2023
DOI: 10.3390/universe9080347
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The ESSnuSB Design Study: Overview and Future Prospects

Abstract: 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 second maximum, the necessary upgrades to the ESS linac in order to produce a neut… Show more

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Cited by 3 publications
(3 citation statements)
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References 41 publications
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“…The ESSnuSB collaboration has proposed an upgrade of this facility, aiming to reduce the proton pulse length from 2.86 ms to 1.3 µs using a proton accumulator. This shortened pulse duration would enable the use of standard magnetic horns for beam focusing, effectively transforming the ESS into a Superbeam facility [59,60]. Operating at the second oscillation maximum, the facility aims to achieve superior sensitivity in detecting the CP violation phase δ.…”
Section: The Second Oscillation Maximummentioning
confidence: 99%
See 1 more Smart Citation
“…The ESSnuSB collaboration has proposed an upgrade of this facility, aiming to reduce the proton pulse length from 2.86 ms to 1.3 µs using a proton accumulator. This shortened pulse duration would enable the use of standard magnetic horns for beam focusing, effectively transforming the ESS into a Superbeam facility [59,60]. Operating at the second oscillation maximum, the facility aims to achieve superior sensitivity in detecting the CP violation phase δ.…”
Section: The Second Oscillation Maximummentioning
confidence: 99%
“…where J ∼ sin θ 13 sin δ is the Jarlskog invariant. Following [60], we can compute the asymmetry ratio between the second and first oscillation maxima, corresponding to ∆ = 3π/2 and ∆ = π/2, respectively,…”
Section: The Second Oscillation Maximummentioning
confidence: 99%
“…We can now try to motivate the choice of the second atmospheric oscillation maximum for ESSnuSB. If we compute A 𝜇→𝑒 CP at the first and at the second maximum (when Δ𝑚 2 31 𝐿/4𝐸 = 𝜋/2, 3𝜋/2), we obtain that [5] A…”
Section: Neutrino Oscillation At the Second Oscillation Maximummentioning
confidence: 99%