Neutrino Beamline Scaling Robert Zwaska Fermilab June 4, 2014 PIP-II Collaboration Meeting.

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Presentation transcript:

Neutrino Beamline Scaling Robert Zwaska Fermilab June 4, 2014 PIP-II Collaboration Meeting

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 2 LBNE “Recent” scope changes Upgrade Issues Primary Beamline: transport p GeV/c. Beam power of 1.2 MW, allowing for upgradeability of the facility to 2.3 MW Neutrino Beamline: wide band, sign selected beam (focusing on E in the GeV range)

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 3 Proton Improvement Plan-II Performance Goals - 80 GeV PIP-II doc: 1232 S. Holmes et al.

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 4  Primary beam window  Baffle and target, and their carrier  Horns  Horn power supply (we were using the NuMI one)  Horn stripline  Cooling panels for target chase  Water cooling at the bottom of support modules for target/baffle and horns  Upstream decay pipe window in the Helium filled decay pipe  Raw systems (Target, Horns, Cooling Chase Panels, Absorber, Decay Pipe windows)  Chillers for air handling and RAW Water systems  Water evaporators  Hadron Monitor  Additional interlock system in the Absorber Hall (on top of thermocouples) to protect from primary beam accident  Target chase shielding roof thickness  Radioactive air releases What will need to be re-evaluated or replaced at 1.2 MW Preliminary Additional $30-35 M in $FY13

Primary beam window Target Horn 1 Baffle and Target carrier Horn 2 Horns Power Supply Stripline US and DS decay pipe windows MARS & ANSYS SIMULATIONS NECESSARY We are here 80% Done Sequence of work needed for designing for 1.2 MW Target chase cooling panels Hadron Monitor Target chase shielding roof thickness RAW systems Baffle Done Will use pre-reconfiguration design

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting MW Target/Horn Considerations When LBNE was reconfigured in 2012, in order to save money we abandoned our LBNE optimized target and horn designs and opted for NuMI designs with small modifications. (e.g. we were able to verify the NuMI horns up to 230 kA instead of their 200 kA design value). March 2012 September 2012 LBNE Sept LBNE March 2012 Beam Power708 kW Horn 1 shapeDouble Parabolic Cylindrical/Parabolic Horn current200 kA300 kA TargetModified MINOS (fins) IHEP cylindrical Target “Carrier”NuMI-style baffle/ target carrier New handler, target attaches to Horn 1 CD1 ~ 25% less flux on the 2 nd oscillation max. ~ 3% more flux on the 1 st oscillation max. Tunable E spectrum

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting MW Target/Horn Considerations Our current plan is to check if modest modifications to the CD-1 (NuMI-like) designs can get us to 1.2 MW,  Minimize the redesign effort and the increase in cost.(Targets and horns are consumables). As a first attempt reduce stress by increasing beam spot size. Use NuMI target as a base but increase the fin width to 10mm and beam sigmas to 1.7mm.  Minor loss of neutrino efficiency  Increased heating in target and horn For the horns try to reduce the joule heating to make room for more beam heating (shorter pulse – cannot use the NuMI power supply).  New supply implements some design innovations

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 8 Preliminary target design for 1.2 MW mm We are simulating this target design and the NuMI horns with MARS and GEANT. It will take a couple more iterations but we see no show stoppers for this design to work. 47 graphite segments, each 2 cm long Graphite fin stress Water line stress

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 9 Preliminary target design for 1.2 MW Target critical safety factors Target is a system that needs R&D in addition to engineering development in order to improve its lifetime and increase operational efficiency Expect to change graphite target ~2-3 a year for 1.2 MW operation  Limited lifetime due to radiation damage of graphite Option remains for Be as target material pending validation.  Radiation damage a factor of 10 less than graphite (subject of R&D) Water hammer effect still to be analyzed

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 10 Horn Operation at 1.2MW Parameters700 kW1.2 MW Current Pulse Width2.1ms0.8ms Cycle Time1.33s1.20s Horn Current230kA Target Width7.4mm10mm Protons Per Spill4.9 X X Beam heating and joule heating on horn 1 generate unacceptable power input into the horn inner conductor with the new target design and the NuMI horn power supply (2.1ms pulse width). Higher energy depositions from the target can be offset by reducing the current pulse width to 0.8ms (requires a new horn power supply). These changes allow the design current to remain at 230kA which is the upper current limit for a NuMI conductor design. We still need to analyze the horn stripline for 230 kA. Increasing the radius of horn 1 neck transitions and moving the upstream weld further upstream may bring the safety factors to comfortable levels. Water Tank

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 11 Lower Beam Energy Certain agitators prefer LBNE operation at energies lower than 120 GeV  If the power can be preserved, may produce a slightly improved neutrino beam for certain analyses More protons are required in these scenarios  Radiation damage and heating of target/horns scales more as the number of protons, rather than the beam power These devices become more challenging with shortened lifetimes, but not impossible Expect reduced uptime in order to replace components  Consumes beam from other users Shorter Cycle time  Increased heating of pulsed elements Magnets, horns Complicated trade-off  Gains in neutrino flux can easily be offset by fewer operational hours and design compromises to deal with greater heating and radiation damage

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 12 Proton Improvement Plan-IV Performance Goals S. Holmes et al., P5 presentation Linac Particle TypeH - Beam Kinetic Energy8.0GeV Pulse rate10Hz Pulse Width6  4.3msec Particles per cycle to Recycler/MI2.5  Beam 8 GeV320kW Main Injector/Recycler Beam Kinetic Energy (maximum)60/120GeV Cycle time0.6/1.2sec Particles per cycle1.5  Beam Power at GeV2400kW LBNE “Facility” built for 2.3 MW  Shielding, Cooling channels, air channels, etc. Beam items  Need to replace target, horns, windows Challenging designs all around – LBNE expends no effort on these items  Incremental upgrade to cooling, air handling systems, etc.

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 13 NuMI High-Power Studies Issues with extended running at high beam power  For 700 kW, most of the issues are only continued running with a few major vulnerabilities  Higher beam powers raise many concerns that need to be addressed  A upper limit of beam power in NuMI exists – likely somewhere between 1.5 and 2.0 MW There have been a number of studies for higher power  The SNuMI effort (which spans the NOvA upgrades) Considered upgrades of 1.2 and 2.0 MW  Project X upgrades  Continued, extended running just for NOvA Reports to LBNE reconfiguration panel and Fermilab PAC Bottom line is that NuMI could likely run at 1.2 MW if PIP-II came online before LBNE  Several uncertainties in facility (radionuclides, cooling)  Need 1.2 MW designs for target & horns from LBNE

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 14 Summary LBNE is now being re-reconfigured to run at 1.2 MW from Day 1  Expect at least one more re-re-reconfiguration Design work is ongoing, but challenges appear tractable for 1.2 MW  Modified target design  Modified horn pulse (and possibly horn itself) 60 – 80 GeV operation of LBNE  May be efficient in terms of neutrinos / kW  Has costs in terms of radiation damage, heating, and capability for other users LBNE facility designed for 2.3 MW  Unreplaceable items designed from the start for high-power  Replaceable items have no designs NuMI could also run at higher power (1.2 MW), if the timing dictated  Some different challenges from LBNE, but same issues with consumables Thanks to Jim Hylen and Vaia Papadimitriou for slides and thoughts for this talk.

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 15 Neutrino Beamline Scaling Robert Zwaska Fermilab June 4, 2014 PIP-II Collaboration Meeting 15

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 16 The NuMI Beam “Neutrinos at the Main Injector” 400 kW design average power 700 kW upgrade for NOvA  1 mm 2 interaction length, C target Produces  , K + mesons Pulsed focusing horns Toroidal magnetic field Parabolic inner conductor profile Focuses meson momentum band 2 m diameter Roughly decay length for 10 GeV  + He-filled Absorbs ~ 40 % of beam power Allows high-energy muons to penetrate Measure hadron & muon fluxes Arrays measure distributions

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 17 Primary Proton Beamline Primary beamline is in mostly good shape  Continued maintenance of magnets, instrumentation, and utilities underground Pre-target window did need replacement  Corrosion around brazing area – hopefully mitigated, but could occur again  Good procedure now exists for the replacement Higher beam power would likely require replacement of some instrumentation and the beam window

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 18 Targets 700 kW target will exist from NOvA  Not suitable for low-energy running  Will have lifetime of ~ 1 year LBNE 700 kW low-energy target could be adopted  Will require additional design and prototyping work if not pursued on LBNE Concepts exist for higher power targets (up to 2 MW)  Often need to compromise in yield with a larger spot size and/or wider target  R&D and design work needed to advance any of these designs

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 19 Horns NuMI horns 1 & 2 for 700 kW will be operating for NOvA  Expect to last a few years each Horn 2 is in medium-energy position  Relocation to the low-energy position is possible, but a big job Low-energy “nest” exists for a possible 3 rd horn installation  Would need study – material interactions may offset any focusing advantage Horn 1 would require some upgrading of cooling capacity to accommodate a low-energy target position  Being pursued within LBNE Horn 1 would require substantial redesign for higher-power operation

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 20 Target Shield Pile Will be operating well for 700 kW  Requires air-cooling at present. Air- handling has been a difficulty in NuMI because of the corrosive, radioactive environment, but it is mostly in-hand now  Much higher beam powers would require water cooling. It has been investigated, but is expensive Radionuclide inventory  Tritium and Na-22 are being handled by an extensive system within NuMI. Challenging, but working well now.  Both will almost be plateauing by 2020.

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 21 Decay Pipe Decay pipe cooling operates very well at 700 kW and could likely accommodate higher-powers with only minor upgrades Beam absorber can be similarly upgraded  Both are quite difficult to repair if major problems arise One major issue is the decay pipe window  Possibility of corrosion build-up  Not designed for replacement  Replacement or mitigation would be costly and time-consuming  Replacement would be thicker

June 4, 2014 Bob Zwaska – Fermilab PIP-II Collaboration Meeting 22 Instrumentation NOvA hadron monitor is designed for 700 kW  Likely to require replacement every few years  Higher-power would require redesign of a difficult system Muon monitor systems are insensitive to beam power  However, they are ageing and could use replacement at some point