Updated physics performance of the ESSnuSB experiment
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 uncerta...
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| Autor*in: |
Alekou, A. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2021 |
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| Anmerkung: |
© The Author(s) 2021 |
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| Übergeordnetes Werk: |
Enthalten in: The European physical journal / C - Springer Berlin Heidelberg, 1998, 81(2021), 12 vom: Dez. |
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| Übergeordnetes Werk: |
volume:81 ; year:2021 ; number:12 ; month:12 |
| Links: |
|---|
| DOI / URN: |
10.1140/epjc/s10052-021-09845-8 |
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| Katalog-ID: |
OLC2077672706 |
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| 100 | 1 | |a Alekou, A. |e verfasserin |4 aut | |
| 245 | 1 | 0 | |a Updated physics performance of the ESSnuSB experiment |
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| 520 | |a 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 $$5\%$$ for signal and $$10\%$$ for background, we find that there is $$10\sigma $$$$(13\sigma )$$ CP violation discovery sensitivity for the baseline option of 540 km (360 km) at $$\delta _\mathrm{CP} = \pm 90^\circ $$. The corresponding fraction of $$\delta _\mathrm{CP}$$ for which CP violation can be discovered at more than $$5 \sigma $$ is $$70\%$$. Regarding CP precision measurements, the $$1\sigma $$ error associated with $$\delta _\mathrm{CP} = 0^\circ $$ is around $$5^\circ $$ and with $$\delta _\mathrm{CP} = -90^\circ $$ is around $$14^\circ $$$$(7^\circ )$$ for the baseline option of 540 km (360 km). For hierarchy sensitivity, one can have $$3\sigma $$ sensitivity for 540 km baseline except $$\delta _\mathrm{CP} = \pm 90^\circ $$ and $$5\sigma $$ sensitivity for 360 km baseline for all values of $$\delta _\mathrm{CP}$$. The octant of $$\theta _{23}$$ can be determined at $$3 \sigma $$ for the values of: $$\theta _{23} > 51^\circ $$ ($$\theta _{23} < 42^\circ $$ and $$\theta _{23} > 49^\circ $$) for baseline of 540 km (360 km). Regarding measurement precision of the atmospheric mixing parameters, the allowed values at $$3 \sigma $$ are: $$40^\circ< \theta _{23} < 52^\circ $$ ($$42^\circ< \theta _{23} < 51.5^\circ $$) and $$2.485 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.545 \times 10^{-3}$$ eV$$^2$$ ($$2.49 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.54 \times 10^{-3}$$ eV$$^2$$) for the baseline of 540 km (360 km). | ||
| 700 | 1 | |a Baussan, E. |4 aut | |
| 700 | 1 | |a Blaskovic Kraljevic, N. |4 aut | |
| 700 | 1 | |a Blennow, M. |4 aut | |
| 700 | 1 | |a Bogomilov, M. |4 aut | |
| 700 | 1 | |a Bouquerel, E. |4 aut | |
| 700 | 1 | |a Burgman, A. |4 aut | |
| 700 | 1 | |a Carlile, C. J. |4 aut | |
| 700 | 1 | |a Cederkall, J. |4 aut | |
| 700 | 1 | |a Christiansen, P. |4 aut | |
| 700 | 1 | |a Collins, M. |4 aut | |
| 700 | 1 | |a Cristaldo Morales, E. |4 aut | |
| 700 | 1 | |a D’Alessi, L. |4 aut | |
| 700 | 1 | |a Danared, H. |4 aut | |
| 700 | 1 | |a de André, J. P. A. M. |4 aut | |
| 700 | 1 | |a Delahaye, J. P. |4 aut | |
| 700 | 1 | |a Dracos, M. |4 aut | |
| 700 | 1 | |a Efthymiopoulos, I. |4 aut | |
| 700 | 1 | |a Ekelöf, T. |4 aut | |
| 700 | 1 | |a Eshraqi, M. |4 aut | |
| 700 | 1 | |a Fanourakis, G. |4 aut | |
| 700 | 1 | |a Fernandez-Martinez, E. |4 aut | |
| 700 | 1 | |a Folsom, B. |4 aut | |
| 700 | 1 | |a Ghosh, M. |4 aut | |
| 700 | 1 | |a Gokbulut, G. |4 aut | |
| 700 | 1 | |a Halić, L. |4 aut | |
| 700 | 1 | |a Kayis Topaksu, A. |4 aut | |
| 700 | 1 | |a Kliček, B. |0 (orcid)0000-0002-5163-8085 |4 aut | |
| 700 | 1 | |a Krhač, K. |4 aut | |
| 700 | 1 | |a Lindroos, M. |4 aut | |
| 700 | 1 | |a Mezzetto, M. |4 aut | |
| 700 | 1 | |a Oglakci, M. |4 aut | |
| 700 | 1 | |a Ohlsson, T. |4 aut | |
| 700 | 1 | |a Olvegård, M. |4 aut | |
| 700 | 1 | |a Ota, T. |4 aut | |
| 700 | 1 | |a Park, J. |4 aut | |
| 700 | 1 | |a Petkov, G. |4 aut | |
| 700 | 1 | |a Poussot, P. |4 aut | |
| 700 | 1 | |a Rosauro-Alcaraz, S. |4 aut | |
| 700 | 1 | |a Stavropoulos, G. |4 aut | |
| 700 | 1 | |a Stipčević, M. |4 aut | |
| 700 | 1 | |a Terranova, F. |4 aut | |
| 700 | 1 | |a Thomas, J. |4 aut | |
| 700 | 1 | |a Tolba, T. |4 aut | |
| 700 | 1 | |a Tsenov, R. |4 aut | |
| 700 | 1 | |a Vankova-Kirilova, G. |4 aut | |
| 700 | 1 | |a Vassilopoulos, N. |4 aut | |
| 700 | 1 | |a Wildner, E. |4 aut | |
| 700 | 1 | |a Wurtz, J. |4 aut | |
| 700 | 1 | |a Zormpa, O. |4 aut | |
| 700 | 1 | |a Zou, Y. |4 aut | |
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10.1140/epjc/s10052-021-09845-8 doi (DE-627)OLC2077672706 (DE-He213)s10052-021-09845-8-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Alekou, A. verfasserin aut Updated physics performance of the ESSnuSB experiment 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2021 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 $$5\%$$ for signal and $$10\%$$ for background, we find that there is $$10\sigma $$$$(13\sigma )$$ CP violation discovery sensitivity for the baseline option of 540 km (360 km) at $$\delta _\mathrm{CP} = \pm 90^\circ $$. The corresponding fraction of $$\delta _\mathrm{CP}$$ for which CP violation can be discovered at more than $$5 \sigma $$ is $$70\%$$. Regarding CP precision measurements, the $$1\sigma $$ error associated with $$\delta _\mathrm{CP} = 0^\circ $$ is around $$5^\circ $$ and with $$\delta _\mathrm{CP} = -90^\circ $$ is around $$14^\circ $$$$(7^\circ )$$ for the baseline option of 540 km (360 km). For hierarchy sensitivity, one can have $$3\sigma $$ sensitivity for 540 km baseline except $$\delta _\mathrm{CP} = \pm 90^\circ $$ and $$5\sigma $$ sensitivity for 360 km baseline for all values of $$\delta _\mathrm{CP}$$. The octant of $$\theta _{23}$$ can be determined at $$3 \sigma $$ for the values of: $$\theta _{23} > 51^\circ $$ ($$\theta _{23} < 42^\circ $$ and $$\theta _{23} > 49^\circ $$) for baseline of 540 km (360 km). Regarding measurement precision of the atmospheric mixing parameters, the allowed values at $$3 \sigma $$ are: $$40^\circ< \theta _{23} < 52^\circ $$ ($$42^\circ< \theta _{23} < 51.5^\circ $$) and $$2.485 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.545 \times 10^{-3}$$ eV$$^2$$ ($$2.49 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.54 \times 10^{-3}$$ eV$$^2$$) for the baseline of 540 km (360 km). Baussan, E. aut Blaskovic Kraljevic, N. aut Blennow, M. aut Bogomilov, M. aut Bouquerel, E. aut Burgman, A. aut Carlile, C. J. aut Cederkall, J. aut Christiansen, P. aut Collins, M. aut Cristaldo Morales, E. aut D’Alessi, L. aut Danared, H. aut de André, J. P. A. M. aut Delahaye, J. P. aut Dracos, M. aut Efthymiopoulos, I. aut Ekelöf, T. aut Eshraqi, M. aut Fanourakis, G. aut Fernandez-Martinez, E. aut Folsom, B. aut Ghosh, M. aut Gokbulut, G. aut Halić, L. aut Kayis Topaksu, A. aut Kliček, B. (orcid)0000-0002-5163-8085 aut Krhač, K. aut Lindroos, M. aut Mezzetto, M. aut Oglakci, M. aut Ohlsson, T. aut Olvegård, M. aut Ota, T. aut Park, J. aut Petkov, G. aut Poussot, P. aut Rosauro-Alcaraz, S. aut Stavropoulos, G. aut Stipčević, M. aut Terranova, F. aut Thomas, J. aut Tolba, T. aut Tsenov, R. aut Vankova-Kirilova, G. aut Vassilopoulos, N. aut Wildner, E. aut Wurtz, J. aut Zormpa, O. aut Zou, Y. aut Enthalten in The European physical journal / C Springer Berlin Heidelberg, 1998 81(2021), 12 vom: Dez. (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:81 year:2021 number:12 month:12 https://doi.org/10.1140/epjc/s10052-021-09845-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY AR 81 2021 12 12 |
| spelling |
10.1140/epjc/s10052-021-09845-8 doi (DE-627)OLC2077672706 (DE-He213)s10052-021-09845-8-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Alekou, A. verfasserin aut Updated physics performance of the ESSnuSB experiment 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2021 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 $$5\%$$ for signal and $$10\%$$ for background, we find that there is $$10\sigma $$$$(13\sigma )$$ CP violation discovery sensitivity for the baseline option of 540 km (360 km) at $$\delta _\mathrm{CP} = \pm 90^\circ $$. The corresponding fraction of $$\delta _\mathrm{CP}$$ for which CP violation can be discovered at more than $$5 \sigma $$ is $$70\%$$. Regarding CP precision measurements, the $$1\sigma $$ error associated with $$\delta _\mathrm{CP} = 0^\circ $$ is around $$5^\circ $$ and with $$\delta _\mathrm{CP} = -90^\circ $$ is around $$14^\circ $$$$(7^\circ )$$ for the baseline option of 540 km (360 km). For hierarchy sensitivity, one can have $$3\sigma $$ sensitivity for 540 km baseline except $$\delta _\mathrm{CP} = \pm 90^\circ $$ and $$5\sigma $$ sensitivity for 360 km baseline for all values of $$\delta _\mathrm{CP}$$. The octant of $$\theta _{23}$$ can be determined at $$3 \sigma $$ for the values of: $$\theta _{23} > 51^\circ $$ ($$\theta _{23} < 42^\circ $$ and $$\theta _{23} > 49^\circ $$) for baseline of 540 km (360 km). Regarding measurement precision of the atmospheric mixing parameters, the allowed values at $$3 \sigma $$ are: $$40^\circ< \theta _{23} < 52^\circ $$ ($$42^\circ< \theta _{23} < 51.5^\circ $$) and $$2.485 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.545 \times 10^{-3}$$ eV$$^2$$ ($$2.49 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.54 \times 10^{-3}$$ eV$$^2$$) for the baseline of 540 km (360 km). Baussan, E. aut Blaskovic Kraljevic, N. aut Blennow, M. aut Bogomilov, M. aut Bouquerel, E. aut Burgman, A. aut Carlile, C. J. aut Cederkall, J. aut Christiansen, P. aut Collins, M. aut Cristaldo Morales, E. aut D’Alessi, L. aut Danared, H. aut de André, J. P. A. M. aut Delahaye, J. P. aut Dracos, M. aut Efthymiopoulos, I. aut Ekelöf, T. aut Eshraqi, M. aut Fanourakis, G. aut Fernandez-Martinez, E. aut Folsom, B. aut Ghosh, M. aut Gokbulut, G. aut Halić, L. aut Kayis Topaksu, A. aut Kliček, B. (orcid)0000-0002-5163-8085 aut Krhač, K. aut Lindroos, M. aut Mezzetto, M. aut Oglakci, M. aut Ohlsson, T. aut Olvegård, M. aut Ota, T. aut Park, J. aut Petkov, G. aut Poussot, P. aut Rosauro-Alcaraz, S. aut Stavropoulos, G. aut Stipčević, M. aut Terranova, F. aut Thomas, J. aut Tolba, T. aut Tsenov, R. aut Vankova-Kirilova, G. aut Vassilopoulos, N. aut Wildner, E. aut Wurtz, J. aut Zormpa, O. aut Zou, Y. aut Enthalten in The European physical journal / C Springer Berlin Heidelberg, 1998 81(2021), 12 vom: Dez. (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:81 year:2021 number:12 month:12 https://doi.org/10.1140/epjc/s10052-021-09845-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY AR 81 2021 12 12 |
| allfields_unstemmed |
10.1140/epjc/s10052-021-09845-8 doi (DE-627)OLC2077672706 (DE-He213)s10052-021-09845-8-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Alekou, A. verfasserin aut Updated physics performance of the ESSnuSB experiment 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2021 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 $$5\%$$ for signal and $$10\%$$ for background, we find that there is $$10\sigma $$$$(13\sigma )$$ CP violation discovery sensitivity for the baseline option of 540 km (360 km) at $$\delta _\mathrm{CP} = \pm 90^\circ $$. The corresponding fraction of $$\delta _\mathrm{CP}$$ for which CP violation can be discovered at more than $$5 \sigma $$ is $$70\%$$. Regarding CP precision measurements, the $$1\sigma $$ error associated with $$\delta _\mathrm{CP} = 0^\circ $$ is around $$5^\circ $$ and with $$\delta _\mathrm{CP} = -90^\circ $$ is around $$14^\circ $$$$(7^\circ )$$ for the baseline option of 540 km (360 km). For hierarchy sensitivity, one can have $$3\sigma $$ sensitivity for 540 km baseline except $$\delta _\mathrm{CP} = \pm 90^\circ $$ and $$5\sigma $$ sensitivity for 360 km baseline for all values of $$\delta _\mathrm{CP}$$. The octant of $$\theta _{23}$$ can be determined at $$3 \sigma $$ for the values of: $$\theta _{23} > 51^\circ $$ ($$\theta _{23} < 42^\circ $$ and $$\theta _{23} > 49^\circ $$) for baseline of 540 km (360 km). Regarding measurement precision of the atmospheric mixing parameters, the allowed values at $$3 \sigma $$ are: $$40^\circ< \theta _{23} < 52^\circ $$ ($$42^\circ< \theta _{23} < 51.5^\circ $$) and $$2.485 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.545 \times 10^{-3}$$ eV$$^2$$ ($$2.49 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.54 \times 10^{-3}$$ eV$$^2$$) for the baseline of 540 km (360 km). Baussan, E. aut Blaskovic Kraljevic, N. aut Blennow, M. aut Bogomilov, M. aut Bouquerel, E. aut Burgman, A. aut Carlile, C. J. aut Cederkall, J. aut Christiansen, P. aut Collins, M. aut Cristaldo Morales, E. aut D’Alessi, L. aut Danared, H. aut de André, J. P. A. M. aut Delahaye, J. P. aut Dracos, M. aut Efthymiopoulos, I. aut Ekelöf, T. aut Eshraqi, M. aut Fanourakis, G. aut Fernandez-Martinez, E. aut Folsom, B. aut Ghosh, M. aut Gokbulut, G. aut Halić, L. aut Kayis Topaksu, A. aut Kliček, B. (orcid)0000-0002-5163-8085 aut Krhač, K. aut Lindroos, M. aut Mezzetto, M. aut Oglakci, M. aut Ohlsson, T. aut Olvegård, M. aut Ota, T. aut Park, J. aut Petkov, G. aut Poussot, P. aut Rosauro-Alcaraz, S. aut Stavropoulos, G. aut Stipčević, M. aut Terranova, F. aut Thomas, J. aut Tolba, T. aut Tsenov, R. aut Vankova-Kirilova, G. aut Vassilopoulos, N. aut Wildner, E. aut Wurtz, J. aut Zormpa, O. aut Zou, Y. aut Enthalten in The European physical journal / C Springer Berlin Heidelberg, 1998 81(2021), 12 vom: Dez. (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:81 year:2021 number:12 month:12 https://doi.org/10.1140/epjc/s10052-021-09845-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY AR 81 2021 12 12 |
| allfieldsGer |
10.1140/epjc/s10052-021-09845-8 doi (DE-627)OLC2077672706 (DE-He213)s10052-021-09845-8-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Alekou, A. verfasserin aut Updated physics performance of the ESSnuSB experiment 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2021 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 $$5\%$$ for signal and $$10\%$$ for background, we find that there is $$10\sigma $$$$(13\sigma )$$ CP violation discovery sensitivity for the baseline option of 540 km (360 km) at $$\delta _\mathrm{CP} = \pm 90^\circ $$. The corresponding fraction of $$\delta _\mathrm{CP}$$ for which CP violation can be discovered at more than $$5 \sigma $$ is $$70\%$$. Regarding CP precision measurements, the $$1\sigma $$ error associated with $$\delta _\mathrm{CP} = 0^\circ $$ is around $$5^\circ $$ and with $$\delta _\mathrm{CP} = -90^\circ $$ is around $$14^\circ $$$$(7^\circ )$$ for the baseline option of 540 km (360 km). For hierarchy sensitivity, one can have $$3\sigma $$ sensitivity for 540 km baseline except $$\delta _\mathrm{CP} = \pm 90^\circ $$ and $$5\sigma $$ sensitivity for 360 km baseline for all values of $$\delta _\mathrm{CP}$$. The octant of $$\theta _{23}$$ can be determined at $$3 \sigma $$ for the values of: $$\theta _{23} > 51^\circ $$ ($$\theta _{23} < 42^\circ $$ and $$\theta _{23} > 49^\circ $$) for baseline of 540 km (360 km). Regarding measurement precision of the atmospheric mixing parameters, the allowed values at $$3 \sigma $$ are: $$40^\circ< \theta _{23} < 52^\circ $$ ($$42^\circ< \theta _{23} < 51.5^\circ $$) and $$2.485 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.545 \times 10^{-3}$$ eV$$^2$$ ($$2.49 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.54 \times 10^{-3}$$ eV$$^2$$) for the baseline of 540 km (360 km). Baussan, E. aut Blaskovic Kraljevic, N. aut Blennow, M. aut Bogomilov, M. aut Bouquerel, E. aut Burgman, A. aut Carlile, C. J. aut Cederkall, J. aut Christiansen, P. aut Collins, M. aut Cristaldo Morales, E. aut D’Alessi, L. aut Danared, H. aut de André, J. P. A. M. aut Delahaye, J. P. aut Dracos, M. aut Efthymiopoulos, I. aut Ekelöf, T. aut Eshraqi, M. aut Fanourakis, G. aut Fernandez-Martinez, E. aut Folsom, B. aut Ghosh, M. aut Gokbulut, G. aut Halić, L. aut Kayis Topaksu, A. aut Kliček, B. (orcid)0000-0002-5163-8085 aut Krhač, K. aut Lindroos, M. aut Mezzetto, M. aut Oglakci, M. aut Ohlsson, T. aut Olvegård, M. aut Ota, T. aut Park, J. aut Petkov, G. aut Poussot, P. aut Rosauro-Alcaraz, S. aut Stavropoulos, G. aut Stipčević, M. aut Terranova, F. aut Thomas, J. aut Tolba, T. aut Tsenov, R. aut Vankova-Kirilova, G. aut Vassilopoulos, N. aut Wildner, E. aut Wurtz, J. aut Zormpa, O. aut Zou, Y. aut Enthalten in The European physical journal / C Springer Berlin Heidelberg, 1998 81(2021), 12 vom: Dez. (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:81 year:2021 number:12 month:12 https://doi.org/10.1140/epjc/s10052-021-09845-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY AR 81 2021 12 12 |
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10.1140/epjc/s10052-021-09845-8 doi (DE-627)OLC2077672706 (DE-He213)s10052-021-09845-8-p DE-627 ger DE-627 rakwb eng 530 VZ 530 VZ Alekou, A. verfasserin aut Updated physics performance of the ESSnuSB experiment 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © The Author(s) 2021 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 $$5\%$$ for signal and $$10\%$$ for background, we find that there is $$10\sigma $$$$(13\sigma )$$ CP violation discovery sensitivity for the baseline option of 540 km (360 km) at $$\delta _\mathrm{CP} = \pm 90^\circ $$. The corresponding fraction of $$\delta _\mathrm{CP}$$ for which CP violation can be discovered at more than $$5 \sigma $$ is $$70\%$$. Regarding CP precision measurements, the $$1\sigma $$ error associated with $$\delta _\mathrm{CP} = 0^\circ $$ is around $$5^\circ $$ and with $$\delta _\mathrm{CP} = -90^\circ $$ is around $$14^\circ $$$$(7^\circ )$$ for the baseline option of 540 km (360 km). For hierarchy sensitivity, one can have $$3\sigma $$ sensitivity for 540 km baseline except $$\delta _\mathrm{CP} = \pm 90^\circ $$ and $$5\sigma $$ sensitivity for 360 km baseline for all values of $$\delta _\mathrm{CP}$$. The octant of $$\theta _{23}$$ can be determined at $$3 \sigma $$ for the values of: $$\theta _{23} > 51^\circ $$ ($$\theta _{23} < 42^\circ $$ and $$\theta _{23} > 49^\circ $$) for baseline of 540 km (360 km). Regarding measurement precision of the atmospheric mixing parameters, the allowed values at $$3 \sigma $$ are: $$40^\circ< \theta _{23} < 52^\circ $$ ($$42^\circ< \theta _{23} < 51.5^\circ $$) and $$2.485 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.545 \times 10^{-3}$$ eV$$^2$$ ($$2.49 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.54 \times 10^{-3}$$ eV$$^2$$) for the baseline of 540 km (360 km). Baussan, E. aut Blaskovic Kraljevic, N. aut Blennow, M. aut Bogomilov, M. aut Bouquerel, E. aut Burgman, A. aut Carlile, C. J. aut Cederkall, J. aut Christiansen, P. aut Collins, M. aut Cristaldo Morales, E. aut D’Alessi, L. aut Danared, H. aut de André, J. P. A. M. aut Delahaye, J. P. aut Dracos, M. aut Efthymiopoulos, I. aut Ekelöf, T. aut Eshraqi, M. aut Fanourakis, G. aut Fernandez-Martinez, E. aut Folsom, B. aut Ghosh, M. aut Gokbulut, G. aut Halić, L. aut Kayis Topaksu, A. aut Kliček, B. (orcid)0000-0002-5163-8085 aut Krhač, K. aut Lindroos, M. aut Mezzetto, M. aut Oglakci, M. aut Ohlsson, T. aut Olvegård, M. aut Ota, T. aut Park, J. aut Petkov, G. aut Poussot, P. aut Rosauro-Alcaraz, S. aut Stavropoulos, G. aut Stipčević, M. aut Terranova, F. aut Thomas, J. aut Tolba, T. aut Tsenov, R. aut Vankova-Kirilova, G. aut Vassilopoulos, N. aut Wildner, E. aut Wurtz, J. aut Zormpa, O. aut Zou, Y. aut Enthalten in The European physical journal / C Springer Berlin Heidelberg, 1998 81(2021), 12 vom: Dez. (DE-627)235469777 (DE-600)1397769-6 (DE-576)061879150 1434-6044 nnns volume:81 year:2021 number:12 month:12 https://doi.org/10.1140/epjc/s10052-021-09845-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY AR 81 2021 12 12 |
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Alekou, A. Baussan, E. Blaskovic Kraljevic, N. Blennow, M. Bogomilov, M. Bouquerel, E. Burgman, A. Carlile, C. J. Cederkall, J. Christiansen, P. Collins, M. Cristaldo Morales, E. D’Alessi, L. Danared, H. de André, J. P. A. M. Delahaye, J. P. Dracos, M. Efthymiopoulos, I. Ekelöf, T. Eshraqi, M. Fanourakis, G. Fernandez-Martinez, E. Folsom, B. Ghosh, M. Gokbulut, G. Halić, L. Kayis Topaksu, A. Kliček, B. Krhač, K. Lindroos, M. Mezzetto, M. Oglakci, M. Ohlsson, T. Olvegård, M. Ota, T. Park, J. Petkov, G. Poussot, P. Rosauro-Alcaraz, S. Stavropoulos, G. Stipčević, M. Terranova, F. Thomas, J. Tolba, T. Tsenov, R. Vankova-Kirilova, G. Vassilopoulos, N. Wildner, E. Wurtz, J. Zormpa, O. Zou, Y. |
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updated physics performance of the essnusb experiment |
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Updated physics performance of the ESSnuSB experiment |
| 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 $$5\%$$ for signal and $$10\%$$ for background, we find that there is $$10\sigma $$$$(13\sigma )$$ CP violation discovery sensitivity for the baseline option of 540 km (360 km) at $$\delta _\mathrm{CP} = \pm 90^\circ $$. The corresponding fraction of $$\delta _\mathrm{CP}$$ for which CP violation can be discovered at more than $$5 \sigma $$ is $$70\%$$. Regarding CP precision measurements, the $$1\sigma $$ error associated with $$\delta _\mathrm{CP} = 0^\circ $$ is around $$5^\circ $$ and with $$\delta _\mathrm{CP} = -90^\circ $$ is around $$14^\circ $$$$(7^\circ )$$ for the baseline option of 540 km (360 km). For hierarchy sensitivity, one can have $$3\sigma $$ sensitivity for 540 km baseline except $$\delta _\mathrm{CP} = \pm 90^\circ $$ and $$5\sigma $$ sensitivity for 360 km baseline for all values of $$\delta _\mathrm{CP}$$. The octant of $$\theta _{23}$$ can be determined at $$3 \sigma $$ for the values of: $$\theta _{23} > 51^\circ $$ ($$\theta _{23} < 42^\circ $$ and $$\theta _{23} > 49^\circ $$) for baseline of 540 km (360 km). Regarding measurement precision of the atmospheric mixing parameters, the allowed values at $$3 \sigma $$ are: $$40^\circ< \theta _{23} < 52^\circ $$ ($$42^\circ< \theta _{23} < 51.5^\circ $$) and $$2.485 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.545 \times 10^{-3}$$ eV$$^2$$ ($$2.49 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.54 \times 10^{-3}$$ eV$$^2$$) for the baseline of 540 km (360 km). © The Author(s) 2021 |
| abstractGer |
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 $$5\%$$ for signal and $$10\%$$ for background, we find that there is $$10\sigma $$$$(13\sigma )$$ CP violation discovery sensitivity for the baseline option of 540 km (360 km) at $$\delta _\mathrm{CP} = \pm 90^\circ $$. The corresponding fraction of $$\delta _\mathrm{CP}$$ for which CP violation can be discovered at more than $$5 \sigma $$ is $$70\%$$. Regarding CP precision measurements, the $$1\sigma $$ error associated with $$\delta _\mathrm{CP} = 0^\circ $$ is around $$5^\circ $$ and with $$\delta _\mathrm{CP} = -90^\circ $$ is around $$14^\circ $$$$(7^\circ )$$ for the baseline option of 540 km (360 km). For hierarchy sensitivity, one can have $$3\sigma $$ sensitivity for 540 km baseline except $$\delta _\mathrm{CP} = \pm 90^\circ $$ and $$5\sigma $$ sensitivity for 360 km baseline for all values of $$\delta _\mathrm{CP}$$. The octant of $$\theta _{23}$$ can be determined at $$3 \sigma $$ for the values of: $$\theta _{23} > 51^\circ $$ ($$\theta _{23} < 42^\circ $$ and $$\theta _{23} > 49^\circ $$) for baseline of 540 km (360 km). Regarding measurement precision of the atmospheric mixing parameters, the allowed values at $$3 \sigma $$ are: $$40^\circ< \theta _{23} < 52^\circ $$ ($$42^\circ< \theta _{23} < 51.5^\circ $$) and $$2.485 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.545 \times 10^{-3}$$ eV$$^2$$ ($$2.49 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.54 \times 10^{-3}$$ eV$$^2$$) for the baseline of 540 km (360 km). © The Author(s) 2021 |
| abstract_unstemmed |
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 $$5\%$$ for signal and $$10\%$$ for background, we find that there is $$10\sigma $$$$(13\sigma )$$ CP violation discovery sensitivity for the baseline option of 540 km (360 km) at $$\delta _\mathrm{CP} = \pm 90^\circ $$. The corresponding fraction of $$\delta _\mathrm{CP}$$ for which CP violation can be discovered at more than $$5 \sigma $$ is $$70\%$$. Regarding CP precision measurements, the $$1\sigma $$ error associated with $$\delta _\mathrm{CP} = 0^\circ $$ is around $$5^\circ $$ and with $$\delta _\mathrm{CP} = -90^\circ $$ is around $$14^\circ $$$$(7^\circ )$$ for the baseline option of 540 km (360 km). For hierarchy sensitivity, one can have $$3\sigma $$ sensitivity for 540 km baseline except $$\delta _\mathrm{CP} = \pm 90^\circ $$ and $$5\sigma $$ sensitivity for 360 km baseline for all values of $$\delta _\mathrm{CP}$$. The octant of $$\theta _{23}$$ can be determined at $$3 \sigma $$ for the values of: $$\theta _{23} > 51^\circ $$ ($$\theta _{23} < 42^\circ $$ and $$\theta _{23} > 49^\circ $$) for baseline of 540 km (360 km). Regarding measurement precision of the atmospheric mixing parameters, the allowed values at $$3 \sigma $$ are: $$40^\circ< \theta _{23} < 52^\circ $$ ($$42^\circ< \theta _{23} < 51.5^\circ $$) and $$2.485 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.545 \times 10^{-3}$$ eV$$^2$$ ($$2.49 \times 10^{-3}$$ eV$$^2< \varDelta m^2_{31} < 2.54 \times 10^{-3}$$ eV$$^2$$) for the baseline of 540 km (360 km). © The Author(s) 2021 |
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Updated physics performance of the ESSnuSB experiment |
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Baussan, E. Blaskovic Kraljevic, N. Blennow, M. Bogomilov, M. Bouquerel, E. Burgman, A. Carlile, C. J. Cederkall, J. Christiansen, P. Collins, M. Cristaldo Morales, E. D’Alessi, L. Danared, H. de André, J. P. A. M. Delahaye, J. P. Dracos, M. Efthymiopoulos, I. Ekelöf, T. Eshraqi, M. Fanourakis, G. Fernandez-Martinez, E. Folsom, B. Ghosh, M. Gokbulut, G. Halić, L. Kayis Topaksu, A. Kliček, B. Krhač, K. Lindroos, M. Mezzetto, M. Oglakci, M. Ohlsson, T. Olvegård, M. Ota, T. Park, J. Petkov, G. Poussot, P. Rosauro-Alcaraz, S. Stavropoulos, G. Stipčević, M. Terranova, F. Thomas, J. Tolba, T. Tsenov, R. Vankova-Kirilova, G. Vassilopoulos, N. Wildner, E. Wurtz, J. Zormpa, O. Zou, Y. |
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Baussan, E. Blaskovic Kraljevic, N. Blennow, M. Bogomilov, M. Bouquerel, E. Burgman, A. Carlile, C. J. Cederkall, J. Christiansen, P. Collins, M. Cristaldo Morales, E. D’Alessi, L. Danared, H. de André, J. P. A. M. Delahaye, J. P. Dracos, M. Efthymiopoulos, I. Ekelöf, T. Eshraqi, M. Fanourakis, G. Fernandez-Martinez, E. Folsom, B. Ghosh, M. Gokbulut, G. Halić, L. Kayis Topaksu, A. Kliček, B. Krhač, K. Lindroos, M. Mezzetto, M. Oglakci, M. Ohlsson, T. Olvegård, M. Ota, T. Park, J. Petkov, G. Poussot, P. Rosauro-Alcaraz, S. Stavropoulos, G. Stipčević, M. Terranova, F. Thomas, J. Tolba, T. Tsenov, R. Vankova-Kirilova, G. Vassilopoulos, N. Wildner, E. Wurtz, J. Zormpa, O. Zou, Y. |
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