The Long-Baseline Neutrino Experiment Project LBNE Project Overview Elaine McCluskey LBNE Project Manager mccluskey@fnal.gov SPAFOA Meeting 13 Nov 2012 Outline • • • • • • Mission need LBNE scope Organization Summary cost and schedule Near term procurements Summary SPAFOA Meeting – 13 Nov 2012 2 Mission Need • The LBNE Project is being planned in response to the Mission Need put forward by the DOE Office of High Energy Physics. • CD-0 was approved by the DOE Deputy Secretary on January 8, 2010. SPAFOA Meeting – 13 Nov 2012 3 The Long-Baseline Neutrino Experiment The LBNE Science Collaboration plans a comprehensive experiment to fully characterize neutrino oscillation phenomenology using • A high-intensity, broad-band neutrino beam • A sophisticated near detector • A 1300 km baseline • An advanced liquid argon time projection chamber far detector The goals of this program are: • Determining leptonic CP violation and neutrino mass ordering The recent discoveries confirm that this a scientifically well motivated, comprehensive, and stunningly beautiful program. • Underground physics, including the exploration of proton decay and supernova neutrinos. SPAFOA Meeting – 13 Nov 2012 4 A Phased Program The U.S. Department of Energy has stated their intention to carry out this program in a phased manner. • The LBNE Project is the first phase – focuses on accelerator neutrino oscillation physics – includes the beam and a 10 kt fiducial mass liquid argon TPC at the surface, 1300 km from Fermilab • Subsequent phases are planned to include: – A highly capable near neutrino detector – A larger far detector, placed deep underground – Higher beam power that will be enabled by Project X Additional national or international collaborators could increase the scope of the first phase of LBNE or accelerate the implementation of subsequent phases. SPAFOA Meeting – 13 Nov 2012 5 New Neutrino Beam at Fermilab… Directed towards a distant detector at the Sanford Underground Research Facility (SURF) in Lead, SD 10 kton Liquid Argon TPC Far Detector just below the surface All the Conventional Facilities at Fermilab and SURF required to support the beam and detectors. SPAFOA Meeting – 13 Nov 2012 6 Neutrino Beamline A new neutrino beam at Fermilab • Aimed at SURF • Spectrum optimized for 1300 km distance • 700kW initial beam power, upgradeable to 2.3 MW Existing Fermilab site Proposed LBNE beamline extracted from the Main Injector SPAFOA Meeting – 13 Nov 2012 7 Neutrino Beamline & its Conventional Facilities • • • • • • • SPAFOA Meeting – 13 Nov 2012 Extracted at MI-10 Conventional magnets Horns & target similar to NuMI Steel decay pipe surrounded by concrete shielding Aluminum, steel, and concrete hadron absorber Embankment for primary beam 3 surface buildings, cut & cover civil construction 8 Near Detector Complex: Tertiary Muon Monitor System • • SPAFOA Meeting – 13 Nov 2012 Positioned just behind Beamline absorber Three types of detectors monitor the neutrino beam 9 Liquid Argon Time Projection Chamber Far Detector 10 kton fiducial mass Liquid Argon (LAr) TPC detector • • Located in a pit just below the surface in Lead, SD (two 5 kton modules) Shielded against hadronic & cosmic ray showers >3m composite cover Detector 2 Septum Detector 1 Concrete liner Insulation SS Membrane Alternating Anode and Cathode Planes 2.3 m drift SPAFOA Meeting – 13 Nov 2012 10 Cryostat Design Using Membrane Cryostat Technology Each LBNE cryostat is 7100 m3 SPAFOA Meeting – 13 Nov 2012 11 Cryogenic Systems 4 1. LAr/GAr Delivery 1 2 2. Gas Purge & Filtering 3. Cryostat with Pumps 4. Refrig & Condensers 5. Liquid Filters & Regeneration 5 3 SPAFOA Meeting – 13 Nov 2012 12 Detector Cross-Section - Beam’s Eye View Side View x u v x 2.5m 2.3m e Anode Plane Ass’y (APA) Standard wire chamber construction e Cathode Plane Ass’y (CPA) – Stn Stl sheet Field cage wraps detector Membrane cryostat 14 m 2 modules x 3 wide x 2 high x 10 long = 120 APA planes SPAFOA Meeting – 13 Nov 2012 13 Far Site Surface Detector Location: Sanford Underground Research Facility (SURF) LBNE Far Detector location at Oro Hondo site SPAFOA Meeting – 13 Nov 2012 14 Far Site Surface Detector Location: Sanford Underground Research Facility (SURF) n beam LAr TPC n beam SPAFOA Meeting – 13 Nov 2012 • Sited against a hill • CF includes rock excavation, buildings, and site work 15 LBNE Project Organization • Fermilab is the lead laboratory. • The Brookhaven and Los Alamos National Laboratories also play major roles. • Universities from the LBNE Science Collaboration also contribute to design & fabrication. DOE Office of HEP J. Siegrist, Assoc Dir M. Procario, LBNE Program Manager • SURF is a partner institution for DOE LBNE Federal Project Director P. Carolan CF at the Far Site. Laboratory Oversight Group Y. K. Kim (FNAL) S. Vigdor (BNL) S. Seestrom (LANL) J. Symons (LBNL) Project Direction & Reporting FNAL P. Oddone, Director Y. K. Kim, Deputy Director Programmatic Advice Scientific Direction Support LBNE Collaboration Co Spokesperson M.Diwan R.Svoboda 130.01 Project Management E.McCluskey (FNAL) LBNE Project J.Strait (FNAL)- Project Director E.McCluskey (FNAL)- Project Manager M.Bishai(BNL) – Project Scientist J.Dolph (BNL) - Systems Engineer M.Andrews (FNAL)– ES&H Manager R. O’Sullivan (FNAL)– P.C. Manager 130.02 Beamline V.Papadimitriou (FNAL) SPAFOA Meeting – 13 Nov 2012 130.03 Near Detector Complex C.Mauger (LANL) 130.05 LAr Far Detector J. Stewart (BNL Project Management Board 130.06 Conventional Facilities T.Lundin (FNAL) 16 Long-Baseline Neutrino Experiment Collaboration Alabama: S.Habib, I.Stancu Argonne: M.D’Agostino, G.Drake.Z.Djurcic, M.Goodman, V.Guarino, S.Magill, J.Paley, H.Sahoo, R.Talaga, M.Wetstein Boston: E.Hazen, E.Kearns, S.Linden Brookhaven: M.Bishai, R.Brown, H.Chen, M.Diwan, J.Dolph, G.Geronimo, R.Gill, T.Haines, D.Lee, W.Louis, C.Mauger, G.Mills, Z.Pavlovic, J.Ramsey, G.Sinnis, W.Sondheim, R.Van de Water, H.White, K.Yarritu Louisiana: J.Insler, T.Kutter, W.Metcalf, M.Tzanov Maryland: E.Blaufuss, S.Eno, R.Hellauer, T.Straszheim, G.Sullivan Michigan State: E.Arrieta-Diaz, C.Bromberg, D.Edmunds, J.Huston, B.Page Minnesota: M.Marshak, W.Miller MIT: W.Barletta, J.Conrad, B.Jones, T.Katori, R.Lanza, A.Prakash, NGA: S.Malys, S.Usman Notre Dame: J.Losecco Oxford: G.Barr, J.de Jong, A.Weber Pennsylvania: S.Grullon, J.Klein, K.Lande, T.Latorre, A.Mann, M.Newcomer, S.Seibert, R.vanBerg Pittsburgh: D.Naples, V.Paolone Princeton: Q.He, K.McDonald Rensselaer: D.Kaminski, J.Napolitano, S.Salon, P.Stoler Rochester: L.Loiacono, K.McFarland, G.Perdue Sheffield: V.Kudryavtsev, M.Richardson, M.Robinson, N.Spooner, L.Thompson 346 members 61 institutions 5 countries SDSMT: X.Bai, C.Christofferson, R.Corey, D.Tiedt SMU.: T.Coan, T.Liu, J.Ye South Carolina: H.Duyang, B.Mercurio, S.Mishra, R.Petti, C.Rosenfeld, X Tian South Dakota: D.Barker, J.Goon, D.Mei, W.Wei, C.Zhang South Dakota State: B.Bleakley, K.McTaggert Syracuse: M.Artuso, S.Blusk, T.Skwarnicki, M.Soderberg, S.Stone Tennessee: W.Bugg, T.Handler, A.Hatzikoutelis, Y.Kamyshkov Texas: S.Kopp, K.Lang, R.Mehdiyev Tufts: H.Gallagher, T.Kafka, W.Mann, J.Schnepps UCLA: K.Arisaka, D.Cline, K.Lee, Y.Meng, A.Teymourian, H.Wang, L.Winslow Virginia Tech.: E.Guarnaccia, J.Link Washington: H.Berns, S.Enomoto, J.Kaspar, N.Tolich, H.K.Tseung Wisconsin: B.Balantekin, F.Feyzi, K.Heeger, A.Karle, R.Maruyama, B.Paulos, D.Webber, C.Wendt Yale: E.Church, B.Fleming, R.Guenette, K.Partyka, A.Szelc MOUs with the Project SPAFOA Meeting – 13 Nov 2012 17 17 September 2012 (346) R.Hackenburg, R.Hahn, S.Hans, Z.Isvan, D.Jaffe, S.Junnarkar, S.H.Kettell, F.Lanni, Y.Li, L.Littenberg, J.Ling, D.Makowiecki, W.Marciano, W.Morse, Z.Parsa, V.Radeka, S.Rescia, N.Samios,R.Sharma, N.Simos, J.Sondericker, J.Stewart, H.Tanaka, H.Themann, C.Thorn, B.Viren, S.White, E.Worcester, M.Yeh, B.Yu, C.Zhang Caltech: R.McKeown, X.Qian Cambridge: A.Blake, M.Thomson Catania/INFN: V.Bellini, F.La Zia, F.Mammoliti, R.Potenza, Chicago: E.Blucher, M.Strait Colorado: S.Coleman, R.Johnson, S.Johnson, A.Marino, E.Zimmerman Colorado State: M.Bass, B.E.Berger, J.Brack, N.Buchanan, D.Cherdack, J.Harton, W.Johnston, W.Toki, T.Wachala, D.Warner, R.J.Wilson Columbia: R.Carr, L.Camillieri, C.Y.Chi, G.Karagiorgi, C.Mariani, M.Shaevitz, W.Sippach, W.Willis Crookston: D.Demuth Dakota State: B.Szcerbinska Davis: M.Bergevin, R.Breedon, D.Danielson, J.Felde, C.Maesano, M.Tripanthi, R.Svoboda, M.Szydagis Drexel: C.Lane, S.Perasso Duke: T.Akiri, J.Fowler, A.Himmel, Z.Li, K.Scholberg, C.Walter, R.Wendell Duluth: R.Gran, A.Habig Fermilab: D.Allspach, M.Andrews, B.Baller, E.Berman, R.Bernstein, V.Bocean, M.Campbell, A.Chen, S.Childress, A.Drozhdin, T.Dykhuis, C.Escobar, H.Greenlee, A.Hahn, S.Hays, A.Heavey, J.Howell, P.Huhr, J.Hylen, C.James, M.Johnson, J.Johnstone, H.Jostlein, T.Junk, B.Kayser, M.Kirby, G.Koizumi, T.Lackowski, P.Lucas, B.Lundberg, T.Lundin, P.Mantsch, A.Marchionni, E .McCluskey, S.Moed Sher, N.Mokhov, C.Moore, J.Morfin, B.Norris, V.Papadimitriou, R.Plunkett, C.Polly, S.Pordes, O.Prokofiev, J.L.Raaf, G.Rameika, B.Rebel, D.Reitzner, K.Riesselmann, R.Rucinski, R.Schmidt, D.Schmitz, P.Shanahan, M.Stancari, A.Stefanik, J.Strait, S.Striganov, K.Vaziri, G.Velev, T.Wyman, G.Zeller, R.Zwaska Hawai’i: S.Dye, J.Kumar, J.Learned, J.Maricic, S.Matsuno, R.Meyhandan, R.Milincic, S.Pakvasa, M.Rosen, G.Varner Houston: L.Whitehead Indian Universities: V.Singh (BHU); B.Choudhary, S.Mandal (DU); B.Bhuyan [IIT(G)]; V.Bhatnagar, A.Kumar, S.Sahijpal(PU) Indiana: W.Fox, C.Johnson, M.Messier, S.Mufson, J.Musser, R.Tayloe, J.Urheim Iowa State: I.Anghel, G.S.Davies, M.Sanchez, T.Xin IPMU/Tokyo: M.Vagins Irvine: G.Carminati, W.Kropp, M.Smy, H.Sobel Kansas State: T.Bolton, G.Horton-Smith LBL: B.Fujikawa, V.M.Gehman, R.Kadel, D.Taylor Livermore: A.Bernstein, R.Bionta, S.Dazeley, S.Ouedraogo London: A.Holin, J.Thomas Los Alamos: M.Akashi-Ronquest, S.Elliott, A.Friedland, G.Garvey, E.Guardincerri, LBNL – SDSTA - LBNE SURF Opera ons Organiza on SDSTA Organiza on LBNE Project Organiza on LBNL P. Alivisatos, Director SDSTA Board of Directors, C.Peterson, Chair R. Wheeler, Execu ve Director FNAL P. Oddone, Director Y.-K. Kim, Deputy Director SURF Opera ons Office K. Lesko, Head Sanford Underground Research Facility LBNE Project Office J. Strait, Project Director M. Gilchriese, Deputy Head M. Headley, Laboratory Director E. McCluskey, Project Manager Sanford Underground Research SDSTA Engineering Facility LBNE Conven onal Facili es J. Willhite, Engineering Director M. Headley, and LBNE CF L3 FarDirector Site Manager T. Lundin, LBNE CF Manager J. Symons, Associate Director General Sciences Line Management / Program Direc on Contract Sanford Underground Research Facility • Host site for the LBNE Far Detector • Provides CF design and construction through contracts with Fermilab • LBNE Level 3 Manager for Far Site CF is SURF employee • Current SURF DOE operations are funded through LBNL SPAFOA Meeting – 13 Nov 2012 18 LBNE Status and Cost Estimate Project had successful DOE CD-1 Review 30 Oct to 1 Nov 2012, and we anticipate CD-1 approval by end of 2012. Estimated cost at CD-1 of the Project in at-year dollars LBNE 130.01 Project Office 130.02 Beamline 130.03 Near Detector Complex M$ 57 129 12 130.05 Liquid Argon Far Detector 130.06 Conventional Facilities Contingency TOTAL SPAFOA Meeting – 13 Nov 2012 181 241 236 867 19 LBNE Critical Path Schedule Summary Two essentially independent schedules, optimized for funding Jan-13 CD-1 Approve Alternate Selection & Cost Range Jan-10 CD-0 Approve Mission Need Apr-15 Apr-17 CD-3a Apr-16 CD-3b Approve CD-2 Approve Long Approve Lead Item Performance Start of Procurement Baseline Construction Jul-22 Near Site KPPs Met Complete Conc Design CF FS Prelim & Final Design & Procurmt CF FS Construction Cryostat Construction Install TPC, Test & Fill Detector Commissioning Sep-22 Far Site KPPs Met Complete Apr-23 CD-4 Approval (Early Finish) Conc Design CF Embankment Design & Procurmt CF Embankment Construction CF Embankment Settlement CF Primary Bm, Target Hall Constn Beamline Installation Beamline Hardware Commissioning Far Site is critical, Near Site near critical, both go through CF FY10 FY11 FY12 FY13 FY14 FY15 FY16 FY17 FY18 FY19 FY20 FY21 FY22 FY23 2 yr schedule contingency on early finish SPAFOA Meeting – 13 Nov 2012 20 Procurement Strategies – Far Detector Major FD engineering/fabrication/construction is planned: • • • Far Detector cryostat: contract with a construction management company under a design-build contract, who will subcontract with one of the two cryostat vendors and coordinate the construction. Expect to award design contract in late FY13, full design-build contract in FY16. Far Detector cryogenic systems: traditional design-build contracts with several sub-components >FY16 • Refrigeration plant/LN2 re-liquefier • Liquid argon storage and liquid nitrogen storage vessels and receiving area • Re-condensers for the cryostats • Purification system vessels and components • LBNE has the responsibility for the interconnections and the integration coordination. Time Projection Chamber (TPC): >FY16 • Major components such as stainless steel frames will be commercially produced in fabrication shops. • Components such as wire and FR4 components are commercially available. • Assembly and testing will be done by labs & universities. SPAFOA Meeting – 13 Nov 2012 21 Procurement Strategies – Conventional Facilities • CF Near Site (Fermilab) – Existing large A/E master contracts are already in place at Fermilab - Burns & McDonnell, HDR, AECOM - selection of one of these A/E’s for design is underway – Similarly with pre-construction CMs: Jacobs, Parsons, PMA/Patrick – FY13: Geotechnical site investigation & test embankment – FY14-16: CF NS design – FY15: Award construction contract for embankment • CF Far Site (SURF) – All design and construction work will be executed through contracts with SURF – SURF will do best value selection for Excavation, Infrastructure, and pre-construction CM consultants in FY13. – FY13: Geotechnical site investigation – FY14-15: Design for CF FS SPAFOA Meeting – 13 Nov 2012 22 Conclusions • The LBNE Project will enable a world-leading program that will address profound questions about nature. • It will deliver – An intense neutrino beam – A near site detector system to characterize the n beam – A 10 kton LAr TPC detector 1300 km from the n source • The Project anticipates CD-1 approval in 2012. • Cryo engineering and CF A/E contracts for design will be initiated with CD-1 approval. • Major construction and fabrication will begin in 2017. SPAFOA Meeting – 13 Nov 2012 23 SPAFOA Meeting – 13 Nov 2012 24 1300 km is an Optimal Baseline SPAFOA Meeting – 13 Nov 2012 25 Time Projection Chamber (TPC) Operation x MIP dE/dx = 2.2 MeV/cm ~ 1fC/mm @ 500 V/cm ~1 MeV/wire 114 kV 2.28m 1.4ms TPC design is modulal. SPAFOA Meeting – 13 Nov 2012 26 LAr TPC Capabilities Simulated neutrino events: • CC nm interaction with a stopped μ followed by a decay Michel electron nm • CCQE ne interaction with a single electron and a proton ne • NC interaction which produced a p0 that then decayed into two g’s with separate conversion vertices nx SPAFOA Meeting – 13 Nov 2012 27 Alternatives Analysis First Pass: Full LBNE LBNE has explored a wide range of “big picture” alternatives, including: • The experimental baseline => 1000 km < L < 1500 km • The location of the proton source: FNAL vs. BNL • Neutrino beamline configuration: deep or shallow; Main Injector extraction points MI-10 vs. MI-60 • The far detector location: Homestake vs. alternates • The far detector technical configuration: Liquid Argon vs. Water Cherenkov; detector depth => 4850 feet • Near Detector technology: scintillator tracker, straw-tube tracker, LAr TPC; with or without magnetic field SPAFOA Meeting – 13 Nov 2012 28 Alternatives Analysis Second Pass: Phase 1 of LBNE Program The 1st pass yielded the configuration of the “full” LBNE, whose cost could not be accommodated by the DOE in a single project => Reopen the alternatives analysis Process led by Fermilab-Directorate-Appointed Steering Committee: www.fnal.gov/directorate/lbne_reconfiguration/ Alternatives considered: • Lower cost alternatives that could achieve some of the scientific goals, with a shorter baseline using the existing NuMI beam. • Phased program that could achieve all the scientific goals in phases over time, with possible first phase options including: – Large detector underground at SURF, beam to be built later – Beam and near detector, far detector to be built later – Beam and small far detector on the surface at SURF, near detector and full-size underground far detector to be built later This is the LBNE Project SPAFOA Meeting – 13 Nov 2012 29