LowEnergy Ionization Cooling - PowerPoint PPT Presentation

1 / 31
About This Presentation
Title:

LowEnergy Ionization Cooling

Description:

Combining Cooling and Heating: Low-Z absorbers (H2, Li, Be, ... C. Rubbia, Ferrari, Kadi, Vlachoudis source of ions for -beams. 5. Cooling/Heating equations ... – PowerPoint PPT presentation

Number of Views:57
Avg rating:3.0/5.0
Slides: 32
Provided by: david1379
Category:

less

Transcript and Presenter's Notes

Title: LowEnergy Ionization Cooling


1
Low-Energy Ionization Cooling
  • David Neuffer
  • Fermilab

2
Outline
  • Low-energy cooling-protons
  • ions and beta-beams
  • Low-energy cooling muons
  • emittance exchange

3
Combining Cooling and Heating
  • Low-Z absorbers (H2, Li, Be, ) to reduce
    multiple scattering
  • High Gradient RF
  • To cool before ?-decay (2.2? ?s)
  • To keep beam bunched
  • Strong-Focusing at absorbers
  • To keep multiple scattering
  • less than beam divergence
  • ? Quad focusing ?
  • ? Li lens focusing ?
  • ? Solenoid focusing?

4
Low-energy cooling of ions
  • Ionization cooling of protons/ ions has been
    unattractive because nuclear reaction rate is
    competitive with energy-loss cooling rate
  • And other cooling methods are available
  • But can have some value if the goal is beam
    storage to obtain nuclear reactions
  • Absorber is also nuclear interaction medium
  • Y. Mori neutron beam source
  • NIM paper
  • C. Rubbia, Ferrari, Kadi, Vlachoudis source of
    ions for ß-beams

5
Cooling/Heating equations
  • Cooling equations are same as used for muons
  • mass a mp, charge z e
  • Some formulae may be inaccurate for small ßv/c
  • Add heating through nuclear interactions
  • Ionization/recombination should be included
  • For small ß, longitudinal dE/dx heating is large
  • At ß 0.1, gL -1.64, ?g 0.36
  • Coupling only with x cannot obtain damping in
    both x and z

0.0
1.0
3.0
5.0
bg
6
µ Cooling Regimes
  • Efficient cooling requires
  • Frictional Cooling (lt1MeV/c) Sg3
  • Ionization Cooling (0.3GeV/c) Sg2
  • Radiative Cooling (gt1TeV/c) Sg4
  • Low-et cooling Sg2ß2
  • (longitudinal heating)

7
Miscellaneous Cooling equations
For small ß
Better for larger mass?
8
Example
  • ERIT-P-storage ring to obtain directed neutron
    beam (Mori-Okabe, FFAG05)
  • 10 MeV protons
  • 9Be target for neutrons
  • s 0.5 barns
  • ß v/c 0.145
  • Large dE heating
  • Baseline Absorber
  • 5µ Be absorber
  • dEp36 keV/turn
  • Design Intensity
  • 1000Hz, 6.51010p/cycle
  • 100W primary beam
  • lt 1.5 kW on foil
  • 0.4 kW at nturns 1000

9
ERIT results
  • With only production reaction, lifetime is 30000
    turns
  • With baseline parameters, cannot cool both x and
    E
  • Optimal x-E exchange increases storage time from
    1000 to 3000 turns (3850 turns 1ms)
  • With x-y-E coupling, can cool 3-D with gi 0.12
  • Cooling time would be 5000 turns
  • With ß?0.2m, ?dErms 0.4MeV, ??,N 0.0004m
    (xrms2.3cm)
  • xrms 7.3cm at ß?2m (would need r 20cm arc
    apertures)
  • (but 1ms refill time would make this
    unnecessary)

10
3-D mixing lattice
  • For 3-D cooling, need to mix with both x and y
  • Possible is Moebius lattice (R. Talman)
  • Single turn includes x-y exchange transport
  • solenoid(s) or skew quads
  • in zero dispersion region for simplicity
  • Solenoid BL p B?
  • For 10 MeV p BL 1.44T-m
  • Complete period is 2 turns

11
Emittance exchange parameters
  • with gL,0 -1.63, ? 0.5m,
  • need G 3.5 to get gL0.12
  • (LW 0.3m)

12
Wedge for thin foil
  • Obtain variable thickness by bent foil (Mori et
    al.)
  • Choose x00.15m, LW0.3, do5µ
  • then a0.15, dR2.5
  • for gL,0 -1.63, ? 0.5m
  • Barely Compatible with ß 0.2m
  • Beam energy loss not too large?
  • lt1kW Power on foil

Beam
a0.15
13
Other heating terms
  • Mixing of transverse heating with longitudinal
    could be larger effect (Wang Kim)

At ERIT parameters ßx 1.0m, ßz 16m, ?0.6m, Be
absorber, dd2/ds 0.00032, d?2/ds 0.0133 only
5, 1.5 changes At ßx 0.2m, 25 change
14
Beta beams for neutrinos (Zuchelli)
  • Number of possible sources is limited (v sources
    easier)
  • Want
  • lifetime 1s
  • large ?-energy
  • ? and ?
  • easily extracted atoms
  • Noble gases easier to extract
  • 6He2 easiest E? 1.94MeV
  • 18Ne10 for ? E? 1.52MeV
  • Noble gas
  • (8B, 8Li) have E ? ,? 7MeV
  • Want 1020 ? and ? / year

v-sources
?-sources
15
ß-beam Scenario
Ion production
Acceleration
Neutrino source
Experiment
Ion Driver 25MeV Li ?
Acceleration to final energy Fermilab Main
Injector
Ion production Target - Ion Conversion Ring
Neutrino Source Decay Ring
Beam preparation ECR pulsed
Decay ring Br 400 Tm B 5 T C 3300
m Lss 1100 m 8B g 80 8Li g 50
Ion acceleration Linac
8z GeV/c
Acceleration to medium energy RCS
16
ß-beam Scenario (Rubbia et al.)
  • Produce Li and inject at 25 MeV
  • Charge exchange injection
  • nuclear interaction at gas jet target produces
    8Li or 8B
  • Multiturn with cooling maximizes ion production
  • 8Li or 8B is caught on stopper(W)
  • heated to reemit as gas
  • 8Li or 8B gas is ion source for ß-beam accelerate
  • Accelerate to B? 400 T-m
  • Fermilab main injector
  • Stack in storage ring for
  • 8B?8Be e? or 8Li?8Be e- ? neutrino
    source

17
Cooling for ß-beams (Rubbia et al.)
  • ß-beam requires ions with appropriate nuclear
    decay
  • 8B?8Be e ?
  • 8Li?8Be e- ?
  • Ions are produced by nuclear interactions
  • 6Li 3He ? 8B n
  • 7Li 2H ? 8Li 1H
  • Secondary ions must be collected and
    reaccelerated
  • Either heavy or light ion could be beam or target
  • Ref. 1 prefers heavy ion beam ions are produced
    more forward (reverse kinematics)
  • Parameters can be chosen such that target cools
    beam
  • (losses and heating from nuclear interactions,
    however)

18
ß-beams example 6Li 3He ? 8B n
  • Beam 25MeV 6Li
  • PLi 529.9 MeV/c B? 0.59 T-m v/c0.09415
  • Absorber3He
  • Z2, A3, I31eV, z3, a6
  • dE/ds 110.6 MeV/cm, LR756cm
  • at (?He-3 0.09375 gm/cm3)Liquid, (?He-3
    0.13410-3P gm/cm3/atm in gas)
  • dE/ds 1180 MeV/gm/cm2, LR 70.9 gm/cm2
  • If gx 0.123 (Sg 0.37), ß- 0.3m at
    absorber
  • eN,eq 0.000046 m-rad
  • sx,rms 1.2 cm at ß- 0.3m,
  • sx,rms 3.14 cm at ß- 2.0m
  • sE,eq is 0.4 MeV
  • ln 5.68,
  • energy straggling
  • underestimated?

19
Cooling time/power 6Li 3He ? 8B n
  • Nuclear cross section for beam loss is 1 barn
    (10-24 cm2) or more
  • s 10-24cm2,corresponds to 5gm/cm2 of 3He
  • 10 3-D cooling e-foldings
  • Cross-section for 8B production is 10 mbarn
  • At best, 10-2 of 6Li is converted
  • Goal is 1013/s of 8B production
  • then at least 1015 Li6/s needed
  • Space charge limit is 1012 6Li/ring
  • Cycle time is lt10-3 s
  • If C10m, t 355 ns, 2820 turns/ms
  • 5/28201.77310-3 gm/cm2 (0.019 cm _at_ liquid
    density )
  • 2.1 MeV/turn energy loss and regain required
    (0.7MV rf)
  • 0.944 MW cooling rf power

20
ß-beams example 7Li 2H ? 8Li 1H
  • Beam 25MeV 7Li
  • PLi 572 MeV/c B? 0.66 T-m v/c0.0872
  • Absorber2H
  • Z1, A2, I19eV, z3, a7
  • dE/ds 184.7 MeV/cm, LR724cm
  • at (?H-2 0.169 gm/cm3)Liquid, (?H-2 0.17910-3P
    gm/cm3/atm in gas)
  • dE/ds 1090 MeV/gm/cm2, LR 70.9 gm/cm2
  • If gx 0.123 (Sg 0.37), ß- 0.3m at
    absorber
  • eN,eq 0.000027 m-rad
  • sx,rms 1.0 cm at ß- 0.3m,
  • sx,rms 2.5 cm at ß- 2.0m
  • sE,eq is 0.36 MeV
  • ln 6.0,
  • Easier than 8B example ?

21
Cooling time/power- 7Li 2H ? 8Li 1H
  • Nuclear cross section for beam loss is 1 barn
    (10-24 cm2) or more
  • s 10-24cm2,corresponds to 3.3gm/cm2 of 2H
  • 9 3-D cooling e-foldings
  • Cross-section for 8Li production is 100 mbarn
  • 10-1 of 7Li is converted ?? 10 better than
    8B neutrinos
  • Goal is 1013/s of 8Li production
  • then at least 1014 Li7/s needed
  • Space charge limit is 1012 7Li/ring
  • Cycle time can be up to 10-2 s, but use 10-3s
  • If C10m, t 355 ns, 2820 turns
  • 3.3/28201.210-3 gm/cm2 (0.007 cm _at_ liquid
    density )
  • 1.3 MeV/turn energy loss and regain required
    (0.43MV rf)
  • 0.06 MW cooling rf power

22
Space charge limitation
  • At N 1012, BF 0.2, ß0.094, z3, a6, eN,rms
    0.000046
  • d? 0.2
  • tolerable ??
  • Space charge sets limit on number of particles in
    beam

23
Inverse vs. Direct Kinematics
  • 6Li3 beam 3He2 target
  • 25 MeV Li
  • gas-jet target
  • tapered nozzle for wedge?
  • product is 8B
  • 8 to 23 MeV
  • Stop in Tantalum absorber
  • penetrates more (5 to 12µ)
  • ? lt14.5
  • Beam divergence 6 (2.5s)
  • Boil out to vapor
  • neutralize to vapor, extract, ionize, accelerate
  • 100 efficiency
  • 3He2 beam 6Li3 target
  • 12.5 MeV He beam
  • Li foil target (or liquid waterfall?)
  • fold to get wedge
  • product is 8B
  • 1 to 8 MeV
  • Stop in Tantalum absorber
  • penetrates less (2 to 5µ)
  • ? lt30
  • Beam divergence is 10 (2.5s)
  • Boil out to vapor

24
X-sections, kinematics
25
Rubbia et al. contains errors
  • Longitudinal emittance growth 2 larger than his
  • synchrotron oscillations reduce energy spread
    growth rate but not emittance growth rate
  • Emittance exchange with only x does not give 3-D
    cooling need x-y coupling and balancing of
    cooling rates
  • Increases equilibrium emittance, beam size
  • increase needed for space charge, however
  • Includes z2 factor in dE/dx but not in multiple
    scattering,

26
Low-Energy cooling-emittance exchange
  • dPµ/ds varies as 1/ß3
  • Cooling distance becomes very short
  • for liquid H at
    Pµ10MeV/c
  • Focusing can get quite strong
  • Solenoid
  • ß?0.002m at 30T, 10MeV/c
  • eN,eq 1.510-4 cm at 10MeV/c
  • Small enough for low-emittance collider

100 cm
Lcool
0.1 cm
200 MeV/c
10

27
Emittance exchange solenoid focusing
  • Solenoid focusing(30T)
  • ??? 0.002m
  • Momentum (30?10 MeV/c)
  • L 5cm
  • R lt 1cm
  • Liquid Hydrogen (or gas)

Lcool
  • eN,eq 1.010-4 cm at 10MeV/c, 50T

0.1cm
Use gas H2 if cooling length too short
-Will need rf to change ?p to ?z
200 MeV/c
10

28
Gas absorbers
  • With gas absorbers can adjust energy loss rate
  • avoid beam loss

29
????? Collider Parameters
30
Summary
31
ß-beams alternate 6Li 3He ? 8B n
  • Beam 12.5MeV 3He
  • PLi 264 MeV/c B? 0.44 T-m v/c0.094
  • Absorber 6Li
  • Z3, A6, I43eV, z2, a3
  • dE/ds 170 MeV/cm, LR155cm
  • at (?Li-6 0.46 gm/cm3)
  • Space charge 2? smaller
  • If gx 0.123 (Sg 0.37), ß- 0.3m at
    absorber
  • eN,eq 0.000133m-rad
  • sx,rms 2.0 cm at ß- 0.3m,
  • sx,rms 5.3 cm at ß- 2.0m
  • sE,eq is 0.3 MeV
  • ln 5.34
Write a Comment
User Comments (0)
About PowerShow.com