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arxiv: 2303.17356 · v3 · pith:MGL54EHTnew · submitted 2023-03-30 · ✦ hep-ex · hep-ph· physics.ins-det

The ESSnuSB design study: overview and future prospects

ESSnuSB Collaboration: A. Alekou , E. Baussan , A.K. Bhattacharyya , N. Blaskovic Kraljevic , M. Blennow , M. Bogomilov , B. Bolling , E. Bouquerel
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F. Bramati A. Branca O. Buchan A. Burgman C.J. Carlile J. Cederkall S. Choubey P. Christiansen M. Collins E. Cristaldo Morales L. D'Alessi H. Danared D. Dancila J.P.A.M. de Andr\'e J.P. Delahaye M. Dracos I. Efthymiopoulos T. Ekel\"of M. Eshraqi G. Fanourakis A. Farricker E. Fernandez-Martinez B. Folsom T. Fukuda N. Gazis B. G\r{a}lnander Th. Geralis M. Ghosh A. Giarnetti G. Gokbulut L. Hali\'c M. Jenssen R. Johansson A. Kayis Topaksu B. Kildetoft B. Kli\v{c}ek M. Kozio{\l} K. Krha\v{c} {\L}. {\L}acny M. Lindroos A. Longhin C. Maiano S. Marangoni C. Marrelli C. Martins D. Meloni M. Mezzetto N. Milas M. Oglakci T. Ohlsson M. Olveg\r{a}rd T. Ota M. Pari J. Park D. Patrzalek G. Petkov P. Poussot F. Pupilli S. Rosauro-Alcaraz D. Saiang J. Snamina A. Sosa G. Stavropoulos M. Stip\v{c}evi\'c B. Szybi\'nski 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
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classification ✦ hep-ex hep-phphysics.ins-det
keywords essnusbmaximumneutrinobeamdesignexperimentfuturemeasurement
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ESSnuSB is a design study for an experiment to measure the CP violation in the leptonic sector at the second neutrino oscillation maximum using a neutrino beam driven by the uniquely powerful ESS linear accelerator. The reduced impact of systematic errors on sensitivity at the second maximum allows for a very precise measurement of the CP violating parameter. This review describes the fundamental advantages of measurement at the 2nd maximum, the necessary upgrades to the ESS linac in order to produce a neutrino beam, the near and far detector complexes, the expected physics reach of the proposed ESSnuSB experiment, concluding with the near future developments aimed at the project realization.

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    With 5.4 Mt·year atmospheric neutrino exposure, ESSnuSB could constrain |ε_eμ^m| < 0.053, |ε_eτ^m| < 0.057, |ε_μτ^m| < 0.021 and related diagonal differences at 90% CL, while NSI would alter mass ordering and θ23 octa...