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

Size: px
Start display at page:

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

Transcription

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

2 Scintillation Efficiency! By Definition: Ratio of light produced by a nuclear recoil to the light produced by an electron recoil of the same energy In Practice: Convert signal -- calibrated to electron recoils -- into nuclear recoil energy S1 signal in pe Light Yield for 122 kev electron recoils in pe/ kevee (with field) Relative scintillation efficiency of NR to 122 kev gammas at zero field E nr = S1/L y /(L eff S nr /S er ) Reduction in light due to electric field for electron recoils (er) and nuclear recoils (nr)

3 Motivation WIMP interacts via nuclear recoil The scintillation efficiency for nuclear recoils is not well understood at energies below 10 kev - within the range of energies probed by the XENON10 experiment Effect of electric field not measured extensively The uncertainty in the Scintillation Efficiency is the dominant contribution to the uncertainty in the XENON10 WIMP-nucleon cross-section limit An accurately determined Scintillation Efficiency at low energies is crucial for calculating the WIMP sensitivity for future dark matter experiments (e.g. XENON100 and LUX)

4 Recent World Values (zero field) XENON10 SEARCH WINDOW* VALUE USED BY XENON10 19% Arneodo 2000 Akimov 2002 Aprile 2006 Chepel 2006 *USING 0.19

5 STAINLESS MESH APPLY E-FIELD Experimental Setup! 3 INCHES SCINTILLATOR COINCIDENCE DEFINES RECOIL ANGLE AND THUS ENERGY 1 meter MESH

6 122 kev GAMMA HIGH QE PMTS: HAMAMATSU 9869MOD (~37%) LIGHT YIELD ~11 phe/kevee

7 Purity measured in two-phase

8 Monte Carlo: GEANT4 MONTE CARLO SPECTRUM: DETECTOR ENERGY RESOLUTION AND SCINTILLATION EFFICIENCY APPLIED 35 DEGREES (7.7 kevr) SINGLE ELASTIC RECOIL IN LXE INELASTIC LXE RECOIL kevee MULTIPLE ELASTIC LXE RECOILS PURE SINGLE ELASTIC LXE RECOIL TIME OF FLIGHT CUT

9 DATA: 110 DEGREES (~56.9 kevr) RECOIL ENERGY TIME OF FLIGHT SCINTILLATOR PULSE SHAPE VS PULSE AREA CUT Cuts Used: SCINTILLATOR PULSE SHAPE CUT QUALITY CUTS (SATURATION, NOISE) TIME OF FLIGHT CUT

10 DATA: 35 DEGREES (7.7 kevr) RECOIL ENERGY TIME OF FLIGHT SCINTILLATOR PULSE SHAPE VS PULSE AREA CUT Cuts Used: SCINTILLATOR PULSE SHAPE CUT QUALITY CUTS (SATURATION, NOISE) TIME OF FLIGHT CUT

11 Data/Monte Carlo Analysis MONTE CARLO SPECTRUM CONSTRUCTED WITH A SCINTILLATION EFFICIENCY EQUAL TO DEGREES (7.7 kevr) DATA MONTE CARLO MONTE CARLO PURE SINGLE ELASTICS χ 2 reduced =0.99

12 Results: No Field (preliminary) XENON10 SEARCH WINDOW* INCLUDES SYSTEMATIC AND STATISTICAL UNCERTAINTY VALUE USED BY XENON10 19% THIS WORK Aprile 2006 Chepel 2006 *USING 0.19

13 Results: with Field (preliminary) S n =0.955 ± S n =0.950 ± (0.73 kv/cm) (1.50 kv/cm) INCLUDES SYSTEMATIC AND STATISTICAL UNCERTAINTY ZERO FIELD 0.73 kv/cm 1.5 kv/cm

14 Sources of Error Statistical Uncertainty: <10% (On the order of several hundreds of events per angle) Calibration uncertainty from PMT gain and light yield drifting: Variation in the measured Light Yield over a period of a couple of months is <5% Background events: Cut with TOF, Use MC to help pick cut Error in Scintillator Position Threshold Efficiency: Relevant for low energy nuclear recoils (below 6 kevr) Analysis is on-going

15 Future Directions Currently taking data in two-phase mode Triggering on proportional light to test threshold effect Verify single-phase data Measure charge yield for mono-energetic nuclear recoils: look for anti-correlation between light and charge

16 Monte Carlo Procedure (back up) Generate events with GEANT4.9.0.p01 Convert energy of points to kevee using different Scintillation efficiencies Also added energy resolution Compared to data using Chi-2 Best fit gives Scintilation Efficiency

17 Monte Carlo: GEANT4 25 DEGREES (~4 kevr) SINGLE ELASTIC RECOIL IN LXE INELASTIC LXE RECOIL MULTIPLE ELASTIC LXE RECOILS PURE SINGLE ELASTIC LXE RECOIL (1 MINUTE) TIME OF FLIGHT CUT

18 Monte Carlo/Data Comparison: Decent agreement with different Time Of Flight Cut (back up) TOF TOF TOF TOF DEGREES

19 Monte Carlo: Understanding Efficiency (back up) Use Monte Carlo at higher energies to help tune the applied threshold efficiency 125 DEGREES UNTUNED TUNED

20 Monte Carlo/Data Comparison:Light Efficiency Uncertainty (back up) 125 DEGREES BEST FIT LIGHT EFFICIENCY = 18.8% +1.2% -1.4%

21 15.00 Measured Mean (kevee) Vs. Recoil Energy (kevr) Peak Energy (kevee)

22

23 Monte Carlo: Understanding Efficiency (back up) Use Monte Carlo to characterize threshold efficiency Curve mostly determined by Trigger level PMT gain dispersion

Nuclear Recoil Scintillation and Ionization Yields in Liquid Xenon

Nuclear Recoil Scintillation and Ionization Yields in Liquid Xenon Nuclear Recoil Scintillation and Ionization Yields in Liquid Xenon Dan McKinsey Yale University Physics Department February, 011 Indirect and Direct Detection of Dark Matter Aspen Center of Physics Energy

More information

Scintillation efficiency measurement of Na recoils in NaI(Tl) below the DAMA/LIBRA energy threshold

Scintillation efficiency measurement of Na recoils in NaI(Tl) below the DAMA/LIBRA energy threshold Scintillation efficiency measurement of Na recoils in NaI(Tl) below the DAMA/LIBRA energy threshold Jingke Xu, Princeton (now @LLNL) Sept 24, 2015 2015 LowECal Workshop, Chicago, IL Outline 1. Overview

More information

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

Measurements of liquid xenon s response to low-energy particle interactions Measurements of liquid xenon s response to low-energy particle interactions Payam Pakarha Supervised by: Prof. L. Baudis May 5, 2013 1 / 37 Outline introduction Direct Dark Matter searches XENON experiment

More information

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

Light Dark Matter and XENON100. For the XENON100 Collaboration Rafael F. Lang Columbia University Light Dark Matter and XENON100 For the XENON100 Collaboration Rafael F. Lang Columbia University rafael.lang@astro.columbia.edu The XENON Collaboration ~60 scientists from 12 institutions: University of

More information

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

XENON100. Marc Schumann. Physik Institut, Universität Zürich. IDM 2010, Montpellier, July 26 th, XENON100 Marc Schumann Physik Institut, Universität Zürich IDM 2010, Montpellier, July 26 th, 2010 www.physik.uzh.ch/groups/groupbaudis/xenon/ Why WIMP search with Xenon? efficient, fast scintillator (178nm)

More information

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

TWO-PHASE DETECTORS USING THE NOBLE LIQUID XENON. Henrique Araújo Imperial College London TWO-PHASE DETECTORS USING THE NOBLE LIQUID XENON Henrique Araújo Imperial College London Oxford University 18 th October 2016 OUTLINE Two-phase xenon for (dark) radiation detection Instrumenting a liquid

More information

Status of the XENON100 Dark Matter Search

Status of the XENON100 Dark Matter Search Status of the XENON Dark Matter Search Guillaume Plante Columbia University on behalf of the XENON Collaboration Exploring Low-Mass Dark Matter Candidates - PITT PACC - November 146, 211 XENON Collaboration

More information

The Search for Dark Matter with the XENON Experiment

The Search for Dark Matter with the XENON Experiment The Search for Dark Matter with the XENON Experiment Elena Aprile Columbia University Paris TPC Workshop December 19, 2008 World Wide Dark Matter Searches Yangyang KIMS Homestake LUX SNOLAB DEAP/CLEAN

More information

arxiv:physics/ v1 3 Aug 2006

arxiv:physics/ v1 3 Aug 2006 Gamma Ray Spectroscopy with Scintillation Light in Liquid Xenon arxiv:physics/6834 v1 3 Aug 26 K. Ni, E. Aprile, K.L. Giboni, P. Majewski, M. Yamashita Physics Department and Columbia Astrophysics Laboratory

More information

Optimization of Non-Gaussian Background Rejection in XENON10

Optimization of Non-Gaussian Background Rejection in XENON10 Optimization of Non-Gaussian Background Rejection in XENON10? Peter Sorensen Brown University Peter Sorensen DSU 2007 p 1 Talk Summary 1. Brief overview of XENON10 installation/detector 2. Trigger Threshold

More information

Liquid Xenon Scintillator for Dark Matter Detection

Liquid Xenon Scintillator for Dark Matter Detection Liquid Xenon Scintillator for Dark Matter Detection Recent Results from the XENON10 Experiment Kaixuan Ni (Yale) IEEE - 9th International Conference on Inorganic Scintillators and their Applications Winston-Salem,

More information

Background and sensitivity predictions for XENON1T

Background and sensitivity predictions for XENON1T Background and sensitivity predictions for XENON1T Marco Selvi INFN - Sezione di Bologna (on behalf of the XENON collaboration) Feb 19 th 016, UCLA Dark Matter 016 1 Outline Description of the detector;

More information

Direct WIMP Detection in Double-Phase Xenon TPCs

Direct WIMP Detection in Double-Phase Xenon TPCs Outline PMTs in the XENON dark matter experiment XENON100 and the weekly gain calibration XENON1T and candidates for the light sensors Tests of Hamamatsu R11410 2 Direct WIMP Detection in Double-Phase

More information

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

The relevance of XENON10 constraints in this low-mass region has been questioned [15] C.E. Aalseth et al. arxiv: v1 The relevance of XENON10 constraints in this low-mass region has been questioned [15] C.E. Aalseth et al. arxiv:1001.2834v1 Peter Sorensen LLNL on behalf of the XENON10 Collaboration at UC Davis HEFTI

More information

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

XENON Dark Matter Search. Juliette Alimena Columbia University REU August 2 nd 2007 XENON Dark Matter Search Juliette Alimena Columbia University REU August 2 nd 2007 Evidence of Dark Matter Missing mass in Coma galaxy cluster (Fritz Zwicky) Flat rotation curves of spiral galaxies (Vera

More information

The XENON Project. M. Selvi The XENON project

The XENON Project. M. Selvi The XENON project The XENON Project M. Selvi Assemblea di Sezione 2011 Dark matter in the Universe Dark matter properties: what we know Direct WIMP search Direct WIMP search Direct WIMP detection Why Xenon? A double-phase

More information

Factors Affecting Detector Performance Goals and Alternative Photo-detectors

Factors Affecting Detector Performance Goals and Alternative Photo-detectors XENON Experiment - SAGENAP Factors Affecting Detector Performance Goals and Alternative Photo-detectors Department of Physics Brown University Source at http://gaitskell.brown.edu Gaitskell Review WIMP

More information

Liquefied noble gases as targets for light dark matter

Liquefied noble gases as targets for light dark matter Liquefied noble gases as targets for light dark matter Dan McKinsey Yale University Physics Department May 1, 2010 HEFTI Workshop on Light Dark Matter UC Davis The Noble Liquid Revolution Noble liquids

More information

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

Searching for Dark Matter From XENON10 to LUX. Luiz de Viveiros FCT - Universidade de Coimbra - Café com Física Searching for Dark Matter From XENON10 to LUX Luiz de Viveiros Brown University Physics Department De Viveiros - Brown University April 2009 v07 Summary

More information

The XENON1T experiment

The XENON1T experiment The XENON1T experiment Ranny Budnik Weizmann Institute of Science For the XENON collaboration 1 The XENON1T experiment Direct detection with xenon The XENON project XENON1T/nT 2 Quick introduction and

More information

XMASS: a large single-phase liquid-xenon detector

XMASS: a large single-phase liquid-xenon detector XMASS: a large single-phase liquid-xenon detector Katsuki Hiraide, the university of Tokyo for the XMASS Collaboration October 3 rd, 2016 IPRD16@Siena, Italy 1 XMASS project XMASS: a multi purpose experiment

More information

SIGN: A Pressurized Noble Gas Approach to WIMP Detection

SIGN: A Pressurized Noble Gas Approach to WIMP Detection SIGN: A Pressurized Noble Gas Approach to WIMP Detection J.T. White Texas A&M University Dark Side of the Universe U. Minnesota, 6/7/2007 Why Gaseous Nobles? Original Motivation: Neon Electron mobility

More information

arxiv:astro-ph/ v1 15 Feb 2005

arxiv:astro-ph/ v1 15 Feb 2005 The XENON Dark Matter Experiment Elena Aprile (on behalf of the XENON collaboration) Physics Department and Columbia Astrophysics Laboratory, Columbia University, New York, New York 10027 age@astro.columbia.edu

More information

Current status of LUX Dark Matter Experiment

Current status of LUX Dark Matter Experiment Current status of LUX Dark Matter Experiment by A. Lyashenko Yale University On behalf of LUX collaboration LUX Large Underground Xenon experiment LUX Collaboration: Yale, CWRU, UC Santa Barbara, Brown,

More information

The Neutron/WIMP Acceptance In XENON100

The Neutron/WIMP Acceptance In XENON100 The Neutron/WIMP Acceptance In XENON100 Symmetries and Fundamental Interactions 01 05 September 2014 Chiemsee Fraueninsel Boris Bauermeister on behalf of the XENON collaboration Boris.Bauermeister@uni-mainz.de

More information

Measurement of nuclear recoil responses of NaI(Tl) crystal for dark matter search

Measurement of nuclear recoil responses of NaI(Tl) crystal for dark matter search Measurement of nuclear recoil responses of NaI(Tl) crystal for dark matter search Hanwool Joo on behalf of the KIMS-NaI collaboration Department of Physics and Astronomy, 1 Gwanak-ro, Gwanak-gu, Seoul

More information

RESPONSE FUNCTION STUDY FOR ENERGY TO LIGHT CONVERSION IN ORGANIC LIQUID SCINTILLATORS

RESPONSE FUNCTION STUDY FOR ENERGY TO LIGHT CONVERSION IN ORGANIC LIQUID SCINTILLATORS RESPONSE FUNCTION STUDY FOR ENERGY TO LIGHT CONVERSION IN ORGANIC LIQUID SCINTILLATORS S. Prasad *, A. Enqvist, S. D. Clarke, S. A. Pozzi, E. W. Larsen 1 Department of Nuclear Engineering and Radiological

More information

arxiv: v1 [physics.ins-det] 27 Sep 2018

arxiv: v1 [physics.ins-det] 27 Sep 2018 Quenching factor measurement for a NaI(Tl) scintillation crystal arxiv:1809.10310v1 [physics.ins-det] 27 Sep 2018 H.W. Joo 1,2, H.S. Park 1,, J.H. Kim 1, S.K. Kim 2,, Y.D. Kim 3 H.S. Lee, 3, S.H. Kim 3

More information

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

DARWIN. Marc Schumann. U Freiburg PATRAS 2017 Thessaloniki, May 19, DARWIN Marc Schumann U Freiburg PATRAS 2017 Thessaloniki, May 19, 2017 marc.schumann@physik.uni-freiburg.de www.app.uni-freiburg.de 1 Dark Matter Searches: Status spin-independent WIMP-nucleon interactions

More information

Dark matter search with the SABRE experiment

Dark matter search with the SABRE experiment Dark matter search with the SABRE experiment Giulia D Imperio* for the SABRE collaboration *INFN Roma 1 25-07-2017 TAUP 2017 Sudbury, Canada 1 Dark matter detection through annual modulation WIMP is one

More information

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

After LUX: The LZ Program. David Malling, Simon Fiorucci Brown University APS DPF Conference August 10, 2011 After LUX: The LZ Program David Malling, Simon Fiorucci Brown University APS DPF Conference August 10, 2011 The LZ Program LZ LUX-ZEPLIN LUX (14 U.S. institutions) + new collaborators from ZEPLIN, other

More information

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

PoS(EPS-HEP2017)074. Darkside Status and Prospects. Charles Jeff Martoff Temple University Temple University E-mail: cmartoff@gmail.com The DarkSide Dark Matter Search Program is a direct-detection search for dark matter using a Liquid Argon Time Projection Chamber. The detector is designed

More information

Direct dark matter search with XMASS. K. Abe for the XMASS collaboration

Direct dark matter search with XMASS. K. Abe for the XMASS collaboration Direct dark matter search with XMASS K. Abe for the XMASS collaboration Outline XMASS experiment. Single phase liquid xenon detector Many targets were searched with XMASS. WIMP search fiducialized volume.

More information

XMASS 1.5, the next step of the XMASS experiment

XMASS 1.5, the next step of the XMASS experiment 1,2 for the XMASS collaboration 1 Kamioka Observatory, Institute for Cosmic Ray Research, the University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu 506-1205, Japan, 2 Kavli Institute for Physics and

More information

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

DARWIN. Marc Schumann Physik Institut, Universität Zürich. Aspera Technology Forum 2010, October 21-22, 2010 21-22 DARWIN Marc Schumann Physik Institut, Universität Zürich Aspera Technology Forum 2010, October 21-22, 2010 www.physik.uzh.ch/groups/groupbaudis/xenon/ Dark Matter: Evidence & Detection NASA/WMAP

More information

Measurement of 39 Ar in Underground Argon for Dark Matter Experiments

Measurement of 39 Ar in Underground Argon for Dark Matter Experiments Measurement of 39 Ar in Underground Argon for Dark Matter Experiments Jingke Xu Princeton University June 7 th, 2013 1 Evidences for Dark Matter Rotation Curve Gravitational Lensing CMB Power Spectrum

More information

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

nerix PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014 Columbia University REU, XENON nerix PMT Calibration and Neutron Generator Simulation Haley Pawlow July 31, 2014 Columbia University REU, XENON Dark Matter XENON nerix Project 1-> PMT Calibration Project 2-> Neutron Generator Simulation

More information

Studies of the XENON100 Electromagnetic Background

Studies of the XENON100 Electromagnetic Background Studies of the XENON100 Electromagnetic Background Daniel Mayani Physik-Institut University of Zurich PhD Seminar PSI, August 26-27, 2015 Searching for elusive particles The main challenge for experiments

More information

Supernova Neutrino Physics with XENON1T and Beyond

Supernova Neutrino Physics with XENON1T and Beyond Supernova Neutrino Physics with XENON1T and Beyond Shayne Reichard* University of Zurich nueclipse 2017 August 22 R. F. Lang*, C. McCabe, M. Selvi*, and I. Tamborra Phys. Rev. D94, arxiv:1606.09243 *Members

More information

WIMP Dark Matter Search with XENON and DARWIN

WIMP Dark Matter Search with XENON and DARWIN WIMP Dark Matter Search with XENON and DARWIN Johannes Gutenberg University Mainz, Germany XENON100 Rice University Houston, TX, USA http://xenon.physics.rice.edu 6th Patras Workshop Zurich July 7, 2010

More information

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

The Dual-Phase Liquid Xenon Time Projection Chamber (TPC) of Münster The Dual-Phase Liquid Xenon Time Projection Chamber (TPC) of Münster Calibration and Safety Aspects Schule für Astroteilchenphysik 2017 10.10.2017 Properties of Xenon as Detector Material Noble gas characterized

More information

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

First Results from the XENON10 Dark Matter Search at Gran Sasso. Elena Aprile Columbia University for the XENON Collaboration First Results from the XENON10 Dark Matter Search at Gran Sasso Columbia University for the XENON Collaboration APS-2007 The XENON10 Collaboration Columbia University (Spokesperson), Karl-Ludwig Giboni,

More information

Background Modeling and Materials Screening for the LUX and LZ Detectors. David Malling Brown University LUX Collaboration AARM Meeting February 2011

Background Modeling and Materials Screening for the LUX and LZ Detectors. David Malling Brown University LUX Collaboration AARM Meeting February 2011 Background Modeling and Materials Screening for the LUX and LZ Detectors David Malling Brown University LUX Collaboration AARM Meeting February 2011 1 Summary LUX screening program limits background contributions

More information

Axion search with Dark Matter detector

Axion search with Dark Matter detector Axion search with Dark Matter detector Paolo Beltrame Durham IPPP, 14th March 2016 1 Direct DM search Dark matter (DM) Milky Way s halo => flux on Earth ~ 10 5 cm -2 s -1 ρχ ~ 0.3 GeV/cm 3 and 100 GeV/c

More information

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

DARWIN. Marc Schumann. U Freiburg LAUNCH 17 Heidelberg, September 15, DARWIN Marc Schumann U Freiburg LAUNCH 17 Heidelberg, September 15, 2017 marc.schumann@physik.uni-freiburg.de www.app.uni-freiburg.de 1 Marc Schumann U Freiburg LAUNCH 17 Heidelberg, September 15, 2017

More information

Physics Letters B 705 (2011) Contents lists available at SciVerse ScienceDirect. Physics Letters B.

Physics Letters B 705 (2011) Contents lists available at SciVerse ScienceDirect. Physics Letters B. Physics Letters B 705 (2011) 471 476 Contents lists available at SciVerse ScienceDirect Physics Letters B www.elsevier.com/locate/physletb Nuclear recoil scintillation and ionisation yields in liquid xenon

More information

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

Paolo Agnes Laboratoire APC, Université Paris 7 on behalf of the DarkSide Collaboration. Dark Matter 2016 UCLA 17th - 19th February 2016 Paolo Agnes Laboratoire APC, Université Paris 7 on behalf of the DarkSide Collaboration Dark Matter 2016 UCLA 17th - 19th February 2016 The DarkSide program 2 Double Phase Liquid Argon TPC, a staged approach:

More information

Measurement of the transverse diffusion coefficient of charge in liquid xenon

Measurement of the transverse diffusion coefficient of charge in liquid xenon Measurement of the transverse diffusion coefficient of charge in liquid xenon W.-T. Chen a, H. Carduner b, J.-P. Cussonneau c, J. Donnard d, S. Duval e, A.-F. Mohamad-Hadi f, J. Lamblin g, O. Lemaire h,

More information

DARK MATTER SEARCH AT BOULBY MINE

DARK MATTER SEARCH AT BOULBY MINE DARK MATTER SEARCH AT BOULBY MINE R. LUSCHER on behalf of the Boulby Dark Matter Collaboration (RAL, Imperial College, Sheffield, UCLA, Texas A&M, Pisa, ITEP, Coimbra, Temple and Occidental) Rutherford

More information

Hands on DarkSide-50: Low Energy Calibration

Hands on DarkSide-50: Low Energy Calibration Hands on DarkSide-50: Low Energy Calibration Kyungwon Kim Seoul National University IBS Center for Underground Physics E-mail: kwkim@hep1.snu.ac.kr University of North Carolina Chapel Hill Triangle Universities

More information

Search for Weakly Interacting Massive Particles with CDMS and XENON

Search for Weakly Interacting Massive Particles with CDMS and XENON Search for Weakly Interacting Massive Particles with CDMS and XENON Elena Aprile 1,2, Laura Baudis 3,4, Blas Cabrera 5,6 1 Physics Department and Columbia Astrophysics Laboratory, Columbia University,

More information

Sensitivity and Backgrounds of the LUX Dark Matter Search

Sensitivity and Backgrounds of the LUX Dark Matter Search Sensitivity and Backgrounds of the LUX Dark Matter Search 1 LUX Goal: Direct Detection of Dark Matter WMAP 5-year data (2008) gives matter densities (Ω) based on best fit to Λ-CDM cosmological model: Ω

More information

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

The XENON Dark Matter Project: Status of the XENON100 Phase. Elena Aprile Columbia University The XENON Dark Matter Project: Status of the XENON100 Phase Elena Aprile Columbia University 8th UCLA Symposium Marina del Rey, Feb 22, 2008 The XENON Dark Matter Phased Program Detect WIMPS through their

More information

Understanding Ionization, Scintillation Light, and the Energy Scale

Understanding Ionization, Scintillation Light, and the Energy Scale Understanding Ionization, Scintillation Light, and the Energy Scale In Noble Element Detectors http://nest.physics.ucdavis.edu/site/ Matthew Szydagis, UC Davis University of Connecticut 12/09/13 1 Why

More information

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

DarkSide-50: performance and results from the first atmospheric argon run DarkSide-50: performance and results from the first atmospheric argon run Yann Guardincerri on behalf of the DarkSide Collaboration August 27th, 2014 1 / 21 DarkSide Direct detection search for WIMP dark

More information

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

Recent results from PandaX- II and status of PandaX-4T Recent results from PandaX- II and status of PandaX-4T Jingkai Xia (Shanghai Jiao Tong University) On behalf of PandaX Collaboration August 2-5, Mini-Workshop@SJTU 2018/8/4 1 Outline Dark Matter direct

More information

The LZ Experiment Tom Shutt SLAC. SURF South Dakota

The LZ Experiment Tom Shutt SLAC. SURF South Dakota The LZ Experiment Tom Shutt SLAC SURF South Dakota 1 LUX - ZEPLIN 31 Institutions, ~200 people 7 ton LXe TPC ( tons LXe total) University of Alabama University at Albany SUNY Berkeley Lab (LBNL), UC Berkeley

More information

Measurement of Scintillation Efficiency for Nuclear Recoils in Liquid Argon

Measurement of Scintillation Efficiency for Nuclear Recoils in Liquid Argon University of Pennsylvania ScholarlyCommons Department of Physics Papers Department of Physics 6-27-212 Measurement of Scintillation Efficiency for Nuclear Recoils in Liquid Argon Dan Gastler Boston University

More information

The XENON100 Dark Matter Experiment at LNGS: Status and Sensitivity

The XENON100 Dark Matter Experiment at LNGS: Status and Sensitivity The XENON100 Dark Matter Experiment at LNGS: Status and Sensitivity Elena Aprile (on behalf of the XENON Collaboration) Columbia University,Physics Department, New York,NY, USA E-mail: age@astro.columbia.edu

More information

Direct Detection of Dark Matter with LUX

Direct Detection of Dark Matter with LUX Direct Detection of Dark Matter with LUX we are a collaboration of 50+ scientists, please see http://lux.brown.edu for more information Peter Sorensen Lawrence Livermore National Laboratory DNP October

More information

Xenon Compton Telescopes at Columbia: the post LXeGRIT phase. E.Aprile. Columbia University

Xenon Compton Telescopes at Columbia: the post LXeGRIT phase. E.Aprile. Columbia University Xenon Compton Telescopes at Columbia: the post LXeGRIT phase E.Aprile Columbia University Seeon 2003 Sensitivity Goals for An Advanced Compton Telescope ~10-7 ph cm -2 s -1 ( 3σ) for narrow lines and ~

More information

Direct dark matter search using liquid noble gases

Direct dark matter search using liquid noble gases Direct dark matter search using liquid noble gases Teresa Marrodán Undagoitia marrodan@physik.uzh.ch Physik Institut Universität Zürich Texas Symposium 2010, Heidelberg, 09.11.2010 Teresa Marrodán Undagoitia

More information

arxiv: v2 [physics.ins-det] 28 Jul 2010

arxiv: v2 [physics.ins-det] 28 Jul 2010 Pulse-Shape Discrimination of CaF 2 (Eu) S. Oguri a,1, Y. Inoue b, M. Minowa a arxiv:1007.4750v2 [physics.ins-det] 28 Jul 2010 a Department of Physics, School of Science, University of Tokyo, 7-3-1, Hongo,

More information

arxiv:physics/ v1 [physics.ins-det] 14 Feb 2005

arxiv:physics/ v1 [physics.ins-det] 14 Feb 2005 arxiv:physics/0502071v1 [physics.ins-det] 14 Feb 2005 Performance of a Large Area Avalanche Photodiode in a Liquid Xenon Ionization and Scintillation Chamber K. Ni a,, E. Aprile a, D. Day a,1, K.L. Giboni

More information

DarkSide new results and prospects

DarkSide new results and prospects DarkSide new results and prospects Stefano Davini - INFN Genova on behalf of the DarkSide collaboration La Thuile, March 20, 2018 The DarkSide WIMP-argon program at LNGS 2011 2012 2013 2014 2015 2016 2017

More information

LARGE UNDERGROUND XENON

LARGE UNDERGROUND XENON LARGE UNDERGROUND XENON Cláudio Silva (LIP Coimbra) On behalf of the LUX Collaboration IDPASC Dark Matter Workshop 17 December 2011 1 THE LUX COLLABORATION Collaboration was formed in 2007 and fully funded

More information

Dark Matter Detection with XENON100 Accomplishments, Challenges and the Future

Dark Matter Detection with XENON100 Accomplishments, Challenges and the Future Dark Matter Detection with XENON0 Accomplishments, Challenges and the Future http://xenon.astro.columbia.edu Kaixuan Ni Columbia University TeV Particle Astrophysics IHEP, Beijing, Sep.4-8, 008 The Challenges

More information

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

Dark Matter Detection and the XENON Experiment. 1 Abstract. 2 Introduction Dark Matter Detection and the XENON Experiment Elena Aprile Physics Department and Columbia Astrophysics Laboratory Columbia University New York, New York 10027 1 Abstract Observations on all fronts strongly

More information

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

XENONNT AND BEYOND. Hardy Simgen. WIN 2015 MPIK Heidelberg. Max-Planck-Institut für Kernphysik Heidelberg XENONNT AND BEYOND Hardy Simgen Max-Planck-Institut für Kernphysik Heidelberg WIN 2015 MPIK Heidelberg THE XENON PROGRAM FOR DIRECT DARK MATTER SEARCH 1 THE PRESENT: XENON1T! LXe TPC under construction

More information

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

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

More information

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

Understanding the response of LXe to electronic and nuclear recoils at low energies Understanding the response of LXe to electronic and nuclear recoils at low energies Christopher W. Geis Johannes-Gutenberg Universität Mainz 2015/01/09 geisch@uni-mainz.de http://xenon.uni-mainz.de 1 /

More information

Doojin Kim University of Wisconsin, WI November 14th, 2017

Doojin Kim University of Wisconsin, WI November 14th, 2017 Doojin Kim, WI November 14th, 2017 Based on DK, J.-C. Park, S. Shin, PRL119, 161801 (2017) G. Giudice, DK, J.-C. Park, S. Shin, 1711. xxxxx Doojin Kim, WI November 14th, 2017 Based on DK, J.-C. Park, S.

More information

The XENON dark matter search. T. Shutt CWRU

The XENON dark matter search. T. Shutt CWRU The XENON dark matter search T. Shutt CWRU The XENON collboration Columbia University Elena Aprile (PI), Edward Baltz,Karl-Ludwig Giboni, Sharmila Kamat, Pawel Majewski,Kaixuan Ni, Bhartendu Singh, and

More information

XENON Dark Matter Experiment (NSF/DOE)

XENON Dark Matter Experiment (NSF/DOE) XENON Dark Matter Experiment (NSF/DOE) Rick Gaitskell Particle Astrophysics Group, Brown University, Department of Physics (Supported by US DOE HEP) see XENON information at http://www.astro.columbia.edu/~lxe/xenon/

More information

Scin/lla/on of liquid neon Photon Detec/on at 27 K

Scin/lla/on of liquid neon Photon Detec/on at 27 K Scin/lla/on of liquid neon Photon Detec/on at 27 K Hugh Lippinco, Fermilab Jin Ping Solar Neutrino Workshop June 9, 2014 1 Why neon? Scin?llates efficiently (of order 20 photons/kev or more) No long lived

More information

Waveform Analysis for DM-Ice17. Zachary Pierpoint University of Wisconsin - Madison October 21, 2013 Yale Weak Interactions Discussions Group

Waveform Analysis for DM-Ice17. Zachary Pierpoint University of Wisconsin - Madison October 21, 2013 Yale Weak Interactions Discussions Group Waveform Analysis for DM-Ice17 Zachary Pierpoint University of Wisconsin - Madison October 21, 213 Yale Weak Interactions Discussions Group DM-Ice17 Energy Spectrum counts / day / kev / kg 1 28 Tl+ 214

More information

LAAPD Performance Measurements in Liquid Xenon

LAAPD Performance Measurements in Liquid Xenon LAAPD Performance Measurements in Liquid Xenon David Day Summer REU 2004 Nevis Laboratories, Columbia University Irvington, NY August 3, 2004 Abstract Performance measurements of a 16mm diameter large

More information

New Physics Results from DarkSide-50. Masayuki Wada Princeton University on behalf of the DarkSide-50 Collaboration Feb

New Physics Results from DarkSide-50. Masayuki Wada Princeton University on behalf of the DarkSide-50 Collaboration Feb New Physics Results from DarkSide5 Masayuki Wada Princeton University on behalf of the DarkSide5 Collaboration Feb. 8 Lake Louise Winter Institute 8 DETECTOR DARKSIDE 5 Radonfree (Rn levels < 5 mbq/m )

More information

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

arxiv: v1 [physics.ins-det] 31 Oct 2015 Alden Fan 1 DPF2015-240 November 4, 2015 Status and Results from DarkSide-50 arxiv:1511.00676v1 [physics.ins-det] 31 Oct 2015 Alden Fan 1 Physics and Astronomy Department University of California, Los Angeles, CA

More information

The XMASS experiment. Y. Kishimoto for the XMASS collaboration March 24 th, 2014 Recontres de Moriond, Cosmology

The XMASS experiment. Y. Kishimoto for the XMASS collaboration March 24 th, 2014 Recontres de Moriond, Cosmology The XMASS experiment Y. Kishimoto for the XMASS collaboration March 24 th, 2014 Recontres de Moriond, Cosmology Contents Introduction to the XMASS Results from XMASS commissioning run Light mass WIMPs

More information

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

LUX: A Large Underground Xenon detector. WIMP Search. Mani Tripathi, INPAC Meeting. Berkeley, May 5, 2007 LUX: A Large Underground Xenon detector WIMP Search Mani Tripathi INPAC Meeting Berkeley, New Collaboration Groups formerly in XENON10: Case Western, Brown, Livermore Natl. Lab (major fraction of the US

More information

PMT Calibration and Neutron Generator Simulation for nerix

PMT Calibration and Neutron Generator Simulation for nerix PMT Calibration and Neutron Generator Simulation for nerix Haley Pawlow Nevis Laboratories, Columbia University, Irvington, NY, 10533, USA (Dated: July 31, 2014) The nuclear and electronic recoils in Xe

More information

Status and Sensitivity Projections for the XENON100 Dark Matter Experiment

Status and Sensitivity Projections for the XENON100 Dark Matter Experiment Status and Sensitivity Projections for the XENON Dark Matter Experiment Elena Aprile Columbia Astrophysics Laboratory, Columbia University, New York, NY 27, USA E-mail: age@astro.columbia.edu Laura Baudis

More information

STUDY ON THE ENERGY RESPONSE OF PLASTIC SCINTILLATION DETECTOR TO MEV NEUTRONS ABSTRACT

STUDY ON THE ENERGY RESPONSE OF PLASTIC SCINTILLATION DETECTOR TO MEV NEUTRONS ABSTRACT STUDY ON THE ENERGY RESPONSE OF PLASTIC SCINTILLATION DETECTOR TO 0.75-14.75 MEV NEUTRONS Jianfu Zhang 1, 2, Xiaoping Ouyang 1, 2, Suizheng Qiu 1, Xichao Ruan 3, Jinlu Ruan 2 1 School of Nuclear Science

More information

SuperCDMS: Recent Results for low-mass WIMPS

SuperCDMS: Recent Results for low-mass WIMPS SuperCDMS: Recent Results for low-mass WIMPS David G. Cerdeño Institute for Theoretical Physics Universidad Autónoma de Madrid for the SuperCDMS Collaboration Hints for low-mass WIMPs in direct detection

More information

THE qualities of liquid xenon (LXe) as an efficient

THE qualities of liquid xenon (LXe) as an efficient 1800 IEEE TRANSACTIONS ON NUCLEAR SCIENCE, VOL. 52, NO. 5, OCTOBER 2005 Fast Timing Measurements of Gamma-Ray Events in Liquid Xenon Karl-Ludwig Giboni, Elena Aprile, Pawel Majewski, Kaixuan Ni, and Masaki

More information

A survey of recent dark matter direct detection results

A survey of recent dark matter direct detection results A survey of recent dark matter direct detection results I where we stand II recent results (CDMS, XENON10, etc) III DAMA results IV a bit about modulation V issues with DAMA results VI what to look for

More information

LXe (part B) Giovanni Signorelli. Istituto Nazionale di Fisica Nucleare, Dipartimento di Fisica and Scuola Normale Superiore, Pisa (Italy)

LXe (part B) Giovanni Signorelli. Istituto Nazionale di Fisica Nucleare, Dipartimento di Fisica and Scuola Normale Superiore, Pisa (Italy) LXe (part B) Giovanni Signorelli Istituto Nazionale di Fisica Nucleare, Dipartimento di Fisica and Scuola Normale Superiore, Pisa (Italy) PSI, February 2003 1 MEG internal meeting 2 MC: Outline shape-qe

More information

DarkSide-20k and the Darkside Program for Dark Matter Searches

DarkSide-20k and the Darkside Program for Dark Matter Searches DarkSide-20k and the Darkside Program for Dark Matter Searches Cristiano Galbiati Princeton University APC Paris Diderot GDR Neutrinos LPSC Grenoble June 6, 2016 DarkSide-20k Institutions [cm 2 ] σ 41

More information

PandaX Dark Matter Search

PandaX Dark Matter Search PandaX Dark Matter Search Xiangdong Ji Shanghai Jiao Tong University University of Maryland On Behalf of the PandaX Collaboration 2017/8/7 1 Outline Introduction to WIMP search and liquid xenon experiments

More information

arxiv: v1 [physics.ins-det] 16 May 2017

arxiv: v1 [physics.ins-det] 16 May 2017 Measurement of the response of a liquid scintillation detector to monoenergetic electrons and neutrons arxiv:175.5532v1 [physics.ins-det] 16 May 217 P. C. Rout a, A. Gandhi b, T. Basak c, R. G. Thomas

More information

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

Background Characterization and Rejection in the LZ Detector. David Malling Brown University IDM 2012 July 25, 2012 Background Characterization and Rejection in the LZ Detector David Malling Brown University IDM 2012 July 25, 2012 LZ Construction 2 Background Sources Ti cryostats 1500 kg

More information

Direct dark matter search using liquid noble gases

Direct dark matter search using liquid noble gases Universität Zürich E-mail: marrodan@physik.uzh.ch Liquid noble gases have proven a great potential as detector medium for dark matter searches. Particles interacting in these media produce ionized and

More information

Direct Detection of! sub-gev Dark Matter

Direct Detection of! sub-gev Dark Matter Direct Detection of! sub-gev Dark Matter Rouven Essig C.N. Yang Institute for Theoretical Physics, Stony Brook Sackler Conference, Harvard, May 18, 2014 An ongoing program Direct Detection of sub-gev Dark

More information

Shedding Light on Dark Matter from Deep Underground with XENON. Kaixuan Ni (Columbia)

Shedding Light on Dark Matter from Deep Underground with XENON. Kaixuan Ni (Columbia) Shedding Light on Dark Matter from Deep Underground with XENON Kaixuan Ni (Columbia) University of Maryland, 11-25-2008 A well-known mystery for astronomers Fritz Zwicky, The Astrophysical Journal, 85

More information

Improving Scintillation Response in Xenon and Implementation in GEANT4

Improving Scintillation Response in Xenon and Implementation in GEANT4 Improving Scintillation Response in Xenon and Implementation in GEANT4 UC Davis and LLNL Faculty Mani Tripathi Bob Svoboda Postdocs and Research Scientists Matthew Szydagis Kareem Kazkaz Undergraduates

More information

SLAC - Advanced Instrumentation Seminars

SLAC - Advanced Instrumentation Seminars Samuele Sangiorgio LLNL Advanced Detector Group SLAC - Advanced Instrumentation Seminars Feb 20, 2013 LLNL-PRES-622432 This work was performed under the auspices of the U.S. Department of Energy by under

More information

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

DarkSide. Bianca Bottino Università di Genova and INFN Sezione di Genova on behalf of the DarkSide collaboration 1 DarkSide Bianca Bottino Università di Genova and INFN Sezione di Genova on behalf of the DarkSide collaboration 1 DARKSIDE MAIN FEATURES Dark Matter direct detection WIMP induced nuclear recoils Double

More information

Dark Matter Search with XENON

Dark Matter Search with XENON Dark Matter Search with XENON Marc Schumann Physik Institut, Universität Zürich Universität Mainz, Seminar, May 2, 2012 www.physik.uzh.ch/groups/groupbaudis/xenon/ 2 Baryonic Matter Dark Matter? Dark Energy????

More information

Monte Carlo Simulation of the Liquid Xenon Detector Response to Low-Energy Neutrons

Monte Carlo Simulation of the Liquid Xenon Detector Response to Low-Energy Neutrons University of Zurich Physics Institute Monte Carlo Simulation of the Liquid Xenon Detector Response to Low-Energy Neutrons July 2, 2014 Bachelor Thesis of Dario Biasini Supervisors: Dr. Alexander Kish

More information