K. Zuber, Uni. Sussex Status of COBRA IDEA Meeting, Zaragoza 7 Nov. 2005.

Slides:



Advertisements
Similar presentations
COBRA A new Approach to -Decay UK HEP Forum, Abingdon, May 11 th, 2003 Daniel Muenstermann University of Dortmund COBRA.
Advertisements

May 2005UK Forum Dark Matter, RAL Neutrino masses from double beta decay Kai Zuber University of Sussex.
Activity for the Gerda-specific part Description of the Gerda setup including shielding (water tank, Cu tank, liquid Nitrogen), crystals array and kapton.
Status of Ultra-low Energy HPGe Detector for low-mass WIMP search Li Xin (Tsinghua University) KIMS collaboration Oct.22nd, 2005.
K. Zuber, University of Sussex Neutrinoless double beta decay SUSSP 61, St. Andrews, 9-23 Aug
K. Zuber, Uni. Sussex IDEA Meeting, Milano 9. Nov Status of COBRA.
COBRA Kai Zuber University of Sussex 5 th SNOLAB Workshop,
M. Dracos 1 Double Beta experiment with emulsions?
GERDA: GERmanium Detector Array
Search for spontaneous muon emission from lead nuclei with OPERA bricks M. Giorgini, V. Popa Bologna Group OPERA Collaboration Meeting, LNGS, 19-22/05/2003.
Erice, Kai Zuber1 Status of the COBRA Experiment K. Zuber, TU Dresden.
Status of COBRA K. Zuber, Univ. of Sussex Blaubeuren, July 2007.
DBD matrix elements Welcome and aim of the workshop Experimental situation Outcome.
Compton Identification Within Single ‘Pixels’ D. Scraggs, A. Boston, H. Boston, R. Cooper, J. Cresswell, A. Grint, A. Mather, P. Nolan University of Liverpool.
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.
Daniel Lenz, University of Wisconsin, Madison 11/05/ APS DNP Cryogenic search for neutrinoless double beta decay Daniel Lenz on behalf of the CUORE.
MUON FLUX MEASUREMENTS AT THE LSC JRA1-N2 Meeting, Zaragoza, Nov 23 rd 2007 Héctor Gómez Maluenda, University of Zaragoza.
No s is good s Sheffield Physoc 21/04/2005 Jeanne Wilson A historical introduction to neutrinoless double beta decay.
The COBRA Double Beta Decay Search Experiment
Potassium Geo-neutrino Detection Mark Chen Queen’s University Neutrino Geophysics, Honolulu, Hawaii December 15, 2005.
M. Dracos, CEA, 10/04/ Double Beta experiment with emulsions?
COBRA Double Beta Decay Experiment D.Y. Stewart, Dr. Y.A. Ramachers, Prof. P.F.Harrison Experimental Particle Physics Group University of Warwick What.
Search for  + EC and ECEC processes in 112 Sn A.S. Barabash 1), Ph. Hubert 2), A. Nachab 2) and V. Umatov 1) 1) ITEP, Moscow, Russia 2) CNBG, Gradignan,
New limits on  + EC and ECEC processes in 74 Se and 120 Te A.S. Barabash 1), F. Hubert 2), Ph. Hubert 2), A. Nachab 2) and V. Umatov 1) 1) ITEP, Moscow,
Contents Lecture 1 General introduction What is measured in DBD ? Neutrino oscillations and DBD Other BSM physics and DBD Nuclear matrix elements Lecture.
CUORICINO and CUORE Chiara Brofferio Università di Milano – Bicocca and INFN, Sez. di Milano NOW 2004 – Otranto 12 – 17 September 2004 On behalf of the.
Background Subtraction in Next Generation 0  Experiments Double-Beta Decay Challenges in 0  Decay Detection Small 0νββ decay half-life leads to low.
GERmanium Detector Array – a Search for Neutrinoless Double Beta Decay X. Liu - MPI für Physik, München Symposium – symmetries and phases in the universe,
Temperature Dependence of the Crystal Properties of 18-fold Segmented HPGe Detector Allen Caldwell, Daniel Lenz, Jing Liu, Xiang Liu, Bela Majorovits,
Status of COBRA 6 th SNOLAB Workshop, Picture courtesy
THE CUORE EXPERIMENT: A SEARCH FOR NEUTRINOLESS DOUBLE BETA DECAY Marco Andrea Carrettoni on behalf of the CUORE collaboration 2 nd International Conference.
LRT2004 Sudbury, December 2004Igor G. Irastorza, CEA Saclay NOSTOS: a spherical TPC to detect low energy neutrinos Igor G. Irastorza CEA/Saclay NOSTOS.
Present status of CUORE / CUORICINO Andrea Giuliani Università dell’Insubria and INFN Milano 3rd IDEA meeting, Orsay, April 14 – 15, 2005.
Upgrade and progess on the COBRA double beta detector Sudbury, 26. August 2010 Kai Zuber.
Status of Surface Sensitive Bolometers University of Insubria – Como, Italy INFN – Milano, Italy Prague, Chiara Salvioni.
The CUORE experiment Thomas Bloxham Lawrence Berkeley National Lab PHENO 2011 May 9th 2011.
M. Wójcik for the GERDA Collaboration Institute of Physics, Jagellonian University Epiphany 2006, Kraków, Poland, 6-7 January 2006.
MINILENS - A Scalable Prototype Detector for LENS LONU-LENS: Mini-Workshop on Low-Energy Solar Neutrinos and LENS Blacksburg, VA, October Mark Pitt.
Experiment TGV II Multi-detector HPGe telescopic spectrometer for the study of double beta processes of 106 Cd and 48 Ca For TGV collaboration: JINR Dubna,
Nd double beta decay search with SNO+ K. Zuber, on behalf of the SNO+ collaboration.
M. Wójcik Instytut Fizyki, Uniwersytet Jagielloński Instytut Fizyki Doświadczalnej, Uniwersytet Warszawski Warszawa, 10 Marca 2006.
Position sensitive CZT detectors for the COBRA neutrinoless double beta decay project Brian Fulton University of York Neutrinoless double beta decay The.
Cracow Epiphany Conference on Physics in Underground Laboratories and its Connection with LHC Cracow, Poland The GERDA Experiment at Gran.
BACKGROUND REJECTION AND SENSITIVITY FOR NEW GENERATION Ge DETECTORS EXPERIMENTS. Héctor Gómez Maluenda University of Zaragoza (SPAIN)
Present and future activities in LSM (2 nd LSM Extension WORKSHOP, Oct.16, 2009) (1) TGV experiment – measurement of 2 EC/EC decay of 106 Cd (2) R&D of.
28 May 2008NEMO-3 Neutrino081 NEMO-3 A search for double beta decay Robert L. Flack University College London On behalf of the NEMO-3 collaboration.
NEMO3 experiment: results G. Broudin-Bay LAL (CNRS/ Université Paris-Sud 11) for the NEMO collaboration Moriond EW conference La Thuile, March 2008.
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.
Results of the NEMO-3 experiment (Summer 2009) Outline   The  decay  The NEMO-3 experiment  Measurement of the backgrounds   and  results.
Double Beta Decay Experiments Jeanne Wilson University of Sussex 29/06/05, RAL.
Background Subtraction in Next Generation 0  Experiments Double-Beta Decay Challenges in 0  Decay Detection Benjamin Spaun Whitworth College Advisors:
Search for double electron capture in 106 Cd using HPGe detectors and Si pixel detectors Ivan Štekl for TGV collaboration Institute of Experimental and.
The COBRA Experiment Jeanne Wilson University of Sussex, UK On behalf of the COBRA Collaboration TAUP 2007, Sendai, Japan.
GERDA – a Search for Neutrinoless Double Beta Decay MPI für Physik, München Neutrinoless double beta decay and the GERDA experimentThe detector array and.
Neutrinoless double electron capture experiment at LSM University of Muenster, Germany (Dieter Frekers et al.) Technical University of Dresden, Germany.
M.Altmann, GERDA Status Report SNOLAB Workshop IV, Investigating Neutrinoless Double Beta Decay Status of the GERDA Experiment Michael Altmann.
Double Beta Decay - status and future Double beta decay basics Double beta decay basics Experimental challenges Experimental challenges Current experimental.
Phase I: Use available 76 Ge diodes from Heidelberg- Moscow and IGEX experiments (~18 kg). Scrutinize with high siginificance current evidence. Phase II:
PyungChang 2006/02/06 HYUNSU LEE CsI(Tl) crystals for WIMP search Hyun Su Lee Seoul National University (For The KIMS Collaboration)
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.
COBRA – CZT detectors for neutrinoless double beta decay measurements Martin Freer, University of Birmingham.
MPI für Physik, Fachbeirat, Béla Majorovits The GERDA experiment Béla Majorovits.
Search for Neutrinoless Double Beta Decay with NEMO-3 Zornitza Daraktchieva University College London On behalf of the NEMO3 collaboration PANIC08, Eilat,
Neutrinoless double beta decay (0  ) CdTe Semico nductor Band gap (eV) Electron mobility (cm 2 /V/s) Hole mobility (cm 2 /V/s) Density (g/cm 3.
Sheffield - Headline News NaI SMALL ARRAY DM55(high gamma background) vs. DM46 -> similar bump rate DM48 -> some evidence for a bump? DM50 (QMW) -> abandoned.
The COBRA Experiment: Future Prospects
Prompt Gamma Activation Analysis on 76Ge
The Heidelberg Dark Matter Search Experiment
Sr-84 0n EC/b+ decay search with SrCl2 crystal
Mo-92 EC/beta+ search with CaMoO4 crystal at Y2L
Presentation transcript:

K. Zuber, Uni. Sussex Status of COBRA IDEA Meeting, Zaragoza 7 Nov. 2005

Contents Introduction Current status of COBRA The 64 detector array Longer term planning Summary

C0BRA Use large amount of CdZnTe Semiconductor Detectors Array of 1cm 3 CdTe detectors K. Zuber, Phys. Lett. B 519,1 (2001)

Cobra - The people C. Gößling, H. Kiel, D. Münstermann, S. Oehl, T. Villett University of Dortmund J. Dawson, C. Montag, D. Polzaird, C. Reeve, J. Wilson, K. Zuber University of Sussex + further interested institutes Laboratori Nazionali del Gran Sasso M. Junker University of Warwick P.F. Harrison, B. Morgan, Y. Ramachers, D. Stewart T. Bloxham, M. Freer P. Seller B. Fulton, A. Smith, R. Wadsworth A. Boston, P. Nolan University of Birmingham University of Liverpool University of York Rutherford Appleton Laboratory

COBRA 2005 some are missing...

Isotopes nat. ab. (%)Q (keV)Decay mode COBRA: CdZnTe semiconductors

Level schemes

Quite a few lines...

 +  + - modes (A,Z)  (A,Z-2) + 2 e + (+2 e )  +  + e - + (A,Z)  (A,Z-2) + e + (+2 e )  +/EC 2 e - + (A,Z)  (A,Z-2) (+2 e ) EC/EC Important to reveal mechanism if 0  is discovered Enhanced sensitivity to right handed weak currents (V+A) n n p p e e In general: Q-4m e c 2 Q-2m e c 2 Q Double charged higgs bosons, R-parity violating SUSY couplings, leptoquarks...

Neutrino mass vs. right handed currents (eV) Possible evidence M. Hirsch et al., Z. Phys. A 347,151 (1994) EC/ß +

Advantages Source = detector Semiconductor (Good energy resolution, clean) Room temperature Tracking („Solid state TPC“) Modular design (Coincidences) Industrial development of CdTe detectors Two isotopes at once 116 Cd above MeV

Contents Introduction Current status of COBRA The 64 detector array Longer term planning Summary

Running periods Running at LNGS since February 2004 Scheme driven by money/manpower CAMAC DAQ - 4 detector prototype CAMAC DAQ - 4 detector prototype mod. VME DAQ - 4 detector prototype modified

Background Cosmogenics neutrons 116 Cd (Q=2805 keV) 2  113 Cd (n th,  ) 114 Cd Measurement: E. Porras et al., NIM B 111, 325 (1996) Alphas, Betas, Gammas muon induced neutrons

2  - decay + Tracking option S. Elliott, P. Vogel, Ann. Rev. Nucl. Part. Sci Energy resolution important  semiconductor Fraction of 2  in 0  peak: Signal/Background: 2  is ultimate, irreducible background

The 2x2 prototype 4 naked 1cm 3 CdZnTe more than 2.5 kg x days of data Setup installed at Gran Sasso Underground Laboratory

Neutrons Worry (if not enriched in 116 Cd): 113 Cd (n th,  ) 114 Cd MCNP simulation of the full set-up

Calibration 2.4% energy resolution at 2614 keV Much better ones available A little bit of cooling helps

Comparison of measurements 0.5 cm 3, surface, no shielding „old“ prototype, LNGS, no shielding „old“ prototype, LNGS, shielding, no veto

The background model Input: Pertinax (grid, base), detectors, paint and copper Currently limiting background: Passivation paint on detectors

Strategies We started a long term R&D with eV-Products to find another passivation (they have alternatives) Alternative providers not using the paint (Freiburg Material Research Centre)

Redesigned prototype Delrin holder and kapton foil Scalable design for larger masses

New versus old prototype Measuring time: 2630 hours, about 0.71 kg x days, Det1 only

Physics Cd T 1/2 = (8.2 ± 0.2 (stat.) (sys)) yrs 113 Cd one of only three 4-fold forbidden  -emitters known in nature C. Goessling et al., nucl-ex/ , acc. by Phys. Rev. C

First results  1/2 close to years obtained 70 Zn1.3 x x Cd8.0 x x Te3.3x x Cd 0  + EC 3.8x x Zn 0  + EC 2.8x x Te 0  + EC 2.2x x  NPA723 Current EC-modes H.Kiel, D. Münstermann, K. Zuber, Nucl. Phys. A 723,499 (2003) Current results are preliminary

Coincidences Aim: Coincidences among crystals should significantly reduce gamma background About 0.2 % of events are coincidences Array too small to prove power of coincidences  Larger Array 2614 keV gamma (MC)

Contents Introduction Current status of COBRA The 64 detector array Longer term planning Summary

The 64 detector array Aim for next 2 years: The next step towards a large scale experiment, Scalable modular design, explore coincidences Include: Cooling Nitrogen flushing Mass is factor 16 higher, about 0.5 kg CdZnTe Physics: - Can access 2 ECEC in theoretically predicted region -Precision measurement of 113Cd - New limits All detectors are at Dortmund

Signatures -  + /EC High granularity  A lot of patterns, interesting to investigate

Contents Introduction Current status of COBRA The 64 detector array Longer term planning Summary

The solid state TPC Single electron spectra Angular correlation coefficient  Introduce tracking properties by using segmented or pixellated electrodes and pulse shape analysis

First own measurements Two detectors: 4x4 pixel, 2mm x 2mm 16x16 pixel, 1.6 mm x 1.6 mm  -  plot Source location Two pixel events

Pixellated detectors 3D - Pixelisation: Solid state TPC

Nobody said it was going to be easy, and nobody was right George W. Bush

Back of the envelope  1/2 = ln2 a N A M t / N  (   T) ( Background free)  50 meV implies half-life measurements of yrs 1 event/yr you need source atoms This is about 1000 moles of isotope, implying 100 kg Now you only can loose: nat. abundance, efficiency, background,...

Dimension it right! 116Cd 116In 116SnA real time low-energy solar neutrino experiment? Threshold energy: 464 keV 7Be contribution g.s. alone: 227 SNU  = 14s K. Zuber, Phys. Lett. B 571,148 (2003) e e e Current idea: 40x40x40 CdZnTe detectors = 420 kg, enriched in 116Cd

Sensitivity 50 meV

Summary COBRA plans to use a large amount of CdZnTe semiconductors for double beta searches Collaboration of about 25 people established Currently preparing a 64 detector array (about 0.5 kg), to be installed at LNGS end of 2005 Design changed to allow easy upgrade to larger scales Work on signal enhancer/active veto and pixellated detectors has started Progress is fast

Einstein was right