Solid Xenon Detector R&D

Size: px
Start display at page:

Download "Solid Xenon Detector R&D"

Transcription

1 Solid Xenon Detector R&D Jonghee Yoo Fermilab 24 Feb 2012 UCLA Dark Matter Symposium

2 Solid Xenon Scintillation ~100 ev/γ Phonons ~100 mev/ph Ionization ~10 ev/el Why Xenon? No long-lived Xe radio isotope (no intrinsic background) High yield of scintillation light Scintillation wavelength : 175nm (optically transparent) Relatively high melting point : T m = 161K Simple crystal structure : fcc (same as Ge) Easy purification (distillation, etc) Self shielding : Z=54 Why Solid? For solar axion search, being a crystal is crucial (Bragg scattering) Even more scintillation light (61 γ/ kev) than LXe (42 γ/ kev) is reported Drifting electrons faster in the crystal Superb low noise superconducting sensors are running at low temperature (mk ~ K) Phonon read out : largest number of quanta (~10,000 phonons / kev) - In principle best energy resolution can be achieved in phonon channel - Luke-phonon readout will provide ionization energy and position information No further background contamination through circulation loop (no convection mix) Optimal detector design for low background experiment - Possible container-free design - No outgassing issue 2

3 Science (1) Solar axion search: crystal - scin5lla5on / (ioniza5on) (2) Dark ma<er search : readout two(or three) signals - scin5lla5on / ioniza5on / (phonon) (3) Neutrinoless double beta decay (0v2b) : 136 Xe enriched - scin5lla5on / ioniza5on / phonon (4) pp- Solar neutrino measurement : 136 Xe depleted (5) Supernova detec5on (6) Neutrino coherent sca<ering (7) Medical usage (MRI/NMR) : hyperpolarized 131 Xe Time-energy plot of the expected event rate for finding photon-converted solar axions with a CDMS germanium crystal detector Full of science topics Strong mo5va5on for R&D But this does not necessarily mean we can ini5ate science experiment. We need proven technology in order to achieve immediate science goal Low background crystal detector 3

4 Solid Xenon Property? ΔT = 4K Compact More electrons / kev? or less?? Faster electron dri\? Slow hole(?) dri\ Single direc5onal Luke- phonon? Not many proper5es are known nor measured in solid phase 4

5 Xenon Crystal? Kramer 1976 : Epitaxial growth of xenon crystal on Carbon- graphite film 5

6 Previous Efforts Fukui Univ. (Miyajima 1999) TAMU (J.White 2004) Measured ioniza.on signal from Solid Argon 6

7 Solid Xenon R&D Phase-1: Frozen Xenon Frozen xenon Frost xenon layers 7

8 Solid Xenon R&D Phase-1 (2010) Liquid Xenon (~200g) Fermilab Center for Par5cle Astrophysics (FCPA) New Ini5a5ve R&D Project Phase- 1 Goal: demonstrated ~1kg size of op.cally transparent solid phase of xenon Collabora5on with T. Saab, D. Balakishiyeva (U.Florida) R.Mahapatra (TAMU) Solid Xenon (~850g) Established Recipe Top T : 160 ± 0.5K BoJom T : 145 ± 0.5K Xenon gas pressure : 1.0 ± 0.1 atm Pa.ence : 3cm growth / 10 hours Phase- 2 Fermilab Par5cle Physics Division (PPD) review panel approved Phase- 2 (April 2010) (1) Automate process (2) Signal readout (scin5lla5on and ioniza5on) Budgetary approval (June 2010) 8

9 Solid Xenon R&D Phase-2 Electric feedthroughs New design of inner glass (xenon) chamber and electric/gas feed throughs Address safety concerns of using glass chamber system Engineering support from Fermilab PPD 4 D glass chamber 9 D glass chamber PMT or TPC Cryobath phase separator Glass chamber pressure simula.on (H.Cease) Max. allowed pressure < 17.5 psig 9

10 New Plumbing 10

11 Automatic control system Touch screen control unit Cryobath level, temperature, pressure and flow rates control Monitoring (graph) tools, remote control (D.Markley) Programmable Logic Controller 11

12 Gas purification/analysis system Noble Gas Purifier (U.Florida) RGA Universal Gas Analyzer 12

13 Photomultiplier Hamamatsu R9869 Spectral Response 169 ~ 650 nm Operating ambient temperature : 163K ~ 323K Quantum Efficiency at 175nm : 20% Gain : 10 6 Anode pulse rise time : 2.3 nsec Weight : 95g Pressure resistance : 5 atm data/ntp/ _pmtv0860ledmv09745_t160k020mhz.root Entry " / ndf / 27 a ± 62.9 µ e+05 ± 4.863e # e+05 ± 3.759e+03 a ± 3.62 µ e+06 ± 1.302e+05 # e+06 ± 1.174e Single p.e. calibration in cold temperature G = 4.2e6 (@860V, 160K) or 33.6pVs at s.p.e Gain 6!10 V.Anjur (IMSA) 13

14 TPC TPC performance test done in gas Argon Δt=at0- ct0 anode t0 (at0) cathode t0 (ct0) 7cm 2cm Anode (+500V) Anode Grid Field shape rings Ground Grid Cathode(- 215V) Photocathod: Gold- coated on Al plate Au Custom Al, PLATYPUS FC MΩ Resistance (W.Jaskierny and E.Skup) TPC design is from LArTPC project at Fermilab 14

15 Solid Xenon Phase-2 Test Stand Safety backup chambers Xenon gas storages and Calibra5on gas storage Gas control DAQ Main chamber System setup completed in 2011 Sep Passed Fermilab safety review Electric safety review 2011 Nov Mechanical safety review 2011 Nov Cryogenic safety review 2012 Dec Opera.onal Readiness Clearness 2012 Nov Approval for system opera5on 2011 Dec System test 2012 Jan ~ Feb 15

16 System Test gas liquid solid 16

17 System test: Scintillation Light (last week) PMT pulses (sequen.al segment readout) Solid Xenon (cosmic ray test) Ini.al test of scin.lla.on light readout Research grade xenon (<ppm for H 2 O, O 2, N 2, ) Radioac.ve source test to be done Amer full system test (coming soon) (1) Measure scin.lla.on efficiencies (2) Measure electron drim (3) Compare proper.es in liquid vs. solid (4) Measure other interes.ng detector parameters 17

18 Summary Solid Xenon Phase- 2 instrument is ready for the opera.on System test is underway - Seeing scin.lla.on light from solid xenon - Detailed system test to be done More to come! 18

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

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

CANDLES Experiment Current Status and Future Plan. X. Li for the CANDLES Collaboration

CANDLES Experiment Current Status and Future Plan. X. Li for the CANDLES Collaboration CANDLES Experiment Current Status and Future Plan X. Li for the CANDLES Collaboration 1 Neutrinoless Double Beta Decay (0νββ) 2νββ decay 0νββ decay (A, Z) => (A, Z+2) + 2e - process beyond Standard Model

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

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

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

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

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 next generation dark matter hunter: XENON1T status and perspective

The next generation dark matter hunter: XENON1T status and perspective The next generation dark matter hunter: XENON1T status and perspective A. Rizzo a on behalf of the XENON Collaboration Department of Astrophysics, Columbia University in the City of New York, USA Abstract.

More information

Rn assay and distillation purification

Rn assay and distillation purification Rn assay and distillation purification of Lq. Xe for Kr Introduction Distillation purification of Xe for Kr Kr assay with API-MS detector Rn assay with XMASS prototype detector Summary Yasuo Takeuchi (Kamioka

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

Low Energy Particles in Noble Liquids

Low Energy Particles in Noble Liquids Low Energy Particles in Noble Liquids Antonio J. Melgarejo Fernandez Columbia University Invisibles School, July 14th 2013, Durham Explaining the title I Noble gases are a group of elements found at the

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

Distillation purification and radon assay of liquid xenon

Distillation purification and radon assay of liquid xenon Distillation purification and radon assay of liquid xenon Yasuo Takeuchi Kamioka Observatory, ICRR, Univ. of Tokyo, Kamioka-cho, Hida-shi, Gifu 56-125, Japan Abstract. We succeeded to reduce the Kr contamination

More information

DARWIN: dark matter WIMP search with noble liquids

DARWIN: dark matter WIMP search with noble liquids DARWIN: dark matter WIMP search with noble liquids Physik Institut, University of Zurich E-mail: laura.baudis@physik.uzh.ch DARWIN (DARk matter WImp search with Noble liquids) is an R&D and design study

More information

The Search for Dark Matter, and Xenon1TP

The Search for Dark Matter, and Xenon1TP The Search for Dark Matter, and Xenon1TP by Jamin Rager Hillsdale College Assistant Prof. Rafael Lang Purdue University Dept. of Physics Galaxy NGC 3198 2 Galaxy NGC 3198 Rotation Curves http://bustard.phys.nd.edu/phys171/lectures/dm.html

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

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

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

Direct detection: results from liquid noble-gas experiments

Direct detection: results from liquid noble-gas experiments Direct detection: results from liquid noble-gas experiments Teresa Marrodán Undagoitia marrodan@mpi-hd.mpg.de DM@LHC Heidelberg, April 5th, 2018 Teresa Marrodán Undagoitia (MPIK) Liquid noble gases Heidelberg,

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

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

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

Technical Specifications and Requirements on Direct detection for Dark Matter Searches

Technical Specifications and Requirements on Direct detection for Dark Matter Searches Technical Specifications and Requirements on Direct detection for Dark Matter Searches Jin Li THU/IHEP Symposium of the Sino-German GDT Cooperation 04/08/2013 Tübingen Outline Introduction Direct detection

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

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

LUX-ZEPLIN (LZ) Status. Attila Dobi Lawrence Berkeley National Laboratory June 10, 2015 WIN Heidelberg LUX-ZEPLIN (LZ) Status Attila Dobi Lawrence Berkeley National Laboratory June 10, 2015 WIN-2015. Heidelberg 1 LZ = LUX + ZEPLIN 29 institutions currently About 160 people Continuing to expand internationally

More information

NEXT ELECTROLUMINESCENCE READOUT

NEXT ELECTROLUMINESCENCE READOUT IFIC - INSTITUTO DE FISICA CORPUSCULAR NEXT ELECTROLUMINESCENCE READOUT Igor Liubarsky Instituto de Fisica Corpuscular CONTENTS Why do it Neutrinoless Double Beta Decay Neutrino Experiments with Xe TPC

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

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

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

PANDA-?? A New Detector for Dark Matter Search

PANDA-?? A New Detector for Dark Matter Search PANDA-?? A New Detector for Dark Matter Search Karl Giboni, Xiangdong Ji, Andy Tan, Li Zhao Shanghai Jiao Tong University Seminar at KEK, Tsukuba Japan 24 November, 2011 PANDA-X Dark Matter Search Jin

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

Status of the AMoRE experiment searching for neutrinoless double beta decay of 100 Mo

Status of the AMoRE experiment searching for neutrinoless double beta decay of 100 Mo Status of the AMoRE experiment searching for neutrinoless double beta decay of 100 Mo Hyon-Suk Jo Center for Underground Physics Institute for Basic Science INPC 2016 - Adelaide Convention Centre, Australia

More information

Direct Dark Matter and Axion Detection with CUORE

Direct Dark Matter and Axion Detection with CUORE Direct Dark Matter and Axion Detection with CUORE Marco Vignati University of Rome La Sapienza & INFN Rome on behalf of the CUORE collaboration Panic 11, July 5, MIT 988 TeO crystals Ton scale bolometric

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

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

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

Dark Matter Searches. Marijke Haffke University of Zürich

Dark Matter Searches. Marijke Haffke University of Zürich University of Zürich Structure Ι. Introduction - Dark Matter - WIMPs Ι Ι. ΙΙΙ. ΙV. V. Detection - Philosophy & Methods - Direct Detection Detectors - Scintillators - Bolometer - Liquid Noble Gas Detectors

More information

AIDA-2020 Advanced European Infrastructures for Detectors at Accelerators. Journal Publication. Photon detection system for ProtoDUNE dual phase

AIDA-2020 Advanced European Infrastructures for Detectors at Accelerators. Journal Publication. Photon detection system for ProtoDUNE dual phase AIDA-2020-PUB-2017-009 AIDA-2020 Advanced European Infrastructures for Detectors at Accelerators Journal Publication Photon detection system for ProtoDUNE dual phase Cuesta, C. (on behalf of DUNE collaboration)

More information

Charge readout and double phase

Charge readout and double phase Charge readout and double phase Vyacheslav Galymov IPN Lyon 1 st annual meeting AIDA-2020 Liquid argon double-phase TPC Concept of double-phase LAr TPC (Not to scale) Anode 0V 2 mm Collection field 5kV/cm

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

Search for double electron capture on 124 Xe with the XMASS-I detector

Search for double electron capture on 124 Xe with the XMASS-I detector Search for double electron capture on 124 Xe with the XMASS-I detector KATSUKI HIRAIDE (ICRR, THE UNIVERSITY OF TOKYO) SEPTEMBER 7 TH, 2015 TAUP2015 1 124 Xe 2n double electron capture Natural xenon contains

More information

PHY 599: How it is usually done

PHY 599: How it is usually done PHY 599: How it is usually done This is Particle Physics and Astro-Cosmology Seminar We meet every Wednesday from 3:30 pm to 4:30 pm in Room 506 Nielsen. This seminar series is mainly intended for graduate

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

can be read by PMTs w/o wave length shifter

can be read by PMTs w/o wave length shifter Liquid-Xe Solar pp 7 Be neutrino detector Y.Suzuki Kamioka Obs. ICRR, U.Tokyo @LowNu 2000-06-15 Detector 1) Liquid Xenon with 10 ton fiducial volume 2) Scintillation detector: 42,000 photons/mev similar

More information

Design, Construction, Operation, and Simulation of a Radioactivity Assay Chamber

Design, Construction, Operation, and Simulation of a Radioactivity Assay Chamber Design, Construction, Operation, and Simulation of a Radioactivity Assay Chamber Wesley Ketchum and Abe Reddy EWI Group, UW REU 2006 Outline Neutrino Physics Background Double Beta Decay and the Majorana

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

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

XENON1T: opening a new era in the search for Dark Matter. Elena Aprile, Columbia University on behalf of the Collaboration, UCLA, February 17, 2016

XENON1T: opening a new era in the search for Dark Matter. Elena Aprile, Columbia University on behalf of the Collaboration, UCLA, February 17, 2016 XENON1T: opening a new era in the search for Dark Matter Elena Aprile, Columbia University on behalf of the Collaboration, UCLA, February 17, 2016 The XENON Dark Matter Program 2005-2007 2007-2015 2012-2022

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

Cherenkov Detector. Cosmic Rays Cherenkov Detector. Lodovico Lappetito. CherenkovDetector_ENG - 28/04/2016 Pag. 1

Cherenkov Detector. Cosmic Rays Cherenkov Detector. Lodovico Lappetito. CherenkovDetector_ENG - 28/04/2016 Pag. 1 Cherenkov Detector Cosmic Rays Cherenkov Detector Lodovico Lappetito CherenkovDetector_ENG - 28/04/2016 Pag. 1 Table of Contents Introduction on Cherenkov Effect... 4 Super - Kamiokande... 6 Construction

More information

the DarkSide project Andrea Pocar University of Massachusetts, Amherst

the DarkSide project Andrea Pocar University of Massachusetts, Amherst the DarkSide project the DarkSide project Andrea Pocar University of Massachusetts, Amherst Dark Matter Workshop, Aspen Physics Institute, 7-11 February, 2011 Outline the DarkSide program and collaboration

More information

The NEXT-100 experiment for Neutrino-less Double Beta decay: Main features, Results from Prototypes and Radiopurity issues.

The NEXT-100 experiment for Neutrino-less Double Beta decay: Main features, Results from Prototypes and Radiopurity issues. The NEXT-100 experiment for Neutrino-less Double Beta decay: Main features, Results from Prototypes and Radiopurity issues. 1 Universidad Autónoma de Madrid Instituto de Física Teórica UAM/CSIC 28049 Cantoblanco

More information

Particle Physics: Neutrinos part II

Particle Physics: Neutrinos part II Particle Physics: Neutrinos part II José I. Crespo-Anadón Week 9: April 1, 2017 Columbia University Science Honors Program Course Policies Attendance Up to four absences Send email notifications of all

More information

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

Prospects for 0-ν ββ Search with a High-Pressure Xenon Gas TPC. What s NEXT? Prospects for 0-ν ββ Search with a High-Pressure Xenon Gas TPC What s NEXT? David Nygren LBNL INT Nu Mass February 2010 1 INT Nu Mass February 2010 2 Xenon for 0 ν ββ Only inert gas with a 0 ν ββ candidate

More information

Neutrinoless Double Beta Decay. Phys 135c Spring 2007 Michael Mendenhall

Neutrinoless Double Beta Decay. Phys 135c Spring 2007 Michael Mendenhall Neutrinoless Double Beta Decay Phys 135c Spring 2007 Michael Mendenhall Theory Overview neutrino Lagrangian ν c iγ 2 γ 0 ν T L ν = M D [ν R ν L + ν c LνR] c }{{} + M L [ν c Lν L + ν L νl] c + M R [ν c

More information

David Caratelli & Angela Fava1

David Caratelli & Angela Fava1 LArCADe: lowering thresholds in LArTPC detectors Magnifcent CEvNS UChicago November 3rd, 2018 ν David Caratelli & Angela Fava1 LArCADe: Liquid Argon Charge Amplifcation Devices LDRD project @ Fermilab

More information

Down-to-earth searches for cosmological dark matter

Down-to-earth searches for cosmological dark matter Down-to-earth searches for cosmological dark matter Carter Hall, University of Maryland October 19, 2016 Astrophysical evidence for dark matter Galaxy cluster collisions Rotation curves Ω 380,000 years

More information

Particle Energy Loss in Matter

Particle Energy Loss in Matter Particle Energy Loss in Matter Charged particles loose energy when passing through material via atomic excitation and ionization These are protons, pions, muons, The energy loss can be described for moderately

More information

Measuring Neutrino Proper0es with Liquid Argon TPCs

Measuring Neutrino Proper0es with Liquid Argon TPCs Measuring Neutrino Proper0es with Liquid Argon TPCs Oxford Seminar 13 October 2015 MaE Bass INTRODUCTION 2 Outline Open ques0ons in Neutrino Physics Liquid Argon Time Projec=on Chambers LAr TPC Experiments

More information

Prospects for WIMP Dark Matter Direct Searches with XENON1T and DARWIN

Prospects for WIMP Dark Matter Direct Searches with XENON1T and DARWIN Via Lactea 2 (2008) Prospects for WIMP Dark Matter Direct Searches with XENON1T and DARWIN NASA/WMAP 8th Patras Workshop on Axions, WIMPs, and WISPs Chicago, 21-July-2012 http://xenon.physik.uni-mainz.de

More information

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

next The NEXT double beta decay experiment Andrew Laing, IFIC (CSIC & UVEG) on behalf of the NEXT collaboration. TAUP2015, Torino, 8/09/2015 a next The NEXT double beta decay experiment Andrew Laing, IFIC (CSIC & UVEG) on behalf of the NEXT collaboration. TAUP2015, Torino, 8/09/2015 NEXT: A light TPC ENERGY PLANE (PMTs) TPB coated surfaces

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

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

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

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

The XENON1T Experiment

The XENON1T Experiment The XENON1T Experiment Ranny Budnik Columbia University On behalf of the XENON1T collaboration 1 Status in WIMP DM Sensitivities (2012) Spin-independent Spin-dependent, n-coupling preliminary Spin-dependent,

More information

EXO experiment. Jesse Wodin EXO group Sept 13, DOE Site Visit: Sept 13-14,

EXO experiment. Jesse Wodin EXO group Sept 13, DOE Site Visit: Sept 13-14, EXO experiment Jesse Wodin EXO group Sept 13, 2010 DOE Site Visit: Sept 13-14, 2010 1 EXO program A phased program aimed at building an enriched xenon double beta decay experiment with a one or more tonne

More information

- JRA2 ADVANCED TECHNIQUES FOR RARE EVENT DETECTION Tentative structure

- JRA2 ADVANCED TECHNIQUES FOR RARE EVENT DETECTION Tentative structure Paris, 26/9/2006 ILIAS-next - JRA2 ADVANCED TECHNIQUES FOR RARE EVENT DETECTION Tentative structure Andrea Giuliani Drafting group: L.Baudis, A. Giuliani, J. Jochum, A. Juillard, H. Kraus, Ch. Marquet,

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

The ICARUS Project FRONTIERS IN CONTEMPORARY PHYSICS II. Vanderbilt University, March 5-10, Sergio Navas (ETH Zürich) " Atmospheric neutrinos

The ICARUS Project FRONTIERS IN CONTEMPORARY PHYSICS II. Vanderbilt University, March 5-10, Sergio Navas (ETH Zürich)  Atmospheric neutrinos The ICARUS Project FRONTIERS IN CONTEMPORARY PHYSICS II Vanderbilt University, March 5-10, 2001 Sergio Navas (ETH Zürich) Detection Principle The T600 Module Physics Programme: " Atmospheric neutrinos

More information

The GERmanium Detector Array

The GERmanium Detector Array The GERmanium Detector Array n n ν=v p e - e - p Outline: Exp. issues of 0νββ-decay of 76 Ge Concept of GERDA Status of the experiment Summary and conclusions Kevin Kröninger (Max-Planck-Institut für Physik,

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

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

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

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

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

Searching for neutrino- less double beta decay with EXO- 200 and nexo

Searching for neutrino- less double beta decay with EXO- 200 and nexo Searching for neutrino- less double beta decay with EXO- 200 and nexo Andrea Pocar University of Massachusetts, Amherst on behalf of the EXO-200 and nexo collaborations The EXO- 200 Collaboration 2 The

More information

Chapter 12. Dark Matter

Chapter 12. Dark Matter Karl-Heinz Kampert Univ. Wuppertal 128 Chapter 12 Dark Matter Karl-Heinz Kampert Univ. Wuppertal Baryonic Dark Matter Brightness & Rotation Curve of NGC3198 Brightness Rotation Curve measured expected

More information

R&D on Astroparticles Detectors. (Activity on CSN )

R&D on Astroparticles Detectors. (Activity on CSN ) R&D on Astroparticles Detectors (Activity on CSN5 2000-2003) Introduction Results obtained with the R&D activity (2000-2003) with some drift chambers prototypes are reported. With different photocathode

More information

Particle Energy Loss in Matter

Particle Energy Loss in Matter Particle Energy Loss in Matter Charged particles, except electrons, loose energy when passing through material via atomic excitation and ionization These are protons, pions, muons, The energy loss can

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

Par$cle and Neutrino Physics. Liang Yang University of Illinois at Urbana- Champaign Physics 403 April 15, 2014

Par$cle and Neutrino Physics. Liang Yang University of Illinois at Urbana- Champaign Physics 403 April 15, 2014 Par$cle and Neutrino Physics Liang Yang University of Illinois at Urbana- Champaign Physics 403 April 15, 2014 1 SNOWMASS on the Mississippi Community study 2013 for the high energy community 10 year plan

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

08 - Miscellaneous and historical detectors

08 - Miscellaneous and historical detectors 08 - Miscellaneous and historical detectors Jaroslav Adam Czech Technical University in Prague Version 2 Jaroslav Adam (CTU, Prague) DPD_08, Miscellaneous and historical detectors Version 2 1 / 25 Streamer

More information

Measurements of Liquid Scintillator Light Yield for Future Neutrino Experiments

Measurements of Liquid Scintillator Light Yield for Future Neutrino Experiments Measurements of Liquid Scintillator Light Yield for Future Neutrino Experiments Athena Ierokomos University of California, Berkeley 2013 University of California, Los Angeles REU Program Abstract Neutrinoless

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

Two-phase and gaseous cryogenic avalanche detectors based on GEMs

Two-phase and gaseous cryogenic avalanche detectors based on GEMs Two-phase and gaseous cryogenic avalanche detectors based on GEMs Budker Institute of Nuclear Physics, Novosibirsk A. Bondar, A. Buzulutskov, A. Grebenuk, D. Pavlyuchenko, R. Snopkov, Y. Tikhonov Outline

More information

PoS(TIPP2014)033. Upgrade of MEG Liquid Xenon Calorimeter. Ryu SAWADA. ICEPP, the University of Tokyo

PoS(TIPP2014)033. Upgrade of MEG Liquid Xenon Calorimeter. Ryu SAWADA. ICEPP, the University of Tokyo ICEPP, the University of Tokyo E-mail: sawada@icepp.s.u-tokyo.ac.jp The MEG experiment yielded the most stringent upper limit on the branching ratio of the flavorviolating muon decay µ + e + γ. A major

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

LUX: The next stage(s) Multi-tonne LXe TPC s (DM08, Marina del Rey, 21 Feb 08)

LUX: The next stage(s) Multi-tonne LXe TPC s (DM08, Marina del Rey, 21 Feb 08) LUX: The next stage(s) Multi-tonne LXe TPC s (DM08, Marina del Rey, 21 Feb 08) Rick Gaitskell Particle Astrophysics Group, Brown University, Department of Physics (Supported by US DOE HEP) see information

More information

Radioactivity. Lecture 6 Detectors and Instrumentation

Radioactivity. Lecture 6 Detectors and Instrumentation Radioactivity Lecture 6 Detectors and Instrumentation The human organs Neither humans nor animals have an organ for detecting radiation from radioactive decay! We can not hear it, smell it, feel it or

More information

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

THE NEXT EXPERIMENT FOR NEUTRINOLESS DOUBLE BETA DECAY SEARCHES ANDER SIMÓN ESTÉVEZ ON BEHALF OF THE NEXT COLLABORATION THE NEXT EXPERIMENT FOR NEUTRINOLESS DOUBLE BETA DECAY SEARCHES ANDER SIMÓN ESTÉVEZ ON BEHALF OF THE NEXT COLLABORATION 2 OUTLOOK NEXT: Neutrino Experiment with a Xenon TPC R&D Phase NEW Detector design

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

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

Recent results from the UK Dark Matter Search at Boulby Mine.

Recent results from the UK Dark Matter Search at Boulby Mine. Recent results from the UK Dark Matter Search at Boulby Mine. Nigel Smith Rutherford Appleton Laboratory on behalf of the UK Dark Matter Collaboration (Imperial College, Sheffield, RAL) NaI scintillation

More information

Cleaning Electronegative Contamination from Gaseous Xenon Through Cryogenic Pumping

Cleaning Electronegative Contamination from Gaseous Xenon Through Cryogenic Pumping Cleaning Electronegative Contamination from Gaseous Xenon Through Cryogenic Pumping Ashton Rutkowski, Columbia University, REU Program, August 7, 2015 Dark Matter Percentage of Observable Universe Baryonic

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

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

Recent results and status of the XENON program

Recent results and status of the XENON program on behalf of the XENON Collaboration Subatech, Ecole des Mines de Nantes, CNRS/In2p3, Université de Nantes, Nantes, France E-mail: julien.masbou@subatech.in2p3.fr The XENON program aims at the direct detection

More information