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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

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 detec...

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Autores principales: Agafonova, N.Yu., Antonioli, P., Ashikhmin, V.V., Bari, G., Bressan, E., Evans, L., Garbini, M., Giusti, P., Malguin, A.S., Persiani, R., Ryasny, V.G., Ryazhskaya, O.G., Sartorelli, G., Scapparone, E., Selvi, M., Shakirianova, I.R., Votano, L., Wenniger, H., Yakushev, V.F., Zichichi, A., Agafonova, N., Alexandrov, A., Bertolin, A., Brugnera, R., Buttner, 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.A., Garfagnini, A., Giacomelli, G., Gollnitz, C., Gornushkin, Yu., 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.T., Naumov, D., Olshevsky, A., Paoloni, A., Pastore, A., Patrizii, L., Pozzato, M., Pupilli, F., Rosa, G., Rostovtseva, I., Russo, A., Ryazhskaya, O., Schembri, A., Shakirianova, I., Sheshukov, A., Simone, S., Sioli, M., Sirignano, C., Sirri, G., Spinetti, M., Stanco, L., Stipcevic, M., Tenti, M., Terranova, F., Tioukov, V., Wonsak, B., Yakushev, V., Zaitsev, Y., Zemskova, S.
Lenguaje:eng
Publicado: 2012
Materias:
Acceso en línea:https://dx.doi.org/10.1140/epjp/i2012-12071-5
http://cds.cern.ch/record/1455799
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author Agafonova, N.Yu.
Antonioli, P.
Ashikhmin, V.V.
Bari, G.
Bressan, E.
Evans, L.
Garbini, M.
Giusti, P.
Malguin, A.S.
Persiani, R.
Ryasny, V.G.
Ryazhskaya, O.G.
Sartorelli, G.
Scapparone, E.
Selvi, M.
Shakirianova, I.R.
Votano, L.
Wenniger, H.
Yakushev, V.F.
Zichichi, A.
Agafonova, N.
Alexandrov, A.
Bertolin, A.
Brugnera, R.
Buttner, 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.A.
Garfagnini, A.
Giacomelli, G.
Gollnitz, C.
Gornushkin, Yu.
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.T.
Naumov, D.
Olshevsky, A.
Paoloni, A.
Pastore, A.
Patrizii, L.
Pozzato, M.
Pupilli, F.
Rosa, G.
Rostovtseva, I.
Russo, A.
Ryazhskaya, O.
Schembri, A.
Shakirianova, I.
Sheshukov, A.
Simone, S.
Sioli, M.
Sirignano, C.
Sirri, G.
Spinetti, M.
Stanco, L.
Stipcevic, M.
Tenti, M.
Terranova, F.
Tioukov, V.
Votano, L.
Wonsak, B.
Yakushev, V.
Zaitsev, Y.
Zemskova, S.
author_facet Agafonova, N.Yu.
Antonioli, P.
Ashikhmin, V.V.
Bari, G.
Bressan, E.
Evans, L.
Garbini, M.
Giusti, P.
Malguin, A.S.
Persiani, R.
Ryasny, V.G.
Ryazhskaya, O.G.
Sartorelli, G.
Scapparone, E.
Selvi, M.
Shakirianova, I.R.
Votano, L.
Wenniger, H.
Yakushev, V.F.
Zichichi, A.
Agafonova, N.
Alexandrov, A.
Bertolin, A.
Brugnera, R.
Buttner, 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.A.
Garfagnini, A.
Giacomelli, G.
Gollnitz, C.
Gornushkin, Yu.
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.T.
Naumov, D.
Olshevsky, A.
Paoloni, A.
Pastore, A.
Patrizii, L.
Pozzato, M.
Pupilli, F.
Rosa, G.
Rostovtseva, I.
Russo, A.
Ryazhskaya, O.
Schembri, A.
Shakirianova, I.
Sheshukov, A.
Simone, S.
Sioli, M.
Sirignano, C.
Sirri, G.
Spinetti, M.
Stanco, L.
Stipcevic, M.
Tenti, M.
Terranova, F.
Tioukov, V.
Votano, L.
Wonsak, B.
Yakushev, V.
Zaitsev, Y.
Zemskova, S.
author_sort Agafonova, N.Yu.
collection CERN
description 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.
id cern-1455799
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2012
record_format invenio
spelling cern-14557992023-04-04T03:42:55Zdoi:10.1140/epjp/i2012-12071-5http://cds.cern.ch/record/1455799engAgafonova, N.Yu.Antonioli, P.Ashikhmin, V.V.Bari, G.Bressan, E.Evans, L.Garbini, M.Giusti, P.Malguin, A.S.Persiani, R.Ryasny, V.G.Ryazhskaya, O.G.Sartorelli, G.Scapparone, E.Selvi, M.Shakirianova, I.R.Votano, L.Wenniger, H.Yakushev, V.F.Zichichi, A.Agafonova, N.Alexandrov, A.Bertolin, A.Brugnera, R.Buttner, 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.A.Garfagnini, A.Giacomelli, G.Gollnitz, C.Gornushkin, Yu.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.T.Naumov, D.Olshevsky, A.Paoloni, A.Pastore, A.Patrizii, L.Pozzato, M.Pupilli, F.Rosa, G.Rostovtseva, I.Russo, A.Ryazhskaya, O.Schembri, A.Shakirianova, I.Sheshukov, A.Simone, S.Sioli, M.Sirignano, C.Sirri, G.Spinetti, M.Stanco, L.Stipcevic, M.Tenti, M.Terranova, F.Tioukov, V.Votano, L.Wonsak, B.Yakushev, V.Zaitsev, Y.Zemskova, S.Determination of a time-shift in the OPERA set-up using high energy horizontal muons in the LVD and OPERA detectorsParticle Physics - ExperimentThe 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.arXiv:1206.2488oai:cds.cern.ch:14557992012-06-13
spellingShingle Particle Physics - Experiment
Agafonova, N.Yu.
Antonioli, P.
Ashikhmin, V.V.
Bari, G.
Bressan, E.
Evans, L.
Garbini, M.
Giusti, P.
Malguin, A.S.
Persiani, R.
Ryasny, V.G.
Ryazhskaya, O.G.
Sartorelli, G.
Scapparone, E.
Selvi, M.
Shakirianova, I.R.
Votano, L.
Wenniger, H.
Yakushev, V.F.
Zichichi, A.
Agafonova, N.
Alexandrov, A.
Bertolin, A.
Brugnera, R.
Buttner, 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.A.
Garfagnini, A.
Giacomelli, G.
Gollnitz, C.
Gornushkin, Yu.
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.T.
Naumov, D.
Olshevsky, A.
Paoloni, A.
Pastore, A.
Patrizii, L.
Pozzato, M.
Pupilli, F.
Rosa, G.
Rostovtseva, I.
Russo, A.
Ryazhskaya, O.
Schembri, A.
Shakirianova, I.
Sheshukov, A.
Simone, S.
Sioli, M.
Sirignano, C.
Sirri, G.
Spinetti, M.
Stanco, L.
Stipcevic, M.
Tenti, M.
Terranova, F.
Tioukov, V.
Votano, L.
Wonsak, B.
Yakushev, V.
Zaitsev, Y.
Zemskova, S.
Determination of a time-shift in the OPERA set-up using high energy horizontal muons in the LVD and OPERA detectors
title Determination of a time-shift in the OPERA set-up using high energy horizontal muons in the LVD and OPERA detectors
title_full Determination of a time-shift in the OPERA set-up using high energy horizontal muons in the LVD and OPERA detectors
title_fullStr Determination of a time-shift in the OPERA set-up using high energy horizontal muons in the LVD and OPERA detectors
title_full_unstemmed Determination of a time-shift in the OPERA set-up using high energy horizontal muons in the LVD and OPERA detectors
title_short Determination of a time-shift in the OPERA set-up using high energy horizontal muons in the LVD and OPERA detectors
title_sort determination of a time-shift in the opera set-up using high energy horizontal muons in the lvd and opera detectors
topic Particle Physics - Experiment
url https://dx.doi.org/10.1140/epjp/i2012-12071-5
http://cds.cern.ch/record/1455799
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AT tioukovv determinationofatimeshiftintheoperasetupusinghighenergyhorizontalmuonsinthelvdandoperadetectors
AT votanol determinationofatimeshiftintheoperasetupusinghighenergyhorizontalmuonsinthelvdandoperadetectors
AT wonsakb determinationofatimeshiftintheoperasetupusinghighenergyhorizontalmuonsinthelvdandoperadetectors
AT yakushevv determinationofatimeshiftintheoperasetupusinghighenergyhorizontalmuonsinthelvdandoperadetectors
AT zaitsevy determinationofatimeshiftintheoperasetupusinghighenergyhorizontalmuonsinthelvdandoperadetectors
AT zemskovas determinationofatimeshiftintheoperasetupusinghighenergyhorizontalmuonsinthelvdandoperadetectors