Cristina Cozzini (Oxford), IDM 2004, Edinburgh CRESST-II background discrimination: detection of 180 W natural decay in a pure alpha spectrum Paper submitted.

Slides:



Advertisements
Similar presentations
EDELWEISS-I last results EDELWEISS-II prospects for dark matter direct detection CEA-Saclay DAPNIA and DRECAM CRTBT Grenoble CSNSM Orsay IAP Paris IPN.
Advertisements

Henrique Araújo Imperial College London on behalf of ZEPLIN-III Collaboration: Edinburgh University (UK), Imperial College London (UK), ITEP-Moscow (Russia),
LNGS (GERmanium Detector Assembly Stefan Schönert MPIK Heidelberg NOW 2004, Sept. 12, 2004.
GERDA: GERmanium Detector Array
Possible merits of high pressure Xe gas for dark matter detection C J Martoff (Temple) & P F Smith (RAL, Temple) most dark matter experiments use cryogenic.
Solotvina Underground Laboratory
Modane, 12/01/2005 Vitaly Kudryavtsev - JRA1 meeting 1 Background simulations: testing Monte Carlo codes V. A. Kudryavtsev Department of Physics and Astronomy.
Present and Future Cryogenic Dark Matter Search in Europe Wolfgang Rau, Technische Universität München CRESSTCRESST EURECA ryogenic are vent earch with.
Present and future activities of the Garching group (E15)
From CUORICINO to CUORE: To probe the inverted hierarchy region On behalf of the CUORE collaboration DUSL Meeting, Washington DC November 2,-4, 2007 Frank.
Radioactivity Polonium and radium X-Rays
The COBRA Double Beta Decay Search Experiment
COBRA Double Beta Decay Experiment D.Y. Stewart, Dr. Y.A. Ramachers, Prof. P.F.Harrison Experimental Particle Physics Group University of Warwick What.
21. October 2004 IDEA DBD Meeting, Heidelberg 150 Nd activities at TUM V. Lazarev 1, E. Nolte 1, L. Oberauer 1, F. Pröbst 2 1 -Technische Universität München,
UKDMC Dark Matter Search with inorganic scintillators Vitaly A. Kudryavtsev University of Sheffield IDM2000 York, UK September 19, 2000.
T. Frank for the CRESST collaboration Laboratori Nazionali del Gran Sasso C. Bucci Max-Planck-Institut für Physik M. Altmann, M. Bruckmayer, C. Cozzini,
CRESST Cryogenic Rare Event Search with Superconducting Thermometers Max-Planck-Institut für Physik University of Oxford Technische Universität München.
Status of COBRA 6 th SNOLAB Workshop, Picture courtesy
A screening facility for next generation low-background experiments Tom Shutt Laura Cadonati Princeton University.
Status of the BOREXINO experiment Hardy Simgen Max-Planck-Institut für Kernphysik / Heidelberg for the BOREXINO collaboration.
Direct Dark Matter Searches
Cryogenic particle detection at the Canfranc Underground Laboratory First International Workshop for the Design of the ANDES Underground Laboratory Centro.
139 Ba decay: precise half-life measurement and gamma-spectroscopy at BARC: an offshoot of ENSDF evaluation work. P.K.Joshi Homi Bhabha Centre for Science.
ICP 9/28/12 Half-life. Warmup Write a balanced nuclear equation for the alpha decay of Uranium-238.
Ultra-low background HPGe detector at ChyeongPyung Underground Laboratory TaeYeon Kim and KIMS(Korea Invisible Mass Search) Collaboration. * Contents *
Present and future detectors for Geo-neutrinos: Borexino and LENA Applied Antineutrino Physics Workshop APC, Paris, Dec L. Oberauer, TU München.
Nuclear Chemistry The Atom The atom consists of two parts: 1. The nucleus which contains: 2. Orbiting electrons. protons neutrons Multiple nuclei is.
HEP-Aachen/16-24 July 2003 L.Chabert IPNL Latest results ot the EDELWEISS experiment : L.Chabert Institut de Physique Nucléaire de Lyon ● CEA-Saclay DAPNIA/DRECAM.
The European Future of Dark Matter Searches with Cryogenic Detectors H Kraus University of Oxford EURECA.
1 IDM2004 Edinburgh, 9 september 2004 Helenia Menghetti Bologna University and INFN Study of the muon-induced neutron background with the LVD detector.
Section 19.1 Radioactivity 1.To learn the types of radioactive decay 2.To learn to write nuclear equations for radioactive decay 3.To learn how one element.
Stellenbosch University
M. Wójcik for the GERDA Collaboration Institute of Physics, Jagellonian University Epiphany 2006, Kraków, Poland, 6-7 January 2006.
Min Kyu Lee ( 이민규 ) Kyoung Beom Lee ( 이경범 ) Yong-Hamb Kim ( 김용함 ) Low Temperature Detectors 2006 Workshop on the Underground Experiment at Yangyang TEXONO-KIMS.
Nuclear Chemistry. The Atom The atom consists of two parts: 1. The nucleus which contains: 2. Orbiting electrons. protons neutrons.
M. Wójcik Instytut Fizyki, Uniwersytet Jagielloński Instytut Fizyki Doświadczalnej, Uniwersytet Warszawski Warszawa, 10 Marca 2006.
The GERDA experiment L. Pandola INFN, Gran Sasso National Laboratory for the GERDA Collaboration WIN2009, Perugia, September 17 th 2009.
Position sensitive CZT detectors for the COBRA neutrinoless double beta decay project Brian Fulton University of York Neutrinoless double beta decay The.
Dark Matter Search with Direction Sensitive Scintillators The10th ICEPP Symposium February 16, 2004, Hakuba H. Sekiya University of Tokyo.
WIMP search Result from KIMS experiments Kim Seung Cheon (DMRC,SNU)
ZEPLIN I: First limits on nuclear recoil events Vitaly A. Kudryavtsev Department of Physics and Astronomy University of Sheffield, UK For the UK Dark Matter.
Yong-Hamb Kim Low Temperature Detectors for Rare Event Search 2 nd Korea-China Joint Seminar on Dark Matter Search.
Activities on double beta decay search experiments in Korea 1.Yangyang Underground laboratory 2.Double beta decay search with HPGe & CsI(Tl) 3.Metal Loaded.
Stefano Torre University College London for NEMO3 and SuperNEMO collaborations Half day IoP Meeting 12 Oct 2011 Outline 0νββ and 2νββ Observation technique.
A screening facility for next generation low-background experiments Tom Shutt Case Western Reserve University.
The COBRA Experiment Jeanne Wilson University of Sussex, UK On behalf of the COBRA Collaboration TAUP 2007, Sendai, Japan.
UNIT 7 NUCLEAR REACTIONS 7.3 Calculating Half Life? May 17, 2011 DO NOW: = /4.5 = If we start with 4.5 grams of Radon-222 and over a period.
GERDA – a Search for Neutrinoless Double Beta Decay MPI für Physik, München Neutrinoless double beta decay and the GERDA experimentThe detector array and.
PMN07 Blaubeuren Segmented germanium detectors in 0νββ-decay experiments Kevin Kröninger (Max-Planck-Institut für Physik, München)
Phase I: Use available 76 Ge diodes from Heidelberg- Moscow and IGEX experiments (~18 kg). Scrutinize with high siginificance current evidence. Phase II:
1 Double Beta Decay of 150 Nd in the NEMO 3 Experiment Nasim Fatemi-Ghomi (On behalf of the NEMO 3 collaboration) The University of Manchester IOP HEPP.
MPI für Physik, Fachbeirat, Béla Majorovits The GERDA experiment Béla Majorovits.
1 CRESST Cryogenic Rare Event Search with Superconducting Thermometers Jens Schmaler for the CRESST group at MPI MPI Project Review December 14, 2009.
Ch 19 Nuclear Chemistry.  Know how nuclear equations are balanced: The same sums of both mass and atomic numbers appear on both sides of the equation.
Scintillating Bolometers – Rejection of background due to standard two-neutrino double beta decay D.M. Chernyak 1,2, F.A. Danevich 2, A. Giuliani 1, M.
18-20 May 2015, Underground Science Conference, SDSM&T 1John Harton, Colorado State University Recent Results from the DRIFT Directional DM Experiment.
CRESST Cryogenic Rare Event Search with Superconducting Thermometers Max-Planck-Institut für Physik University of Oxford Technische Universität München.
5/13/11 FCPA Mini-RetreatDarkSide - S.Pordes1 DarkSide 10 kg Prototype at Princeton Distillation Column for Depleted Argon at Fermilab DarkSide 50 at Gran.
1 st : Mass Spectrometry on Heavy Molecules with Cryogenic Detectors - status Project Review 2004 PROTEOM 2 nd : Measurement of the Quenching Factors in.
WIMPs Direct Search with Dual Light-emitting Crystals Xilei Sun IHEP International Symposium on Neutrino Physics and Beyond
Leo Stodolsky 80th anniversary
The CRESST Dark Matter Search Status Report
Fast neutron flux measurement in CJPL
Pulse-shape discrimination with Cs2HfCl6 crystal
Prompt Gamma Activation Analysis on 76Ge
CRESST Cryogenic Rare Event Search with Superconducting Thermometers
Irina Bavykina, MPI f. Physik
Progress with cryogenic dark matter searches
Direct Dark Matter Searches
BACKGROUND STUDY IN CRESST
Presentation transcript:

Cristina Cozzini (Oxford), IDM 2004, Edinburgh CRESST-II background discrimination: detection of 180 W natural decay in a pure alpha spectrum Paper submitted to Physical Review C (also available on nucl-ex/ )

Cristina Cozzini (Oxford), IDM 2004, Edinburgh C. Cozzini 1, G. Angloher 2, C. Bucci 3, F. von Feilitzsch 4, D. Hauff 2, S. Henry 1, Th. Jagemann 4, J. Jochum, H. Kraus 1, B. Majorovits 1, V. Mikhailik 1, J. Ninkovic 2, F. Petricca 2, W. Potzel 4, F. Proebst 2, Y. Ramachers 1,*, W. Rau 2, M. Razeti 4, W. Seidel 2, M. Stark 4, L. Stodolsky 2, A. J. B. Tolhurst 1, W. Westphal 4, H. Wulandari 4 1. University of Oxford, U.K. 2. MPI für Physik, Munich, Germany 3. Laboratori Nazionali del Gran Sasso, Italy 4. Technische Universität München, Germany 5. Eberhard-Karls-Universität Tübingen, Germany * Permanent address: University of Warwick, U.K.

Cristina Cozzini (Oxford), IDM 2004, Edinburgh light reflector 300 g CaWO 4 crystal separate cryogenic light detector thermometer Superconducting film as thermometer simultaneous measurement of phonons and scintillation light to discriminate nuclear recoil signals from radioactive background CRESST PhaseII detector module

Cristina Cozzini (Oxford), IDM 2004, Edinburgh irradiation with e - and  with e -  und neutrons Background Suppression: 98 % keV 99.7% keV 99.9% > 20 keV

Cristina Cozzini (Oxford), IDM 2004, Edinburgh U-Th >

Cristina Cozzini (Oxford), IDM 2004, Edinburgh ICP-MS (inductively coupled plasma mass- spectrometry) analysis of the impurities in CaWO 4 X-ray luminescence of CaWO 4 RE- impurities in Russian (Y, Nd, Gd and Er all >1 ppm) and Pb (~1 ppm ) in Ukrainian samples Russian Ukrainian

Cristina Cozzini (Oxford), IDM 2004, Edinburgh 147 Sm 152 Gd 144 Nd 180 W

Cristina Cozzini (Oxford), IDM 2004, Edinburgh 180 W Run 28 crystal D

Cristina Cozzini (Oxford), IDM 2004, Edinburgh Half-life for the  -decay of 180 W obtained independently in four different runs Counts Exposure Half-life [kg days] [years] Run 28 Crystal D35± (1.7±0.2)  Run 27 Crystal D28.5± (1.9±0.4)  Run 23 Crystal E ≥1.1  (90% C.L.) Run 22 Crystal B ≥6.7  (90% C.L.)

Cristina Cozzini (Oxford), IDM 2004, Edinburgh Half-life for the  -decay of 180 W obtained from the total exposure (28.62 kg days) Half life T 1/2 = (1.8±0.2)  years Energy Q = (2516.4±1.1 (stat.)±1.2(sys.)) keV Previous indication (Danevich et al. Phys. Rev. C 67 (2003)) Half life T 1/2 = ( (stat.)±0.3(sys.))  years

Cristina Cozzini (Oxford), IDM 2004, Edinburgh Lower limits (90% C.L) for the half-life times of the non-observed  -decay on the other naturally occurring W isotopes (exposure kg days) 182 W T 1/2 ≥ 7.7  years 183 W T 1/2 ≥ 4.1  years 184 W T 1/2 ≥ 8.9  years 186 W T 1/2 ≥ 8.2  years

Cristina Cozzini (Oxford), IDM 2004, Edinburgh Summary Strength of CRESST discrimination techniques High sensitivity (~1µBq/kg) Detection of the alpha decay of 180 W 182 W 183 W 184 W 186 W: improving by a factor of 50 the best previously published limits