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NuFACT07 Summer School Factory Front End and Cooling

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Force is perpendicular to motion , =v/c, P remain constant ... C. Rubbia, Ferrari, Kadi, Vlachoudis source of ions for -beams. Cooling/Heating equations ... – PowerPoint PPT presentation

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Title: NuFACT07 Summer School Factory Front End and Cooling


1
NuFACT07 Summer School?-Factory Front Endand
Cooling
  • David Neuffer
  • Fermilab

2
Beam Optics, Tutorial
  • Longitudinal Beam dynamics
  • Equations of motion
  • Discussion
  • Optics transverse dynamics
  • General introduction
  • Betatron functions
  • Focusing fields
  • Quadrupoles
  • Solenoids
  • Li lens, Magnetic horn
  • Cooling
  • Sample parameters
  • Cooling of ions

3
Basic Equations
  • Maxwells equations
  • Equation of motion
  • Transport/focusing uses magnetic fields
  • Dipoles, quads, solenoids,
  • Horns, Li lens,
  • Acceleration uses rf electric fields
  • rf cavities
  • Induction modules

4
Magnetic motion
  • Force is perpendicular to motion
  • ?, ßv/c, P remain constant
  • If v, B are perpendicular, motion is circular
  • m?v/q BR P/q is called the magnetic rigidity
    or B?
  • 1 GeV/c particle has B?109/c 3.33 T-m
  • Bending angle in magnet with field B, length L is
    ?BL/ B?

Bending radius
What is B? for a 300 MeV/c muon?
5
Homework problems
  • Target
  • How many 24 GeV protons per second are in a 4 MW
    beam?
  • PRISM
  • Homework rewrite equations of motion in F-dp
    units (ddp/p)

6
Longitudinal Beam Dynamics
  • Longitudinal equations of motion (????)

In dz-dE/mc2 units
7
Longitudinal motion stuff
  • Distance for oscillation
  • Adiabatic ( if L gt ?osc)
  • Longitudinal Cooling equations
  • Rf Bucket energy width

8
Betatron Functions
  • Assume focusing is linear around the orbit
  • Harmonic oscillator ( k(s))
  • Solution
  • where
  • Focussing forces
  • Quads kx(s) B(s)/B?
  • ky(s) - kx(s)
  • Solenoids k(s) (B/2B?)2
  • With x-y rotation
  • Need starting amplitude and derivative to specify
    motion
  • ßx(0), ßx'(0)
  • In periodic structure these are set by requiring
    that ßx(s) be periodic.

At equilibrium ßx (1/k)½
Exercise show that these equations are consistent
9
At a focus (with kx0)
To minimize beam heating Labsorber lt
ß? unless kx is non-zero
10
Solenoidal Focussing
  • Magnetic field
  • Cylindrical symmetry
  • Change to R-f notation
  • Solution is rotation in f, focussing in R

11
Comparison of focussing
  • Quadrupole
  • Focuses x or y
  • Proportional to 1/P
  • Solenoid
  • Focuses both x and y
  • Focuses both ? and ?-
  • Proportional to 1/P2
  • Solenoid better for low-energy
  • For B? lt Bo a (1 T-m ?)

12
Betatron function discussion
  • Beam optics typically described in terms of
    betatron functions
  • Use rms Emittance (beam phase space area)
  • Emittance also defined as
  • References are often unclear on whether
    normalized or normalized emittance is used also
  • Fermilab convention ?f 6p?rms
  • CERN convention ?CERN 4p?rms

13
Solenoidal lattices (with field flips)
  • Magnets used
  • FOFO lattice
  • Used in study 2A (B2.5T)
  • Produces constant focusing
  • ß? ? Lcell
  • Super FOFO
  • Used in study 2
  • Bmax ? 5.5T
  • Produces small ß? between strong coils
  • ß? ? 0.2m
  • Single flip, double flip
  • ß? ? 2 B?/B

14
Magnetic horn
  • Current along horn creates magnetic field B?
    outside surface (B0 inside)
  • Focussing field from Fr qvzB?
  • If horn profile is parabolic, ?z?r2, integrated
    force is linear
  • Focuses only one sign
  • S. van der Meer

NUMI horn 205 kA peak current 3.0 Tesla peak
field 2.6 milli-sec half-sine wave pulse 1.87 sec
repetition rate
15
Li-lens cooling
  • Lithium Lens provides strong-focusing and low-Z
    absorber in same device
  • Liquid Li-lens may be needed for highest-field,
    high rep. rate lens
  • BINP (Silvestrov) was testing prototype liquid Li
    lens for FNAL
  • But FNAL support was stopped - and prototypes
    were not successful ...

ß? 0.026m (200 MeV/c, 1000 T/m) ß? 0.004m (40
MeV/c, 8000 T/m)
16
Adiabatic damping and normalized emittance
  • Under acceleration
  • dx dpx remain constant (normalized emittance)
  • dx dx' dx dpx/p is proportional to (1/p)
  • geometric emittance decreases (beam size
    decreases)
  • Similarly,
  • dct dE remain constant
  • dz dp/p decreases as 1/p (acceptances set by
    dp/p)
  • Acceptances improve as beam is accelerated
  • Use higher-frequency rf, weaker transverse
    focusing

17
Cooling requirements
  • Set by acceptance of downstream accelerators and
    storage ring
  • Study 2 200MHz, Pµ 200MeV/c
  • ex,max lt 0.015m, ey,max lt 0.015m, ez, maxlt0.15m
  • xmax,, ymax lt 8.5cm (at ß?1m), zb lt 0.5m
  • ex,rms lt 0.06
  • Study 2A 200MHz, Pµ 200MeV/c
  • ex,max lt 0.03m, ey,max lt 0.03m, ez, maxlt0.15m
  • xmax,, ymax lt 12cm (at ß?1m), zb lt 0.5m
  • ex,rms lt 0.12
  • May change in future redesign

18
Homework Problem
  • 1300MHz Superconducting rf is cheap and
    available
  • Internal aperture is r3cm
  • Assume
  • 1300 MHz rf is used in 1m long cavities, with a
    quad magnet between cavities , 1.3 m half-cell
    (ß?,max 4m)
  • How small must the emittance be to allow muon
    acceleration ?
  • Require 2.5 ? aperture
  • Guesstimate an acceptable injection energy/
    cooled emittance
  • Redo exercise for 800MHz (r5cm)

19
Problem
  • Plug in some sample values for the cooling
    equations solve for ?t equilibrium and ?t(s)
  • try dE/ds 5 MV/m, p 300 MeV/c,
  • ?t 0.1m, Li absorbers ?N(0)0.01

20
Solution
  • Lithium density is 5/84.8 of solid

21
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

22
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

23
Example
  • ERIT-P-storage ring to obtain directed neutron
    beam (Mori-Okabe)
  • 10 MeV protons
  • 10Be target for neutrons
  • ? v/c 0.145
  • Large dE heating

24
RMS Cooling equations
For small ß
Better for larger mass?
25
Problem set
  • Use above discussion and equations to set up
    cooling constraints and possible parameters for
    Li6 cooling by He3.
  • Are the phase-space mixed heating terms greater
    than the direct terms ? (see Wang and Kim)
  • Track cooling with an appropriate tracking
    code compare with analytic numbers
  • Suitable for publication/Ph. D. thesis

26
ß-beams example 6Li 3He ? 8B n
  • Beam 25MeV 6Li
  • PLi 529.9 MeV/c B? 0.59 T-m v/c0.09415
    Jz,0-1.6
  • Absorber3He
  • Z2, A3, I31eV, z3, a6
  • dE/ds 110.6 MeV/cm,
  • (?He-3 0.09375 gm/cm3)if Liquid,
  • dE/ds 1180 MeV/gm/cm2, LR 70.9 gm/cm2
  • If gx,y,z 0.13 (Sg 0.4), ß- 0.3m at
    absorber
  • Must mix both x and y with z
  • eN,eq 0.000046 m-rad,
  • sx,rms 2 cm at ß- 1m
  • sE,eq is 0.4 MeV
  • Promising but many problems

27
References
  • Beam transport codes (linear optics fitting)
  • TRANSPORT, MAD, DIMAD, OPTIM, COSY
  • Not always good for unusual optics
  • Do not include absorber effects
  • Tracking codes
  • ICOOL and DP4GEANT
  • Accelerator physics texts S. Y. Lee, Edwards and
    Syphers,etc.
  • Handbook of Accelerator Physics and Engineering
    (A. Chao and M. Tigner, eds.)
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