2022
DOI: 10.1007/s41365-022-01049-3
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Reconstruction of a muon bundle in the JUNO central detector

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Cited by 8 publications
(2 citation statements)
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“…The response function is dened as average function of Poisson process 𝑅 𝑗 (𝑑; π‘Ÿ, πœƒ, 𝐸) for point source event 𝛿(Γ¬ π‘Ÿ, 𝐸). As the result of energy linearity, we can extract the energy 𝐸 from intensity function 𝑅 𝑗 (𝑑; π‘Ÿ, πœƒ, 𝐸) = 𝐸 𝑅 𝑗 (𝑑; π‘Ÿ, πœƒ), (1) then we use polynomials to express 𝑅 𝑗 (𝑑; π‘Ÿ, πœƒ)…”
Section: Pmt Expected Response Functionmentioning
confidence: 99%
“…The response function is dened as average function of Poisson process 𝑅 𝑗 (𝑑; π‘Ÿ, πœƒ, 𝐸) for point source event 𝛿(Γ¬ π‘Ÿ, 𝐸). As the result of energy linearity, we can extract the energy 𝐸 from intensity function 𝑅 𝑗 (𝑑; π‘Ÿ, πœƒ, 𝐸) = 𝐸 𝑅 𝑗 (𝑑; π‘Ÿ, πœƒ), (1) then we use polynomials to express 𝑅 𝑗 (𝑑; π‘Ÿ, πœƒ)…”
Section: Pmt Expected Response Functionmentioning
confidence: 99%
“…Moreover, atmospheric neutrinos at JUNO can provide complementary measurements for the CP violation phase Ξ΄ CP . We are currently developing a more realistic sensitivity analysis with the recent progress and performance of atmospheric neutrino reconstructions [5][6][7][8]. We are also performing a combined analysis with the reactor antineutrinos that will further improve JUNO's NMO sensitivity.…”
Section: Atmospheric Neutrinosmentioning
confidence: 99%