LBNF Neutrino Beam Jim Strait, Fermilab For the LBNF/DUNE Team

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Presentation transcript:

LBNF Neutrino Beam Jim Strait, Fermilab For the LBNF/DUNE Team NuFact 2015 Rio de Janeiro, Brazil 14 August 2015

Outline Overview of LBNF/DUNE Current and expected capabilities of the Main Injector complex Reference design of the LBNF Neutrino Beam Optimizing the focusing system for greater physics reach Summary 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Long-Baseline Neutrino Facility A facility to enable a world-leading experimental program in neutrino physics, nucleon decay, and astroparticle physics. LBNF comprises: Underground and surface facilities at the Sanford Underground Research Facility capable of hosting a modular LAr TPC of fiducial mass ≥ 40 kt (~70 kt liquid mass) Cryostats, refrigeration and purification systems to operate the detectors A high-power, wide-band, tunable, n beam at Fermilab Underground and surface facilities to host a highly-capable near detector at Fermilab … and potentially other non-oscillation neutrino experiments 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

LBNF/DUNE LBNF is a DOE/Fermilab hosted project with international participation. Major partners include CERN and SURF. DUNE Collaboration will build and operate the experiment* in LBNF. 32 km *See DUNE talks: DUNE Physics (WG1 Monday) DUNE Near Detector (WG1-2 Tuesday) DUNE Systematics (WG1-2-3 Thursday) 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Fermilab Main Injector Capabilities Routine operation >400 kW since March With Fixed Target Beam Operations Dedicated Neutrino Operations Record beam power 520 kW just before summer shutdown. Goal is 700 kW for NOvA by next Spring 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

LBNF Beam Operating Parameters: Main Injector Complex with PIP-II and PIP-III upgrades Summary of key Beamline design parameters for ≤1.2 MW and ≤2.4 MW operation Pulse duration: 10 ms Beam size at target: tunable 1.0-4.0 mm (1.1 – 1.9)x1021 POT/yr PIP-II PIP-III 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

LBNF Neutrino Beam To SURF 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Primary Beam and Lattice Functions The LBNF Primary Beam will transport 60 - 120 GeV protons from MI-10 to the LBNF target to create a neutrino beam. The beam lattice points to 79 conventional magnets (25 dipoles, 21 quadrupoles, 23 correctors, 6 kickers, 3 Lambertsons and 1 C magnet). Beam size at target tunable between 1.0-4.0 mm Horizontal (solid) and vertical (dashed) lattice functions of the LBNF transfer line 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Neutrino Beam Configuration multi-­ply geosynthetic barriers, separated by a drainage layer Support modules for target/baffle carrier and horns Decay Pipe Decay Pipe snout and window Beam slopes down at 101 mrad towards the Far Detector 1300 km away Work cell Water cooled panels Space reserved for more optimized horn system 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

~40% of the beam energy deposited in the target chase Target Shield Pile steel shielding surrounds the beamline components (baffle, target, Horn 1, Horn 2, and the decay pipe upstream window) installed in the target chase Water-cooled chase panels ~40% of the beam energy deposited in the target chase Cooling: combination of forced air & water-cooled panels 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Target and Focusing System – Reference Design Protection Baffle 150 cm Ten graphite cores, 17 mm Ø hole, enclosed by an aluminum tube Target NuMI-style target: 47 graphite segments, each 2 cm long and spaced 0.2 mm apart, for a total target core length of 95 cm, 2 λI. Viable for 1.2 MW beam power. Horns: identical to NuMI, but operated at 230 kA current and subjected to a maximum beam power of 1.2 MW new Horn Power Supply necessary to reduce pulse width to 0.8 ms Target starting 45 cm upstream of MCZERO 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Initial Modifications for 1.2 MW 700 kW design 7.4 mm Proton Beam Wider target material (still graphite): 7.4 10.0 mm Dual cooling pipes – greater surface area Slightly larger outer vessel diameter: 30 36 mm (Move target upstream 10 cm from horn) cm 47 graphite segments, each 2 cm long mm 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Upstream Decay Pipe Window ~ 20 cm He cooling supply temporary blind thin replaceable window 1.25 mm beryllium or beryllium-aluminum alloy foil welded to a heavier aluminum ring heavier ring includes a seal groove for an all metal seal viable design for 60-120 GeV/c protons, 1.03-1.20 MW beam power 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Decay Pipe 194 m long, 4 m inside diameter Helium filled double-wall decay pipe, 20 cm annular gap 5.6 m thick concrete shielding It collects ~30% of the beam power, removed by an air cooling system Porous cellular concrete drainage layer 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Target Chase & Decay Pipe Cooling Combination of forced air & water cooling panels for Target Shield Pile Air-cooled Decay pipe 2 separate air systems for target Chase and Decay Pipe Possible need to replace air in the target chase with N2 or He under study 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Absorber building Absorber goes here 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Beam Absorber Configuration ~30% of the beam energy deposited in the Absorber Core: replaceable water-cooled blocks, each 1 foot thick Outside of the core is forced-air cooled steel and concrete shielding Viable for 60-120 GeV/c protons, 2.06-2.4 MW beam power, including both steady-state operations and accident conditions 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Absorber Hall components and shielding allow future replacement Remote Handling Remote Handling systems are integrated into the infrastructure of the Target complex, they must be designed to be sufficient for 2.4-MW beam power Shield doors (will incorporate air seals) Lifting fixtures, vision system Morgue/Maintenance areas, Rail System Hot Storage Rack and Work Cell Absorber Hall components and shielding allow future replacement Low probability of complete failure, final design and construction of remote handling equipment not included in the LBNF project No Work Cell needed in Absorber Hall Transfer cart Cask Work Cell Replaceable core blocks Beam 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Beam Simulation Extensive MARS simulations for energy deposition and radiological studies as well as for Beamline configuration optimization studies. ~40% of the beam power is deposited to the Target Hall Complex, 30% to the Decay Pipe region and 30% to the Absorber Hall complex. GEANT simulations for Beamline configuration optimization studies, neutrino fluxes, sensitivity and systematic studies. Target Complex (mSv/hr) Absorber Complex (mSv/hr) 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

What is being designed for 2.4 MW Designed for 2.4 MW, since upgrading later would be prohibitively expensive and inconsistent with ALARA: Size of enclosures (primary proton beamline, target chase, target hall, decay pipe, absorber hall) Radiological shielding of enclosures (except from the roof of the target hall, that can be easily upgraded for 2.4 MW when needed) Primary Beamline components The water cooled target chase cooling panels The decay pipe and its cooling and the decay pipe downstream window beam absorber remote handling equipment radioactive water system piping horn support structures are designed to last for the lifetime of the Facility 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Neutrino Flux – Reference Configuration Focusing positive particles (nm beam) 120 GeV protons 230 kA horn current Focusing negative particles (n̅m beam) 2nd 1st osc max 2nd 1st osc max 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Studies for an optimal beam design - Physics Proton energy choice in the range 60-120 GeV (some programmatic consequences). Horns Shape/size current (power supply up to 300 kA, just completed new conceptual design) Target (currently two interaction lengths) Size/shape/position with respect to Horn 1 Material(s) (higher longevity can increase up time - ongoing R&D) Studied Decay Pipe length and diameter. Current length 194 m (studied 170 m - 250 m). Current diameter 4 m (studied 2-6 m). Recently fixed at 194 m long x 4 m diameter. 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Optimizing the focusing system for greater physics reach Genetic algorithm, inspired by work done by LBNO Collaboration to optimize for CP Violation sensitivity Genetic algorithm and new shape of Horn 1 Horn 2 is NuMI shape in this case but rescaled radially and longitudinally 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Target chase allows for optimized focusing systems Reference Design Target Chase indicating the positions of the reference design horns (in red) and the optimized horns (in blue) 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Neutrino Flux of best configurations compared with Reference Design 80 GeV protons Enhanced: thinner and shorter cylindrical Be target, 25 cm upstream of 1st horn 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

CPV and MH sensitivity improvement with optimized beam 40% less exposure req’d 5 % ⊕ 1 % 5 % ⊕ 3 % 5 % ⊕ 2 % 50 % CP Violation Sensitivity 30% less exposure req’d 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Further work required on optimized target-horn system Engineering needed to determine feasibility of horn designs selected by genetic algorithm Study effect of 2 -> 3 horn system Search phase-space of horn design more broadly, and consider other optimization criteria, e.g. for nt appearance. Alternate target designs and materials Target and horn R&D towards 2.4 MW operation Alternate ideas to “classical” horn focusing? => Ideas from new collaborators are needed! 14 Aug 2015 Jim Strait | LBNF Neutrino Beam

Summary The Fermilab Main Injector is delivering the world’s highest beam power for neutrinos ... 0.5 MW now, 0.7 MW next year, 1.2 MW -> 2.4 MW with PIP-II and eventually PIP-III The LBNF beamline design is well developed, based on NuMI experience All systems designed for 1.2 MW All elements that cannot be replaced later are designed for 2.4 MW Further optimization can have a big impact on the physics reach of DUNE … new ideas and new collaborators are needed now to realize this potential. 14 Aug 2015 Jim Strait | LBNF Neutrino Beam