Current Status of the Construction of the Angra Antineutrino Detector
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1 Current Status of the Construction of the Angra Antineutrino Detector
2 ANGRA Collaboration: Brazilian Institutions: CBPF J.C. Anjos, G.L. Azzi, A.F. Barbosa, R.M.O. Galvão, H. Lima Jr, M. Vaz Graduate Students: Marcelo Nascimento Souza (PhD) Thamys Abrahão (MSc) Marcio Nunes (MSc) Andre G. Oliveira (MSc) Rafael Gama (MSc) Wallace R. Ferreira (MSc) Aridio Schiapazza (MSc) Vitor Ferraz (MSc) Undergraduate Students: Upiratan Beatriz 15/09/11 J.C.Anjos-AAP
3 The ANGRA Collaboration: UNICAMP E. Kemp, T. Bezerra, L. F. González, T. Junqueira UFABC Marcelo Leigui, R. Da Maceno, P. Chimenti UFJF Luciano M. Andrade, Rafael A. Nóbrega, Augusto S. Cerqueira UFBA Iuri M. Pepe Paulo Farias UEFS Germano P. Guedes PUC-RJ Hiroshi Nunokawa 15/09/11 J.C.Anjos-AAP
4 The ANGRA Collaboration: International group A. Bernstein, N. Bowden D. Reyna L. Villaseñor, E. Casimiro Linares Walter Fulgione, M.Aglietta 15/09/11 J.C.Anjos-AAP
5 Neutrinos Angra Project Development of new techniques for nuclear reactor monitoring 15/09/11 J.C.Anjos-AAP
6 15/09/11 J.C.Anjos-AAP
7 15/09/11 J.C.Anjos-AAP
8 DETECTOR STATUS 15/09/11 J.C.Anjos-AAP
9 Existing Infrastructure at ANGRA - Old 20 HC container placed next to reactor containment - Currently measuring background muon flux - Remote data acquisition from Angra-CBPF 15/09/11 J.C.Anjos-AAP
10 New container being prepared: size 40 High Cube model, for better shielding Top view of the container showing detector position 15/09/11 J.C.Anjos-AAP
11 external water shield Central detector: Gd loaded water with 40 PMTs to detector Cherenkov radiation 15/09/11 J.C.Anjos-AAP
12 Detector design (2011) Optimisation of number of PMTs: (detector + muon veto) Simulation with GEANT4 (2 MeV positrons at the center of the detector) Central detector: Gd loaded water with 40 PMTs to detector Cherenkov radiation 15/09/11 J.C.Anjos-AAP
13 Modeling of PMT fixture 15/09/11 J.C.Anjos-AAP
14 Prototype of the central detector Mechanical Project of Sarcophage ] External box: iron Internal box: Polypropilene PMT test setup 15/09/11 J.C.Anjos-AAP
15 Setup for testing efficiency of PMT photo-cathode Mounting of PMTs in the prototype tank 15/09/11 J.C.Anjos-AAP
16 Setup for testing efficiency of PMT photo-cathode Mounting of the prototype tank 15/09/11 J.C.Anjos-AAP
17 Setup for testing efficiency of PMT photo-cathode Mechanical project PMT Hat Mounting of the PMT hat 15/09/11 J.C.Anjos-AAP
18 Single Photoelectron Charge Spectrum Nu-DAQ 15/09/11 J.C.Anjos-AAP
19 Construction of a 50 l prototype for neutron detection in Gd loaded water ( 1 PMT) 252 Californium source donated by CDTN / MG (2010); Instalation of a small laboratory in the old CBPF linear accelerator tunnel; Authorization to use the neutron source given by CNEN in 2011; Some work still needs to be done Instalation of water purification station concluded; 15/09/11 J.C.Anjos-AAP
20 Muon outer veto project 15/09/11 J.C.Anjos-AAP
21 Testing Setup to test the multi-anode PMT H7546B 15/09/11 J.C.Anjos-AAP
22 ELECTRONICS STATUS 15/09/11 J.C.Anjos-AAP
23 Muon electronics - conceptual diagram (2007) PMT trigger logic FPGAs control and status registers Front-end electronics signal conditioning ADC 125 MHz 10 bits leading-edge discriminator stop TDC 81 ps 28 bits time encoding data builder DC level-1 trigger start* FIFO * trigger pulse from previous event control addr VME bus data 15/09/11 J.C.Anjos-AAP
24 Herman Lima Jr VII Encontro Neutrinos Angra UFJF 1-3 de junho de 2011
25 Lay-out of VME board developed in collaboration with Brazilian industry CADSERVICE Ten units produced for tests Components mounted by CADSERVICE (Campinas, SP) 15/09/11 J.C.Anjos-AAP
26 Optimized Digital Detection for the Trigger System. Luciano M. de A. Filho (UFJF) Augusto Santiago (UFJF) A. F. Barbosa (CBPF) 26 15/09/11 J.C.Anjos-AAP
27 Proposal Digital Filter to maximize signal/background ra8on before the trigger. Implementa8on Filter FIR. Two methods tested 1. Joint Filter. 2. Op8mized Filter for amplitude es8mate. Similar results for both filters. Op8mized filter has advantage of output in Volts. Central FPGA of NDAQ ADC Digital Filter Trigger Decision Increase signal/ background ra8o 15/09/11 J.C.Anjos-AAP
28 Optimal filter for amplitude estimate Signal before the filter Signal aier the filter 15/09/11 J.C.Anjos-AAP
29 Results Peak/Valley = 2.5 Peak/Valley = 5.0 ANTES DEPOIS Variance of the measurement: Error in the measurement: 15/09/11 J.C.Anjos-AAP
30 Detector Simulation Studies 15/09/11 J.C.Anjos-AAP
31 Simulation Software for photon propagation in the Central Detector Rafael Antunes Nóbrega Universidade Federal de Juiz de Fora - UFJF Faculdade de Engenharia Elétrica 15/09/11 J.C.Anjos-AAP
32 Event Generation 15/09/11 J.C.Anjos-AAP
33 Detector Geometry Studies: With or without Winston cones? Configuration 1 UP Média / 100 Ev. 77 (+19%) Hits/100 Ev./PMT < > 85 FRONT BACK DOWN Gustavo Valdiviesso (UFAlfenas) 15/09/11 J.C.Anjos-AAP
34 Conclusion of the Detector Geometry Studies Geometric configuration of the 40 PMTs does not affect neutrino signal. Final configuration to optimize muon rejection. Better signal with Winston cones (16% more light), but technical difficulties to implement (construction, cost... ). Polyethilene Shielding generates at least the double of neutrons by spallation than water Internal surface should be reflective but does not need to be polished. 15/09/11 J.C.Anjos-AAP
35 Data Analysis: simulation of expected signal and background Signal and background Simulation: Positrons (from neutrino interaction) Neutrons (from neutrino interaction) Cosmic Muons Cosmic Neutrons 15/09/11 J.C.Anjos-AAP
36 GEANT4: antineutrino signal positron signal (prompt) Neutron capture in Gd signal Distribuition of total number of photo electrons (p.e.) observed 15/09/11 J.C.Anjos-AAP
37 GEANT4: muon background Cherenkov signal of a muon in the target 15/09/11 J.C.Anjos-AAP
38 10 MeV neutron GEANT4: study of neutron shielding Fluxo Experimental medido no LNGS (1000 m): En > 10 MeV N_flux = 75 n/m 2.s Angra (nível do mar): redução 3x N_flux = 25 n/m 2.s Atenuação da blindagem ( ~ 85% acima de 10 MeV) N_flux = 4 n/m 2.s ~ 5% de contaminação 15/09/11 J.C.Anjos-AAP
39 Counts The time interval for both neutron capture in Gd and consecutive cosmic rays arrival follow a Poisson distribution The probability for an event to occur after a time interval t is: One day neutrino detection time spectrum 1/λ = average time interval between events 1/λ ν 30µs = time average for n capture Average 30µs µs 1/λ μ 1ms = time average for cosmic muons 39 15/09/11 J.C.Anjos-AAP
40 Data acquisition simulation Simulated data for one day of data taking and data reduction by each selection criteria 15/09/11 J.C.Anjos-AAP
41 Data acquisition simulation Simulated data for one day of data taking and data reduction by each selection criteria 15/09/11 J.C.Anjos-AAP
42 Data acquisition simulation 15/09/11 J.C.Anjos-AAP
43 Data acquisition simulation Fit Result: Neutrino events estimated within ~ 8% uncertainty 15/09/11 J.C.Anjos-AAP
44 Conclusions Previous experiments demonstrated a good capability of using antineutrinos for nuclear reactor distant monitoring. Neutrino laboratory already installed in Angra Muon detection (background estimate) and remote data acquisition (CBPF-Angra link) working. Simulation is running and guiding final detector design. Electronics is ready for production phase Expected data taking by beginning 2012 Good opportunity to develop experimental neutrino physics in Brazil and to contribute to new safeguards techniques. Good opportunity to interact with local industry. 15/09/11 J.C.Anjos-AAP
45 Thank you!
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