Fluorescence time profile measurement of LAB based liquid scintillator in response to medium relativistic ion particles
Xiaojie Luo, Shuya Jin, Gaosong Li, Zepeng Li, Fenhua Lu, Yazhou Sun, Shitao Wang, Yaoguang Wang, Yifang Wang, Xiaobao Wei, Liangjian Wen
TL;DR
The study addresses how LAB-based liquid scintillator time profiles depend on the ionization density $dE/dX$ by measuring fluorescence timing for high-energy ions ($Z=1$, $Z=2$, and Krypton) and comparing to MeV-scale radioactive sources. A thin 5 mm LAB-based scintillator sample read out by fast PMTs, coupled with a downstream energy detector, is used to capture detailed time spectra, which are analyzed with a four-component exponential model convolved with the PMT response. GEANT4 simulations guide particle identification and energy deposition, enabling separation of Z=1 and Z=2 samples and assessment of the role of secondary electrons in Kr interactions. The results reveal that ions with similar $dE/dX$ can exhibit timing close to electron-like responses, while Kr shows reduced long-time tails due to secondary-electron contributions, underscoring the importance of $dE/dX$ in scintillation timing and offering a path toward a unified time model for PSD in large detectors like JUNO and for DSNB searches.
Abstract
Liquid scintillator is widely used in particle physics experiments due to its high light yield, good timing resolution, scalability and low cost. Certain liquid scintillators exhibit pulse shape discrimination capabilities because of difference in fluorescence timing properties induced by different particles. Its fluoresence timing properties have been measured mostly for radioactive decay sources at MeV energies. We present a novel measurement of fluorescence time properties of LAB based liquid scintillator in response to high-energy ions of hydrogen (Z = 1), helium (Z = 2) and Krypton at around 200-300 MeV/u for the first time. We compared the results to those from radioactive sources and observed a distinct $dE/dX$ dependence, regardless of the particle type. These findings are essential for physics searches such as the diffuse supernova neutrino background in large liquid scintillator detectors like JUNO, and are also critical towards understanding the underlying scintillation timing mechanism.
