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Cooling Scenarios Recycler

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Both electron cooling (EC) and stochastic cooling (SC) are supposed to do the job. ... There is no Landau damping up to frequencies ... – PowerPoint PPT presentation

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Title: Cooling Scenarios Recycler


1
Cooling Scenarios _at_ Recycler
  • Alexey Burov
  • DOE Review
  • July 2003

2
Introduction
  • Recycler 3 km, 8.9 GeV/c, 40 p mm mrad ring for
    cooling and stacking of pbars from the
    Accumulator.
  • The goal is to stack (2-6)E12 pbars inside
    (100-30) eVs and (10-7) p mm mrad with flux
    (20-45)E10 pbars/hr (tougher numbers electron
    cooling goal).
  • Both electron cooling (EC) and stochastic
    cooling (SC) are supposed to do the job.
  • Requires
  • Good vacuum
  • Good MI shielding
  • Suppression of longitudinal IBS diffusion

3
Stochastic Cooling Only
  • Before EC gets functioning, what can be done with
    SC only?
  • SC (0.5-1)?(1-2) GHz for 2-4 GHz for ?.
  • Scenario
  • batches arrive from Accumulator every 3-4 hours
  • stacked longitudinally inside 100 eVs and
    cooled transversely against gas diffusion to be
    inside 10 p µm
  • IBS-driven longitudinal emittance growth is
    suppressed with proper bunching.
  • Modeling
  • Longitudinal Fokker-Planck equation where both
    friction and diffusion include SC and IBS terms.
  • Transverse SC gas diffusion equilibrium

4
Stochastic Cooling Only Results
  • Losses longitudinal (efficiency of coalescing in
    MI is a function of the initial phase space) and
    transverse (finite lifetime due to gas
    scattering).
  • Results
  • For as good vacuum as 4 µm/hr (eff. pressure only
    2x of Accumulator), and lt10 of total phase space
    dilution, MI can get 2E12 pbars in 36?3 eVs.
  • For 8 µm/hr, MI gets 1.4E12 pbars
  • Conclusion
  • With SC only (no EC), benefits of Recycler
    integration are marginal.

5
Longitudinal Distribution
  • Longitudinal evolution after the last injection
    (SC-IBS equilibrium).
  • Black before the injection, red just after,
    all other changes after every ¾ hour. The number
    of particles 3E12, the total time is 3 hours.

6
Efficiency of Coalescing in MI
Efficiency of coalescing, , as a function of
the initial phase space area (by I. Kourbanis).
7
S-Cooling, Gas Heating and Lifetime
dependence of the lifetime on the beam emittance
(by V. Lebedev)
8
E-Cool Tools Goals
9
Cooling Process
  • Every repetition interval, a new pbar batch is
    injected in RR.
  • The batch can be either kept separated from the
    accumulated stack for one more repetition
    interval, or immediately merged with the stack.
  • A reason for separation is batch transverse
    stochastic pre-cooling (BSC), which would make
    the following EC more effective. To make BSC
    faster, the batch phase space can be deliberately
    inflated. The goal for BSC is to make batch and
    stack emittances equal.
  • EC may be off for the batch.
  • After BSC, the batch is merged with the stack,
    and a new batch is injected on its place.
  • The stack is both e-cooled and s-cooled (?,
    gated, for tail pbars).
  • The stack is properly compressed , to suppress
    longitudinal IBS emittance growth (? IBS is weak
    for RR).
  • After the merger, the stack phase space is
    increased by the batch. EC has to cool it down to
    design value (30 eVs) for rep. time (1 hr).
  • Transverse EC acts against gas diffusion.
  • To prevent core over-cooling, e-beam can be
    deliberately misalign.

10
Cooling Simulations
  • The whole process is modeled by Monte-Carlo
    simulations.
  • SC cooling diffusion.
  • EC cooling rates are functions of 3 pbar actions
    for given e-beam parameters (current?length,
    radius, effective temperature).
  • EC rates have been analytically calculated by
    averaging of the friction power over pbar phases
    and e-beam angle distribution, assuming it
    Gaussian (5D integrals).
  • Two-stage simulation 1. BSC and 2. after-merger
    ECSC
  • IBS diffusion can be neglected for proper
    compression (checked by Bjorken-Mtingwa
    formulae).
  • Several scenarios are presented to show a space
    of possibilities.

11
IBS
  • (Phase space diffusion) ? (bunching)2 x
    (momentum diffusion).
  • With more compression, IBS diffusion goes down
    due to
  • bunching2
  • vz/vx gets closer to equilibrium (Fig. below with
    red as direct B-M calculation).

12
Small emittance, nominal e-current
13
Small emittance vacuum for e-current
14
Nominal emittance, nominal e-current
15
Nominal emittance vacuum for e-current
16
Space Charge and Coherent Instabilities
  • The space charge tune shift for max number of
    stacked pbars, small emittance scenario is as
    high as 0.08, which is not far from the
    conventional limit 0.10-0.15 .
  • There is no Landau damping up to frequencies
  • Thus, a broadband feedback up to SC lower
    frequency is required.
  • Growth time due to resistive wall is calculated
    as 300 turns at lowest frequency.

17
Conclusions
  • Pbar stacking goals require to be inside a
    certain volume in the space of parameters
    (vacuum, e-current, e-angles, s-cool, acceptance,
    ).
  • For moderately good vacuum
  • eff pressure 4x AA ? pencil beam lifetime
    200 hr
  • and good alignment
  • rms e-angle (1D) 0.2 mrad
  • e-current 0.5 A is sufficient.
  • For better vacuum, current requirements are
    reduced.
  • The stack bunching varies during cooling.
    E-current may be either DC or pulse with the same
    pattern.
  • For the same e-current, e-angles and vacuum, the
    stack emittance can be as any value between 3 and
    10 mm mrad.
  • Discussions with D. McGinnis and V. Lebedev were
    essential for this work.

18
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