Abulencia, A. et al. (CDF Collaboration)A. et al. (CDF Collaboration)AbulenciaYEE HSIUNG2021-07-282021-07-2820211689002https://www.scopus.com/inward/record.uri?eid=2-s2.0-85097731900&doi=10.1016%2fj.nima.2020.164823&partnerID=40&md5=3f67bbb655f97aadb03256d7a44b048ahttps://scholars.lib.ntu.edu.tw/handle/123456789/575151To maximize the light yield of the liquid scintillator (LS) for the Jiangmen Underground Neutrino Observatory (JUNO), a 20 t LS sample was produced in a pilot plant at Daya Bay. The optical properties of the new LS in various compositions were studied by replacing the gadolinium-loaded LS in one antineutrino detector. The concentrations of the fluor, PPO, and the wavelength shifter, bis-MSB, were increased in 12 steps from 0.5 g/L and <0.01 mg/L to 4 g/L and 13 mg/L, respectively. The numbers of total detected photoelectrons suggest that, with the optically purified solvent, the bis-MSB concentration does not need to be more than 4 mg/L. To bridge the one order of magnitude in the detector size difference between Daya Bay and JUNO, the Daya Bay data were used to tune the parameters of a newly developed optical model. Then, the model and tuned parameters were used in the JUNO simulation. This enabled to determine the optimal composition for the JUNO LS: purified solvent LAB with 2.5 g/L PPO, and 1 to 4 mg/L bis-MSB. ? 2020 Elsevier B.V.Optical properties; Pilot plants; Purification; Daya Bay; Detector size; Light yield; Liquid scintillator; Optical modeling; Optimal composition; Wavelength shifter; Scintillation counters[SDGs]SDG14Optimization of the JUNO liquid scintillator composition using a Daya Bay antineutrino detectorjournal article10.1016/j.nima.2020.1648232-s2.0-85097731900