A multi-stage liquid Xe based Dark Matter experiment at China JinPing Lab (location: Sichuan Province) Deepest dark matter facility, covered with 2,500m.

Slides:



Advertisements
Similar presentations
Masaki Yamashita XMASS at Kamioka Large Scale Cryogenic detector in the underground laboratory Masaki Yamashita Kamioka observatory, ICRR, Univ. Of Tokyo.
Advertisements

First Xenon Liquefaction at Nantes by using Pulse Tube Cryocooler Workshop FJPPL’07, 9-12 May 2007, KEK, Japan Tom Haruyama (KEK) Eric Morteau, Patrick.
1 Experimental Nuclear Physics at UMass UMass, February 1st, 2010.
Status of XMASS experiment Shigetaka Moriyama Institute for Cosmic Ray Research, University of Tokyo For the XMASS collaboration September 10 th, 2013.
DMSAG 14/8/06 Mark Boulay Towards Dark Matter with DEAP at SNOLAB Mark Boulay Canada Research Chair in Particle Astrophysics Queen’s University DEAP-1:
Dark Matter Searches with Dual-Phase Noble Liquid Detectors Imperial HEP 1st Year Talks ‒ Evidence and Motivation ‒ Dual-phase Noble Liquid Detectors ‒
The XENON Project A 1 tonne Liquid Xenon experiment for a sensitive Dark Matter Search Elena Aprile Columbia University.
PANDAX Results and Outlook
Search for Dark Matter at CJPL with PANDAX
Proportional Light in a Dual Phase Xenon Chamber
Cygnus 2013/06/05 Nagoya univ. H.Uchida for XMASS collaboration 1.
Carter Hall, University of Maryland August 7, 2015 DPF 2015, Ann Arbor, MI The LZ WIMP dark matter search.
NSF Dark Matter Program P5 Meeting, Sept 24-25, Dark Matter Searches Summary of NSF Dark Matter Projects Direct Detection (including co-funds with.
 Dark matter forms a giant sea, enclosing the milky way. The earth and solar system like a small fish, swimming in it.  Dark Matter particle has a small.
My Element Foldable for Lithium (as an example). Element Symbol Li 3 7.
New developments in Energy Havesting: US-China collaboration on Magnetocaloric Effect Materials Joseph H. Ross Jr., Texas A&M University Main Campus, DMR.
Dark Matter Detection with Liquid Xenon Masahiro Morii Harvard University Laboratory for Particle Physics and Cosmology 21 August
The Shaping of China’s Postdoctoral Community Andrea Lynn Stith, PhD Shanghai Jiao Tong University AC21 Annual Forum 2010 October 19-20, 2010.
Future work Kamioka Kyoto We feel WIMP wind oh the earth NEWAGE ~ Direction Sensitive Direct Dark Matter Search ~ Kyoto University Hironobu Nishimura
Bei Cai and Mark Boulay For the DEAP-1 Collaboration Queen’s University, Canada Pulse Shape Discrimination (PSD) in Liquid Argon from DEAP-1 APS meeting,
EUROPE Nov 27 –Dec 10 November 27 - Dec 10.
IPPOG masterclass working group May 15, Building an IceCube Collaboration outreach activity Inspired by the International Masterclasses for hands-
E. Beise, U MarylandJune E906 Targets Betsy Beise, U Maryland in collaboration with Wolfgang Lorenzon + Richard Raymond, U Michigan June 2008 collaboration.
Kamioka Kyoto We feel WIMP wind on the earth NEWAGE Direction-sensitive direct dark matter search with μ-TPC * 1.Dark.
Mechanics Physics12 Mass & weight Mechanics Physics12 Mass & weight.
Fermilab: Present and Future Young-Kee Kim Data Preservation Workshop May 16, 2011.
 Everything in the universe that has mass and takes up space.
DARK MATTER SEARCH Carter Hall, University of Maryland.
I. Giomataris, CEA-Irfu-France
The 4 th International Workshop on Future High Energy Circular Colliders 第四届未来高能环形对撞机国际研讨会 Shanghai Jiao Tong.
PandaX 实验中的电子学概述 郭国栋 Outline Introduction Original scheme Improved scheme PMT base design in PandaX I and PandaX II Decoupler design in.
Physics in Underground Laboratories G Gerbier IRFU-CEA & slides from Hue Qian (THU) Underground Labs uopdate Current programs Status of FCPPL 012 activities.
The Liquid Argon Test Facility in THU Qinghao Chen Tsinghua Univ. CDEX Tuebingen April 9, 2013 Development of High Purity Germanium.
Enter the DarkSide Stefano Davini University of Houston RICAP-13.
The INPAC A SJTU Xiao-Gang He INPAC Department of Physics and Astronomy Shanghai Jiao Tong University
China Deep Underground Laboratory and Dark Matter Search Hesheng Chen Institute of High Energy Physics.
0νDBD Experimental Review and 136 Xe With HP Gas at CJPL 季向 东.
Summary of the workshop Sun Kee Kim. Brief History of this meeting  Mini-workshop on WIMP search with crystals, Seoul (Henry Wong, Jin Li)
Roles of integrin β3 cytoplasmic tail in bidirectional signal transduction in a trans-dominant inhibition model Jiansong Huang,Yulan Zhou,Xiaoyu Su,Yuanjing.
P. Chaiyabin1, J. Lomon1, Prayoon Songsiriritthigul1. , P
LBNF/DUNE Update Public Meeting Sanford Lab Update
Fast neutron flux measurement in CJPL
PandaX DM Search Exp Xiangdong Ji (季向东)
GEM and MicroMegas R&D Xiaomei Li Science and Technology
Xiangyi Cui Shanghai Jiao Tong U. On Behalf of the Collaboration
Low-level impurity measurements in Xenon with cold traps
Special UCLA High Energy & Astro-Particle (HEAP) Seminar
UK Dark Matter Collaboration
Status and Future Developments of TPC’s with MPGD readout systems
Work on neutrino and dark matter experiments
TPC Conference, Paris 5 -7 December, 2016
PandaX-III 原型探测器进展 上海交通大学 林横
Large Area Cryogenic Gaseous Photo Multipliers
Low-Energy Neutrino and Dark Matter Physics with TEXONO Program
Direct Dark Matter Searches
Clicker #1 The two balloons above are the same size but contain different gases. How do the pressures inside the balloons compare? A) The pressures are.
جمهوری خلق چین گردآورندگان : محبوبه تقي زاده بهبهاني
تحليل الحساسية Sensitive Analysis.
杨勇 上海交通大学 On Behalf of the Collaboration 粒子物理数据分析基础和前沿研讨会,2016/9/13
China’s Provinces and Capitals
4th Grade Vocabulary Part Four
Clicker #1 The two balloons above are the same size but contain different gases. How do the pressures inside the balloons compare? A) The pressures are.
UCLA High Energy & Astro-Particle (HEAP) Seminar
LUX: Shedding Light on Dark Matter
Clicker #1 The two balloons above are the same size but contain different gases. How do the pressures inside the balloons compare? A) The pressures are.
Clicker #1 The two balloons above are the same size but contain different gases. How do the pressures inside the balloons compare? A) The pressures are.
Clicker #1 The two balloons above are the same size but contain different gases. How do the pressures inside the balloons compare? A) The pressures are.
Global liver disease burdens and research trends: Analysis from a Chinese perspective  Jia Xiao, Fei Wang, Nai-Kei Wong, Jinhan He, Rui Zhang, Ruijuan.
Lab Mass and Weight Page 51 – November 1, 2017.
Presentation transcript:

A multi-stage liquid Xe based Dark Matter experiment at China JinPing Lab (location: Sichuan Province) Deepest dark matter facility, covered with 2,500m of marble PandaX-1: Time Projection Chamber (TPC) design optimized for low mass dark matter PandaX-2: increase the fiducial mass: optimized for large mass dark matter PandaX location at CJPL PandaX-1a TPC (Particle AND Astrophysical Xenon TPC)

PandaX-1a: exposure: 25 kg x 300 days start Nov 2012 PandaX-2 (ton-scale): exposure: 1,200 kg x 600 days start 2015 expected sensitivity PandaX-2: world’s most sensitive Dark Matter search experiment

3 December 2011 collaboration meeting Wolfgang Lorenzon (PI - U-M) Xiangdong Ji (PI - PandaX) Member institutions: Shanghai Jiao Tong University (SJTU) Shanghai Institute of Applied Physics Shandong University Peking University University of Michigan (U-M) MOU between U-M & SJTU signed in September 2011