Table of Contents
Luminosity Upgrade Projects Fermi National Accelerator LaboratoryDOE Annual ProgramReviewApril 1-3, 1997
Luminosity Formula
Outline
Run II Parameters
Run II Luminosity Goal2?1032 cm?? sec?1
How higherantiproton intensitywill be obtained
Antiproton Production
Beam SweepingYield versus Sweep Radius
Debuncher Cooling AIP
4-8 GHz Pickup R&D
4-8 GHz PickupE-Field Over Full Length
4-8 GHz PickupE-Field at a Slot
Stack Tail
Accumulator LatticeModification
Proton Source
Tevatron Modifications
Tevatron 1 TeV Upgrade(Possible Elements)
Proton Removal byScraping at E0
Need forBump Kicker Magnet
Need forShort Batch Kicker
Multi-bunchCoalescing Intensities
Reliability ModificationsIncluding Diagnostics
Controls Modifications
Critical Run II Issues
7 rf bucket Bunch Spacing & Crossing Angles
7 rf bucket spacing
The Need for a Crossing Angle
Luminosity vs Crossing Angle
Linear Beam-Beam Tune Shiftwith Crossing Angle Effect
Longitudinal Distribution of Vertices for ?*=0.5 m
Tune Spread0 ?rad Crossing Angle
Tune Spread100 ?rad Crossing Angle
Tune Spread170 ?rad Crossing Angle
Beam-Beam Tune Spread 100 ?rad Crossing Angle
Beam-Beam Tune Spread170 ?rad Crossing Angle
Beam-Beam InteractionConsiderations
Design for 7 rf bucket spacing
C0 Low Beta
C0 Low Beta(Continued)
C0 Low Beta(Continued)
C0 Low Beta Conceptual Design
C0 Low BetaMagnet Gradients
Goal of TeV33
Elements of TeV33
Elements of TeV33(Continued)
Antiproton Productionthe key to higher luminosity
Luminosity versus TimeFor a Nominal Store
Antiproton Intensityversus Time in a Store
Antiproton Requirements
Luminosity Leveling
Luminosity Leveling
Antiproton Production
Slip Stacking Cartoon
Slip Stacking Simulation
Debuncher Bunch Rotation
Slip Stackingrf Voltage & Frequency
Slip StackingBeam Loading Voltage
Slip Stacking Issues(in progress)
Yield versus Lens Field
Cooling Issues
Transverse Coolingin the Debuncher
Momentum Coolingin the Debuncher
TeV Dipole MagnetsQuench Currents
TeV33 Stack Tail System
Stacking in the Accumulator
Future Plans
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