129 citations · 382 across the 23 of their papers we have counts for
25 papers
Natural Chlorine Enhances Antineutrino Detection in the Deep Ocean
Ruike Cao, Iwan Morton-Blake, Donglian Xu +16
Large-volume neutrino telescopes such as IceCube and KM3NeT exploit natural ice or water as detection media, but their sparse instrumentation makes MeV neutrino interactions diffic…
Final assessment of radioactive impurities in the JUNO detector
Thomas Adam, Fengpeng An, Costas Andreopoulos +569
The Jiangmen Underground Neutrino Observatory (JUNO) collaboration has completed the construction of the 20,000-ton liquid scintillator detector and the associated muon veto detect…
A Low-energy Threshold and Multi-messenger Trigger System for the JUNO Experiment
Thomas Adam, Fengpeng An, Costas Andreopoulos +563
The Jiangmen Underground Neutrino Observatory (JUNO) is a 20-kiloton liquid scintillator neutrino detector, located 650 meters (1800 m.w.e.) underground in Jiangmen, Guangdong, Chi…
Embedded underwater front-end electronics for the 3-inch photomultipliers in the JUNO experiment
Cédric Cerna, Miao He, Xiaoshan Jiang +591
The Jiangmen Underground Neutrino Observatory (JUNO) is a 20-kton liquid scintillator-based, low-radioactivity, multi-purpose neutrino detector located 693 meters (1800 m.w.e.) und…
Probing Dark Matter annihilation in the Galactic Centre with TRIDENT
Yingwei Wang, Xinhui Chu, Andrew Cheek +7
We determine the future sensitivity of the TRIDENT neutrino telescope to dark matter annihilation in the Galactic Centre. By applying the full detector design and assuming an NFW h…
Prospects for geoneutrino detection with JUNO
Thomas Adam, Shakeel Ahmad, Rizwan Ahmed +625
Geoneutrinos, which are antineutrinos emitted during the decay of long-lived radioactive elements inside Earth, serve as a unique tool for studying the composition and heat budget…
Optimising Underwater Neutrino Telescopes for All-Flavour Point Source Sensitivity
Iwan Morton-Blake, Fuyudi Zhang, Qichao Chang +7
High-energy neutrino astronomy has advanced rapidly in recent years, with IceCube, KM3NeT, and Baikal-GVD establishing a diffuse astrophysical flux and pointing to promising source…
Design, waterproofing, and mass production of the 3-inch PMT frontend system of JUNO
Jilei Xu, Miao He, Cédric Cerna +628
Over 25,600 3-inch photomultiplier tubes (PMTs) have been instrumented for the central detector of the Jiangmen Underground Neutrino Observatory. Each PMT is equipped with a high-v…
A Cost Effective Optimization of the hybrid-DOM Design for TRIDENT
Hengbin Shao, Fuyudi Zhang, Qichao Chang +11
TRIDENT is a planned multi-cubic-kilometer deep-sea neutrino telescope to be built in the South China Sea, designed to rapidly discover high-energy astrophysical neutrino sources w…
Simulation of the Background from CO Reaction in the JUNO Scintillator
JUNO Collaboration, Thomas Adam, Kai Adamowicz +627
Large-scale organic liquid scintillator detectors are highly efficient in the detection of MeV-scale electron antineutrinos. These signal events can be detected through inverse bet…
Measurement of reactor antineutrino oscillation at SNO+
SNO+ Collaboration, :, M. Abreu +298
The SNO+ collaboration reports its second spectral analysis of reactor antineutrino oscillation using 286 tonne-years of new data. The measured energies of reactor antineutrino can…
Neutron source-based event reconstruction algorithm in large liquid scintillator detectors
Akira Takenaka, Zhangming Chen, Arran Freegard +10
We developed an event reconstruction algorithm, applicable to large liquid scintillator detectors, built primarily upon neutron calibration data. We employ a likelihood method usin…
Initial measurement of reactor antineutrino oscillation at SNO+
SNO+ Collaboration, :, A. Allega +119
The SNO+ collaboration reports its first spectral analysis of long-baseline reactor antineutrino oscillation using 114 tonne-years of data. Fitting the neutrino oscillation probabi…
Real-time Monitoring for the Next Core-Collapse Supernova in JUNO
Angel Abusleme, Thomas Adam, Shakeel Ahmad +623
The core-collapse supernova (CCSN) is considered one of the most energetic astrophysical events in the universe. The early and prompt detection of neutrinos before (pre-SN) and dur…
Event-by-Event Direction Reconstruction of Solar Neutrinos in a High Light-Yield Liquid Scintillator
A. Allega, M. R. Anderson, S. Andringa +116
The direction of individual B solar neutrinos has been reconstructed using the SNO+ liquid scintillator detector. Prompt, directional Cherenkov light was separated from the slo…
Evidence of Antineutrinos from Distant Reactors using Pure Water at SNO+
SNO+ Collaboration, :, A. Allega +114
The SNO+ Collaboration reports the first evidence of reactor antineutrinos in a Cherenkov detector. The nearest nuclear reactors are located 240~km away in Ontario, Canada. This an…
A multi-cubic-kilometre neutrino telescope in the western Pacific Ocean
Z. P. Ye, F. Hu, W. Tian +54
Next-generation neutrino telescopes with significantly improved sensitivity are required to pinpoint the sources of the diffuse astrophysical neutrino flux detected by IceCube and…
Improved search for invisible modes of nucleon decay in water with the SNO+ detector
SNO+ Collaboration, :, A. Allega +116
This paper reports results from a search for single and multi-nucleon disappearance from the O nucleus in water within the \snoplus{} detector using all of the available dat…
An Alternative Design for Large Scale Liquid Scintillator Detectors
Iwan Morton-Blake, Steven D. Biller
The construction of large-scale liquid scintillator detectors is complicated by the need to separate the scintillation region from photomultiplier tubes (PMTs) due to their intrins…
Optical calibration of the SNO+ detector in the water phase with deployed sources
SNO+ Collaboration, :, M. R. Anderson +120
SNO+ is a large-scale liquid scintillator experiment with the primary goal of searching for neutrinoless double beta decay, and is located approximately 2 km underground in SNOLAB,…
The SNO+ Experiment
SNO+ Collaboration, :, V. Albanese +251
The SNO+ experiment is located 2 km underground at SNOLAB in Sudbury, Canada. A low background search for neutrinoless double beta () decay will be conducted using 780 tonnes…
Development, characterisation, and deployment of the SNO+ liquid scintillator
SNO+ Collaboration, :, M. R. Anderson +223
A liquid scintillator consisting of linear alkylbenzene as the solvent and 2,5-diphenyloxazole as the fluor was developed for the SNO+ experiment. This mixture was chosen as it is…
Measurement of neutron-proton capture in the SNO+ water phase
The SNO+ Collaboration, :, M. R. Anderson +130
The SNO+ experiment collected data as a low-threshold water Cherenkov detector from September 2017 to July 2019. Measurements of the 2.2-MeV produced by neutron capture on hydr…
Measurement of the B Solar Neutrino Flux in SNO+ with Very Low Backgrounds
The SNO+ Collaboration, :, M. Anderson +120
A measurement of the B solar neutrino flux has been made using a 69.2 kt-day dataset acquired with the SNO+ detector during its water commissioning phase. At energies above 6 M…