J.S. Jang Chonnam National University for RENO collaboration Oct. 24, 2010.

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Presentation transcript:

J.S. Jang Chonnam National University for RENO collaboration Oct. 24, 2010

 Overview of the RENO Experiment - Experimental Method - YongGwang Power Plant & Experimental Setup - Statistical & Systematic Uncertainties - Expected  13 Sensitivity - Schedule  Construction Status of the RENO Experiment - Tunnel - Detector - DAQ & Data Analysis Tools Outline

νeνe νeνe νeνe νeνe νeνe νeνe Distance Probability ν e to 1800 meters flux before oscillation Oscillations observed as a deficit of anti-neutrinos sin 2 2θ 13  Find disappearance of e fluxes due to neutrino oscillation as a function of energy Experimental Method of  13 Measurement  Identical detectors reduce the systematic errors in 1% level.

Detection of Reactor Neutrinos in Gd-LS detector

 Located in the west coast of southern part of Korea  ~400km from Seoul  6 reactors are lined up in roughly equal distances and span ~1.3 km  Total average thermal output ~16.4GW th (2 nd largest in the world) YongGwang Nuclear Power Plant YongGwang : 靈光 (Glorious light)

Google Satellite View of Experimental Site ~290m ~1380m

(13 institutions and 40 physicists)  Chonnam National University  Chonbuk National University  Dongshin University  Gyeongsang National University  Kyungpook National University  Pusan National University  Sejong University  Seokang Information University  Seokyeong University  Seoul National University  Sungkyunkwan University  Institute of Nuclear Research RAS (Russia)  Institute of Physical Chemistry and Electrochemistry RAS (Russia) RENO collaboration

RENO Experimental Setup ExperimentsLocation Thermal Power (GW) Distances Near/Far (m) Depth Near/Far (mwe) Target Mass (tons) Cost (US $) # of people Double- CHOOZ France8.7410/ /30010/10?> 160 RENOKorea / /45016/16~10M40 Daya BayChina (500)/1985(1613)260/  2/80 ?> 230

RENO Detector (Gd loaded liquid scintilllation detector) RENO Detector (Gd loaded liquid scintilllation detector)  354, 10” Inner PMTs : 14% surface coverage  67, 10” Outer PMTs

2.73 GW per reactor ⅹ 6 reactors 1.21x10 30 free protons per targets (16 tons) Near : 1,280/day, 468,000/year Far : 114/day, 41,600/year 3 years of data taking with 70% efficiency Near : 9.83x10 5 ≈ 10 6 (0.1% error) Far : 8.74x10 4 ≈ 10 5 (0.3% error) Expected Number of Neutrino Events at RENO

Systematic SourceCHOOZ (%)RENO (%) Reactor related absolute normalization Reactor antineutrino flux and cross section 1.9< 0.1 Reactor power Energy released per fission0.6< 0.1 Number of protons in target H/C ratio Target mass0.3< 0.1 Detector Efficiency Positron energy Positron geode distance Neutron capture (H/Gd ratio)1.0< 0.1 Capture energy containment Neutron geode distance Neutron delay Positron-neutron distance Neutron multiplicity combined 2.7< 0.5 Expected Systematic Uncertainty

10x better sensitivity than current limit New!! (full analysis) RENO Expected Sensitivity

 Tunnel facility, detector structure & buffer steel tanks completed  June 2010 : Acrylic containers installed  Aug : PMT test completed  Aug. ~ Oct : Installation of PMTs, veto tyvek and liquid handling system  Nov. ~ Jan : Installation of DAQ & HV and filling with liquid scintillator  Jan : Closing and detector commissioning  Feb : Start data taking Schedule

~11 : Geological survey and tunnel design are completed ~12 : Construction of both near and far tunnels are completed ~ : Veto tanks and peripheral facilities (electricity, air circulation, drainage, network, etc.) are completed : SK new electronics were adopted and ready ~11 : Buffer steel tanks are installed : Acrylic containers are installed : PMT test is completed Installation of PMTs, Electronics and liquid handling system are underway : Both near and far detectors are expected to be ready for data-taking. Construction status

Near detector site: - tunnel length : 110m - overburden height : 46.1m Far detector site: - tunnel length : 272m - overburden height : 168.1m Geological survey (2007.3~2007.8) Rock Quality Map

Experimental hall Wing tunnel(L) Wing tunnel(R) Detector Wing tunnel(R) Access tunnel Detectorv ertical hall Tunnel design (2007.9~ ) Design of Tunnel

Tunnel construction (2008.6~ ) by Daewoo Eng. Co. Korea Tunnel Construction

by Daewoo Eng. Co. Korea Tunnel completion (2009.3) Near siteFar site Near & far tunnels are completed

by NIVAK Co. Korea Vertical detector halls & steel structure are ready ( ~ ) Vertical detector halls & steel structure are ready ( ~ )

Experimental Hall

by NIVAK Co. Korea Buffer steel tanks are installed (2009.6~ )

Installation of Acrylic Vessels ( ) by KOA Tech. Korea

PMT test ( ~ 08) 890 PMTs were tested and 6 PMTs were returned to Hamamatsu.

Production of PMT Holder ( ~12) & PMT Mounting ( ~10) Production of PMT Holder ( ~12) & PMT Mounting ( ~10)

Installation of 1 st PMT ( ) & bottom PMTs

PMT assembling & barrel PMTs

Installation of VETO tyvek & outer PMTs Installation of laser injector

At present, PMT installation of near and far detectors has been done except for top PMTs. On going work (Middle of Oct. 2010) Installation of top PMTs Installation of liquid handling system Preparing Installation of DAQ and PMT HV system Filling the liquid Inner PMT installation of only far detector was done NOW conference Sep NuFact conference, Oct PMT installation including the VETO tyvek & VETO PMTs of near and far detector was done

HV Supply System CAEN SY1527 CAEN A1932A HV Supplier DAQ system All of system is ready to install.

DAQ System 24 channel input 60MHz clock 0.1pC, 0.52nsec resolution ~2500pC/ch large dynamic range No dead time (w/o hardware trigger) Fast data transfer via Ethernet R/W QBEE (QTC Based Electronics w/ Ethernet) All of DAQ system is ready to install & online DAQ programs are ready.

 Recipe of Liquid Scintillator Aromatic Solvent & Flour WLSGd-compound LABPPO + Bis-MSB 0.1% Gd+TMHA (trimethylhexanoic acid)  Target is filled with 0.1% Gd(with CBX) loaded liquid Scintillator C n H 2n+1 -C 6 H 5 (n=10~14) High Light Yield : not likely Mineral oil(MO) replace MO and even Pseudocume(PC) Good transparency (better than PC) High Flash point : 147 o C (PC : 48 o C) Environmentally friendly (PC : toxic) Components well known (MO : not well known) Domestically available: Isu Chemical Ltd. Gd Loaded Liquid Scintillator Liquid filling system is under construction.

R Analysis Control RENO Analysis Control Raw/MCDataProductionModulesReconstructionModulesUserAnalysisModulesUserntuples RACFrameWork RENO Event Display & Analysis Code Online event display and offline analysis code are ready.

 RENO is suitable for measuring  13 (sin 2 (2  13 ) > 0.02).  RENO is near completion.  Data taking with two detector is expected to start in Feb Summary Thank you!

Backup

J μ [cm -2 s -1 ] [GeV] Far 250 m2.9× m8.5× Near70 m5.5× Muon intensity at the sea level using modified Gaisser parametrization + MUSIC or Geant4 (the code for propagating muon through rock) Calculation of Muon Rate at the RENO Underground

Calculation of Background Rates due to Radioactivity Concentration 40 K (ppb) Concentration 232 Th (ppb) Concentration 238 U (ppb) 40 K [Hz] 232 Th [Hz] 238 U [Hz] Total [Hz] Rock4.33(ppm)7.58(ppm)2.32(ppm) LS in Target Target Contatiner LS in Gamma Catcher Gamma Catcher Container LS in Buffer ~ Buffer Tank PMT Total~24

Error bar = RMS of pC/sqrt(#of hits) * Error bar is too small in this plot Typical Plot by Malfunction PMTs