NEMO3 analysis and SuperNEMO development Benjamin Richards D14.

Slides:



Advertisements
Similar presentations
11 Mar 2004Nemo Collaboration Meeting1 Preliminary Study of 214 Bi Background in Mo foils Preliminary Study of 214 Bi Background in Mo foils Leo Jenner,
Advertisements

SuperNEMO Thoughts about next generation NEMO experiment Ruben Saakyan UCL.
Measurement of 40 Ar(n,p) reaction and neutron capture on 40 Ar and 136 Xe TUNL and Duke Univ. Megha Bhike and Werner Tornow Duke University and Triangle.
Status of XMASS experiment Shigetaka Moriyama Institute for Cosmic Ray Research, University of Tokyo For the XMASS collaboration September 10 th, 2013.
June 6 th, 2011 N. Cartiglia 1 “Measurement of the pp inelastic cross section using pile-up events with the CMS detector” How to use pile-up.
 Decay of 48 Ca, Preliminary Results Shiva King NEMO Meeting Aussois December 2005.
M. Dracos 1 Double Beta experiment with emulsions?
TeVPA, July , SLAC 1 Cosmic rays at the knee and above with IceTop and IceCube Serap Tilav for The IceCube Collaboration South Pole 4 Feb 2009.
Status of  b Scan Jianchun Wang Syracuse University Representing L b scanners CLEO Meeting 05/11/02.
27 Jun 2005S. Kahn -- Tof/Ckov Status1 Status of TOF and Ckov Sub- packages in G4Mice Steve Kahn 27 June 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.
First results from NEMO 3 Experiment V. Vasiliev (ITEP), H. Ohsumi (Saga) and Ch. Marquet Nara, Japan, June 2003 NEMO collaboration.
Background Subtraction in Next Generation 0  Experiments Double-Beta Decay Challenges in 0  Decay Detection Small 0νββ decay half-life leads to low.
NEMO-3  experiment First Results and Future Prospects Ruben Saakyan, UCL UK HEP Neutrino Forum The Cosener’s House, Abingdon.
Warsaw - NEMO initiative group Zenon Janas for Search for neutrinoless double  decay in NEMO-3 and SuperNEMO experiments Warszawa,
NEMO-3 Double Beta Decay Experiment: Last Results A.S. Barabash ITEP, Moscow (On behalf of the NEMO Collaboration)
The Summery of the NEMO 3 meeting. The topic Discussed 1) Some problems in variation of the gain of the counters and resoulution of the counters (for.
Development of A Scintillation Simulation for Carleton EXO Project Rick Ueno Under supervision of Dr. Kevin Graham.
Status of R&D of the SuperNEMO experiment Gwénaëlle Broudin-Bay LAL Orsay GDR neutrino – Bordeaux – Oct
FIRST RESULTS OF THE NEMO 3 EXPERIMENT Laurent SIMARD LAL Orsay (France) HEP-EPS 2003 conference CENBG, IN2P3-CNRS et Université de Bordeaux, France CFR,
SuperNEMO Simulations Darren Price University of Manchester July, 2005.
Updates on GEMs characterization with APV electronics K. Gnanvo, N. Liyanage, K. Saenboonruang.
Recent Results of the NEMO 3 Experiment Ladislav VÁLA Czech Technical University in Prague NOW2006, 9 th – 16 th September 2006, Conca Specchiulla, Italy.
Double beta decay and neutrino physics Osaka University M. Nomachi.
Spasimir Balev /CERN/ mrad 3 LKr simulation: – very slow, so only events with interesting topology are fully simulated: –  + with.
9-June-2003NDM2003 M. Nomachi M. Nomachi OSAKA University and MOON collaboration MOON (Mo Observatory Of Neutrinos) for double beta decay Photo by
2007/9/13N. Ishihara, TAUP2007, Sendai1 DCBA DCBA experiment for searching for Neutrinoless Double Beta Decay Nobuhiro Ishihara (KEK, Tsukuba) TAUP2007.
Start Counter Collaboration Meeting September 2004 W. Boeglin FIU.
1 Energy loss correction for a crystal calorimeter He Miao Institute of High Energy Physics Beijing, P.R.China.
Neutrinoless double-beta decay and the SuperNEMO project. Darren Price University of Manchester 24 November, 2004.
1 Performance of a Magnetised Scintillating Detector for a Neutrino Factory Scoping Study Meeting Rutherford Appleton Lab Tuesday 25 th April 2006 M. Ellis.
VIeme rencontres du Vietnam
Tracking (wire chamber) Shield radon, neutron,  Source foil (40 mg/cm 2 ) Scintillator + PMT 2 modules 2  3 m 2 → 12 m 2 Background < 1 event / month.
IOP HEPP Matthew Kauer Double beta decay of Zr96 using NEMO- 3 and calorimeter R&D for SuperNEMO IOP HEPP April Matthew Kauer UCL London.
DOUBLE BETA DECAY TO THE EXCITED STATES (EXPERIMENTAL REVIEW) A.S. BARABASH ITEP, MOSCOW.
Muon flux at Y2L and reconstruction of muon tracks
Neutrino Ettore Majorana Observatory
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.
Results of the NEMO-3 experiment (Summer 2009) Outline   The  decay  The NEMO-3 experiment  Measurement of the backgrounds   and  results.
Stefano Torre University College London for NEMO3 and SuperNEMO collaborations Half day IoP Meeting 12 Oct 2011 Outline 0νββ and 2νββ Observation technique.
Background Subtraction in Next Generation 0  Experiments Double-Beta Decay Challenges in 0  Decay Detection Benjamin Spaun Whitworth College Advisors:
Medium baseline neutrino oscillation searches Andrew Bazarko, Princeton University Les Houches, 20 June 2001 LSND: MeVdecay at rest MeVdecay in flight.
1st Year Talk1 PEP Violation Analysis with NEMO3 and Calorimeter R&D for SuperNEMO Anastasia Freshville.
By Matthew Kauer First Year Report – 15 June 07 Measurement of 2b2ν Half-Life of Zr96 and Lightguide Studies for SuperNEMO Calorimeter Matthew Kauer UCL.
Data vs MC … issues of the K +- group 1.Accidentals … contribution from Erika & Roberto 2.DC background.
Second Workshop on large TPC for low energy rare event detection, Paris, December 21 st, 2004.
Nasim Fatemi-Ghomi, Group Christmass Meeting December Nasim Fatemi-Ghomi Double Beta Decay Study of 150 Nd at NEMO3 (The magic isotope!!)
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.
Search for Neutrinoless Double Beta Decay with NEMO-3 Zornitza Daraktchieva University College London On behalf of the NEMO3 collaboration PANIC08, Eilat,
The NEMO3 Double Beta Decay Experiment Ruben Saakyan IoP meeting on Double Beta Decay Manchester 21 November 2007.
1 Cosmic Ray Physics with IceTop and IceCube Serap Tilav University of Delaware for The IceCube Collaboration ISVHECRI2010 June 28 - July 2, 2010 Fermilab.
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.
Calor 2010Anastasia Freshville1 SuperNEMO Calorimetry Anastasia Freshville (On behalf of the SuperNEMO Collaboration) Calor2010 – 12 th May.
Yuri Shitov Imperial College London On behalf of the NEMO Collaboration A search for neutrinoless double beta decay: from NEMO-3 to SuperNEMO Moriond EW.
Search for Neutrinoless Double-Beta Decay Werner Tornow Duke University & Triangle Universities Nuclear Laboratory (TUNL) & Kavli-Tokyo Institute of the.
ICARUS T600: low energy electrons
Transversal calibration of Geiger Cells
Status of 100Mo based DBD experiment
Deep learning possibilities for GERDA
Very preliminary study of the random background for the BiPo detector (PhoSwich configuration) Work done by Jonathan Ferracci.
Preliminary Study of 214Bi Background in 100Mo foils
XAX Can DM and DBD detectors combined?
Sr-84 0n EC/b+ decay search with SrCl2 crystal
The time-of-flight reconstruction & calibration
• • • Ge measurements for SuperNEMO
Some Comments to the Neutrinoless Double Beta-Decay
Recent works on AMS TANG Zhi-Cheng.
Presentation transcript:

NEMO3 analysis and SuperNEMO development Benjamin Richards D14

Brief Nemo3 Intro The Neutrino Ettore Majorana Observatory (NEMO 3) detector, which is now running in the Frejus Underground Laboratory and was begun more than ten years ago.

Description of detector parts Tracking wires PMTsSource foil Scintillator blocks wrapped in mylar

Last year: PMT coating / Analysis fit Development of PMT coating. Development of PMT coating. Shows Shows 10% ~ 15% increase in Q.E. Wrote an automated fit for Bi 207 energy spectrum Wrote an automated fit for Bi 207 energy spectrum Experimented with Phoswich idea Experimented with Phoswich idea Photons From LED Coating Photo cathode layer dynodes No. of Events ADC counts (Energy)

This year: Uniformity study of scintillator block for SuperNEMO PMT 8” Source Energy bins Frequency Scintilator wrapped in PTFE 976 KeV electron peak

Model of NEMO3 from TDR TDR Drawings 3D Reconstruction

Model of NEMO3 from TDR

Neutrinoless double beta decay

Theory for molybdenum to ground state and excited states We can calculate the matrix elements of other decay modes of 100 Mo, To more accurately estimate the matrix element for the neutrinoless double beta decay. We can calculate the matrix elements of other decay modes of 100 Mo, To more accurately estimate the matrix element for the neutrinoless double beta decay. 100 Mo γ γ 100 Ru 2e2ν

Cuts Made No. of scintillator hits = 2 No. of scintillator hits = 2 No. of tracks = 2 No. of tracks = 2 Check if scintillator hits have associated tracks Check if scintillator hits have associated tracks Both tracks are from negatively charged particles Both tracks are from negatively charged particles Cut if track reconstruction fails Cut if track reconstruction fails Cut on the source used (Mo only) Cut on the source used (Mo only) Cut if PMT is above max energy threshold Cut if PMT is above max energy threshold Cut if electrons are below 200KeV Cut if electrons are below 200KeV Check track starts from first 4 tracking wires Check track starts from first 4 tracking wires Check track end on last 3 tracking wires Check track end on last 3 tracking wires TOF cut to check its an internal electron TOF cut to check its an internal electron Check if scintillator is isolated Check if scintillator is isolated

Results Energy (MeV) Frequency Cos (θ) 1 Months data

Results Active time over which data was used = days Active time over which data was used = days No. of events that passed cuts = ±135 No. of events that passed cuts = ±135 Efficiency calculated from MC = Efficiency calculated from MC = Half-life calculated = (6.90 ± 0.05) x10 18 yr Half-life calculated = (6.90 ± 0.05) x10 18 yr

What I will do in the future Understand the backgrounds of the experiment Understand the backgrounds of the experiment Make analysis of 100 Mo transitions to excited states for Ph II Make analysis of 100 Mo transitions to excited states for Ph II Work on development for SuperNemo, including work on the module prototype. Work on development for SuperNemo, including work on the module prototype.