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Long-Baseline Neutrino FacilityLBNF
LBNF MARS Modeling for Optimized
Beamline
Nikolai Mokhov
Beam Optimization Review - FNAL
October 5-6, 2017
LBNF
Outline
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization2
• Target Station
• Decay Channel and DS Window at Normal Operation
• Hadron Absorber at Normal Operation
• Beam Accidents
MARS LBNF Modeling Team:
N. Mokhov, I. Rakhno, D. Reitzner, S. Striganov and I. Tropin
LBNF
e95 = 20p mm-mrad, Np = 1.5×1014 pppBeam starts at z = -7.3 m from MC0, tilt = 0.101074
N. Mokhov | MARS Modeling for Beamline Optimization3
Scenarios & Beam Parameters
Scenario Ep (GeV) P (MW)Q (MJ)
s0 (mm)at MC0
b0 (m)at MC0
Cycle (s) × 1014
Normal 120 2.40 MW 1.7 110.8837 1.2 1.25 p/s
No-targetaccident*
120 2.88 MJ 2.4 221.03 1.2 1.5 ppp
Off-axis accident**
120 2.88 MJ 2.4 221.03 1.2 1.5 ppp
Normal 60 2.06 MW 1.7 55.44 0.7 2.14 p/s
*) On-axis
**) Beam points to absorber cooling water pipes
10/05/2017
LBNF
Target Station Configurations
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization4
Reference Design 2016 (RD)95-cm target, first 6 cm winged
2 NuMI-type horns, Air
Optimized Design 2017 (OD)198-cm target, first 12 cm winged,
3 optimized horns, Nitrogen
LBNF
Longer Target with Winged Fins at Upstream End
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization5
AirAl
Ti
He
Air
• In RD, 0.3% of beam miss targetentirely, giving 0.9-cm RMSon absorber (7 kW) addwinged fins on target upstream,6-cm (RD) and 12-cm (OD) long,to lower the peak EDEP
• In RD, 13% of proton beam do notparticipate in inelastic nuclearinteractions with target,experiencing just Coulomb andnuclear elastic scattering. Latterresults in a 4.9-cm RMS footprinton absorber(~300 kW) maketarget longer to lower pedestaland total power on absorber
Lines - analytical
LBNF
EDEP in Optimized Target/Horns (1)
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization6
Horn A Horn B Horn C
Energy Deposition (GeV/cm3/pot) vs longitudinal position (cm) in horn IC
0 50 100 150 200 250Position Along IC (cm)
0.0
0.5
1.0
1.5
2.0
2.5
ED
EP
(G
eV
/cm
3/p
) (
10
-3) Horn A IC
0 100 200 300 400Position Along IC (cm)
0.0
0.5
1.0
1.5
2.0
2.5
ED
EP
(G
eV
/cm
3/p
) (
10
-4) Horn B IC
0 50 100 150 200 2500 50 100 150 200 250Position Along IC (cm)
0.5
1.0
1.5
2.0
2.5
3.0
3.5
0.5
1.0
1.5
2.0
2.5
3.0
3.5
ED
EP
(G
eV
/cm
3/p
) (
10
-5) Horn C IC
LBNF
0 100 200 300 4000 100 200 300 400Position Along IC (cm)
2.1
2.2
2.3
2.4
2.5
2.6
2.7
2.8
2.9
2.1
2.2
2.3
2.4
2.5
2.6
2.7
2.8
2.9
ED
EP
Ratio
(12
0G
eV
/60G
eV
)
EDEP in Optimized Target/Horns (2)
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization7
Target tube: R=2.5cm, Ti
120GeV/60GeV Ratio
2.8 at peak
Horn B IC
Energy Deposition (GeV/cm3/pot)
-50 0 50 100 150 200 250-50 0 50 100 150 200 250Position Along Target Tube (cm)
0
1
2
3
4
5
0
1
2
3
4
5
ED
EP
(G
eV
/cm
3/p
) (
10
-3)
OD
~RD
OD/RD ~2 at peaks
Target tube
LBNF
EDEP (r) in US Decay Pipe Window: 120 vs 60 GeV
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization8
Transition from AlBeMet to Al (thinner bin)
LBNF
EDEP (r) in US DK Window: Nominal vs Accident
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization9
Transition from AlBeMet to Al (thinner bin)
LBNF
EDEP in Target Station Cooling Panels
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization10
Floor Max: 4.9×10-6 GeV/cm3/p
T-Blocks Max: 6.0×10-6 GeV/cm3/p
MARS EDEP mapsprovided to ANSYS team
LBNF
Target Station Model: Extracting EDEP for FEA
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization11
Extracting new MARS15 EDEP results for FEA analysisEspecially for the shielding block / module / stripline block studies
Shielding block binning
Diane
LBNF
EDEP in Target Station Components
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization12
Component REF OPT OPT/REF
Target/horns 153.70* 193.84* 1.26
Steel blocks/elements 769.9 1,004.04 1.30
Concrete blocks 0.201 0.132 0.66
Miscellaneous 27.7 39.71 1.43
Total 951.5 1,237.72 1.30
Power dissipation (kW)
*) REF (OPT): Baffle – 0.42 (0.41), target fins -23.55 (44.45), other target components –5.62 (11.26), Horn1 – 79.66 (A: 47.42), Horn2 – 41.76 (B: 60.66, C: 26.64), tanks – 2.69 (3.00) kW
LBNF
Double-Walled Steel Decay Pipe EDEP vs DK
Length: Optimized Design
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization13
350 kW total over entire length
ANSYS analysis was already performed using this as input
LBNF
DK Concrete EDEP in First 50cm Radially vs DK
Length
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization14
EDEP maps for entire DK including DS window are available in DUNE-doc-3303-v2 for ANSYS analysis
LBNF
EDEP and Star Density in DK Concrete for OD
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization15
For heat load & ground-water activation analysesat two longitudinal maxima and DK-averaged
Design limit
LBNF
EDEP (kW/m3) in DK DS Steel Window and Frame
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization16
3.42-mm Steel window 12.7-mm Steel frame
The peak value at the beam axis:RD: 190 kW/m3 in 3.42-mm stainless steel
90 kW/cm3 in 6.35-mm aluminumOD: 45 kW/m3 in 3.42-mm stainless steel
The peak value in 12.7-mm steel frame:RD: 26.5 kW/m3 at r=55 cmOD: 24.0 kW/m3 at r=55 cm
Peak OD/RD = 0.24
LBNF
EDEP in DK and DS Stainless Steel Window
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization17
Element REF OPT OPT/REF
Double-walled steel decay pipe
291 350 1.20
Concrete 158.3 189.3 1.20
SS window 0.08 0.06 0.75
Steel frame 2.7 2.8 1.04
Total 452.08 542.16 1.20
Power dissipation (kW)
LBNF
Hadron Absorber Configurations
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization18
Ref. Hadron Absorber (RHA)Non-uniformity, sculpting needed for RDwith a 30% safety margin
Uniform Hadron Abs (UHA)No sculpting, larger uniform masks, largercore blocks (60”->67”), 1/16” windows on maskblocks, simpler cooling and interface to hadronmonitor with a large safety margin for OD
LBNF
Proton and Energy Flux at Hadron Absorber
System at Normal Operation
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization19
Total Power: 854 kW (RD)and 436 kW (OD) OD/RD = 0.50Peak: OD/RD = 0.17
Lines - analytical
Eth=115 GeV
LBNF
Power Density (mW/cm3) in Hadron Absorber
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization20
RD Peak: 1.6 W/cm3 Peak: 0.24 W/cm3OD
Thanks to longer target and longer wings in OD, instantaneous (EDEP)and accumulated (DPA) peaks are down by a factor of 6.7 and totalheat load is down by a factor of 2 (for normal operation ) !
LBNF
EDEP (mW/cm3) in Reference Hadron Absorber
for RD and OD Beams
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization21
Axial Lateral
LBNF
EDEP in Reference Hadron Absorber Components (OD)
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization22
No Component kW
1 Spoiler 47.52
2 Masks 1-5 139.42
3 Al sculpted blocks 60.58
4 Al solid blocks 7.07
5 Steel core blocks 1-4 3.78
6 Steel shielding 134.5
7 Concrete 2.7
8 Miscellaneous 4.0
9 Total 400.0
1
23
4 5 6
66
6
7
7
7
LBNF
2.4-MW LBNF EDEP (kW) in OD vs RD
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization23
System RD OD OD/RD
Target Station 951.5 1,237.7 1.30
Decay Channel 452.1 542.2 1.20
Hadron Absorber 786.0 400 0.51
4-p Neutrino power 66 69 1.05
Misc: infrastructure,binding energy & sub-threshold ptcls
144.4 151.1 1.05
Total 2400 2400
LBNF
DS DK Window, Hadron Monitor and Spoiler
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization24
Peak EDEP (J/cm3) per 1.5×1014 ppp no-target accident:80 3.42-mm stainless steel window48 Hadron monitor (aluminum)235 Spoiler downstream (aluminum)
LBNF
DK DS Window at Beam Accident: EDEP & DT
per 1.5×1014 ppp
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization25
sx = sy = 2.4 mm at the missed targetentrance3.42-mm Stainless Steel windowT0 = 27 0CPeak DT = 23 0C
LBNF
Summary
10/05/2017 N. Mokhov | MARS Modeling for Beamline Optimization26
• EDEP is well under control
• Hadron absorber system – EDEP, muon monitoring and radiological - is
under thorough optimization MARS calculations (uniform absorber etc.)
• The Optimized Design vs Reference Design: 30% n-flux improvement,
increase of heat and radiation loads in Target Station (30%) and Decay
Channel (20%), substantial mitigation of EDEP problems in Hadron
Absorber system
• Thorough search and elimination of differences in
MARS15LBNF and G4LBNF models were
performed (#3408): geometry, materials, magnetic
fields etc. n-fluxes at Far Detector calculated with
MARS15 and Geant4 now agree within 10%. The
code related uncertainties were reduced to the
differences in the event generators, especially for
K- and K0 mesons (need data!)