Measurement of cosmogenic Li 9 and He 8 production rates at RENO

H. G. Lee, J. H. Choi, H. I. Jang, J. S. Jang, S. H. Jeon, K. K. Joo, D. E. Jung, J. G. Kim, J. H. Kim, J. Y. Kim, S. B. Kim, S. Y. Kim, W. Kim, E. Kwon, D. H. Lee, W. J. Lee, I. T. Lim, D. H. Moon, M. Y. Pac, J. S. ParkR. G. Park, H. Seo, J. W. Seo, C. D. Shin, B. S. Yang, J. Yoo, S. G. Yoon, I. S. Yeo, I. Yu

Research output: Contribution to journalArticlepeer-review

2 Scopus citations

Abstract

We report the measured production rates of unstable isotopes Li9 and He8 produced by cosmic muon spallation on C12 using two identical detectors of the RENO experiment. Their β decays accompanied by a neutron make a significant contribution to backgrounds of reactor antineutrino events in precise determination of the smallest neutrino mixing angle. The mean muon energy of its near (far) detector with an overburden of 120 (450) m.w.e. is estimated as 33.1±2.3(73.6±4.4) GeV. Based on roughly 3100 days of data, the cosmogenic production rate of Li9(He8) isotope is measured to be 44.2±3.1(10.6±7.4) per day at near detector and 10.0±1.1(2.1±1.5) per day at far detector. This corresponds to yields of Li9(He8), 4.80±0.36(1.15±0.81) and 9.9±1.1(2.1±1.5) at near and far detectors, respectively, in a unit of 10-8 μ-1 g-1 cm2. Combining the measured Li9 yields with other available underground measurements, an excellent power-law relationship of the yield with respect to the mean muon energy is found to have an exponent of α=0.75±0.05.

Original languageEnglish
Article number012005
JournalPhysical Review D
Volume106
Issue number1
DOIs
StatePublished - 1 Jul 2022

Fingerprint

Dive into the research topics of 'Measurement of cosmogenic Li 9 and He 8 production rates at RENO'. Together they form a unique fingerprint.

Cite this