24–29 Aug 2014
Hamburg University
Europe/Berlin timezone

Liquid scintillators for Daya Bay neutrino experiment and JUNO experiment

Not scheduled
1m
Main Building (Hamburg University)

Main Building

Hamburg University

Edmund-Siemers-Allee 1 Hamburg <a href="https://www.google.com/maps/place/Edmund-Siemers-Allee+1/@53.56303,9.98782,17z/data=!3m1!4b1!4m2!3m1!1s0x47b18f3cbed7b4f1:0xffb72ee7b0f3c774">PANIC14 venue at University Hamburg</a>
Poster 3) Neutrinos and related astrophysical implications

Speaker

Dr Yayun Ding (Institute of High Energy Physics, Chinese Academy of Sciences)

Description

Daya Bay Reactor Neutrino Experiment is designed to measure the mixing angle θ13 using 8 identical Anti-neutrino detectors (AD). Each AD contains 20-ton Gadolinium-loaded liquid scintillator (Gd-LS) as the target for catching neutrino. Optical properties and stability of Gd-LS are of great important for the experiment. Here we report the choice of Gd-LS recipe and the preparation procedures of 185-ton Gd-LS. Both results based on periodical characterization of Gd-LS and data taken from AD show 185-ton Gd-LS meets the requirements of Daya Bay experiment. Jiangmen Underground Neutrino Observatory (JUNO) is a multipurpose neutrino experiment which is going to use a huge detector containing 20-kiloton liquid scintillator for catching neutrino. Requirements for JUNO LS, such as attenuation length, light yield and radio-impurity content, are very strict because of the size of the detector. Pre-study of LS at IHEP show production of 20-kt qualified LS are very promising.

Primary author

Dr Yayun Ding (Institute of High Energy Physics, Chinese Academy of Sciences)

Presentation materials