Future Neutrino Beams at Fermilab
Gina Rameika NNN10 – Toyama, Japan December 14-16, 2010
Future Neutrino Beams at Fermilab Gina Rameika NNN10 Toyama, - - PowerPoint PPT Presentation
Future Neutrino Beams at Fermilab Gina Rameika NNN10 Toyama, Japan December 14-16, 2010 Outline Neutrinos and the Intensity Frontier Neutrino Beams at Fermilab Booster Neutrino Beam (BNB) : MiniBooNE NuMI : MINOS, MINERvA
Gina Rameika NNN10 – Toyama, Japan December 14-16, 2010
future expt.
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MINOS MiniBooNE MINERvA SeaQuest NOvA MicroBooNE g-2? SeaQuest Now 2016 LBNE Mu2e Project X+LBNE mu, K, nuclear, … Factory ?? 2013 2019 2022
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to go in the desired direction
neutrinos
neutrinos or anti-neutrinos are (predominantly) generated
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Short baseline – Near surface
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e e /µ
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Depends on other demands for the protons
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Energy configuration)
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second cycle
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cycle 5 Hz from Booster 7.8e16/hour 9 Hz from Booster 1.4e17/hour
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Primary Beamline Horn Power Supply
Target Pile Air Cooling System
(above shielding)
Target & Baffle Work Cell
(above shielding)
Horn 1 Horn 2 Low Energy Configuration
Stripline
Horn
Configuration
Morgue
NuMI Design
NOvA†
Beam Power (kW)
400 700
Energy Spectrum Low Energy Medium Energy Cycle time (s)
1.87 1.33
Intensity (ppp)
4.0×1013 4.9×1013
Spot Size (mm)
1.0 1.3
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Aperture Increased from 11 mm to 13 mm diameter Alternative Clamp Material
No Remote Longitudinal Motion Larger Target Casing Same Graphite Material, but wider target fins
No Remote Longitudinal Motion Simpler Construction
Thinner Outer Conductor Modified Stripline Geometry Additional Spray Cooling
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and the efficiency need to be maximized
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Hardware capable of ~9 Hz
aperture improvements and loss reduction
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hr at peak power
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Booster performance near NOvA levels (at peak)
question and is not accounted for in the extrapolation
years?
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additional improvements
Booster Solid State Upgrade
Improved reliability of RF Power Amplifiers
Increase repetition rate to 15 Hz
Improved electrical infrastructure Improved cooling for RF cavities Requires solid state upgrade
New shielding assessment and associated shielding improvements
Operational limits Additional shielding in tunnel Office occupancy
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efficiency of the Booster complex will be required if the currently approved physics program is to be successful
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(GeV)
!
E 1 10 POT
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CC evts/GeV/100kT/10
!
! 1000 2000 3000 4000 5000 6000 7000 8000 9000 10000
2
= 2.5e-03 eV
31 2
m " CC spectrum at 1300km,
!
! Appearance Probability 0.01 0.02 0.03 0.04 0.05 0.06 0.07 0.08 0.09 0.1
/2 # =
cp$ = 0.02,
13% 2
2sin =0
cp$ = 0.02,
13% 2
2sin
/2 # =-
cp$ = 0.02,
13% 2
2sin
= n/a
cp
$ =0,
13
% 2
2
sin (GeV)
!
E 1 10 POT
21
CC evts/GeV/100kT/10
!
! 1000 2000 3000 4000 5000 6000 7000 8000 9000 10000
2
= -2.5e-03 eV
31 2
m " CC spectrum at 1300km,
!
! Appearance Probability 0.01 0.02 0.03 0.04 0.05 0.06 0.07 0.08 0.09 0.1
/2 # =
cp$ = 0.02,
13% 2
2sin =0
cp$ = 0.02,
13% 2
2sin
/2 # =-
cp$ = 0.02,
13% 2
2sin
= n/a
cp
$ =0,
13
% 2
2
sin
s
e
50 100 150 200 250 300 350 400
e
20 40 60 80 100 120 140 160 180 200
=1.
s
e
50 100 150 200 250 300 350 400
e
10 20 30 40 50 60 70 80 90 100
=1.
sin2 2θ13 = 0.08,0.04,0.02,0.01
sin2 2θ13 = 0.04
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neutrino program
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20x1020 POT/yr 10x1020 POT/yr : not current plan 6 - 7x1020 POT/yr 3x1020 POT/yr
NuMI to MINOS
ProjectX