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Peng Zhang , Ping Zhang , Qingmin Zhang , Rongping Zhang , Rui Zhang , Shaoping Zhang , Shiqi Zhang , Shu Zhang , Shuihan Zhang , Siyuan Zhang , Tao Zhang , Xiaofeng Zhang , Xiaomei Zhang , Xin Zhang , Xu Zhang , Xuan Zhang , Xuantong Zhang , Xuesong Zhang , Xueyao Zhang , Yan Zhang , Yibing Zhang , Yinhong Zhang , Yiyu Zhang , Yizhou Zhang , Yongjie Zhang , Yongpeng Zhang , Yu Zhang , Yuanyuan Zhang , Yue Zhang , Yueyuan Zhang , Yumei Zhang , Yuning Zhang , Zhenyu Zhang , Zhicheng Zhang , Zhijian Zhang , Zhixuan Zhang , Baoqi Zhao , Fengyi Zhao , Jie Zhao , Liang Zhao , Mei Zhao , Rong Zhao , Runze Zhao , Shujun Zhao , Tianchi Zhao , Tianhao Zhao , Yubin Zhao , Dongqin Zheng , Hua Zheng , Xiangyu Zheng , Yangheng Zheng , Weili Zhong , Weirong Zhong , Albert Zhou , Guorong Zhou , Li Zhou , Lishui Zhou , Min Zhou , Shun Zhou , Tong Zhou , Xiang Zhou , Xing Zhou , Yan Zhou , Haiwen Zhu , Jiang Zhu , Jingsen Zhu , Jingyu Zhu , Kangfu Zhu , Kejun Zhu , Zhihang Zhu , Ivan Zhutikov , Bo Zhuang , Honglin Zhuang , Liang Zong , Jiaheng Zou , Sebastian Zwickel , Jan Züfle
The Sudbury Neutrino Observatory (SNO) has unique capabilities as a supernova detector. In the event of a galactic supernova there are opportunities, with the data that SNO would collect, to constrain certain intrinsic neutrino properties…
We report on the results of a Monte Carlo simulation study of a km^3 scale deep underwater Cherenkov detector aimed at detecting neutrinos of astrophysical origin. This analysis has been undertaken as part of the NEMO R&D project to develop…
The Accelerator Neutrino Neutron Interaction Experiment (ANNIE) is a 26-ton Gd-doped water Cherenkov detector installed in the Booster Neutrino Beam (BNB) at Fermilab. The primary physics goal of ANNIE is to study the multiplicity of final…
The optical properties of the Sudbury Neutrino Observatory (SNO) heavy water Cherenkov neutrino detector are measured in situ using a light diffusing sphere ("laserball"). This diffuser is connected to a pulsed nitrogen/dye laser via…
Nuclear Experiment · Physics
2009-11-11
B. A. Moffat , R. J. Ford , F. A. Duncan , K. Graham , A. L. Hallin , C. A. W. Hearns , J. Maneira , P. Skensved , D. R. Grant
The IceCube Neutrino Observatory is a kilometer-scale detector currently under construction at the South Pole. The full detector will comprise 5,160 photomultipliers (PMTs) deployed on 86 strings from 1.45-2.45 km deep within the ice. As of…
Neutrino-electron scattering can be used to probe neutrino electromagnetic properties at low-threshold underground detectors with good angular and recoil electron energy resolution. We propose to do this using a number of artificial…
High Energy Physics - Phenomenology · Physics
2007-05-23
O. G. Miranda , J. Segura , V. B. Semikoz , J. W. F. Valle
Neutrinos from a future Galactic supernova will be detected by several large underground detectors, in particular by SuperKamiokande (SK) and the Sudbury Neutrino Observatory (SNO). If, as expected, the $\nu_{\mu}$ and $\nu_{\tau}$…
Water Cherenkov detectors offer a robust and economical solution for real-time radiation monitoring by detecting Cherenkov light from charged particles moving faster than light in water. This work presents a novel two-stage classification…
Instrumentation and Detectors · Physics
2026-01-27
Alejandro Núñez-Selin , Iván Sidelnik , Christian Sarmiento-Cano , Hernán Asorey , Luis A. Núñez
ANTARES is a project aiming at the operation of an underwater detector at a depth of 2.5 km close to Toulon in the South of France. The detector is expected to be completed at the beginning of 2007. The main purpose of the experiment is the…
Neutrinos in water can be detected thanks to several reactions. The most important one is the inverse beta decay $\bar\nu_{e}+p \rightarrow n+e^{+}$ . The detection of 2.2 MeV from neutron capture on free protons is very difficult. The…