Y. X. Chen
North China Electric Power University
Network
Latest external collaboration on country level. Dive into details by clicking on the dots.
Publication
Featured researches published by Y. X. Chen.
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 1999
P. Cennini; J.-P. Revol; C. Rubbia; F. Sergiampietri; A. Bueno; M. Campanelli; P Goudsmit; A. Rubbia; L. Periale; S. Suzuki; C. Chen; Y. X. Chen; K. He; X. T. Huang; Z. Li; F. Lu; J. Ma; G. Xu; Z. Xu; C. C. Zhang; Qingmin Zhang; S.C. Zheng; F. Cavanna; D. Mazza; G. Piano Mortari; S. Petrera; C. Rossi; G. Mannocchi; P. Picchi; F. Arneodo
A system to detect light from liquid argon scintillation has been implemented in a small, ICARUS-like, liquid argon time projection chamber. The system, which uses a VUV-sensitive photomultiplier to collect the light, has recorded many ionizing tracks from cosmic-rays in coincidence with scintillation signals. Our measurements demonstrate that scintillation light detection can provide an effective method for absolute time measurement of events and eventually a useful trigger signal
Nuclear Instruments & Methods in Physics Research Section A-accelerators Spectrometers Detectors and Associated Equipment | 2000
F. Arneodo; A. Badertscher; S Baibussinov; P. Benetti; A.Borio di Tigliole; R. Brunetti; A. Bueno; E. Calligarich; M. Campanelli; C. Carpanese; D. Cavalli; F. Cavanna; P. Cennini; S. Centro; A. Cesana; C. Chen; Y. X. Chen; D. Cline; I. De Mitri; R. Dolfini; A. Ferrari; A. Gigli Berzolari; P Goudsmit; K. He; X. T. Huang; Z. Li; F. Lu; J. Ma; G. Mannocchi; M Maris
Abstract The ICARUS time projection chamber can yield sound information on 8 B solar neutrinos. Owing to the high-energy resolution and the good capability of event reconstruction it can make a contribution to our understanding of neutrino intensities and their energy spectrum. Moreover, the MSW oscillation probability for sterile and active neutrinos can be well studied because both elastic scattering by electrons and absorption reaction on argon nuclei can be measured independently. The main problem in detecting the low-energy neutrino interactions arises from the environmental radioactivity. In the present work we study by Monte Carlo simulation the topology and the rates of the events, induced by neutrinos and background neutrons, in a 470 t (fiducial mass) liquid-argon TPC detector. For neutrino interactions we use the standard solar model BP98 and the recent experimental confirmation of the shell model computation of absorption cross section. The noise is estimated from new data on natural neutron background, collected in the hall C of the Gran Sasso laboratory. It is confirmed that, with a relatively modest neutron shielding and particular off-line event triggers, the weight of spurious events can be made to have little influence on the ICARUS solar neutrino measurement. Indeed, we expect 6 (26) background events per year in the 212 (759) elastic scattering (absorption reaction) sample.
Nuclear Physics B - Proceedings Supplements | 2000
C. Vignoli; F. Arneodo; A. Badertscher; E. Barbieri; P. Benetti; A.Borio di Tigliole; R. Brunetti; A. Bueno; E. Calligarich; M. Campanelli; F. Carli; C. Carpanese; D. Cavalli; F. Cavanna; P. Cennini; S. Centro; A. Cesana; C. Chen; Y. X. Chen; C. Cinquini; D. Cline; I. De Mitri; R. Dolfini; D. Favaretto; A. Ferrari; A. Gigli Berzolari; P Goudsmit; K. He; X. T. Huang; Z. Li
The goal of the ICARUS Project is the installation of a multi-kiloton LAr TPC in the underground Gran Sasso Laboratory. The programme foresees the realization of the detector in a modular way. The first step is the construction of a 600 ton module which is now at an advanced phase. It will be mounted and tested in Pavia in one year and then it will be moved to Gran Sasso for the final operation. The major cryogenic and purification systems and the mechanical components of the detector have been constructed and tested in a 10 m3 prototype. The results of these tests are here summarized.
Physical Review C | 2013
X.B. Ma; W. L. Zhong; L.Z. Wang; Y. X. Chen; Jun Cao
arXiv: Nuclear Experiment | 2014
X.B. Ma; F. Lu; L.Z. Wang; Y. X. Chen; W. L. Zhong; F. P. An
arXiv: High Energy Physics - Experiment | 2018
D. Adey; F.P. An; A. B. Balantekin; H. R. Band; M. Bishai; S. Blyth; D. Cao; G. F. Cao; Jun Cao; Y. L. Chan; J. F. Chang; Y. Chang; H. S. Chen; Shaomin Chen; Y. B. Chen; Y. X. Chen; J. H. Cheng; Z.K. Cheng; J. J. Cherwinka; M. C. Chu; A. Chukanov; J.P. Cummings; F.S. Deng; Y. Y. Ding; M. V. Diwan; M. Dolgareva; D.A. Dwyer; W. R. Edwards; M. Gonchar; G. H. Gong
arXiv: Instrumentation and Detectors | 2015
X.B. Ma; Y.F. Zhao; W.L. Zhong; F.P. An; Y. X. Chen
Proceedings of the 7th International Conference on ICATPP-7 | 2002
C. Vignoli; F. Arneodo; B. Babussinov; B. Badełek; A. Badertscher; M. Baldo-Ceolin; G. Battistoni; B. Bekman; P. Benetti; E. Bernardini; M. Bischofberger; A. Borio di Tigliole; R. Brunetti; A. Bueno; E. Calligarich; D. Cavalli; F. Cavanna; P. Cennini; S. Centro; A. Cesana; C. Chen; Y. X. Chen; D. Cline; A. Dabrowska; M. Daszkiewicz; C. De Vecchi; R. Dolfini; A. Ferrari; F. Ferri; A. Gigli Berzolari