European Physical Journal C: Particles and Fields (Dec 2021)
Updated physics performance of the ESSnuSB experiment
- A. Alekou,
- E. Baussan,
- N. Blaskovic Kraljevic,
- M. Blennow,
- M. Bogomilov,
- E. Bouquerel,
- A. Burgman,
- C. J. Carlile,
- J. Cederkall,
- P. Christiansen,
- M. Collins,
- E. Cristaldo Morales,
- L. D’Alessi,
- H. Danared,
- J. P. A. M. de André,
- J. P. Delahaye,
- M. Dracos,
- I. Efthymiopoulos,
- T. Ekelöf,
- M. Eshraqi,
- G. Fanourakis,
- E. Fernandez-Martinez,
- B. Folsom,
- M. Ghosh,
- G. Gokbulut,
- L. Halić,
- A. Kayis Topaksu,
- B. Kliček,
- K. Krhač,
- M. Lindroos,
- M. Mezzetto,
- M. Oglakci,
- T. Ohlsson,
- M. Olvegård,
- T. Ota,
- J. Park,
- G. Petkov,
- P. Poussot,
- S. Rosauro-Alcaraz,
- G. Stavropoulos,
- M. Stipčević,
- F. Terranova,
- J. Thomas,
- T. Tolba,
- R. Tsenov,
- G. Vankova-Kirilova,
- N. Vassilopoulos,
- E. Wildner,
- J. Wurtz,
- O. Zormpa,
- Y. Zou
Affiliations
- A. Alekou
- CERN
- E. Baussan
- IPHC, Université de Strasbourg, CNRS/IN2P3
- N. Blaskovic Kraljevic
- European Spallation Source
- M. Blennow
- Department of Physics, School of Engineering Sciences, KTH Royal Institute of Technology
- M. Bogomilov
- Faculty of Physics, Sofia University St. Kliment Ohridski
- E. Bouquerel
- IPHC, Université de Strasbourg, CNRS/IN2P3
- A. Burgman
- Department of Physics, Lund University
- C. J. Carlile
- Department of Physics and Astronomy, FREIA, Uppsala University
- J. Cederkall
- Department of Physics, Lund University
- P. Christiansen
- Department of Physics, Lund University
- M. Collins
- European Spallation Source
- E. Cristaldo Morales
- University of Milano-Bicocca and INFN sez. di Milano-Bicocca
- L. D’Alessi
- IPHC, Université de Strasbourg, CNRS/IN2P3
- H. Danared
- European Spallation Source
- J. P. A. M. de André
- IPHC, Université de Strasbourg, CNRS/IN2P3
- J. P. Delahaye
- CERN
- M. Dracos
- IPHC, Université de Strasbourg, CNRS/IN2P3
- I. Efthymiopoulos
- CERN
- T. Ekelöf
- Uppsala University
- M. Eshraqi
- European Spallation Source
- G. Fanourakis
- Institute of Nuclear and Particle Physics, NCSR Demokritos
- E. Fernandez-Martinez
- Departamento de Fisica Teorica and Instituto de Fisica Teorica, IFT-UAM/CSIC, Universidad Autonoma de Madrid
- B. Folsom
- European Spallation Source
- M. Ghosh
- Center of Excellence for Advanced Materials and Sensing Devices, Ruder Bošković Institute
- G. Gokbulut
- Department of Physics, Faculty of Science and Letters, University of Cukurova
- L. Halić
- Center of Excellence for Advanced Materials and Sensing Devices, Ruder Bošković Institute
- A. Kayis Topaksu
- Department of Physics, Faculty of Science and Letters, University of Cukurova
- B. Kliček
- Center of Excellence for Advanced Materials and Sensing Devices, Ruder Bošković Institute
- K. Krhač
- Center of Excellence for Advanced Materials and Sensing Devices, Ruder Bošković Institute
- M. Lindroos
- European Spallation Source
- M. Mezzetto
- INFN sez. di Padova
- M. Oglakci
- Department of Physics, Faculty of Science and Letters, University of Cukurova
- T. Ohlsson
- Department of Physics, School of Engineering Sciences, KTH Royal Institute of Technology
- M. Olvegård
- Uppsala University
- T. Ota
- Departamento de Fisica Teorica and Instituto de Fisica Teorica, IFT-UAM/CSIC, Universidad Autonoma de Madrid
- J. Park
- Department of Physics, Lund University
- G. Petkov
- Faculty of Physics, Sofia University St. Kliment Ohridski
- P. Poussot
- IPHC, Université de Strasbourg, CNRS/IN2P3
- S. Rosauro-Alcaraz
- Departamento de Fisica Teorica and Instituto de Fisica Teorica, IFT-UAM/CSIC, Universidad Autonoma de Madrid
- G. Stavropoulos
- Institute of Nuclear and Particle Physics, NCSR Demokritos
- M. Stipčević
- Center of Excellence for Advanced Materials and Sensing Devices, Ruder Bošković Institute
- F. Terranova
- University of Milano-Bicocca and INFN sez. di Milano-Bicocca
- J. Thomas
- IPHC, Université de Strasbourg, CNRS/IN2P3
- T. Tolba
- Institute for Experimental Physics, Hamburg University
- R. Tsenov
- Faculty of Physics, Sofia University St. Kliment Ohridski
- G. Vankova-Kirilova
- Faculty of Physics, Sofia University St. Kliment Ohridski
- N. Vassilopoulos
- Spallation Neutron Science Center
- E. Wildner
- CERN
- J. Wurtz
- IPHC, Université de Strasbourg, CNRS/IN2P3
- O. Zormpa
- Institute of Nuclear and Particle Physics, NCSR Demokritos
- Y. Zou
- Uppsala University
- DOI
- https://doi.org/10.1140/epjc/s10052-021-09845-8
- Journal volume & issue
-
Vol. 81,
no. 12
pp. 1 – 12
Abstract
Abstract In this paper, we present the physics performance of the ESSnuSB experiment in the standard three flavor scenario using the updated neutrino flux calculated specifically for the ESSnuSB configuration and updated migration matrices for the far detector. Taking conservative systematic uncertainties corresponding to a normalization error of $$5\%$$ 5 % for signal and $$10\%$$ 10 % for background, we find that there is $$10\sigma $$ 10 σ $$(13\sigma )$$ ( 13 σ ) CP violation discovery sensitivity for the baseline option of 540 km (360 km) at $$\delta _\mathrm{CP} = \pm 90^\circ $$ δ CP = ± 90 ∘ . The corresponding fraction of $$\delta _\mathrm{CP}$$ δ CP for which CP violation can be discovered at more than $$5 \sigma $$ 5 σ is $$70\%$$ 70 % . Regarding CP precision measurements, the $$1\sigma $$ 1 σ error associated with $$\delta _\mathrm{CP} = 0^\circ $$ δ CP = 0 ∘ is around $$5^\circ $$ 5 ∘ and with $$\delta _\mathrm{CP} = -90^\circ $$ δ CP = - 90 ∘ is around $$14^\circ $$ 14 ∘ $$(7^\circ )$$ ( 7 ∘ ) for the baseline option of 540 km (360 km). For hierarchy sensitivity, one can have $$3\sigma $$ 3 σ sensitivity for 540 km baseline except $$\delta _\mathrm{CP} = \pm 90^\circ $$ δ CP = ± 90 ∘ and $$5\sigma $$ 5 σ sensitivity for 360 km baseline for all values of $$\delta _\mathrm{CP}$$ δ CP . The octant of $$\theta _{23}$$ θ 23 can be determined at $$3 \sigma $$ 3 σ for the values of: $$\theta _{23} > 51^\circ $$ θ 23 > 51 ∘ ( $$\theta _{23} 49^\circ $$ θ 23 > 49 ∘ ) for baseline of 540 km (360 km). Regarding measurement precision of the atmospheric mixing parameters, the allowed values at $$3 \sigma $$ 3 σ are: $$40^\circ< \theta _{23} < 52^\circ $$ 40 ∘ < θ 23 < 52 ∘ ( $$42^\circ< \theta _{23} < 51.5^\circ $$ 42 ∘ < θ 23 < 51 . 5 ∘ ) and $$2.485 \times 10^{-3}$$ 2.485 × 10 - 3 eV $$^2< \varDelta m^2_{31} < 2.545 \times 10^{-3}$$ 2 < Δ m 31 2 < 2.545 × 10 - 3 eV $$^2$$ 2 ( $$2.49 \times 10^{-3}$$ 2.49 × 10 - 3 eV $$^2< \varDelta m^2_{31} < 2.54 \times 10^{-3}$$ 2 < Δ m 31 2 < 2.54 × 10 - 3 eV $$^2$$ 2 ) for the baseline of 540 km (360 km).