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Determination of a time-shift in the OPERA set-up using high-energy horizontal muons in the LVD and OPERA detectors

Authors :
A. Di Crescenzo
Ante Ljubičić
J. Ebert
Alessandro Paoloni
N. Yu. Agafonova
N. Di Marco
I. Shakirianova
M. Garbini
R. A. Fini
Andrey Alexandrov
M. T. Muciaccia
Björn Wonsak
P. Giusti
V. G. Ryasny
Eugenio Scapparone
M. Hierholzer
Nicola D'Ambrosio
M. Spinetti
Dmitry V. Naumov
L. Patrizii
Maximiliano Sioli
M. Pozzato
J. Lenkeit
Vitaliano Chiarella
N. Mauri
M. Tenti
G. De Lellis
G. Mandrioli
C. Jollet
E. Medinaceli
A. Russo
V. A. Matveev
O. G. Ryazhskaya
S. Dusini
B. Klicek
I. Rostovtseva
V. Yakushev
A. Longhin
Pietro Antonioli
A. Meregaglia
R. Brugnera
Y. A. Gornushkin
C. Gustavino
Krešimir Jakovčić
V. F. Yakushev
A. S. Malgin
L. Votano
A. Garfagnini
G. Sirri
Artem Chukanov
A. Bertolin
F. Grianti
Torben Ferber
A. Schembri
G. Bari
Antonio Ereditato
F. Pupilli
D. Di Ferdinando
A. S. Malguin
Yu. Zaitsev
Caren Hagner
Chiara Sirignano
G. Giacomelli
A.G. Olshevsky
V. V. Ashikhmin
M. Selvi
Utku Kose
S. Simone
S. Zemskova
R. Persiani
S. Dmitrievsky
F. Terranova
A. Sheshukov
B. Büttner
Gianfranca De Rosa
E. Bressan
V. Tioukov
N. Agafonova
M. Dracos
H. Wenniger
O. Ryazhskaya
C. Göllnitz
L. Evans
L. Stanco
A. Hollnagel
Antonino Zichichi
Alessandro Pastore
Mario Stipčević
G. Sartorelli
DE LELLIS, Giovanni
DI CRESCENZO, Antonia
Agafonova, N
Antonioli, P
Ashikhmin, V
Bari, G
Bressan, E
Evans, L
Garbini, M
Giusti, P
Malguin, A
Persiani, R
Ryasny, V
Ryazhskaya, O
Sartorelli, G
Scapparone, E
Selvi, M
Shakirianova, I
Votano, L
Wenniger, H
Yakushev, V
Zichichi, A
Alexandrov, A
Bertolin, A
Brugnera, R
Büttner, B
Chiarella, V
Chukanov, A
D’Ambrosio, N
De Lellis, G
Di Crescenzo, A
Di Ferdinando, D
Di Marco, N
Dmitrievsky, S
Dracos, M
Dusini, S
Ebert, J
Ereditato, A
Ferber, T
Fini, R
Garfagnini, A
Giacomelli, G
Göllnitz, C
Gornushkin, Y
Grianti, F
Gustavino, C
Hagner, C
Hierholzer, M
Hollnagel, A
Jakovcic, K
Jollet, C
Klicek, B
Kose, U
Lenkeit, J
Ljubicic, A
Longhin, A
Malgin, A
Mandrioli, G
Matveev, V
Mauri, N
Medinaceli, E
Meregaglia, A
Muciaccia, M
Naumov, D
Olshevsky, A
Paoloni, A
Pastore, A
Patrizii, L
Pozzato, M
Pupilli, F
Rosa, G
Rostovtseva, I
Russo, A
Schembri, A
Sheshukov, A
Simone, S
Sioli, M
Sirignano, C
Sirri, G
Spinetti, M
Stanco, L
Stipcevic, M
Tenti, M
Terranova, F
Tioukov, V
Wonsak, B
Zaitsev, Y
Zemskova, S
N.Yu. Agafonova
P. Antonioli
V.V. Ashikhmin
G. Bari
E. Bressan
L. Evan
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. Wenniger
V.F. Yakushev
A. Zichichi
N. Agafonova
A. Alexandrov
A. Bertolin
R. Brugnera
B. B¨uttner
V. Chiarella
A. Chukanov
N. D’Ambrosio
G. De Lelli
A. Di Crescenzo
D. Di Ferdinando
N. Di Marco
S. Dmitrievsky
M. Draco
S. Dusini
J. Ebert
A. Ereditato
T. Ferber
R.A. Fini
A. Garfagnini
G. Giacomelli
C. G¨ollnitz
Y. Gornushkin
F. Grianti
C. Gustavino
C. Hagner
M. Hierholzer
A. Hollnagel
K. Jakovcic
C. Jollet
B. Klicek
U. Kose
J. Lenkeit
A. Ljubicic
A. Longhin
A. Malgin
G. Mandrioli
V. Matveev
N. Mauri
E. Medinaceli
A. Meregaglia
M.T. Muciaccia
D. Naumov
A. Olshevsky
A. Paoloni
A. Pastore
L. Patrizii
M. Pozzato
F. Pupilli
G. Rosa
I. Rostovtseva
A. Russo
O. Ryazhskaya
A. Schembri
I. Shakirianova
A. Sheshukov
S. Simone
M. Sioli
C. Sirignano
G. Sirri
M. Spinetti
L. Stanco
M. Stipcevic
M. Tenti
F. Terranova
V. Tioukov
B. Wonsak
V. Yakushev
Y. Zaitsev
S. Zemskova
Source :
Ereditato, Antonio (2012). Determination of a time-shift in the OPERA set-up using high-energy horizontal muons in the LVD and OPERA detectors. European physical journal-plus, 127(6), p. 71. Les Ulis (F): EDP Sciences 10.1140/epjp/i2012-12071-5
Publication Year :
2012
Publisher :
EDP Sciences, 2012.

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 through LVD and OPERA exist because of this anomaly in the mountain orography. The total live time of the data in coincidence correspond to 1200 days from mid 2007 until March 2012. The time coincidence study of LVD and OPERA detectors is based on 306 cosmic horizontal muon events and shows the existence of a negative time shift in the OPERA set-up of the order of deltaT(AB) = - (73 \pm 9) ns when two calendar periods, A and B, are compared. This result shows a systematic effect in the OPERA timing system from August 2008 until December 2011. The size of the effect is comparable with the neutrino velocity excess recently measured by OPERA. It is probably interesting not to forget that with the MRPC technology developed by the ALICE Bologna group the TOF world record accuracy of 20 ps was reached. That technology can be implemented at LNGS for a high precision determination of TOF with the CNGS neutrino beams of an order of magnitude smaller than the value of the OPERA systematic effect. 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 through LVD and OPERA exist because of this anomaly in the mountain orography. The total live time of the data in coincidence correspond to 1200 days from mid 2007 until March 2012. The time coincidence study of LVD and OPERA detectors is based on 306 cosmic horizontal muon events and shows the existence of a negative time shift in the OPERA set-up of the order of deltaT(AB) = - (73 \pm 9) ns when two calendar periods, A and B, are compared. This result shows a systematic effect in the OPERA timing system from August 2008 until December 2011. The size of the effect is comparable with the neutrino velocity excess recently measured by OPERA. It is probably interesting not to forget that with the MRPC technology developed by the ALICE Bologna group the TOF world record accuracy of 20 ps was reached. That technology can be implemented at LNGS for a high precision determination of TOF with the CNGS neutrino beams of an order of magnitude smaller than the value of the OPERA systematic effect.

Details

Database :
OpenAIRE
Journal :
Ereditato, Antonio (2012). Determination of a time-shift in the OPERA set-up using high-energy horizontal muons in the LVD and OPERA detectors. European physical journal-plus, 127(6), p. 71. Les Ulis (F): EDP Sciences 10.1140/epjp/i2012-12071-5 <http://dx.doi.org/10.1140/epjp/i2012-12071-5>
Accession number :
edsair.doi.dedup.....6eb92e9433c8b28748064784ef09cf90
Full Text :
https://doi.org/10.48350/17949