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Your search keyword '"M. Olvegård"' showing total 2 results
Start Over Author "M. Olvegård" Journal journal of high energy physics
2 results on '"M. Olvegård"'

1. Exploring atmospheric neutrino oscillations at ESSnuSB

Author

The ESSnuSB collaboration, J. Aguilar, M. Anastasopoulos, E. Baussan, A. K. Bhattacharyya, A. Bignami, M. Blennow, M. Bogomilov, B. Bolling, E. Bouquerel, F. Bramati, A. Branca, G. Brunetti, I. Bustinduy, C. J. Carlile, J. Cederkall, T. W. Choi, S. Choubey, P. Christiansen, M. Collins, E. Cristaldo Morales, P. Cupiał, H. Danared, J. P. A. M. de André, M. Dracos, I. Efthymiopoulos, T. Ekelöf, M. Eshraqi, G. Fanourakis, A. Farricker, E. Fasoula, T. Fukuda, N. Gazis, Th. Geralis, M. Ghosh, A. Giarnetti, G. Gokbulut, C. Hagner, L. Halić, M. Hooft, K. E. Iversen, N. Jachowicz, M. Jenssen, R. Johansson, E. Kasimi, A. Kayis Topaksu, B. Kildetoft, K. Kordas, A. Leisos, M. Lindroos, A. Longhin, C. Maiano, S. Marangoni, C. Marrelli, D. Meloni, M. Mezzetto, N. Milas, J. L. Muñoz, K. Niewczas, M. Oglakci, T. Ohlsson, M. Olvegård, M. Pari, D. Patrzalek, G. Petkov, Ch. Petridou, P. Poussot, A. Psallidas, F. Pupilli, D. Saiang, D. Sampsonidis, C. Schwab, F. Sordo, A. Sosa, G. Stavropoulos, R. Tarkeshian, F. Terranova, T. Tolba, E. Trachanas, R. Tsenov, A. Tsirigotis, S. E. Tzamarias, G. Vankova-Kirilova, N. Vassilopoulos, S. Vihonen, J. Wurtz, V. Zeter, and O. Zormpa

Subjects
Flavour Physics, Neutrino Detectors and Telescopes (experiments), Oscillation, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract

Abstract This study provides an analysis of atmospheric neutrino oscillations at the ESSnuSB far detector facility. The prospects of the two cylindrical Water Cherenkov detectors with a total fiducial mass of 540 kt are investigated over 10 years of data taking in the standard three-flavor oscillation scenario. We present the confidence intervals for the determination of mass ordering, θ 23 octant as well as for the precisions on sin2 θ 23 and Δ m 31 2 $$ \left|\Delta {m}_{31}^2\right| $$ . It is shown that mass ordering can be resolved by 3σ CL (5σ CL) after 4 years (10 years) regardless of the true neutrino mass ordering. Correspondingly, the wrong θ 23 octant could be excluded by 3σ CL after 4 years (8 years) in the case where the true neutrino mass ordering is normal ordering (inverted ordering). The results presented in this work are complementary to the accelerator neutrino program in the ESSnuSB project.

Published
2024
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2. Decoherence in neutrino oscillation at the ESSnuSB experiment

Author

The ESSnuSB collaboration, J. Aguilar, M. Anastasopoulos, E. Baussan, A. K. Bhattacharyya, A. Bignami, M. Blennow, M. Bogomilov, B. Bolling, E. Bouquerel, F. Bramati, A. Branca, G. Brunetti, I. Bustinduy, C. J. Carlile, J. Cederkall, T. W. Choi, S. Choubey, P. Christiansen, M. Collins, E. Cristaldo Morales, P. Cupiał, H. Danared, D. Dancila, J. P. A. M. de André, M. Dracos, I. Efthymiopoulos, T. Ekelöf, M. Eshraqi, G. Fanourakis, A. Farricker, E. Fasoula, T. Fukuda, N. Gazis, Th. Geralis, M. Ghosh, A. Giarnetti, G. Gokbulut, A. Gupta, C. Hagner, L. Halić, V. T. Hariharan, M. Hooft, K. E. Iversen, N. Jachowicz, M. Jenssen, R. Johansson, E. Kasimi, A. Kayis Topaksu, B. Kildetof, B. Kliček, K. Kordas, A. Leisos, M. Lindroos, A. Longhin, C. Maiano, D. Majumdar, S. Marangoni, C. Marrelli, C. Martins, D. Meloni, M. Mezzetto, N. Milas, J. Muñoz, K. Niewczas, M. Oglakci, T. Ohlsson, M. Olvegård, M. Pari, D. Patrzalek, G. Petkov, Ch. Petridou, P. Poussot, A. Psallidas, F. Pupilli, D. Saiang, D. Sampsonidis, C. Schwab, F. Sordo, A. Sosa, G. Stavropoulos, M. Stipčević, R. Tarkeshian, F. Terranova, T. Tolba, E. Trachanas, R. Tsenov, A. Tsirigotis, S. E. Tzamarias, G. Vankova-Kirilova, N. Vassilopoulos, S. Vihonen, J. Wurtz, V. Zeter, O. Zormpa, and Y. Zou

Subjects
Long-Baseline Neutrino Experiments, Oscillation, Nuclear and particle physics. Atomic energy. Radioactivity, QC770-798
Abstract

Abstract Neutrino oscillation experiments provide a unique window in exploring several new physics scenarios beyond the standard three flavour. One such scenario is quantum decoherence in neutrino oscillation which tends to destroy the interference pattern of neutrinos reaching the far detector from the source. In this work, we study the decoherence in neutrino oscillation in the context of the ESSnuSB experiment. We consider the energy-independent decoherence parameter and derive the analytical expressions for P μe and P μμ probabilities in vacuum. We have computed the capability of ESSnuSB to put bounds on the decoherence parameters namely, Γ21 and Γ32 and found that the constraints on Γ21 are competitive compared to the DUNE bounds and better than the most stringent LBL ones from MINOS/MINOS+. We have also investigated the impact of decoherence on the ESSnuSB measurement of the Dirac CP phase δ CP and concluded that it remains robust in the presence of new physics.

Published
2024
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