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Transcript of The Physics of Accelerators C.R. Prior Rutherford Appleton Laboratory and Trinity College, Oxford...
The Physics of Accelerators
C.R. Prior
Rutherford Appleton Laboratory
and Trinity College, Oxford
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory
Contents• Basic concepts in the study of Particle
Accelerators (including relativistic effects)
• Methods of Acceleration– linacs and rings
• Controlling the beam– confinement, acceleration, focusing– animations– synchrotron radiation
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory
Introduction• Basic knowledge for the study of particle
beams:– applications of relativistic particle dynamics– classical theory of electromagnetism (Maxwell’s
equations)
• More advanced studies require– Hamiltonian mechanics– optical concepts– quantum scattering theory, radiation by charged
particlesCERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory
Applications of Accelerators• Based on
– possibility of directing beams to hit specific targets
– production of thin beams of synchrotron light
• Bombardment of targets used to obtain new materials with different chemical, physical and mechanical properties
• Synchrotron radiation covers spectroscopy, X-ray diffraction, x-
ray microscopy, crystallography of proteins. Techniques used to manufacture products for aeronautics, medicine, pharmacology, steel production, chemical, car, oil and space industries.
• In medicine, beams are used for Positron Emission Tomography (PET), therapy of tumours, and for surgery.
Basic ConceptsEnergy of a relativistic particle
where c=speed of light = 3x108
m/s
is the “relativistic -factor”
For v<<c,
20 cmE
2
21
1
cv
202
120 vmcmE
Rest energy Classical kinetic energy
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory
Relativistic kinetic energy 120 cmT
MomentumConnection between E and p:
so for ultra-relativistic particlesUnits: 1eV = 1.6021 x 10-19 joule.
E[eV] = m0c2/e where e=electron charge
Rest energies: Electron E0 = 511 keV
Proton E0 = 938 MeV
vmp 0
220
22
2cmp
cE
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Basic Concepts
pcE
Velocity v. Kinetic Energy
Low energies:
E E0+½m0v2
High energies:
2
201
EEcv
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Basic Concepts
At low energies, Newtonian mechanics may be used; relativistic formulae necessary at high energies
Equation of motion and Lorentz force
Acceleration in direction of constant E-field
Constant energy and spiralling about constant B-field.
BvEqdt
pd
EpE
cq
dt
dE
2
qB
p
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Basic Concepts
v
E
qBc
2
Radius FrequencyqvBvm
2
0
Methods of AccelerationLinacsLinacs
Vacuum chamber with one or more DC
accelerating structures with E-field aligned in
direction of motion.– Avoids expensive magnets– no loss of energy from synchrotron radiation– but many structures, limited energy gain/metre– large energy increase requires long accelerator
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory
CyclotronCyclotron
Use magnetic fields to force particles to pass
through accelerating cells periodically
R.F. electric field
•Constant B, constant accelerating frequency f.
•Spiral trajectories
• For synchronism
=> approximately constant energy, so only possible at low velocities ~1.
Use for heavy particles (protons, deuterons, -particles)
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Methods of Acceleration
~
B
nf
qB
p
v
E
qBc
2
Isochronous CyclotronIsochronous CyclotronHigher energies => relativistic effects
=> no longer constant.
Particles get out of phase with accelerating
fields; eventually no overall acceleration.
Solution: vary B to compensate and keep f
constant.
Thomas (1938): need both radial (because varies) and azimuthal B-field variation for stable orbits.
Construction difficulties.
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Methods of Acceleration
v
E
qBc
2
nf
qB
p
Synchro-cyclotronSynchro-cyclotronModulate frequency f of accelerating structure instead.
McMillan & Veksler (1945): oscillations are stable.
Betatron (Kerst 1941)Betatron (Kerst 1941)Particles accelerated by rotational electric field generated by time varying B:
Theory of “betatron” oscillations.Overtaken by development of synchrotron.
t
BE
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Methods of Acceleration
qB
p
v
E
qBc
2
nf
SynchrotronSynchrotron
Principle of frequency modulation but in addition variation in time of B-field to match increase in energy and keep revolution radius constant.
Magnetic field produced by several dipoles, increases linearly with momentum. At high energies:
B= p/q E/qc
E[GeV]=0.29979 B[T] [m]
per unit charge. Limitations of magnetic fields => high energies only at large radius
e.g. LHC E = 8 TeV, B = 10 T, = 2.7 km
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Methods of Acceleration
qB
p
v
E
qBc
2
nf
(i) storage rings: accumulate particles and keep circulating for long periods; used for high intensity beams to inject into more powerful machines or synchrotron radiation factories.
(ii) colliders: two beams circulating in opposite directions, made to intersect; maximises energy in centre of mass frame.
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Methods of Acceleration
Example of variation of parameters with time in a synchrotron:
Important types of Synchrotron:
B
E
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory
Confinement, Acceleration and Focusing of Particles
Confinement
By increasing E (hence p) and B together, possible to maintain cyclotron at constant radius and accelerate a beam of particles.
In a synchrotron, confining magnetic field comes from a system of several magnetic dipoles forming a closed arc. Dipoles are mounted apart, separated by straight sections/vacuum chambers including equipment for focusing, acceleration, injection, extraction, experimental areas, vacuum pumps.
qB
p
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Confinement
ISIS dipole (RAL)
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Confinement
Hence mean radius of ring R>
e.g. CERN SPS
R=1100m, =225m
Can also have large machines with a large number of dipoles each of small bending angle.
e.g. CERN SPS
744 magnets, 6.26m long, angle =0.48o
Injection
Extraction
Collimation
R.F.
Dipoles
Focusing elements
Dipoles
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Acceleration
Acceleration
A positive charge crossing uniform E-fields is
accelerated according to Eqdt
pd
Simple model of an RF cavity: uniform field between parallel plates of a condenser containing small holes to allow for the passage of the beam
Revolution period when vc.
Revolution frequency Hz.
If several bunches in machine, introduce RF cavities in
straight sections with oscillating fields
h is the harmonic number.
Energy increase E when particles pass RF cavities can
increase energy only so far as can increase B-field in dipoles
to keep constant .
Magnetic rigidity
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Acceleration
c
L
v
R
2
L
c
1
L
hchrf
q
pB
Bunch passing cavity: centre of bunch called the synchronous particle.
Particles see voltage
For synchronous particle s = 0 (no acceleration)
Particles arriving early see < 0
Particles arriving late see > 0
energy of those in advance is decreased and vice versa.
To accelerate, make 0 < s< so that synchronous particle gains energy CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Acceleration
tVtV rf sin2sin 00
sqVE sin0
Bunching effect
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Acceleration
Not all particles are stable. There is a limit to the stable region (the separatrix or “bucket”) and, at high intensity, it is important to design the machine so that all particles are confined within this region and are “trapped”.
Weak FocusingParticles injected horizontally into a uniform magnetic field follow a circular orbit.
Misalignment errors, difficulty in perfect injection cause particles to drift vertically and radially and to hit walls.
severe limitations to a machine.
Require some kind of stability mechanism:
Vertical stability requires negative field gradient.
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory
rifqBvr
vm 20 i.e. horizontal restoring force
is towards the design orbit.
10
d
dB
Bn Weak focusing
Overall stability:
Focusing
Strong FocusingAlternating gradient (AG) principle (1950’s)A sequence of focusing-defocusing fields provides a
stronger net focusing force.Quadrupoles focus horizontally, defocus vertically or vice
versa. Forces are proportional to displacement from axis.
Focusing
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory
A succession of opposed elements enable particles to follow stable trajectories, making small oscillations about the design orbit.
Technological limits on magnets are high.
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Focusing
Fermilab quadrupole
Sextupoles are used to correct longitudinal momentum errors.
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory
Thin lens analogy of AG focusing:
x
finout
x
x
fx
x
1
101
F-drift-D system:
f
l
f
ll
f
l
f
fl
1
1
11
01
10
11
101
2
Thin lens of focal length f 2/l, focusing overall, if l f. Same for D-drift-F (f -f ), so system of AG lenses can focus in both planes simultaneously.
lB
B
f
1
f
xx
Drift: unchanged, xlxxx inout
x
xl
x
x
10
1
Focusing
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Focusing
Matched beam oscillations in simple FODO cell
Matched beam oscillations in a proton driver for a
neutrino factory
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Focusing
Typical example of ring design:
• basic lattice
• beam envelopes
• phase advances
• phase space non-linearities
• Poincaré maps
Electrons and Synchrotron Radiation
• Particles radiate when they are accelerated, so charged particles crossing the magnetic dipoles of a lattice in a ring (centrifugal acceleration) emit radiation in a direction tangential to their trajectory.
• After one turn of a circular accelerator, total energy loss by synchrotron radiation is
• Proton mass : electron mass = 1836. For the same energy and radius,
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory
4
20
18
/GeVm
10034.6GeV
cm
GeVEE
1310: pe EE
Synchrotron Radiation
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory
• In electron machines, strong dependence of radiated energy on E.
• Losses must be compensated by cavities
• Technological limit on maximum energy a cavity can deliver upper band for electron energy in an accelerator:
• Better to have larger accelerator for same power from RF cavities at high energies.
• To reach twice LEP energy with same cavities would require a machine 16 times as large.
Synchrotron Radiation
4/1maxmax m10GeV EE
e.g. LEP 50 GeV electrons, = 3.1 km, circumference = 27 km.
Energy loss per turn = 0.18 GeV per particle
• Radiation within a light cone of angle
• For electrons in the range 90 MeV to 1 GeV, is in the range 10-4 - 10-5 degs.
• Such collimated beams can be directed with high precision to a target - many applications.
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory Synchrotron Radiation
cE
toclosespeedsforkeV
5111
Luminosity
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory
Area, A
• Measures interaction rate per unit cross section - an important concept for colliders.
• Simple model: Two cylindrical bunches of area A. Any particle in one bunch sees a fraction N/A of the other bunch. (=interaction cross section). Number of interactions between the two bunches is N2 /A.
Interaction rate is R=f N2 /A, and• Luminosity
• CERN and Fermilab colliders
have L ~ 1030 cm-2s-1. SSC was
aiming for L ~ 1033 cm-2s-1
A
Nf
2
L
pp
Reading• E.J.N. Wilson: Introduction to Accelerators• S.Y. Lee: Accelerator Physics• M. Reiser: Theory and Design of Charged Particle
Beams• D. Edwards & M. Syphers: An Introduction to the
Physics of High Energy Accelerators• M. Conte & W. MacKay: An Introduction to the
Physics of Particle Accelerators• R. Dilao & R. Alves-Pires: Nonlinear Dynamics in
Particle Accelerators• M. Livingston & J. Blewett: Particle Accelerators
CERN Accelerator School Loutraki, Greece, Oct 2000
C.R. Prior, Rutherford Appleton Laboratory