The High-Emittance Muon Collider
David Neuffer
June 2009 Low Emittance Muon Collider Workshop Preview
1
Outline
Introduction
Motivation
Scenario Outline and Features
Parameters Proton Driver Front End Accelerator Collider
Upgrade Path(s)
to Low-Emittance Muon Collider
2
Motivation- E. Eichten
3
Other physics
Higgs at high energy
ζ ≈ 0.6pb
0.01 fb-1 is 1030 for 107s
need more to sweep nearby energy
First SuperDimensional DarkMatterEnergy HyperSymmetric Particle??
ζ > pb !!
4
2A
2 TeV
5
HEMC Parameters
Proton Linac 8 GeV
Parameter
Proton Beam Power Bunch frequency Protons per bunch Proton beam energy Number of muon bunches +/-/ bunch
Symbol
Pp Fp Np Ep nB N
Value
2.4 MW 60 Hz 3×1013 8 GeV 12 1011
Accumulator, Buncher Hg target
Drift, Bunch, Cool
Transverse emittance
t,N
* * x,y x,y max E+,E_ Nt L0
0.003m
0.05m 10000m 0.013cm 0.55cm 5.4cm 1 TeV (2TeV total) 1000 4×1030
6
Linac RLAs
Collision * Collision max Beam size at collision Beam size (arcs) Beam size IR quad Collision Beam Energy Storage turns
Collider Ring
Luminosity
Proton Driver
Proton Driver is variant of Project X
Other variations possible 8 GeV at Fermilab 1.2×1014/cycle Drift, Bunch, Cool Proton Linac 8 GeV Accumulator, Buncher
8 GeV SRF linac , 15 Hz
Hg target
Accumulate, Bunch to form 4 bunches
3×1013/bunch
extract at 60Hz
• •
εN6π =120π mm-mrad, BF = 0.005 2 2 B F N δν = 0.4
3 rp N tot
Linac RLAs
Detector
Collider Ring
7
Solenoid lens capture
Target is immersed in high field solenoid Particles are trapped in Larmor orbits
B= 20T -> ~2T Particles with p < 0.3 BsolRsol/2=0.225GeV/c are trapped
π→μ Focuses both + and – particles
Drift, Bunch and phase-energy rotation
p
8
High-frequency Buncher and φ-E Rotator
Drift (π→μ) “Adiabatically” bunch beam first (weak 320 to 240 MHz rf) Φ-E rotate bunches – align bunches to ~equal energies
240to 202 MHz, 15MV/m
Cool beam
p
201.25MHz
π→μ
FE Targ Solenoid et 10 m
Drift
~50 m
Buncher
~30m
Rotator
36m
Cooler ~80 m
9
Adiabatic Buncher; φ-E rotation
Set rf phase to be zero for reference energies
Spacing is N rf rf increases gradually increase rf gradient
Match to rf= ~1.5m at end:
After bunching rephase rf so that higher energy bunches accelerate, low energy bunches
Finish when bunch energies are aligned in E
Transfer to cooling
Captures both μ+ and μ born from same proton bunch Example: rf : 0.901.5m
10
Bunch train for Collider
Drift, buncher, rotator to get “short” bunch train (nB = 10):
217m ⇒ 125m 57m drift, 31m buncher, 36m rotator Rf voltages up to 15MV/m (×2/3) At < 0.03, AL <0.2 Choose best 12 bunches
Obtains ~0.1 μ/p8 in ref. acceptance
3 × 1013 protons
• •
~0.008 μ/p8 per bunch ~0.005 μ/p8 in acceptance
1.5× 1011 μ/bunch in acceptance εt,rms, normalized ≈ 0.003m (accepted μ’s) εL,rms, normalized≈ 0.034m (accepted μ’s)
11
Simulations (NB=10)
s = 1m s = 89m
Drift and Bunch
Rotate
500 MeV/c
s = 125m
s = 219m
Cool
0 -30m 12
30m
HEMC collider bunches
Scenario is unoptimized
~60% of μ’s in best 12 bunches ~75% in best 16
13
Acceleration-RLA’s ?
244 MeV
300 m 160 m
1.8 GeV
A. Bogacz – Dogbone RLAs
1.2 GeV/pass
7.2 GeV
528 m
32.5GeV 5 GeV/pass
Dogbone RLA II example
7 pass
Ef
E0
= 30
Beam is probably too big for 1300MHz. 800 MHz - OK
32.5 GeV
1000 GeV Linac 140 GeV/pass
Dogbone geometry is long.
(140 GeV @20MV/m is 7km.) Racetrack is more compact.
14
Collider Ring
12 bunches of μ+ and μ 1011 μ/bunch
β* = 3 to 10 cm
ζ= 0.01 to 0.016cm
βmax = 10000m
ζ=5.5cm (1TeV) IR quads are large aperture (20cm radius) δE ~0.12 GeV if ζz = 3cm δE/E = 10-4 Δν=0.000036
εL =0.012 eV-s
Collider is not beam-beam limited
beam beam
N r 4 p N , rm s
15
Upgrade path
More cooling
εt,N→ 0.0005, β*→1cm L→1032
Bunch recombination
12→1 L →1033
More cooling
low emittance εt,N→ 0.00003, β*→0.3cm L→1034
More Protons
2.4→5MW or more L→1035
16
Conclusions
An Initial Muon Collider (0.5 to 4 TeV) with low luminosity could be constructed, particularly if motivated by a clear physics goal. Uses trains of μ+ and μ- bunches for acceleration and storage (~ 20m trains)
L= ~4×1030 cm-2s-1 needs little cooling does need front end (captures both μ+ and μ-)
Could be upgraded to high-luminosity
more cooling smaller β* bunch recombination
17
First μ Collider may not be perfect …
18