; Płoński, P.; Rappoldi, A.; Raselli, G. L.; Rossella, M.; Rubbia, C.; Sala, P.; Scaramelli, A.; Segreto, E.; Stefan, D.; Steṕaniak, J.; Sulej, R.; Суворова, О. В.; Terrani, M.; Tlisov, D.; Water, R. G. Van de; Trinchero, G.; Turcato, M.; Varanini, F.; Ventura, S.; Vignoli, C.; Wang, H. G.; Yang, Xinzheng; Zani, A.; Заремба, К.; Benettoni, M.; Bernardini, P.; Bertolin, A.; Bozza, C.; Brugnera, R.; Cecchetti, A.; Cecchini, S.; Collazuol, G.; Creti, P.; Corso, F. Dal; Mitri, I. De; Robertis, G. De; Serio, M. De; Esposti, L. Degli; Ferdinando, D. Di; Dore, U.; Dusini, S.; Fabbricatore, P.; Fanin, C.; Fini, R. A.; Fiore, Gaetano; Garfagnini, A.; Giacomelli, G.; Giacomelli, Roberto; Grelli, G.; Guandalini, C.; Guerzoni, M.; Köse, U.; Laurenti, G.; Laveder, M.; Lippi, I.; Loddo, F.; Longhin, A.; Loverre, P.; Mancarella, G.; Mandrioli, G.; Margiotta, A.; Marsella, G.; Mauri, N.; Medinaceli, E.; Mengucci, A.; Mezzetto, M.; Michinelli, R.; Muciaccia, M. T.; Orecchini, D.; Paoloni, A.; Pastore, Alessandro; Patrizii, L.; Pozzato, M.; Rescigno, R.; Rosa, G.; Simone, S.; Sioli, M.; Sirri, G.; Spurio, M.; Stančo, L.; Stellacci, Francesco; Surdo, A.; Tenti, M.; Togo, V.; Ventura, M.; Zago, M.

doi:10.48550/arxiv.1203.3432

Cited by 19 publications

(12 citation statements)

References 9 publications

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“…That powerful trio of detectors would yield precise measurements of both electron-neutrino appearance and muon neutrino disappearance, which are tightly coupled in nearly all sterile-neutrino oscillation models 18. Search for anomalies with muon spectrometers and large LArTPC imaging detectors at CERN 43 An experimental search for sterile neutrinos at new CERN-SPS neutrino beam has been recently proposed [704]. The experiment is based on two identical LAr-TPCs [705,706] followed by magnetized spectrometers [707], observing the electron and muon neutrino events at the Far and Near positions 1600 and 300 m from the proton target, respectively (Figure 139).…”

Section: The Boone Proposal 42mentioning

confidence: 99%

Light Sterile Neutrinos: A White Paper

Abazajian,

Acero,

Agarwalla

et al. 2012

Preprint

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471

864

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In memoriamRamaswami "Raju" S. Raghavan 1937 -2011 CONTENTS Executive summary I. Theory and Motivation A. Introduction: What is a Sterile Neutrino? B. Theoretical Motivations and Symmetries Behind the Existence of Light Sterile Neutrinos Sterile neutrinos in "standard approaches" Sterile neutrinos in "non-standard approaches" C. The Low-Energy Seesaw and Minimal Models General Aspects eV-scale Seesaw The νMSM D. Sterile Neutrino Dark Matter Dark matter in the νMSM Neutrinos in gauge multiplets -thermal production of DM neutrinos Primordial generation of DM neutrinos Other models E. Light Sterile Neutrinos as Messengers of New Physics F. Non-Standard Neutrino Interactions (NSI) CC-like NSI NC-like NSI Models to evade charged lepton NSI Summary of the present status on NSI G. Extra Forces H. Lorentz Violation Violation of Lorentz invariance in the standard model Lorentz-violating neutrinos Global models using Lorentz violation Some types of Lorentz violation: CPT violation, non-standard interactions, and lepton-number-violating oscillations i I. CPT Violation in Neutrino Oscillations and the Early Universe as an Alternative to Sterile Neutrinos II. Astrophysical Evidence A. Cosmology Sterile neutrino thermalization Big Bang Nucleosynthesis Cosmic microwave background and large-scale structure B. Core Collapse Supernovae III. Evidence from Oscillation Experiments A. The LSND Signal Description of the Experiment Event Selection Neutrino Oscillation Signal and Background Reactions LSND Oscillation Results B. The KARMEN Constraint Description of the Experiment Event Selection Neutrino Oscillation Signal and Background Reactions KARMEN Neutrino Oscillation Results C. Joint Analysis of LSND and KARMEN Data D. Sterile Neutrino Analysis of Super-K Comparison of ν µ → ν τ and ν µ → ν s Oscillations An Admixture Model E. The MiniBooNE ν e and νe Appearance Searches Description of the Experiment Neutrino Oscillation Event Selection Neutrino Oscillation Signal and Background Reactions MiniBooNE Neutrino Oscillation Results MiniBooNE Antineutrino Oscillation Results F. Disappearance Results from Accelerator Experiments

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Section: The Boone Proposal 42mentioning

confidence: 99%

Light Sterile Neutrinos: A White Paper

Abazajian,

Acero,

Agarwalla

et al. 2012

Preprint

Self Cite

471

864

View full text Add to dashboard Cite

show abstract

“…The proposed ICARUS@CERN experiment [61][62][63] is based on two Liquid-Argon Time-Projection-Chamber imaging detectors at 300 m and 1.6 km from the source. Since the beam will have an average neutrino energy of about 2 GeV, the oscillation length is larger than the distance of the near detector for ∆m 2 41 20 eV 2 .…”

mentioning

confidence: 99%

Short-baseline electron neutrino oscillation length after the Troitsk experiment

Giunti

Laveder

et al. 2013

Phys. Rev. D

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We discuss the implications for short-baseline electron neutrino disappearance in the 3+1 mixing scheme of the recent Troitsk bounds on the mixing of a neutrino with mass between 2 and 100 eV. Considering the Troitsk data in combination with the results of short-baseline νe and ν̅ e disappearance experiments, which include the reactor and Gallium anomalies, we derive a 2σ allowed range for the effective neutrino squared-mass difference between 0.85 and 43 eV2. The upper bound implies that it is likely that oscillations in distance and/or energy can be observed in radioactive source experiments. It is also favorable for the ICARUS@CERN experiment, in which it is likely that oscillations are not washed out in the near detector. We discuss also the implications for neutrinoless double-β decay

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“…Field lines in the detector module area between 0 and +45cm on both vertical and horizontal axes can be inferred from measurements made with the probe along the gap length. 4 The Totally Active Scintillator Detector (TASD) prototype…”

Section: Mind Prototype Testsmentioning

confidence: 99%

Proposal for SPS beam time for the baby MIND and TASD neutrino detector prototypes

Asfandiyarov,

Bayes,

Blondel

et al. 2014

Preprint

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The design, construction and testing of neutrino detector prototypes at CERN are ongoing activities. This document reports on the design of solid state baby MIND and TASD detector prototypes and outlines requirements for a test beam at CERN to test these, tentatively planned on the H8 beamline in the North Area, which is equipped with a large aperture magnet. It is hoped that this will allow for the current proposal to be considered in light of the recently approved projects related to neutrino activities with the SPS in the North Area in the medium term 2015-2020.

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Search for "anomalies" from neutrino and anti-neutrino oscillations at Delta_m^2 ~ 1eV^2 with muon spectrometers and large LAr-TPC imaging detectors

Cited by 19 publications

References 9 publications

Light Sterile Neutrinos: A White Paper

Light Sterile Neutrinos: A White Paper

Short-baseline electron neutrino oscillation length after the Troitsk experiment

Proposal for SPS beam time for the baby MIND and TASD neutrino detector prototypes

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