Determination of a time-shift in the OPERA set-up using high energy horizontal muons in the LVD and OPERA detectors
N. Yu. Agafonova, P. Antonioli, V. V. Ashikhmin, G. Bari, E. Bressan,, L. Evans, M. Garbini, P. Giusti, A. S. Malguin, R. Persiani, V. G. Ryasny, O., G. Ryazhskaya, G. Sartorelli, E. Scapparone, M. Selvi, I. R. Shakirianova, L., Votano, H. Wenninger, V. F. Yakushev

TL;DR
This study independently measures a systematic negative time shift in the OPERA detector using high-energy horizontal muons crossing both LVD and OPERA, revealing a timing anomaly that could explain the neutrino velocity excess reported by OPERA.
Contribution
It introduces a novel, independent TOF calibration method using horizontal muons to identify a systematic timing shift in OPERA's setup.
Findings
Detected a -73 ns time shift in OPERA's timing system
Identified a systematic effect in OPERA from 2008 to 2011
The effect size is comparable to the neutrino velocity anomaly reported by OPERA
Abstract
The purpose of this work is to report the measurement of a time-shift in the OPERA set-up in a totally independent way from Time Of Flight (TOF) measurements of CNGS neutrino events. The LVD and OPERA experiments are both installed in the same laboratory: LNGS. The relative position of the two detectors, separated by an average distance of ~ 160 m, allows the use of very high energy horizontal muons to cross-calibrate the timing systems of the two detectors, using a TOF technique which is totally independent from TOF of CNGS neutrino events. Indeed, the OPERA-LVD direction lies along the so-called "Teramo anomaly", a region in the Gran Sasso massif where LVD has established, many years ago, the existence of an anomaly in the mountain structure, which exhibits a low m. w. e. thickness for horizontal directions. The "abundant" high-energy horizontal muons (nearly 100 per year) going…
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Taxonomy
TopicsAdvanced Frequency and Time Standards · Astrophysics and Cosmic Phenomena · Radioactive Decay and Measurement Techniques
