introduction to accelerators -...
TRANSCRIPT
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US Particle Accelerator School
Introduction to Accelerators
Lecture 4
Basic Properties of Particle Beams
William A. Barletta
Director, United States Particle Accelerator School
Dept. of Physics, MIT
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Homework item
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From the last lecture
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We computed the B-field from currentloop with I = constant
By the Biot-Savart law we found that on the z-axis
What happens if we drive the current to
have a time variation?
B =I
cr2 Rsin d ˆ z = 2 IR2
c R2 + z2( )3 / 2
0
2
ˆ z
R
r
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The far field B-field hasa static dipole form
Importantly the ring of current does not radiate
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Question to ponder:What is the field from this situation?
R
r
We’ll return to this question in the second half of the course
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Is this really paradoxical?
Let’s look at Maxwell’s equations
Take the curl of xE
Hence
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The dipole radiation field: note thesimilarity to the static dipole
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Now on to beams
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Ions - either missing electrons (+) or with extra electrons (-)
Electrons or positrons
Plasma - ions plus electrons
Source techniques depend on type of beam & on application
Beams: particle buncheswith directed velocity
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Electron sources - thermionic
Heated metals
Some electrons have energies above potential barrier
# o
f el
ectr
ons
Cannot escape
Enough energy
to escape
Work function =
dn(E)
dE= A E
1
e(E EF ) / kT +1[ ]
+ HV
Electrons in a metal obey Fermi statistics
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Electrons with enough momentum canescape the metal
Integrating over electrons going in the z direction with
yields
some considerable manipulation yields the Richardson-Dushman
equation
I AT 2 expq
kBT
A=1202 mA/mm2K2
pz2 /2m > EF +
Je = dpx dpy dpxpz , free
(2 /h3) f (E)vz
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Brightness of a beam source
A figure of merit for the performance of a beam source isthe brightness
Typically the normalized brightness is quoted for = 1
B =Beam current
Beam area o Beam Divergence=
Emissivity (J)
Temperature/mass
=Je
kT
moc2
2 =Je
kTmoc
2
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Other ways to get electronsover the potential barrier
Field emission
Sharp needle enhances electric field
Photoemission from metals & semi-conductors
Photon energy exceeds the work function
These sources produce beams with high current densities and low
thermal energy
This is a topic for a separate lecture
+ HV
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Anatomy of an ion source
Gas in
Energy in to
ionize gas
Plasma
Container
for plasma
Electron filter
Extraction
electrodes
Beam
out
Electron beams can also be used to ionize the gas or sputter ions from a solid
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What properties characterize particle beams?
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Beams have directed energy
The beam momentum refers to the average value of pz of
the particles
pbeam = <pz>
The beam energy refers to the mean value of
For highly relativistic beams pc>>mc2, therefore
Ebeam = pz2c 2 + m2c 4[ ]
1/ 2
Ebeam = pz c
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Measuring beam energy & energy spread
Magnetic spectrometer - for good resolution, p one needs
small sample emittance , (parallel particle velocities)
a large beamwidth w in the bending magnet
a large angle
p =w
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Beam carry a current
I ~ ne<vz>
Imacro
I
pulse
QI peak =
Qpulse
Iave =Qtot
T
Duty factor =pulse
T
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Measuring the beam current
Examples:
Non-intercepting: Wall current monitors, waveguide pick-ups
Intercepting: Collect the charge; let it drain through a current meter
• Faraday Cup
Beam current
Return current
Voltage meter
eam pipe
Beam current
Stripline waveguide
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Collecting the charge: Right & wrong ways
Proper Faraday cupSimple collector
The Faraday cup
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Bunch dimensions
X
Y
Z
For uniform charge distributions
We may use “hard edge values
For gaussian charge distributions
Use rms values x, y, z
We will discuss measurements of
bunch size and charge distribution laterx,
y
z,
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But rms values can be misleading
Gaussian beam Beam with halo
We need to measure the particle distribution
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Measuring beam size & distribution
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Beams particles have random (thermal) motion
Beams must be confined against thermal expansion during
transport
Some other characteristics of beams
x =px
x
pz2
1/ 2
> 0
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Beams have internal (self-forces)
Space charge forces
Like charges repel
Like currents attract
For a long thin beam
Esp (V /cm) =60 Ibeam (A)
Rbeam (cm)
B (gauss) = Ibeam (A)
5 Rbeam (cm)
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Net force due to transverse self-fields
In vacuum:
Beam’s transverse self-force scale as 1/ 2
Space charge repulsion: Esp, ~ Nbeam
Pinch field: B ~ Ibeam ~ vz Nbeam ~ vz Esp
Fsp , = q (Esp, + vz x B ) ~ (1-v2) Nbeam ~ Nbeam/ 2
Beams in collision are not in vacuum (beam-beam effects)
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Example: Megagauss fieldsin linear collider
electrons positrons
At Interaction Point space charge cancels; currents add==> strong beam-beam focus
--> Luminosity enhancement--> Strong synchrotron radiation
Consider 250 GeV beams with 1 kA focused to 100 nm
Bpeak ~ 40 Mgauss
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Applications determine the desiredbeam characteristics
Energy E = mc2 MeV to Te V
Energy Spread (rms)
Momentum spread
E/E,
/
p/p
~0.1%
Beam current (peak ) I 10 – 104 A
Pulse duration (FWH M ) Tp 50 fs - 50 ps
Pulse length
(Standard deviation)
z mm - cm
Charge per pulse
# of Particles number
Qb
Nb
1 nC
Emittance (rms)
Normalized emittance
n =
1 mm-mrad /
Bunches per
macropul s e
Mb 1- 100
Pulse repetition rate f 1 - 107
Effective bunch rate f Mb 1 - 109
Emittance is a
measure of beam
quality
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What is this thing called beam quality?
or
How can one describe the dynamics of
a bunch of particles?
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Coordinate space
Each of Nb particles is tracked in ordinary 3-D space
Not too helpful
Orbit traces
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Configuration space:
6Nb-dimensional space for Nb particles; coordinates (xi, pi), i = 1,…, Nb
The bunch is represented by a single point that moves in time
Useful for Hamiltonian dynamics
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Configuration space example:1 particle in an harmonic potential
px
x
But for many problems this description carries
much more information than needed :
We don’t care about each of 1010 individual particles
But seeing both the x & px looks useful
b constant
Fx = kx = m˙ ̇ x
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Option 3: Phase space(gas space in statistical mechanics)
6-dimensional space for Nb particles
The ith particle has coordinates (xi, pi), i = x, y, z
The bunch is represented by Nb points that move in time
px
x
In most cases, the three planes are to very good approximation decoupled
==> One can study the particle evolution independently in each planes:
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Particles Systems & Ensembles
The set of possible states for a system of N particles is referred as an
ensemble in statistical mechanics.
In the statistical approach, particles lose their individuality.
Properties of the whole system are fully represented by particle density
functions f6D and f2D :
where
f6D x, px,y, py,z, pz( ) dx dpx dy dpy dz dpz f2D xi, pi( )dxi dpi i =1,2,3
Ndpdzdpdydpdxf zyxD =6
From: Sannibale USPAS lectures
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Longitudinal phase space
In most accelerators the phase space planes are only weakly coupled.
Treat the longitudinal plane independently from the transverse one
Effects of weak coupling can be treated as a perturbation of theuncoupled solution
In the longitudinal plane, electric fields accelerate the particles
Use energy as longitudinal variable together with its canonicalconjugate time
Frequently, we use relative energy variation & relative time withrespect to a reference particle
According to Liouville, in the presence of Hamiltonian forces, the areaoccupied by the beam in the longitudinal phase space is conserved
=E E0
E00
tt=
From: Sannibale USPAS lectures
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Transverse phase space
For transverse planes {x, px} and {y, py}, use a modified phase space
where the momentum components are replaced by:
where s is the direction of motion
We can relate the old and new variables (for Bz 0 ) by
Note: xi and pi are canonical conjugate variables while x and xi’ are not,
unless there is no acceleration ( and constant)
From: Sannibale USPAS lectures
ds
dxxpxi =
ds
dyypyi =
w
s
PROJECTIONWSp
w
pi = m0
dxi
dt= m0 vs
dxi
ds= m0 c x i i = x,y
( ) 212
1== andc
vwhere
s
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Look again at ourensemble of harmonic oscillators
px
x
Particles stay on their energy contour.
Again the phase area of the ensemble is conserved
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Emittance describes the area in phasespace of the ensemble of beam particles
Phase space of anharmonic oscillator
Emittance - Phase space volume of beam
2 R2(V 2 ( R )2) /c 2
RMS emittance
k (x) - frequency ofrotation of a phase
volume
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Twiss representation of the emittance
A beam with arbitrary phase space distribution can be represented by
an equivalent ellipse with area equal to the rms emittance divided by .
The equation for such an ellipse can be written as
Accelerator physicists often write this equation in terms of
the so-called Twiss Parameters T, T and T
where
x
x
w 2
w ,rms
w2+
w2
w,rms
w 2 2w w
w,rms
w w = w,rms w = x,y
yxwwwww wTwTwTw ,222
==++
yxwwwww wTwwTwwTw ,22
====
From: Sannibale USPAS lectures
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Force-free expansion of a beam
px
x
px
x
Notice: The phase space area is conserved
Drift distance L
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Matrix representation of a drift
From the diagram we can write by inspection
Now write these last equations in terms of T, T and T
0
00
0
0
10
1
xx
xLxx
x
xL
x
x
=
+==
( )
( )00
2
0000
2
0
2
00
2
0
22
0
2
00
22
xxxLxxLxxx
xx
xxLxLxxLxx
+=+=
=
++=+=
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Recalling the definition of the Twissparameters
=
0
0
0
2
10
010
21
T
T
T
T
T
T
L
LL
T = T 0 + L2T 0 2L T 0
T = T 0
T = L T 0 T 0
![Page 44: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/44.jpg)
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A numerical example
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For your notes, as shown in many books:
![Page 46: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/46.jpg)
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The rms emittance is a measure of the mean non-
directed (thermal) energy of the beam
This emittance is the phase space area
occupied by the system of particles, divided by
![Page 47: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/47.jpg)
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Why is emittance an important concept
@ t1
@ t21) Liouville: Under conservative forces phase space
evolves like an incompressible fluid ==>
Z = /12
Z = /8Z = /4
Z = 0x
x’
2) Under linear forces macroscopic(such as focusing magnets) &
=constantemittance is an invariant of motion
3) Under acceleration = n
is an adiabatic invariant
![Page 48: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/48.jpg)
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An axial Bz field, (e.g.,solenoidal lenses) couples transverse planes
The 2-D Phase space area occupied by the system in each transverse plane
is no longer conserved
Liouville’s theorem still applies to the 4D transverse phase space
the 4-D hypervolume is an invariant of the motion
In a frame rotating around the z axis by the Larmor frequency
L = qBz / 2g m0, the transverse planes decouple
The phase space area in each of the planes is conserved again
Emittance conservation with Bz
![Page 49: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/49.jpg)
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Emittance during acceleration
When the beam is accelerated, & change
x and x’ are no longer canonical
Liouville theorem does not apply & emittance is not invariant
0yp
0zp
0
0p
energykineticT
pcmTT
cTmTp zz
+
+=
02
00
2
0
2
0
2
2
2
Accelerate by Ez
0yp p
pz
From: Sannibale USPAS lectures
![Page 50: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/50.jpg)
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Then…
Therefore, the quantity is invariant during acceleration.
Define a conserved normalized emittance
Acceleration couples the longitudinal plane with the transverse planes
The 6D emittance is still conserved but the transverse ones are not
cm
p
p
py
y
z
y
0
0
tan ===cm
p
p
py
y
z
y
000
0
0
0
00tan === 00
0
=y
y
In this case y
y0
= y y 0
000 yy===>
n i = i i = x,y
From: Sannibale USPAS lectures
![Page 51: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/51.jpg)
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Consider a cold beam with a
Gaussian charge distribution
entering a dense plasma
At the beam head the plasma
shorts out the Er leaving only
the azimuthal B-field
The beam begins to pinch trying
to find an equilibrium radius
Nonlinear space-charge fields filamentphase space
![Page 52: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/52.jpg)
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![Page 53: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/53.jpg)
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Example 2: Filamentation oflongitudinal phase space
Data from CERN PS
The emittance according to Liouville is still conserved
Macroscopic (rms) emittance is not conserved
0=t
w
w
![Page 55: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/55.jpg)
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Non-conservative forces (scattering)increases emittance
Scatterer
Scatterer<Vx> <Vx + Vx>
Px/Pz
X
Px/Pz
X
Px/Pz
X
Px/Pz
X
![Page 56: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/56.jpg)
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The Concept of Acceptance
Example: Acceptance of a slit
y
y’
-h/2
h/d
-h/d
-h/2h
d
Electron
Trajectories
Matched beam
emittance
Acceptance at
the slit entrance
Unmatched beam
emittance
From: Sannibale USPAS lectures
![Page 57: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/57.jpg)
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Is there any way to decrease the emittance?
This means taking away mean transverse momentum,
but
keeping mean longitudinal momentum
We’ll leave the details for later in the course.
![Page 58: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/58.jpg)
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Measuring the emittance of the beam
RMS emittance
Determine rms values of velocity & spatial distribution
Ideally determine distribution functions & compute rms
values
Destructive and non-destructive diagnostics
2= R2(V 2 ( R )2) /c 2
![Page 59: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/59.jpg)
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Example of pepperpot diagnostic
Size of image ==> R
Spread in overall image ==> R´
Spread in beamlets ==> V
Intensity of beamlets ==> current density
![Page 60: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/60.jpg)
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Wire scanning to measure R and
SNS Wire Scanner
Measure x-ray signal from beam
scattering from thin tungsten wires
Requires at least 3 measurements along
the beamline
![Page 61: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/61.jpg)
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Horizontal, 0.22 pi mm mrad Vertical, 0.15 pi mm mrad
111
mra
d, fu
ll sc
ale
10.1 mm full scale 5.9 mm full scale
1 0 . 7 5 0 . 5 0 . 3 0 . 1 4 0 . 0 7 0 . 0 4 0 . 0 2 1 0 . 7 5 0 . 5 0 . 2 5 0 . 1 0 . 0 5 0 . 0 3 0 . 0 1 3
111
mra
d, fu
ll sc
ale
Measured 33-mA Beam RMS Emittances
![Page 62: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/62.jpg)
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Matching beams & accelerators
to the task
![Page 63: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/63.jpg)
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What are the design constraints?
Beam particle
Beam format
Type of accelerator
Machine parameters
![Page 64: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/64.jpg)
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Accelerator designer needs figures ofmerit to compare machine alternatives
Physics based
Colliders
• Energy reach, Collision rate (Luminosity), Energy resolution
Light sources
• Spectral range, Spectral brilliance
Economics based
Total cost, $/Watt, /Joule, operating cost
Lifetime, Reliability, Availability
Facility based
Size, Weight, power consumption
==> Accelerating gradient, efficiency
Technology based
Technical risk, expansion potential
![Page 65: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/65.jpg)
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Figure of Merit 1: Beam Energy ==>Energy frontier of discovery
SLED
SC cable
Stochastic
cooling
Wakefields, impedances
Strong
focusing
Colliding beams
![Page 66: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/66.jpg)
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High Energy Physics Figure of Merit 2:Number of events
Events = Cross - section Collision Rate Time
Beam energy: sets scale of physics accessible
Luminosity = N1 N2 frequency
Overlap Area=
N1 N2 f
4 x y Correction factors
We want large charge/bunch, high collision frequency & small spot size
1
2
![Page 67: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/67.jpg)
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Log
lum
inos
ity (
cm-2
s-1
)
ILC
SLHC
VLHC
Example from high energy physics:Discovery space for future accelerators
Luminosity =
Energy Current
Focal depth Beam quality
$, , M
W
![Page 68: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/68.jpg)
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FOM 1 from condensed matter studies:Light source brilliance v. photon energy
Duty factor
correctionfor
pulsed linacsERLsERLs
![Page 69: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/69.jpg)
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FOM 2 from condensed matter studies:Ultra-fast light sources
![Page 70: Introduction to Accelerators - USPASuspas.fnal.gov/materials/09UNM/Unit_2_Lecture_4_Beam_Properties.pdfIntroduction to Accelerators ... Director, United States Particle Accelerator](https://reader034.vdocuments.mx/reader034/viewer/2022052313/5aecd3f87f8b9ad73f90340b/html5/thumbnails/70.jpg)
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Primary, secondary, & tertiary design
constraints
Part
icle
type
Energ
y
Curr
ent
Quality
E/E
Pulse rate
Pulse length
Micro
-bunch
Pola
rize
HEP. NP p, i, e 1 2 2 1 2 2 1 1/3
Light sources e 2 1 1 1 2 3 1 –
FELs e 2 1 1 1 2 1 3 –
Spallation sources p, i 3 1 2 1 2 2 3 –
Radiography e, p 2 1 1 2 3 1 2 –
Therapy e, p 1 1 2 2 3 3 3 –
Cargo screening i 2 1 3 3 2 3 3 –