Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, 2006 A High-Precision Measurement of sin 2 2  13 with the Daya Bay Reactor Antineutrino.

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Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, 2006 A High-Precision Measurement of sin 2 2  13 with the Daya Bay Reactor Antineutrino Experiment Karsten Heeger University of Wisconsin-Madison for the Daya Bay Collaboration DNP2006, Nashville, TN

Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, 2006 Understanding Neutrino Mixing What is  e fraction of 3 ? Is there  symmetry in neutrino mixing? ? Is there CP? What are the elements of the neutrino mixing matrix U MNSP ?

Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, 2006 Precise measurement of   3 - key in understanding neutrino mixing  13 and  23 are 2 of the 26 parameters of the SM, worthy of precision measurements Synergy of reactor + accelerator experiments (NOvA, T2K) - resolves  23 degeneracy - early indications of mass hierarchy - constraints on  CP -with enhanced beam rates NOvA+T2K will have good coverage for sin 2 2  13 > Ref: hep-ex/ Reactor experiments set the scale for future studies. Measuring  13 & Towards the Search for Leptonic CP Violation

Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, 2006 Direct search At  m 2 31 = 2.5x10 -3 eV 2, sin 2 2  13 < 0.15 allowed region Current Knowledge of  13 Ref: Fogli et al., hep-ph/ Global fit sin 2 2  13 < 0.11 (90% CL) Best fit value of  m 2 32 = 2.4x10- 3 eV 2 sin 2 2  13 = 0.04

Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, 2006 Measuring  13 with Reactor Antineutrinos Search for  13 in new e disappearance experiment ~1-1.8 km > 0.1 km  13 Large-amplitude oscillation due to  12 Small-amplitude oscillation due to  13 integrated over E  m 2 13 ≈  m 2 23 detector 1 detector 2

Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, 2006 How To Reach A Precision of sin 2 2  13 < 0.01 ? Concepts of a Next-Generation Reactor Neutrino Experiment High Statistics - Powerful source of e : commercial nuclear plant - Large detectors Optimization of Detector Locations - Optimize baseline for best sensitivity and smaller residual reactor- related errors Control of Systematics - Minimize reactor-related errors:  Use multiple, “identical” near and far detectors  Relative measurement - Cancel detector systematic uncertainties:  no position cuts for event selection  Interchange near and far detectors - Ensuring high detector efficiency through multi-zone antineutrino detector  Comprehensive calibration/monitoring of detectors Reduction of Backgrounds - Reduce background-related uncertainties through sufficient overburden and active shielding

Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, 2006 Daya Bay, China Multiple reactor cores. (at present 4 units 11.6 GW th, in units with 17.4 GW th ) Up to 1000 mwe overburden nearby. Adjacent to mountains.

Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, m 290 m 730 m 570 m 910 m Daya Bay Near 363 m from Daya Bay Overburden: 98 m Ling Ao Near 481 m from Ling Ao Overburden: 112 m Far Site 1615 m from Ling Ao 1985 m from Daya Overburden: 355 m Mid Site ~1000 m from Daya Overburden: 208 m Daya Bay - Site Layout Ling Ao ll (under construction) Ling Ao Daya Bay

Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, 2006 Detecting Reactor  e  e  p  e + + n  + p  D +  (2.2 MeV) (delayed)  + Gd  Gd*  Gd +  ’s (8 MeV) (delayed)  Time- and energy-tagged signal is a good tool to suppress background events. Energy of  e is given by: E   T e+ + T n + (m n - m p ) + m e+  T e MeV keV Inverse  -decay in 0.1% Gd-doped liquid scintillator 0.3b 50,000b Proton-rich target Easily identifiable n-capture signal above radioactive backgrounds Short capture time (  ~28  s) Good light yield

Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, 2006  Catcher thickness 92%  -catcher thickness (cm) Antineutrino Detector Design Cylindrical 3-Zone Structure I. Target: 0.1% Gd-loaded liquid scintillator, 1.6m II.  -catcher: liquid scintillator, 45cm III. Buffer shielding: mineral oil, ~45cm 12.2% 13cm 20 t Gd-LS liquid scintillator mineral oil With 224 PMT’s on circumference and diffuse reflector on top and bottom: Resolution  Catcher Efficiency Transparent acrylic vessels

Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, 2006 Event Rates and Signal Antineutrino Interaction Rate (events/day per 20 ton module) Daya Bay near site 960 Ling Ao near site760 Far site 90 Delayed Energy Signal Prompt Energy Signal Statistics comparable to single detector in far hall Distances to Sites (m)

Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, 2006 Systematic Errors from the Detector Number of Protons - reproducability: volume flow < 0.02%, mass flow < 0.1% - combustion analysis, NMR or neutron beam to determine H/C ratio Low-energy threshold: Routine calibration using positron annihilation source ( 68 Ge) Energy Cuts Calibrate the 6 MeV cut  relative uncertainty in neutron efficiency <0.2%. Position & Time Cuts - no position cuts: volume defined by neutron capture on Gd. - time cuts:time window  s, precision <10ns,uncertainty < 0.03% Gd/H Ratio 1% mass uncertainty causes 0.12% change in n-capture efficiency

Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, 2006 Detector-Related Uncertainties Baseline: currently achievable relative uncertainty without R&D Goal: expected relative uncertainty after R&D Absolute measurement Relative measurement Swapping: can reduce relative uncertainty further Ref: Daya Bay CDR

Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, near + far (3 years) near (40t) + mid (40 t) 1 year Near-mid Assume backgrounds are measured to < 0.2%. Use rate and spectral shape. Input relative detector systematic error of 0.2%. Sensitivity of Daya Bay Reactor  13 Experiment Milestones April 07 Begin civil construction June 09Start commissioning first two detectors Sep 09Begin data taking with near-mid June 10 Begin data taking with near-far 90% confidence level 1 year of data taking = 300 days

Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, 2006 June 2011 June 2010 June 2013 Baseline Configuration 9 months with near-mid 3 years with near-far Daya Bay Sensitivity by Year 20 t detector module

Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, 2006 Daya Bay Collaboration Asia (13) IHEP, CIAE,Tsinghua Univ., Zhongshan Univ.,Nankai Univ., Beijing Normal Univ., Nanjing Univ., Shenzhen Univ., Hong Kong Univ., Chinese Hong Kong Univ., Taiwan Univ., Chiao Tung Univ., National United Univ. ~ 125 collaborators Europe (3) JINR, Dubna, Russia Kurchatov Institute, Russia Charles University, Czech Republic North America (13) BNL, Caltech, LBNL, Iowa State Univ., Illinois Inst. Tech., Princeton, RPI, UC Berkeley, UCLA,Univ. of Houston, Univ. of Wisconsin, Virginia Tech, Univ. of Illinois Urbana-Champaign

Karsten Heeger, Univ. of WisconsinDNP2006, Nashville, October 28, 2006