PandaX detector calibration and response. 报告人 : 肖梦姣 Shanghai Jiao Tong University (On behalf of the Panda-X Collaboration)

Similar documents
Paolo Agnes Laboratoire APC, Université Paris 7 on behalf of the DarkSide Collaboration. Dark Matter 2016 UCLA 17th - 19th February 2016

Light Dark Matter and XENON100. For the XENON100 Collaboration Rafael F. Lang Columbia University

PANDA-X A New Detector for Dark Matter Search. Karl Giboni Shanghai Jiao Tong University

DarkSide-50: performance and results from the first atmospheric argon run

DarkSide. Bianca Bottino Università di Genova and INFN Sezione di Genova on behalf of the DarkSide collaboration 1

Factors Affecting Detector Performance Goals and Alternative Photo-detectors

The XENON Project. M. Selvi The XENON project

arxiv:physics/ v1 3 Aug 2006

nerix PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014 Columbia University REU, XENON

Direct WIMP Detection in Double-Phase Xenon TPCs

Recent results from PandaX- II and status of PandaX-4T

XMASS: a large single-phase liquid-xenon detector

Recent Results from the PandaX Experiment

XENON100. Marc Schumann. Physik Institut, Universität Zürich. IDM 2010, Montpellier, July 26 th,

arxiv:astro-ph/ v1 15 Feb 2005

PoS(EPS-HEP2017)074. Darkside Status and Prospects. Charles Jeff Martoff Temple University

PANDA-?? A New Detector for Dark Matter Search

Background and sensitivity predictions for XENON1T

Low Energy Particles in Noble Liquids

arxiv: v1 [physics.ins-det] 31 Oct 2015 Alden Fan 1

Understanding the response of LXe to electronic and nuclear recoils at low energies

The Neutron/WIMP Acceptance In XENON100

Down-to-earth searches for cosmological dark matter

DARWIN. Marc Schumann. U Freiburg LAUNCH 17 Heidelberg, September 15,

The relevance of XENON10 constraints in this low-mass region has been questioned [15] C.E. Aalseth et al. arxiv: v1

The XENON1T experiment

TWO-PHASE DETECTORS USING THE NOBLE LIQUID XENON. Henrique Araújo Imperial College London

LUX: A Large Underground Xenon detector. WIMP Search. Mani Tripathi, INPAC Meeting. Berkeley, May 5, 2007

Measurement of 39 Ar in Underground Argon for Dark Matter Experiments

The LZ Experiment Tom Shutt SLAC. SURF South Dakota

PandaX Dark Matter Search

DARK MATTER SEARCH AT BOULBY MINE

LARGE UNDERGROUND XENON

Nuclear Recoil Scintillation and Ionization Yields in Liquid Xenon

Status of the XENON100 Dark Matter Search

LUX-ZEPLIN (LZ) Status. Attila Dobi Lawrence Berkeley National Laboratory June 10, 2015 WIN Heidelberg

Dark Matter Detection and the XENON Experiment. 1 Abstract. 2 Introduction

DarkSide new results and prospects

Studies of the XENON100 Electromagnetic Background

Search for Weakly Interacting Massive Particles with CDMS and XENON

The XENON100 Dark Matter Experiment at LNGS: Status and Sensitivity

Scintillation Efficiency of Nuclear Recoils in Liquid Xenon. T. Wongjirad, L. Kastens, A. Manzur, K. Ni, and D.N. McKinsey Yale University

Measurements of liquid xenon s response to low-energy particle interactions

Results from DarkSide-50 with underground argon

Oddities of light production in the noble elements. James Nikkel

Current status of LUX Dark Matter Experiment

Direct dark matter search using liquid noble gases

The Dual-Phase Liquid Xenon Time Projection Chamber (TPC) of Münster

The XENON dark matter search. T. Shutt CWRU

PHY 599: How it is usually done

Chung-Yao Fellowship 2016 interview

SIGN: A Pressurized Noble Gas Approach to WIMP Detection

DARWIN. Marc Schumann. U Freiburg PATRAS 2017 Thessaloniki, May 19,

arxiv: v1 [physics.ins-det] 14 May 2015

Probing the Intrinsic Electron Recoil Rejection Power in Liquid Xenon for Dark Matter Searches

First Results from the XENON10 Dark Matter Search at Gran Sasso. Elena Aprile Columbia University for the XENON Collaboration

XENON Dark Matter Search. Juliette Alimena Columbia University REU August 2 nd 2007

arxiv: v2 [physics.ins-det] 26 Oct 2015

DARWIN. Marc Schumann Physik Institut, Universität Zürich. Aspera Technology Forum 2010, October 21-22, 2010

X-ray ionization yields and energy spectra in liquid argon

The XENON Dark Matter Project: Status of the XENON100 Phase. Elena Aprile Columbia University

Calibration of Single Phase Liquid Argon Detectors

Luca Grandi.

Dark matter search activities at CIEMAT

Optimization of Non-Gaussian Background Rejection in XENON10

arxiv: v1 [physics.ins-det] 5 Nov 2015

Direct dark matter search using liquid noble gases

Prospects for WIMP Dark Matter Direct Searches with XENON1T and DARWIN

Technical Specifications and Requirements on Direct detection for Dark Matter Searches

the DarkSide project Andrea Pocar University of Massachusetts, Amherst

The Search for Dark Matter with the XENON Experiment

The XENON100 Dark Matter Experiment

After LUX: The LZ Program. David Malling, Simon Fiorucci Brown University APS DPF Conference August 10, 2011

Supernova Neutrino Physics with XENON1T and Beyond

The ArDM Experiment. A Double Phase Argon Calorimeter and TPC for Direct Detection of Dark Matter

LOW ENERGY SOLAR NEUTRINOS WITH BOREXINO. Lea Di Noto on behalf of the Borexino collaboration

Prospects for 0-ν ββ Search with a High-Pressure Xenon Gas TPC. What s NEXT?

Searching for Dark Matter From XENON10 to LUX. Luiz de Viveiros

Hands on DarkSide-50: Low Energy Calibration

DarkSide-20k and the future Liquid Argon Dark Matter program. Giuliana Fiorillo Università degli Studi di Napoli Federico II & INFN Napoli

THE NEXT EXPERIMENT FOR NEUTRINOLESS DOUBLE BETA DECAY SEARCHES ANDER SIMÓN ESTÉVEZ ON BEHALF OF THE NEXT COLLABORATION

The next generation dark matter hunter: XENON1T status and perspective

PMT Calibration and Neutron Generator Simulation for nerix

XENONNT AND BEYOND. Hardy Simgen. WIN 2015 MPIK Heidelberg. Max-Planck-Institut für Kernphysik Heidelberg

The ArDM project: A Liquid Argon TPC for Dark Matter Detection

Performance of the Gamma-ray Imaging Detector with Micro-TPC

next The NEXT double beta decay experiment Andrew Laing, IFIC (CSIC & UVEG) on behalf of the NEXT collaboration. TAUP2015, Torino, 8/09/2015

LAAPD Performance Measurements in Liquid Xenon

Background Characterization and Rejection in the LZ Detector. David Malling Brown University IDM 2012 July 25, 2012

Current and Future of WIMP Search in DarkSide

Status of the ANAIS experiment at Canfranc

Recent results and status of the XENON program

Status and Sensitivity Projections for the XENON100 Dark Matter Experiment

Testing the Purity Monitor for the XENON Dark Matter Search

WIMP Dark Matter Search with XENON and DARWIN

Recent Progress from the DEAP-3600 Dark Matter Direct Detection Experiment

Laboratori Nazionali del GranSasso Alfredo G. Cocco Istituto Nazionale di Fisica Nucleare Sezione di Napoli

The XENON1T Experiment

X-ray ionization yields and energy spectra in liquid argon

Micro Pixel Chamber Operation with Gas Electron Multiplier

Transcription:

PandaX detector calibration and response 报告人 : 肖梦姣 Shanghai Jiao Tong University (On behalf of the Panda-X Collaboration) 1

Outline 1. Detector running conditions 2. LED calibration Setup of the optical system PMTs gain and SPE resolution calibration 3. Radioactive source calibration Geometry of the source position Detector response and position reconstructed Gamma calibration (light yield, electron lifetime, resolution) Electron recoil band 4. Summary 2

1. Detector running conditions Inner Pressure: ~1.05 barg, Outer Vacuum: <1.0E-3 Pa; Cathode HV: -10 kv (drift field ~390 V/cm); Grid HV: -4.2 kv (extraction field ~7 kv/cm); Detected both scintillation (S1) and proportional (S2) light. 3

2. LED calibration The optical system: 1). Setup the LEDs outside the detector to void to induce the EMI; 2). Install 2 teflon balls as the diffusers on the top PMTs array; 3). LEDs and diffusers are coupled to the optical fibers and feedthroughs. 4

Calibration: Gain and SPE resolution Top pmt Gain were balanced ~2E6 Bottom pmt 5

3. Radioactive source calibration 1). Geometry of the source position SS tube PE tube 6

2). Detector response and position reconstructed 7

2). Detector response and position reconstructed Double scatter event 8

3). Gamma calibration: light yield at zero field Light yield at zero field: ~6.0 pe/kev for 662 kev (~6.42 pe/kev for122 kev) (Xenon100: 3.8 pe/kevee for 122 kevee) 9

3). Gamma calibration: light yield at field Light Yield at field (drift field ~390 V/cm and extraction field ~7 kv/cm): ~2.8 pe/kev Co60 Cs137 10

3). Gamma calibration: electron lifetime N=N0*exp(-dt/τ). N: number of electron drifting to gas/liquid interface; N0: number of initial free electrons; dt: the drift time; τ: electron lifetime, strongly dependent of impurity level. Average electron drift velocity ~2 mm/μs 165μs~33cm (maximum drfit length TPC is 15cm.) 11

3). Gamma calibration: resolution Resolution with only light (S1) or charge signal S2 Resolution with S1_only: 10.20% at Cs137 peak (662 kev) Resolution with S2_only: 7.36% at Cs137 peak (662 kev) 12

3). Gamma calibration: resolution Resolution with combined energy (S1+S2): ~3.5% Combine the energy through the anti-correlation of S2 and S1 Correlation of S1 and S2 Spectrum of combined energy 13

4.) Electron recoil band Discrimination between electron and nuclear recoils with S2/S1: S1: electrons recombination signal (scintillation) S2: ionized electrons escaped from recombination (ionization) 14

4.) Electron recoil band 15

Summary The detector of PandaX is working stable now and we are learning more and more about the detector. We carried out the LED calibration and the pmts and DAQ are working well. Many gamma calibration runs were taken and gave us much information about the detector, such as light/charge yield, electron lifetime, energy resolution and so on. We roughly got the electron recoil band now. The uniformity and neutron calibration will be carried on soon for the further study. 16

Thank you! 17