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Featured researches published by H. Gong.


Physical Review D | 2014

Limits on light weakly interacting massive particles from the CDEX-1 experiment with ap-type point-contact germanium detector at the China Jinping Underground Laboratory

Q. Yue; Q. Du; H.J. He; N. Chen; Z.Z. Xianyu; J.M. Wang; M.B. Shen; J.Q. Qin; Shin-Ted Lin; H. Jiang; S.K. Liu; M. G. Zhao; Y.C. Chuang; Laxman Singh; Henry T. Wong; Jianping Cheng; Y. Li; H.X. Huang; Z. Y. Deng; W. Zhao; L. Zhang; X. Ruan; Haichan Yu; S.J. Mao; X.H. Zeng; H. B. Li; C.J. Tang; Y. H. Zhang; T. Xue; N. Yi

We report results of a search for light Dark Matter WIMPs with CDEX-1 experiment at the China Jinping Underground Laboratory, based on 53.9 kg-days of data from a p-type point-contact germanium detector enclosed by a NaI(Tl) crystal scintillator as anti-Compton detector. The event rate and spectrum above the analysis threshold of 475 eVee are consistent with the understood background model. Part of the allowed regions for WIMP-nucleus coherent elastic scattering at WIMP mass of 6-20 GeV are probed and excluded. Independent of interaction channels, this result contradicts the interpretation that the anomalous excesses of the CoGeNT experiment are induced by Dark Matter, since identical detector techniques are used in both experiments.


Frontiers of Physics in China | 2013

Introduction to the CDEX experiment

Kejun Kang; Jianping Cheng; Jin Li; Y.L. Li; Qian Yue; Yang Bai; Yong Bi; J.P. Chang; Nan Chen; Ning Chen; Qing-Hao Chen; Y.H. Chen; Yo-Chun Chuang; Zhi Deng; Qiang Du; H. Gong; X.Q. Hao; Hong-Jian He; Q.J. He; Xin-Hui Hu; H.X. Huang; T.R. Huang; H. Jiang; Hau-Bin Li; J.M. Li; Jun Li; Xia Li; Xin-Ying Li; Xue-Qian Li; Y. Li

It is believed that weakly interacting massive particles (WIMPs) are candidates for dark matter (DM) in our universe which come from outer space and might interact with the standard model (SM) matter of our detectors on the earth. Many collaborations in the world are carrying out various experiments to directly detect DM particles. China Jinping underground Laboratory (CJPL) is the deepest underground laboratory in the world and provides a very promising environment for DM search. China Dark matter EXperiment (CDEX) is going to directly detect the WIMP flux with high sensitivity in the low WIMP-mass region. Both CJPL and CDEX have achieved a remarkable progress in recent three years. CDEX employs a point-contact germanium (PCGe) semi-conductor detector whose energy threshold is less than 300 eV. In this report we present the measurement results of muon flux, monitoring of radioactivity and radon concentration carried out in CJPL, as well describing the structure and performance of the 1 kg-PCGe detector in CDEX-1 and 10 kg-PCGe detector array in CDEX-10 including the detectors, electronics, shielding and cooling systems. Finally we discuss the physics goals of CDEX-1, CDEX-10 and the future CDEX-1T experiments.


Physical Review D | 2013

First results on low-mass WIMPs from the CDEX-1 experiment at the China Jinping underground laboratory

W. Zhao; Q. Du; H.J. He; Nan Chen; Z.Z. Xianyu; J.M. Wang; M.B. Shen; J.Q. Qin; Shin-Ted Lin; H. Jiang; S.K. Liu; M. G. Zhao; Y.C. Chuang; Lakhwinder Singh; Su-Ning Zhong; Zhi Zeng; Henry T. Wong; Jianping Cheng; Y. Li; Xin-Hua Hu; Z. Y. Deng; J.P. Chang; L. Zhang; Kejun Kang; H. Yu; S.J. Mao; Wei Wu; Y. Bai; H. B. Li; Q. Yue

The China Dark matter Experiment collaboration reports the first experimental limit on WIMP dark matter from 14.6 kg-day of data taken with a 994 g p-type point-contact germanium detector at the China Jinping underground Laboratory where the rock overburden is more than 2400 m. The energy threshold achieved was 400 eVee. According to the 14.6 kg-day live data, we placed the limit of N= 1.75 * 10^{-40} cm^{2} at 90% confidence level on the spin-independent cross-section at WIMP mass of 7 GeV before differentiating bulk signals from the surface backgrounds.


Physical Review D | 2016

A Search of Low-Mass WIMPs with p-type Point Contact Germanium Detector in the CDEX-1 Experiment

W. Zhao; Q. Yue; K.J. Kang; Jianping Cheng; Y. Li; Henry T. Wong; Shin-Ted Lin; J.P. Chang; JingHan Chen; Qing-Hao Chen; Y.H. Chen; Z. Y. Deng; Q. Du; H. Gong; X.Q. Hao; H.J. He; Q.J. He; H.X. Huang; T.R. Huang; H. Jiang; H. B. Li; J. Li; J.M. Li; X. Q. Li; Xia Li; Y.L. Li; F.K. Lin; S.K. Liu; L.C. Lu; H. L. Ma

The CDEX-1 experiment conducted a search of low-mass (< 10 GeV/c2) Weakly Interacting Massive Particles (WIMPs) dark matter at the China Jinping Underground Laboratory using a p-type point-contact germanium detector with a fiducial mass of 915 g at a physics analysis threshold of 475 eVee. We report the hardware set-up, detector characterization, data acquisition and analysis procedures of this experiment. No excess of unidentified events are observed after subtraction of known background. Using 335.6 kg-days of data, exclusion constraints on the WIMP-nucleon spin-independent and spin-dependent couplings are derived.


Chinese Physics C | 2017

Physics prospects of the Jinping neutrino experiment

John F. Beacom; Shaomin Chen; Jianping Cheng; Sayed N. Doustimotlagh; Yuanning Gao; Guanghua Gong; H. Gong; L. Guo; Ran Han; Hong-Jian He; Xing-Tao Huang; Jianmin Li; Jin Li; Mohan Li; X. Q. Li; Wei Liao; Guey-Lin Lin; Zuowei Liu; William F. McDonough; Ondřej Šrámek; Jian Tang; Linyan Wan; Yuanqing Wang; Zhe Wang; Zongyi Wang; H.Y. Wei; Yufei Xi; Ye Xu; Xun-Jie Xu; Zhenwei Yang

Jinping Neutrino Experiment (Jinping) is proposed to significantly improve measurements on solar neutrinos and geoneutrinos in China Jinping Laboratory - a lab with a number of unparalleled features, thickest overburden, lowest reactor neutrino background, etc., which identify it as the world-best low-energy neutrino laboratory. The proposed experiment will have target mass of 4 kilotons of liquid scintillator or water-based liquid scintillator, with a fiducial mass of 2 kilotons for neutrino-electron scattering events and 3 kilotons for inverse-beta interaction events. A number of initial sensitivities studies have been carried out, including on the transition phase for the solar neutrinos oscillation from the vacuum to the matter effect, the discovery of solar neutrinos from the carbon-nitrogen-oxygen (CNO) cycle, the resolution of the high and low metallicity hypotheses, and the unambiguous separation on U and Th cascade decays from the dominant crustal anti-electron neutrinos in China.The China Jinping Underground Laboratory (CJPL), which has the lowest cosmic-ray muon flux and the lowest reactor neutrino flux of any laboratory, is ideal to carry out low-energy neutrino experiments. With two detectors and a total fiducial mass of 2000 tons for solar neutrino physics (equivalently, 3000 tons for geo-neutrino and supernova neutrino physics), the Jinping neutrino experiment will have the potential to identify the neutrinos from the CNO fusion cycles of the Sun, to cover the transition phase for the solar neutrino oscillation from vacuum to matter mixing, and to measure the geo-neutrino flux, including the Th/U ratio. These goals can be fulfilled with mature existing techniques. Efforts on increasing the target mass with multi-modular neutrino detectors and on developing the slow liquid scintillator will increase the Jinping discovery potential in the study of solar neutrinos, geo-neutrinos, supernova neutrinos, and dark matter.


Chinese Physics C | 2013

CDEX-1 1 kg point-contact germanium detector for low mass dark matter searches

Kejun Kang; Zhi Zeng; H. Jiang; Z.H. Zhu; Heng-Ye Liao; Ming-Gang Zhao; Yuan-Jing Li; Wei Wu; Xia Li; Zu-Ying Zhou; Manoj Kumar Singh; Su-Ning Zhong; X.H. Zeng; SongWei Yang; Chun-Xu Yu; HauBin Li; M.B. Shen; Y. Li; Li Wang; J.M. Wang; Q.J. He; Jianping Cheng; Xue-Qian Li; H. Yu; Qing-Hao Chen; A. K. Soma; J. Ren; Qian Yue; J.P. Chang; W.B. Zhu

The CDEX collaboration has been established for direct detection of light dark matter particles, using ultra-low energy threshold point-contact p-type germanium detectors, in China JinPing underground Laboratory (CJPL). The first 1 kg point-contact germanium detector with a sub-keV energy threshold has been tested in a passive shielding system located in CJPL. The outputs from both the point-contact P+ electrode and the outside N+ electrode make it possible to scan the lower energy range of less than 1 keV and at the same time to detect the higher energy range up to 3 MeV. The outputs from both P+ and N+ electrode may also provide a more powerful method for signal discrimination for dark matter experiment. Some key parameters, including energy resolution, dead time, decay times of internal X-rays, and system stability, have been tested and measured. The results show that the 1 kg point-contact germanium detector, together with its shielding system and electronics, can run smoothly with good performances. This detector system will be deployed for dark matter search experiments.


Chinese Physics C | 2018

Limits on light WIMPs with a 1 kg-scale germanium detector at 160 eVee physics threshold at the China Jinping Underground Laboratory*

L.T. Yang; Hau-Bin Li; Q. Yue; Kejun Kang; Jianping Cheng; Yuanjing Li; Henry T. Wong; M Aǧartioǧlu; HaiPeng An; J.P. Chang; JingHan Chen; Y.H. Chen; Zhi Deng; Q. Du; H. Gong; Li He; JinWei Hu; QingDong Hu; H.X. Huang; LiPing Jia; H. Jiang; Hong Li; Jianmin Li; Jin Li; Xia Li; Xue-Qian Li; Y. Li; F.K. Lin; Shin-Ted Lin; S.K. Liu

We report results of a search for light weakly interacting massive particle (WIMP) dark matter from the CDEX-1 experiment at the China Jinping Underground Laboratory (CJPL). Constraints on WIMP-nucleon spin-independent (SI) and spin-dependent (SD) couplings are derived with a physics threshold of 160 eVee, from an exposure of 737.1 kg-days. The SI and SD limits extend the lower reach of light WIMPs to 2 GeV and improve over our earlier bounds at WIMP mass less than 6 GeV.


nuclear science symposium and medical imaging conference | 2010

A 20ps resolution wave union FPGA TDC with on-chip real time correction

Ji Qi; Zhi Deng; H. Gong; Yinong Liu

Benefit from wave union, the bins (especially the ultra-wide bins) are sub-divided by each other, making FPGA TDC achieve a resolution beyond its cell delay. At such high level resolution, delay chain becomes very sensitive to the environment disturbance, including power supply voltage, temperature and current surge. On chip calibration needs lots of events and hence cannot follow fast delay changes of the chain. On-chip real time correction method proposed in this article gives one correcting parameter for each sample, making the FPGA TDC stronger when exposed to fast disturbance. A fast encoding logic is also implemented in our design and the dead time can be reduced to 1 clock cycle in the best case. Test results show a typical RMS of 20ps and the max RMS is below 30ps.


IEEE Transactions on Nuclear Science | 2012

On-Chip Real-Time Correction for a 20-ps Wave Union Time-To-Digital Converter (TDC) in a Field-Programmable Gate Array (FPGA)

Ji Qi; H. Gong; Yinong Liu

The latest delay chain-based FPGA TDCs can achieve resolutions around 10 ps. At such high levels of accuracy, delay chains become very sensitive to parasitic electromagnetic perturbations, including power supply voltage, temperature, and current surge. This paper describes how common-mode fast perturbation can deteriorate the spectra and make the root mean square (RMS) periodical as the input time interval increases. Based on this observation, an on-chip real-time correction method can be implemented, giving a correcting reference for each sample. Results show a typical RMS of 20 ps, with a maximum value below 30 ps, under the perturbation of around 100 mV and 20 kHz coming from the DC-DC module.


ieee nuclear science symposium | 2008

Design of prototyping PMT electronic system for Daya Bay Reactor Neutrino Experiment

Zheng Wang; Qiuju Li; Xiaonan Li; S. Chen; Y. C. Lin; Guanghua Gong; H. Gong; Christophe White; Qun Wu

This paper describes the design of the PMT Readout VME System developed by IHEP and Tsinghua University for the detector prototype of Daya Bay Reactor Neutrino Experiment. The readout electronics and the trigger event selection, with estimated rates, are presented along with the timing synchronization between all of the electronic elements. The processing of the data from the front-end modules through data storage is discussed, along with the detector control system.

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Y. Li

Tsinghua University

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Q. Yue

Tsinghua University

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