002776281 001__ 2776281
002776281 005__ 20240614055749.0
002776281 0248_ $$aoai:cds.cern.ch:2776281$$pcerncds:FULLTEXT$$pcerncds:CERN:FULLTEXT$$pcerncds:CERN
002776281 0247_ $$2DOI$$9arXiv$$a10.1140/epjc/s10052-021-09845-8$$qpublication
002776281 037__ $$9arXiv$$aarXiv:2107.07585$$chep-ex
002776281 035__ $$9arXiv$$aoai:arXiv.org:2107.07585
002776281 035__ $$9Inspire$$aoai:inspirehep.net:1886386$$d2021-10-27T14:48:30Z$$h2021-10-29T02:02:43Z$$mmarcxml$$ttrue$$uhttps://inspirehep.net/api/oai2d
002776281 035__ $$9Inspire$$a1886386
002776281 041__ $$aeng
002776281 100__ $$aAlekou, A.$$tGRID:grid.9132.9$$tGRID:grid.8993.b$$uCERN$$uUppsala U.$$vCERN, 1211 Geneva 23, Switzerland$$vUppsala University, P.O. Box 256, 751 05 Uppsala, Sweden
002776281 245__ $$9arXiv$$aUpdated physics performance of the ESSnuSB experiment
002776281 246__ $$9submitter$$aUpdated physics performance of the ESSnuSB experiment
002776281 269__ $$c2021-06-25
002776281 260__ $$c2021-12-23
002776281 260__ $$c2021-12
002776281 300__ $$a12 p
002776281 500__ $$9arXiv$$a13 pages, 8 figures, 3 tables. Changes: Text updated, this is a
published version
002776281 520__ $$9Springer$$aIn 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).
002776281 520__ $$9submitter$$an 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
10𝜎
10σ
(13𝜎)
(13σ) CP violation discovery sensitivity for the baseline option of 540 km (360 km) at
𝛿
CP
=±
90
∘
δCP=±90∘. The corresponding fraction of
𝛿
CP
δCP for which CP violation can be discovered at more than
5𝜎
5σ is
70%
70%. Regarding CP precision measurements, the
1𝜎
1σ error associated with
𝛿
CP
=
0
∘
δCP=0∘ is around
5
∘
5∘ and with
𝛿
CP
=−
90
∘
δCP=−90∘ is around
14
∘
14∘
(
7
∘
)
(7∘) for the baseline option of 540 km (360 km). For hierarchy sensitivity, one can have
3𝜎
3σ sensitivity for 540 km baseline except
𝛿
CP
=±
90
∘
δCP=±90∘ and
5𝜎
5σ sensitivity for 360 km baseline for all values of
𝛿
CP
δCP. The octant of
𝜃
23
θ23 can be determined at
3𝜎
3σ for the values of:
𝜃
23
>
51
∘
θ23>51∘ (
𝜃
23
<
42
∘
θ23<42∘ and
𝜃
23
>
49
∘
θ23>49∘) for baseline of 540 km (360 km). Regarding measurement precision of the atmospheric mixing parameters, the allowed values at
3𝜎
3σ are:
40
∘
<
𝜃
23
<
52
∘
40∘<θ23<52∘ (
42
∘
<
𝜃
23
<
51.5
∘
42∘<θ23<51.5∘) and
2.485×
10
−3
2.485×10−3 eV
2
<𝛥
𝑚
2
31
<2.545×
10
−3
2<Δm312<2.545×10−3 eV
2
2 (
2.49×
10
−3
2.49×10−3 eV
2
<𝛥
𝑚
2
31
<2.54×
10
−3
2<Δm312<2.54×10−3 eV
2
2) for the baseline of 540 km (360 km).`
002776281 520__ $$9arXiv$$aIn 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$$(13\sigma)$ CP violation discovery sensitivity for the baseline option of 540 km (360 km) at $\delta_{\rm CP} = \pm 90^\circ$. The corresponding fraction of $\delta_{\rm CP}$ for which CP violation can be discovered at more than $5 \sigma$ is $70\%$. Regarding CP precision measurements, the $1\sigma$ error associated with $\delta_{\rm CP} = 0^\circ$ is around $5^\circ$ and with $\delta_{\rm CP} = -90^\circ$ is around $14^\circ$$(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 $\delta_{\rm CP} = \pm 90^\circ$ and $5\sigma$ sensitivity for 360 km baseline for all values of $\delta_{\rm CP}$. 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$^2 < \Delta m^2_{31} < 2.545 \times 10^{-3}$ eV$^2$ ($2.49 \times 10^{-3}$ eV$^2 < \Delta m^2_{31} < 2.54 \times 10^{-3}$ eV$^2$) for the baseline of 540 km (360 km).
002776281 540__ $$3preprint$$aarXiv nonexclusive-distrib 1.0$$uhttp://arxiv.org/licenses/nonexclusive-distrib/1.0/
002776281 540__ $$3publication$$aCC-BY-4.0$$bSpringer$$uhttp://creativecommons.org/licenses/by/4.0/
002776281 542__ $$3publication$$dThe Author(s)$$g2021
002776281 65017 $$2arXiv$$aphysics.ins-det
002776281 65017 $$2SzGeCERN$$aDetectors and Experimental Techniques
002776281 65017 $$2arXiv$$ahep-ph
002776281 65017 $$2SzGeCERN$$aParticle Physics - Phenomenology
002776281 65017 $$2arXiv$$ahep-ex
002776281 65017 $$2SzGeCERN$$aParticle Physics - Experiment
002776281 690C_ $$aCERN
002776281 690C_ $$aARTICLE
002776281 693__ $$aESSnuSB
002776281 700__ $$aBaussan, E.$$tGRID:grid.462076.1$$uStrasbourg, IPHC$$vIPHC, Université de Strasbourg, CNRS/IN2P3, Strasbourg, France
002776281 700__ $$aBlaskovic Kraljevic, N. $$tGRID:grid.434715.0$$uESS, Lund$$vEuropean Spallation Source, Box 176, 221 00 Lund, Sweden
002776281 700__ $$aBlennow, M.$$tGRID:grid.5037.1$$tGRID:grid.411313.5$$uRoyal Inst. Tech., Sodertalje$$uStockholm U., OKC$$uRoyal Inst. Tech., Stockholm$$uStockholm Observ.$$vDepartment of Physics, School of Engineering Sciences, KTH Royal Institute of Technology, Roslagstullsbacken 21, 106 91 Stockholm, Sweden$$vThe Oskar Klein Centre, AlbaNova University Center, Roslagstullsbacken 21, 106 91 Stockholm, Sweden
002776281 700__ $$aBogomilov, M.$$tGRID:grid.11355.33$$uSofiya U.$$vFaculty of Physics, Sofia University St. Kliment Ohridski, 1164 Sofia, Bulgaria
002776281 700__ $$aBouquerel, E.$$tGRID:grid.462076.1$$uStrasbourg, IPHC$$vIPHC, Université de Strasbourg, CNRS/IN2P3, Strasbourg, France
002776281 700__ $$aBurgman, A.$$tGRID:grid.4514.4$$uLund U.$$vDepartment of Physics, Lund University, P.O Box 118, 221 00 Lund, Sweden
002776281 700__ $$aCarlile, C.J.$$tGRID:grid.8993.b$$uUppsala U. (main)$$uUppsala U.$$vDepartment of Physics and Astronomy, FREIA, Uppsala University, Box 516, 751 20 Uppsala, Sweden
002776281 700__ $$aCederkall, J.$$tGRID:grid.4514.4$$uLund U.$$vDepartment of Physics, Lund University, P.O Box 118, 221 00 Lund, Sweden
002776281 700__ $$aChristiansen, P.$$tGRID:grid.4514.4$$uLund U.$$vDepartment of Physics, Lund University, P.O Box 118, 221 00 Lund, Sweden
002776281 700__ $$aCollins, M.$$tGRID:grid.434715.0$$tGRID:grid.4514.4$$uESS, Lund$$uLund U.$$vEuropean Spallation Source, Box 176, 221 00 Lund, Sweden$$vFaculty of Engineering, Lund University, P.O Box 118, 221 00 Lund, Sweden
002776281 700__ $$aCristaldo Morales, E. $$tGRID:grid.7563.7$$uMilan Bicocca U.$$uINFN, Milan Bicocca$$vUniversity of Milano-Bicocca and INFN sez. di Milano-Bicocca, Milan, Italy
002776281 700__ $$aD'Alessi, [email protected]$$tGRID:grid.462076.1$$uMilan Bicocca U.$$uStrasbourg, IPHC$$vIPHC, Université de Strasbourg, CNRS/IN2P3, Strasbourg, France
002776281 700__ $$aDanared, H.$$tGRID:grid.434715.0$$uESS, Lund$$vEuropean Spallation Source, Box 176, 221 00 Lund, Sweden
002776281 700__ $$ade André, J.P. A.M.$$tGRID:grid.462076.1$$uStrasbourg, IPHC$$vIPHC, Université de Strasbourg, CNRS/IN2P3, Strasbourg, France
002776281 700__ $$aDelahaye, J.P.$$tGRID:grid.9132.9$$uCERN$$vCERN, 1211 Geneva 23, Switzerland
002776281 700__ $$aDracos, M.$$tGRID:grid.462076.1$$uStrasbourg, IPHC$$vIPHC, Université de Strasbourg, CNRS/IN2P3, Strasbourg, France
002776281 700__ $$aEfthymiopoulos, I.$$tGRID:grid.9132.9$$uCERN$$vCERN, 1211 Geneva 23, Switzerland
002776281 700__ $$aEkelöf, T.$$tGRID:grid.8993.b$$uUppsala U.$$vUppsala University, P.O. Box 256, 751 05 Uppsala, Sweden
002776281 700__ $$aEshraqi, M.$$tGRID:grid.434715.0$$uESS, Lund$$vEuropean Spallation Source, Box 176, 221 00 Lund, Sweden
002776281 700__ $$aFanourakis, G.$$tGRID:grid.450262.7$$uDemocritos Nucl. Res. Ctr.$$vInstitute of Nuclear and Particle Physics, NCSR Demokritos, Neapoleos 27, 15341 Agia Paraskevi, Greece
002776281 700__ $$aFernandez-Martinez, E.$$tGRID:grid.5515.4$$uMadrid, IFT$$uMadrid, Autonoma U.$$vDepartamento de Fisica Teorica and Instituto de Fisica Teorica, IFT-UAM/CSIC, Universidad Autonoma de Madrid, Cantoblanco, 28049 Madrid, Spain
002776281 700__ $$aFolsom, B.$$tGRID:grid.434715.0$$uESS, Lund$$vEuropean Spallation Source, Box 176, 221 00 Lund, Sweden
002776281 700__ $$aGhosh, [email protected]$$tGRID:grid.4905.8$$tGRID:grid.18048.35$$uBoskovic Inst., Zagreb$$uHyderabad U.$$vCenter of Excellence for Advanced Materials and Sensing Devices, Ruder Bošković Institute, 10000 Zagreb, Croatia$$vSchool of Physics, University of Hyderabad, 500046 Hyderabad, India
002776281 700__ $$aGokbulut, G.$$tGRID:grid.98622.37$$uCukurova U.$$vDepartment of Physics, Faculty of Science and Letters, University of Cukurova, 01330 Adana, Turkey
002776281 700__ $$aHalić, L.$$tGRID:grid.4905.8$$tGRID:grid.22939.33$$uBoskovic Inst., Zagreb$$uRijeka U.$$vCenter of Excellence for Advanced Materials and Sensing Devices, Ruder Bošković Institute, 10000 Zagreb, Croatia$$vDepartment of Physics, University of Rijeka, 51000 Rijeka, Croatia
002776281 700__ $$aKayis Topaksu, A.$$tGRID:grid.98622.37$$uCukurova U.$$vDepartment of Physics, Faculty of Science and Letters, University of Cukurova, 01330 Adana, Turkey
002776281 700__ $$aKliček, B.$$jORCID:[email protected]$$tGRID:grid.4905.8$$uBoskovic Inst., Zagreb$$vCenter of Excellence for Advanced Materials and Sensing Devices, Ruder Bošković Institute, 10000 Zagreb, Croatia
002776281 700__ $$aKrhač, K.$$tGRID:grid.4905.8$$uBoskovic Inst., Zagreb$$vCenter of Excellence for Advanced Materials and Sensing Devices, Ruder Bošković Institute, 10000 Zagreb, Croatia
002776281 700__ $$aLindroos, M.$$tGRID:grid.434715.0$$uESS, Lund$$vEuropean Spallation Source, Box 176, 221 00 Lund, Sweden
002776281 700__ $$aMezzetto, M.$$uINFN, Padua$$vINFN sez. di Padova, Padua, Italy
002776281 700__ $$aOglakci, M.$$tGRID:grid.98622.37$$uCukurova U.$$vDepartment of Physics, Faculty of Science and Letters, University of Cukurova, 01330 Adana, Turkey
002776281 700__ $$aOhlsson, T.$$tGRID:grid.5037.1$$tGRID:grid.411313.5$$uStockholm U., OKC$$uRoyal Inst. Tech., Stockholm$$uStockholm Observ.$$vDepartment of Physics, School of Engineering Sciences, KTH Royal Institute of Technology, Roslagstullsbacken 21, 106 91 Stockholm, Sweden$$vThe Oskar Klein Centre, AlbaNova University Center, Roslagstullsbacken 21, 106 91 Stockholm, Sweden
002776281 700__ $$aOlvegård, M.$$tGRID:grid.8993.b$$uUppsala U.$$vUppsala University, P.O. Box 256, 751 05 Uppsala, Sweden
002776281 700__ $$aOta, T.$$tGRID:grid.5515.4$$uMadrid, IFT$$uMadrid, Autonoma U.$$vDepartamento de Fisica Teorica and Instituto de Fisica Teorica, IFT-UAM/CSIC, Universidad Autonoma de Madrid, Cantoblanco, 28049 Madrid, Spain
002776281 700__ $$aPark, J.$$tGRID:grid.4514.4$$tGRID:grid.410720.0$$uIBS, Daejeon$$uLund U.$$vDepartment of Physics, Lund University, P.O Box 118, 221 00 Lund, Sweden$$vresent address: The center for Exotic Nuclear Studies, Institute for Basic Science, 34126 Daejeon, Korea
002776281 700__ $$aPetkov, G.$$tGRID:grid.11355.33$$uSofiya U.$$vFaculty of Physics, Sofia University St. Kliment Ohridski, 1164 Sofia, Bulgaria
002776281 700__ $$aPoussot, P.$$tGRID:grid.462076.1$$uStrasbourg, IPHC$$vIPHC, Université de Strasbourg, CNRS/IN2P3, Strasbourg, France
002776281 700__ $$aRosauro-Alcaraz, S.$$tGRID:grid.5515.4$$uMadrid, IFT$$uMadrid, Autonoma U.$$vDepartamento de Fisica Teorica and Instituto de Fisica Teorica, IFT-UAM/CSIC, Universidad Autonoma de Madrid, Cantoblanco, 28049 Madrid, Spain
002776281 700__ $$aStavropoulos, G.$$tGRID:grid.450262.7$$uDemocritos Nucl. Res. Ctr.$$vInstitute of Nuclear and Particle Physics, NCSR Demokritos, Neapoleos 27, 15341 Agia Paraskevi, Greece
002776281 700__ $$aStipčević, M.$$tGRID:grid.4905.8$$uBoskovic Inst., Zagreb$$vCenter of Excellence for Advanced Materials and Sensing Devices, Ruder Bošković Institute, 10000 Zagreb, Croatia
002776281 700__ $$aTerranova, F.$$tGRID:grid.7563.7$$uMilan Bicocca U.$$vUniversity of Milano-Bicocca and INFN sez. di Milano-Bicocca, Milan, Italy
002776281 700__ $$aThomas, J.$$tGRID:grid.462076.1$$uStrasbourg, IPHC$$vIPHC, Université de Strasbourg, CNRS/IN2P3, Strasbourg, France
002776281 700__ $$aTolba, T.$$tGRID:grid.9026.d$$uHamburg U.$$vInstitute for Experimental Physics, Hamburg University, 22761 Hamburg, Germany
002776281 700__ $$aTsenov, R.$$tGRID:grid.11355.33$$uSofiya U.$$vFaculty of Physics, Sofia University St. Kliment Ohridski, 1164 Sofia, Bulgaria
002776281 700__ $$aVankova-Kirilova, G.$$tGRID:grid.11355.33$$uSofiya U.$$vFaculty of Physics, Sofia University St. Kliment Ohridski, 1164 Sofia, Bulgaria
002776281 700__ $$aVassilopoulos, N.$$uCAS, IHEP, Dongguan$$vSpallation Neutron Science Center, 523803 Dongguan, China
002776281 700__ $$aWildner, E.$$tGRID:grid.9132.9$$uCERN$$vCERN, 1211 Geneva 23, Switzerland
002776281 700__ $$aWurtz, J.$$tGRID:grid.462076.1$$uStrasbourg, IPHC$$vIPHC, Université de Strasbourg, CNRS/IN2P3, Strasbourg, France
002776281 700__ $$aZormpa, O.$$tGRID:grid.450262.7$$uDemocritos Nucl. Res. Ctr.$$vInstitute of Nuclear and Particle Physics, NCSR Demokritos, Neapoleos 27, 15341 Agia Paraskevi, Greece
002776281 700__ $$aZou, Y.$$tGRID:grid.8993.b$$uUppsala U.$$vUppsala University, P.O. Box 256, 751 05 Uppsala, Sweden
002776281 710__ $$gESSnuSB Collaboration
002776281 773__ $$c1130$$n12$$pEur. Phys. J. C$$v81$$y2021
002776281 8564_ $$82311095$$s12281$$uhttps://cds.cern.ch/record/2776281/files/precision_360.png$$y00022 Sensitivity to the precision measurement of the atmospheric mixing parameters $\theta_{23}$ - $\Delta m^2_{31}$. The left and right panels are for the baseline options of 540 km and 360 km respectively.
002776281 8564_ $$82311096$$s10888$$uhttps://cds.cern.ch/record/2776281/files/event_ap_anu_540.png$$y00004 Appearance channel event spectrum vs reconstructed energy. The upper panels are for the baseline option of 540 km and the lower panels are for the baseline option of 360 km. Note the difference in scales between upper and lower panels.
002776281 8564_ $$82311097$$s11018$$uhttps://cds.cern.ch/record/2776281/files/cpv_expo.png$$y00013 CP violation discovery sensitivity of ESSnuSB. The top left panel shows the sensitivity as a function of true $\delta_{\rm CP}$. The top right panel shows the fraction of true values of $\delta_{\rm CP}$ for which CP violation can be discovered at $5 \sigma$ as a function of run-time. The left bottom panel shows the sensitivity corresponding to $\delta_{\rm CP}=-90^\circ$ as a function of run-time and the right panel shows the dependence of the sensitivity on the systematics uncertainties assuming 10 years of data collection.
002776281 8564_ $$82311098$$s10678$$uhttps://cds.cern.ch/record/2776281/files/event_disap_anu_540.png$$y00008 Disappearance channel event spectrum vs reconstructed energy. The upper panels are for the baseline option of 540 km and the lower panels are for the baseline option of 360 km. Note the difference in scales between upper and lower panels.
002776281 8564_ $$82311099$$s21628$$uhttps://cds.cern.ch/record/2776281/files/event_ap_nu_540.png$$y00003 Appearance channel event spectrum vs reconstructed energy. The upper panels are for the baseline option of 540 km and the lower panels are for the baseline option of 360 km. Note the difference in scales between upper and lower panels.
002776281 8564_ $$82311100$$s13984$$uhttps://cds.cern.ch/record/2776281/files/oct_540.png$$y00019 Hierarchy and octant sensitivity of ESSnuSB. The left panel corresponds to the hierarchy sensitivity as a function of $\delta_{\rm CP}$ (true). The middle and right panels correspond to the octant sensitivity in the $\theta_{23}$ (true) - $\delta_{\rm CP}$ (true) plane.
002776281 8564_ $$82311101$$s14180$$uhttps://cds.cern.ch/record/2776281/files/cpp_test_360.png$$y00017 CP precision sensitivity of ESSnuSB. Left panel shows the $1 \sigma$ error associated with a value of $\delta_{\rm CP}$ as a function of $\delta_{\rm CP}$ (true). The middle and right panels depict the CP precision in the $\delta_{\rm CP}$ (true) vs $\delta_{\rm CP}$ (test) plane.
002776281 8564_ $$82311102$$s10860$$uhttps://cds.cern.ch/record/2776281/files/event_disap_anu_360.png$$y00010 Disappearance channel event spectrum vs reconstructed energy. The upper panels are for the baseline option of 540 km and the lower panels are for the baseline option of 360 km. Note the difference in scales between upper and lower panels.
002776281 8564_ $$82311103$$s38935$$uhttps://cds.cern.ch/record/2776281/files/prob_nu.png$$y00000 Appearance channel probability and flux $\times$ cross-section vs energy. The left panel is for neutrinos and the right panel is for antineutrinos.
002776281 8564_ $$82311104$$s34915$$uhttps://cds.cern.ch/record/2776281/files/prob_anu.png$$y00001 Appearance channel probability and flux $\times$ cross-section vs energy. The left panel is for neutrinos and the right panel is for antineutrinos.
002776281 8564_ $$82311105$$s11158$$uhttps://cds.cern.ch/record/2776281/files/event_ap_anu_360.png$$y00006 Appearance channel event spectrum vs reconstructed energy. The upper panels are for the baseline option of 540 km and the lower panels are for the baseline option of 360 km. Note the difference in scales between upper and lower panels.
002776281 8564_ $$82311106$$s11006$$uhttps://cds.cern.ch/record/2776281/files/event_disap_nu_360.png$$y00009 Disappearance channel event spectrum vs reconstructed energy. The upper panels are for the baseline option of 540 km and the lower panels are for the baseline option of 360 km. Note the difference in scales between upper and lower panels.
002776281 8564_ $$82311107$$s22119$$uhttps://cds.cern.ch/record/2776281/files/event_ap_nu_360.png$$y00005 Appearance channel event spectrum vs reconstructed energy. The upper panels are for the baseline option of 540 km and the lower panels are for the baseline option of 360 km. Note the difference in scales between upper and lower panels.
002776281 8564_ $$82311108$$s13143$$uhttps://cds.cern.ch/record/2776281/files/precision_540.png$$y00021 Sensitivity to the precision measurement of the atmospheric mixing parameters $\theta_{23}$ - $\Delta m^2_{31}$. The left and right panels are for the baseline options of 540 km and 360 km respectively.
002776281 8564_ $$82311109$$s14345$$uhttps://cds.cern.ch/record/2776281/files/oct_360.png$$y00020 Hierarchy and octant sensitivity of ESSnuSB. The left panel corresponds to the hierarchy sensitivity as a function of $\delta_{\rm CP}$ (true). The middle and right panels correspond to the octant sensitivity in the $\theta_{23}$ (true) - $\delta_{\rm CP}$ (true) plane.
002776281 8564_ $$82311110$$s15911$$uhttps://cds.cern.ch/record/2776281/files/cpp_test_540.png$$y00016 CP precision sensitivity of ESSnuSB. Left panel shows the $1 \sigma$ error associated with a value of $\delta_{\rm CP}$ as a function of $\delta_{\rm CP}$ (true). The middle and right panels depict the CP precision in the $\delta_{\rm CP}$ (true) vs $\delta_{\rm CP}$ (test) plane.
002776281 8564_ $$82311111$$s12816$$uhttps://cds.cern.ch/record/2776281/files/bi_events.png$$y00002 The bi-event distribution for both baselines in the $\nu_e$ events vs $\bar{\nu}_e$ events plane. Different values of $\delta_{\rm CP}$ are shown by black markers.
002776281 8564_ $$82311112$$s10374$$uhttps://cds.cern.ch/record/2776281/files/cpv_frac_expo.png$$y00012 CP violation discovery sensitivity of ESSnuSB. The top left panel shows the sensitivity as a function of true $\delta_{\rm CP}$. The top right panel shows the fraction of true values of $\delta_{\rm CP}$ for which CP violation can be discovered at $5 \sigma$ as a function of run-time. The left bottom panel shows the sensitivity corresponding to $\delta_{\rm CP}=-90^\circ$ as a function of run-time and the right panel shows the dependence of the sensitivity on the systematics uncertainties assuming 10 years of data collection.
002776281 8564_ $$82311113$$s11101$$uhttps://cds.cern.ch/record/2776281/files/event_disap_nu_540.png$$y00007 Disappearance channel event spectrum vs reconstructed energy. The upper panels are for the baseline option of 540 km and the lower panels are for the baseline option of 360 km. Note the difference in scales between upper and lower panels.
002776281 8564_ $$82311114$$s9641$$uhttps://cds.cern.ch/record/2776281/files/hier.png$$y00018 Hierarchy and octant sensitivity of ESSnuSB. The left panel corresponds to the hierarchy sensitivity as a function of $\delta_{\rm CP}$ (true). The middle and right panels correspond to the octant sensitivity in the $\theta_{23}$ (true) - $\delta_{\rm CP}$ (true) plane.
002776281 8564_ $$82311115$$s11550$$uhttps://cds.cern.ch/record/2776281/files/cpp.png$$y00015 CP precision sensitivity of ESSnuSB. Left panel shows the $1 \sigma$ error associated with a value of $\delta_{\rm CP}$ as a function of $\delta_{\rm CP}$ (true). The middle and right panels depict the CP precision in the $\delta_{\rm CP}$ (true) vs $\delta_{\rm CP}$ (test) plane.
002776281 8564_ $$82311116$$s11040$$uhttps://cds.cern.ch/record/2776281/files/cpv_sys.png$$y00014 CP violation discovery sensitivity of ESSnuSB. The top left panel shows the sensitivity as a function of true $\delta_{\rm CP}$. The top right panel shows the fraction of true values of $\delta_{\rm CP}$ for which CP violation can be discovered at $5 \sigma$ as a function of run-time. The left bottom panel shows the sensitivity corresponding to $\delta_{\rm CP}=-90^\circ$ as a function of run-time and the right panel shows the dependence of the sensitivity on the systematics uncertainties assuming 10 years of data collection.
002776281 8564_ $$82311117$$s25547$$uhttps://cds.cern.ch/record/2776281/files/cpv.png$$y00011 CP violation discovery sensitivity of ESSnuSB. The top left panel shows the sensitivity as a function of true $\delta_{\rm CP}$. The top right panel shows the fraction of true values of $\delta_{\rm CP}$ for which CP violation can be discovered at $5 \sigma$ as a function of run-time. The left bottom panel shows the sensitivity corresponding to $\delta_{\rm CP}=-90^\circ$ as a function of run-time and the right panel shows the dependence of the sensitivity on the systematics uncertainties assuming 10 years of data collection.
002776281 8564_ $$82314199$$s1025897$$uhttps://cds.cern.ch/record/2776281/files/2107.07585.pdf$$yFulltext
002776281 8564_ $$82344618$$s1025897$$uhttps://cds.cern.ch/record/2776281/files/document.pdf$$yFulltext
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