BeamandLargeDetectorsforthe USLongBaselineNeutrinoExperiment - - PowerPoint PPT Presentation
BeamandLargeDetectorsforthe USLongBaselineNeutrinoExperiment - - PowerPoint PPT Presentation
BeamandLargeDetectorsforthe USLongBaselineNeutrinoExperiment JonUrheim IndianaUniversity 16December2010 Outline TheLBNEProject:
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Outline
- The LBNE Project:
– Origins, CD‐0 (“mission need”), Scope & Status
- The LBNE Beam Line
– General CharacterisTcs, Technical Components
- Water Cherenkov (WCD) Far Detector
– Cavern, Vessel, PMT’s
- Liquid Argon TPC (LArTPC) Far Detector
– Cavern, Membrane cryostat, TPC mechanics & electronics
Disclaimer: “reference designs” described here evolving rapidly!
2 16 Dec. 2010
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
What is LBNE?
3 16 Dec. 2010
- LBNE = Long Baseline Neutrino Experiment
– It is the name of the “Project” being proposed to U.S. funding agencies. – Its impetus was provided by the very influenTal 2008 P5 report. – LBNE represents the “next generaTon” of osc’n experiments following T2K & NOvA accelerator + Double Chooz, Daya Bay, & Reno reactor expts
- Nominally it involves:
– A new intense wide‐band “low‐energy” neutrino beam line at FNAL. – A “Near Detector” facility located at the edge of the FNAL site – A “Far Detector” facility 1290 km away at DUSEL (Homestake mine in SD)
- Liquid Argon TPC (17‐51 kt) and/or Water Cherenkov (100‐300 kt)
- Timescale: Bulk of data‐taking in the 2020’s (!!)
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Status of PreparaTon
- f Conceptual Design
4 16 Dec. 2010
- Design Efforts
– By Fall 2008, considerable momentum already established. – Science CollaboraTon forming then
- Denoted as “Homestake Neutrino Detector” collaboraTon in fall 2009
– Water Cherenkov proponents awarded NSF “S4” funds for engineering support – Liquid Argon efforts grown out of Fermilab R&D acTviTes, incl. MicroBooNE – AcTviTes formalized/accelerated w/ formaTon of “LBNE” Project in 2009
- establishment of project management structure/personnel
– DOE grants “CriTcal Decision 0” in January 2010 authorizaTon to develop conceptual design for 2 x 100‐kt Water Cherenkov Module Equivalents
- 3rd module could be built if funded internaTonally
- Deliverable for CD‐1 approval: “Conceptual Design Report”
– Current Drao well over 1,000 pages. CD‐1 review planned in 2011.
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
The LBNE Beam Line
5 16 Dec. 2010
- Highlights:
– Wide‐band on‐axis beam (0.5‐5 GeV + HE tail) – Pitched down at 5.6o (10% grade) – 700 kW beam line, upgradable to 2.3 MW – Builds on experTse gained with NuMI:
- Focus on reliability, safety, finite lifeTme of components, and
need for remote handling & storage of spent components.
See also slides from G. Rameika
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10 16 Dec. 2010 6
Slide courtesy V. Papadimitriou
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10 16 Dec. 2010 7
Slide courtesy G. Rameika
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Beam Line Parameters
8 16 Dec. 2010
Beam Parameter Value Protons per cycle 4.9 x 1013 Cycle Tme (120 GeV) 1.33 sec Pulse duraTon 1.0 x 10‐5 sec Proton beam energy 60 to 120 GeV Beam power at 120 GeV 708 kW OperaTonal efficiency 63% Protons at target per year 7.3 x 1020 Beam size at focus 1.5 mm Beam divergence x,y 0.017 mrad
Compare w/ NuMI: Design: 400 kW OperaTng at: 300 kW ~ 3 x 1013 ppp ~ 2 sec cycle Tme
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10 9 16 Dec. 2010
Primary Beam Line
- Requirements/SpecificaTons:
– Minimize Losses:
- Extensive beam permit system w/ 250 parameters
- Open extracTon channel, large magnet apertures
(> 47mm x 120 mm for dipoles, 72 mm for quads) to accommodate
varied beam condiTons (beyond 500 π Main Injector dynamic aperture)
- Strong focusing opTcs, automated beam pos’n control
- Power supply regulaTon to few ppm.
- Robust instrumentaTon.
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Neutrino Beam Technical Components
10 16 Dec. 2010
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Recent repair to Horn 1 made difficult due to high radiation levels: 75 r/hr ( 0.75 Sv/hr) on contact 35 r/hr ( 0.35 Sv/hr) at 1 foot Repair worker gets weekly dose limit in a few seconds! 2 minute repair job distributed over crew of 10, total 371 mr.
NuMI Horn 1, aoer 1st year of running
Slide from 2004, Courtesy J. Hylen
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Target Hall Layout
12 16 Dec. 2010
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Target and Horns
13 16 Dec. 2010
Target
– Nominally Graphite core – Design for 700 kW target proceding at IHEP Protvino, upgradable to 2.3 kW – Fully inserted into Horn 1, but can be removed w/ remote handling
Horns
– Horn 1 u/s: cylindrical – Horn 1 d/s: parabolic – Horn 2: parabolic – Polarity under external control
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Far Detector OpTons:
14 16 Dec. 2010
- 2 x 100‐kt (fid.) Water Cherenkov Modules (WCD) ?
– w/wo Gadolinium doping (for relic SN neutrinos) ??
- 2 x 17‐kt (fid.) Liquid Argon TPC Modules (LAr20) ?
– w/wo scinTllaTon/cherenkov photon detectors ??
- 1 x WCD + 1 x LAr20 ?
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
The “WCD” Far Detector Module
15 16 Dec. 2010
- 100kt (fiducial) 138 kt total water mass
- 20% coverage: 50,000 x 10” diameter PMTs
– Hamamatsu R7081’s are candidate tubes
- Located at the DUSEL 4850’ level (4290 mwe)
– Cosmic muon rate ~ 0.1 Hz – SubstanTal cavern excavaTon project
- Builds on substanTal experience from SK and earlier
detectors.
See also slides from L. Whitehead
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
100 kt Water Cherenkov Detector Module
16 16 Dec. 2010
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
100 kt WCD: 4850’ & 5060’ Levels
17 16 Dec. 2010
Support rooms for water treatment, MEP, control & clean rooms Sumps Mucking egress and operaTonal sump access drio and secondary egress @ 5060L Secondary egress from LC1
Slide courtesy E. McCluskey
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Water Cherenkov Module
18 16 Dec. 2010
Highly integrated design
– Water containment/cavern interface – MagneTc compensaTon coils – PMT InstallaTon Units – Water recirculaTon manifolds – Deck & electronics / PMT interface
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Water Containment System
19 16 Dec. 2010
Vessel liner material:
– Polymeric sheet liner is a preferred opTon – 3mm stainless steel (304) is in baseline for now, as polymeric materials are under study
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
WCD Photodetector
20 16 Dec. 2010
- Requirements and SpecificaTons
– Aim for 20% coverage, w/ Quantum Efficiency > 20% – Wavelength range 300 to 600 nm – Gain 107 @ < 2 kV, charge resoluTon 50% – Aoerpulsing < 5%, pre‐pulsing < 1%, dark rate 2500 Hz @ 13C – Long‐term stability; Pressure resistance up to 700 kPa
- 50,000 Hamamatsu R7081 HQE version array meets requirements
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
WCD PMT Assembly & Support Structure
21 16 Dec. 2010
Housing Base EncapsulaTon Sleeve or Cup Base Electronics Cable Assembly
PMTs mounted onto “PIU”s:
– 6 PMT’s/PA’s per PIU – Note ‘cable trays’, light barrier – Note 100m cable spools (spools removed aoer install)
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
WCD Water CirculaTon System
22 16 Dec. 2010
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
ImplementaTon:
- Horizontal, verTcal and saddle coils
- Conductor is copper in single or 4 strand cable
- All feed and power supplies on deck
- Coils buried between cavern rock and concrete
vessel
- Proximity to PMTs may result in less than opTmal
compensaTon
Goal:
Less than 50 mG on at least 75% of all PMT posiTons Less than 100 mG on at least 95% Less than 150 mG everywhere
MagneTc CompensaTon
Slide courtesy F. Feyzi
16 Dec. 2010 23
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
The “LAr20” Far Detector Module
24 16 Dec. 2010
See also slides from B. Rebel, M. Soderberg
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
How to build a 20‐kt scale LArTPC ?
- 0. Draw from previous experience – ICARUS
- 1. Need a large cavern deep enough to provide
adequate shielding (most important for proton decay)
- 2. Need a vessel w/ low heat loss & no leaks
- 3. Need a cryogenics system to remove heat, re‐
liquefy boil‐off, & achieve required argon purity
- 4. Need a simple, modular TPC structure
- 5. Need low‐power, low‐noise electronics
- 6. Need high‐bandwidth readout & DAQ
25 16 Dec. 2010
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Cavern: to be sited at 800‐o level, w/ drive‐in access
26 16 Dec. 2010
Ross Shaft Ramp From 300L to 800L Existing 800 Level Yates Shaft LArTPC Cavern 1 Existing 300 Level Kirk Portal LArTPC Cavern 2 Utility Shafts To Surface
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Layout of the proposed cavern
27 16 Dec. 2010
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
LAr20 Module ConfiguraTon
28 16 Dec. 2010
Key Elements:
1) 16m x 15m x 74m of LAr in vessel: 25 kt (total), 17 kt (fiducial) 2) 2.47 m maximum drio: 123 kV on cathodes 1.6 mm/µs max drio Tme 1.6 ms 3) Aim for < 0.2 ppb O2 contaminaTon: ensures e lifeTme > 1.4 ms 4) 3 R/O planes: verTcal (coll.), +/‐ 45o (ind.) wire pitch 3.0 mm (Y) / 3.3 mm (U,V) 5) Segmented as “Anode Plane Assemblies”: 3840 readout wires per APA x 3 x 2 x 28 = 645k channels, sampled @ 2 Msps
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
“Membrane Cryostat”
inspired by LNG Tanker Ships…
29 16 Dec. 2010
Person scale
Source: GTT & Russ Rucinski
Membrane Cryostat for LNG ship tanker. This tank is 35 m high x ~45 m wide, 40,000 m3. LAr20 will be 15 m high x 16 m wide x 74 m long = 19,000 m3.
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Cryostat Structure/ InsulaTon
30 16 Dec. 2010
- Key Elements
- Cavity drain
- Shotcrete
- Concrete liner
- Steel roof
- HeaTng system
- Vapor barrier
- InsulaTon
- Secondary barrier
- Primary membrane
Source: ARUP
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
TPC Assembly in the Cryostat
31
70m 14m 2.5m
168 APAs 224 CPAs Total weight: ~70 tons
Source: Bo Yu 16 Dec. 2010
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Anode Plane Assembly (APA)
7mx2.5m, stainless steel construcTon, 250kg 4 planes of wires @ 3mm pitch 3840 sense wires, 5520 wires total Electronics on one end of the frame
Source: Bo Yu 16 Dec. 2010 32
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Front‐end electronics
33 16 Dec. 2010
Low‐power, low‐noise CMOS ASIC, designed for operaTon in LAr – work by BNL ASIC group in collaboraTon w/ other experts at
Ga Tech on “hot carrier” effects
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Cryogenics System Overview
- LAr System
– Deliver liq. Argon from 300’ level cryopiping – Circulate to purify: 4 x 600 liter/min submersible pumps. Use one during operaTon: ~1.2 kt exchanged per day. – Pump out to 300’ level if needed
- GAr System
– 5 W/m2 heat load + pumps + electronics 45 kW boil‐off = 24 tons/day (0.1%) recondense/repurify – RefrigeraTon/Heat exchange system (w/ LN2 ?)
34 16 Dec. 2010
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
LAr20: Issues & QuesTons
- Cavern / Membrane Cryostat issues
– Heat loss into cryostat freezing of rock will install heaTng elements – Nominally no evacuaTon of interior volume to eliminate contaminants (though not impossible). LAPD (see M. Soderberg talk) will test purity quesTons.
- Auxiliary detector systems
– LAr20 is self‐shielding, and CR muon rate into detector is low (~100 Hz), but… – Adding CR veto system in surrounding rock would protect against neutrals, produced in CR muon interacTons, entering and mimicking, e.g., p K ν – Adding scinTllaTon/cherenkov photon detecTon capability would enhance
- verall performance. What should this look like?
- DemonstraTon of constructability
– 800 ton prototype planned for construcTon at FNAL
35 16 Dec. 2010
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Near Detector Reference ConfiguraTon
36 16 Dec. 2010
70‐ton LArTPC (MicroBooNE‐like) MagneTzed straw‐tube tracker, and calorimeter/muon range stack
Alternate configuraTons also under consideraTon.
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Summary
- Reference conceptual designs for LBNE beam and detectors are well
advanced
– Much engineering effort invested already – These systems appear technically feasible
- The physics arguments for realizing LBNE are strong
– See, e.g., previous talks by L. Whitehead and B. Rebel – The case grows stronger in proporTon to detector mass and beam power
- Many interesTng challenges lie ahead
- Lots of room for new, creaTve ideas on all fronts
37 16 Dec. 2010
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Backup Slides
38 16 Dec. 2010
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
WCD Deck ConfiguraTon
39 16 Dec. 2010
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Access to 800L LAr Cavern via Kirk Portal @ 300L
16 Dec. 2010 40
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Source: ARUP
Plan view of LAr20 cryostat & cavern at 800L
16 Dec. 2010 41
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
LAr20 Cryostat Parameter List
Parameter Value Total Volume 18,500 m3 LAr Total Mass 25 kton Inner/Outer Height of Tank 16 m/19 m Inner/Outer Width of Tank 16 m/19 m Inner/Outer Length of Tank 74 m/77 m Inner Liner Thin membrane stainless steel InsulaTon Reinforced Polyurethane; Inner layer 30 cm,
- uter layer 70 cm
Secondary Containment 0.07 mm thick aluminum between fiberglass cloth. Overall thickness is 0.8 mm located between insulaTon layers Outer Concrete Layer 0.5 m thick, inner surface treated with vapor barrier
16 Dec. 2010 42
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Cryostat Parameter List
– cont’d
Parameter Value LAr Temperature 89 K Depth of the Liquid (Liquid Head) 15.0 m Design OperaTng Pressure (Above Liquid) 0.113 MPa Design OperaTng Pressure (Bo|om of Liquid) 0.316 MPa Rated Pressure Capacity of Tank 0.52 MPa (calculated according to BS EN 14620)
16 Dec. 2010 43
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Cryostat
16 Dec. 2010 44
- GTT system
- Onshore / floaTng LNG storage
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
On the freezing of cavern wall
(Glen Morgan, LBNE docdb‐120)
- Without heaters, rock surface freezes in ~5 months.
16 Dec. 2010 45
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
Channels: up to 700,000 Chips: ~ 65,000 (assume > 90% yield, > 15% spares) Technology: CMOS 0.18µm (a main stream, available Tll 2020) mask cost $ 210k, wafer cost $2.2k; packaging cost $ 1.75 each FabricaTon cost esTmate: chips per wafer: ~ 330 (6/ret.) number of wafers: ~ 200 Total cost: 210k$ + 2.2k$×200 + $1.75×65k ≈ 760 k$ Cost per channel: ≈ 0.7 $
14 x 20 package (cavity 11x13)
requirement challenge status Low‐noise front‐end
ENC < 1000e‐ at 200pF ~ 5mW, 300fC range moderate‐high ASIC fabricated, being tested
ADC
12‐bit, 2MS/s, ~ 4mW moderate‐high design in progress
Design
reliable models at 90K low structures fabricated, being tested
Life<me
> 20 year operaTon at 90K low structures to be fabricated
LAr20 Front‐end ASIC
(slide courtesy H. Chen, BNL)
16 Dec. 2010 46
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
LAr20 Rate EsTmate Summary
47
Rates/data sizes of dominaTng processes – All numbers are per APA – Zero‐suppression assumed, unless noted otherwise – “Instantaneous data rates” are for 1.6ms Tmeframe – “Avg data rates” factors in rate for ‘rare’ processes
16 Dec. 2010
1 APA (out of 168) = 2.5m x 7m x (2 x 2.47m drio) = 119 tons LAr = 3840 wires x 3088 sample (@2 Msps)
Beam and Detectors for LBNE – J. Urheim, Indiana University – NNN10
LAr20 DAQ System Overview
48 16 Dec. 2010
Total: 168 APA’s
1 APA = 2.5m x 7m x (2 x 2.47m drio) = 119 tons LAr = 3840 wires x 3088 samples (@ 2 Msps)