1. The European Spallation Source neutrino super-beam conceptual design report
- Author
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A. Alekou, E. Baussan, A. K. Bhattacharyya, N. Blaskovic Kraljevic, M. Blennow, M. Bogomilov, B. Bolling, E. Bouquerel, O. Buchan, A. Burgman, C. J. Carlile, J. Cederkall, P. Christiansen, M. Collins, E. Cristaldo Morales, P. Cupiał, L. D’Alessi, H. Danared, D. Dancila, J. P. A. M. de André, J. P. Delahaye, M. Dracos, I. Efthymiopoulos, T. Ekelöf, M. Eshraqi, G. Fanourakis, A. Farricker, E. Fernandez-Martinez, B. Folsom, T. Fukuda, N. Gazis, B. Gålnander, Th. Geralis, M. Ghosh, G. Gokbulut, L. Halić, M. Jenssen, A. Kayis Topaksu, B. Kildetoft, B. Kliček, M. Kozioł, K. Krhač, Ł. Łacny, M. Lindroos, C. Maiano, C. Marrelli, C. Martins, M. Mezzetto, N. Milas, M. Oglakci, T. Ohlsson, M. Olvegård, T. Ota, J. Park, D. Patrzalek, G. Petkov, P. Poussot, R. Johansson, S. Rosauro-Alcaraz, D. Saiang, B. Szybiński, J. Snamina, A. G. Sosa, G. Stavropoulos, M. Stipčević, R. Tarkeshian, F. Terranova, J. Thomas, T. Tolba, E. Trachanas, R. Tsenov, G. Vankova-Kirilova, N. Vassilopoulos, E. Wildner, J. Wurtz, O. Zormpa, Y. Zou, Alekou, A, Baussan, E, Bhattacharyya, A, Kraljevic, N, Blennow, M, Bogomilov, M, Bolling, B, Bouquerel, E, Buchan, O, Burgman, A, Carlile, C, Cederkall, J, Christiansen, P, Collins, M, Cristaldo Morales, E, Cupial, P, D'Alessi, L, Danared, H, Dancila, D, de Andre, J, Delahaye, J, Dracos, M, Efthymiopoulos, I, Ekelof, T, Eshraqi, M, Fanourakis, G, Farricker, A, Fernandez-Martinez, E, Folsom, B, Fukuda, T, Gazis, N, Galnander, B, Geralis, T, Ghosh, M, Gokbulut, G, Halic, L, Jenssen, M, Topaksu, A, Kildetoft, B, Klicek, B, Koziol, M, Krhac, K, Lacny, L, Lindroos, M, Maiano, C, Marrelli, C, Martins, C, Mezzetto, M, Milas, N, Oglakci, M, Ohlsson, T, Olvegard, M, Ota, T, Park, J, Patrzalek, D, Petkov, G, Poussot, P, Johansson, R, Rosauro-Alcaraz, S, Saiang, D, Szybinski, B, Snamina, J, Sosa, A, Stavropoulos, G, Stipcevic, M, Tarkeshian, R, Terranova, F, Thomas, J, Tolba, T, Trachanas, E, Tsenov, R, Vankova-Kirilova, G, Vassilopoulos, N, Wildner, E, Wurtz, J, Zormpa, O, and Zou, Y
- Subjects
Accelerator Physics (physics.acc-ph) ,Physics::Instrumentation and Detectors ,FOS: Physical sciences ,General Physics and Astronomy ,Accelerator Physics and Instrumentation ,High Energy Physics - Experiment ,Subatomär fysik ,High Energy Physics - Experiment (hep-ex) ,neutrino ,High Energy Physics - Phenomenology (hep-ph) ,Subatomic Physics ,General Materials Science ,Physical and Theoretical Chemistry ,physics.acc-ph ,Particle Physics - Phenomenology ,hep-ex ,Physics ,Acceleratorfysik och instrumentering ,hep-ph ,Accelerators and Storage Rings ,High Energy Physics - Phenomenology ,Physics::Accelerator Physics ,High Energy Physics::Experiment ,Physics - Accelerator Physics ,essnusb ,cp violation ,cdr ,Particle Physics - Experiment - Abstract
This conceptual design report provides a detailed account of the European Spallation Source neutrino Super Beam (ESS$\nu$SB) feasibility study. This facility has been proposed after the measurements reported in 2012 of a relatively large value of the neutrino mixing angle $\theta_{13}$, which raised the possibility of observing potential CP violation in the leptonic sector with conventional neutrino beams. The measured value of $\theta_{13}$ also privileges the $2^{nd}$ oscillation maximum for the discovery of CP violation instead of the more typically studied $1^{st}$ maximum. The sensitivity at this $2^{nd}$ oscillation maximum is about three times higher than at the $1^{st}$ one, which implies a reduced influence of systematic errors. Working at the $2^{nd}$ oscillation maximum requires a very intense neutrino beam with an appropriate energy. The world's most intense pulsed spallation neutron source, the European Spallation Source (ESS), will have a proton linac operating at 5\,MW power, 2\,GeV kinetic energy and 14~Hz repetition rate (3~ms pulse duration, 4\% duty cycle) for neutron production. In this design study it is proposed to double the repetition rate and compress the beam pulses to the level of microseconds in order to provide an additional 5~MW proton beam for neutrino production. The physics performance has been evaluated for such a neutrino super beam, in conjunction with a megaton-scale underground water Cherenkov neutrino detector installed at a distance of 360--550\,km from ESS. The ESS proton linac upgrades, the accumulator ring required for proton-pulse compression, the target station design and optimisation, the near and far detector complexes, and the physics potential of the facility are all described in this report. The ESS linac will be operational by 2025, at which point the implementation of upgrades for the neutrino facility could begin., Comment: 216 pages
- Published
- 2022