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Cockcroft Education Lectures 2009 M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

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Page 1: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Introduction to AcceleratorsPart 1

M W PooleDirector, ASTeC

Page 2: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Daresbury Campus

Cockcroft Institute

Page 3: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Basic Acceleration Principle

A voltage drop accelerates charged particles

Electrostatic acceleration in cathode ray tubes:

• televisions

• computer monitors

• oscilloscopes

Page 4: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Birth of Particle Physics and Accelerators

• 1909 Geiger/Marsden MeV backscattering - Manchester

• 1919 Rutherford disintegrates Nitrogen - Manchester

• 1927 Rutherford demands accelerator development

Particle accelerator studies start - Cavendish

• 1929 Cockcroft and Walton start high voltage experiments

• 1932 The prize achieved: Cockcroft + Walton split Li !!!!

‘High’ voltage generation is UK achievement at this stage – brute force

UK grid initiated (132 kV) and industrial base started

Page 5: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Walton, Rutherford, Cockcroft - 1932

Start of the modern era – particle accelerators

NOBEL PRIZE !

Page 6: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Cockcroft-Walton Generator

ISIS 665 kV

Removed 2005

Greinacher 1921See our Atrium !

Page 7: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Electrostatic Monster: the NSF• 1936 van der Graaff pioneers electrostatic solution (2.5 MeV)

• 1961 6 MeV machine at Liverpool (Manchester collaboration)

• 1972 Design Study of 20-30 MV facility at Daresbury

• 1974 Civil construction starts

• 1983 NSF commissioned

• 1992 Closure

World’s highest voltage machine

No nuclear physics replacement

Page 8: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Daresbury Nuclear Structure Facility (NSF)

Last of the line !

Van de Graaf 20+ MV

Page 9: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Seriously high voltages !

Page 10: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Resonant Accelerator Concept

The acceleration occurs in the electric field between cylindrical drift tubes.

The RF power must be synchronised with the motion of the electrons, so that acceleration occurs in every cavity.

This naturally produces bunches of electrons

Wideroe - 1928Linear Accelerator = LINAC

Page 11: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Recirculation Concept - Cyclotron

Radio frequency alternating voltage

Hollow metal drift tubes

time t =0

time t =½ RF period

SynchronisationNecessary

D-shaped RF cavities

Orbit radius increaseswith energy

Expensive/impractical forhigh energies (1 GeV)

Lawrence:4” – 80 keV11” - 1.2 MeV

q v B = mv2 / r

r = mv / qBT = 2pm / qB

Page 12: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Phase Synchronism

Synchronous particle (A) crosses cavity after one turn at same phase relative to RF peak

Particle B delayed behind A receives higher accelerating voltage and therefore after next turn returns nearer or even ahead of A

Particles undergo harmonic synchrotron oscillations about A as they orbit the accelerator

NOTE: This leads to BUNCHING about A

Page 13: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Accelerator Developments

• Cyclotrons have huge magnets - spiral orbits

• Also complicated by relativistic mass increase

• Solution:

Raise magnetic field strength as particle energy increases

Produces annular orbit geometry

SYNCHROTRON

Page 14: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Synchrotron Ring Schematic

Focusing magnets

Vacuumtube

Accelerating cavity

Bending magnets

Bending and focussing often combined

Page 15: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Magnet Focusing

FQUADs (shown above) focus the beam horizontally.

DQUADs (as above, rotated 90º) focus the beam vertically.

Quadrupole magnets are used to focus the beam.

Page 16: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

RF Accelerating Cavities

Single cell example

Page 17: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Klystrons

Page 18: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Simple Accelerator Lattice

Dipole

F Quadrupole

D Quadrupole

FODO Cellfinite dispersion

Page 19: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Betatron Oscillations

Transverse motion of particles in both planes is harmonic - as they deviate from the design orbit a restoring force increases with displacement

The particles follow betatron oscillations as they orbit the accelerator

The amplitude and wavelength of this motion is characterised by the beta functions of the accelerator

Off-energy particles follow a dispersion function

Page 20: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Phase Space

Beta function givestransverse envelope

Emittance measuresphase space area

Page 21: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

The Double Bend Achromat Cell

Dipole

Quadrupoles

Sextupoles

Dipole

Quadrupole

Dispersive Path

Dipole

Non - Dispersive

Page 22: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Lattice Functions - DBA Example

Lattice Functions

-10

-5

0

5

10

15

20

25

30

0 10 20 30 40 50Distance (m)

Bet

a fu

nctio

ns (

m)

0.0

0.2

0.4

0.6

0.8

1.0

Dis

pers

ion

(m)

Page 23: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Sextupole Magnets

Chromatic Correction

(off energy particles)

In finite dispersion region focussing matches energy

Page 24: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Penalty: Collapse of Dynamic Stability

No sextupoles Corrected to zero chromaticity

Page 25: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Four families

Six families

Eight families

Recovery of Stability - Sextupoles in Patterns

Page 26: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Early (UK) History

(Synchro)CyclotronsBerkeley (Lawrence) 60” (1939)Liverpool 37” 20 MeV (1939)Harwell 110” 175 MeV (1949)Liverpool 156” 380 MeV (1954) (extraction)

LinacsHarwell 3.5 MeV (1947) 15 (Mullard), 55 (Met Vickers), 136 MeV

SynchrotronsWoolwich Arsenal - Goward & Barnes 8 MeV (1946) (Betatron 1943)Malvern 30 MeV (1950)Oxford 125 MeV (1952)Birmingham 1 GeV p (1953)Glasgow 350 MeV (1954)NIMROD RAL 7 GeV p (1960)NINA DL 5 GeV (1966)

Clatterbridge Oncology Centre65 MeV

Page 27: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Origins of Daresbury Laboratory

• 1957 Wilkinson proposes HE electron synchrotron

• 1960 Cockcroft + Cassels propose 4 GeV version

• 1961 Cockcroft proposes Cheshire site !!!!

• 1962 NINA approved - £3.5M

Many local sites considered

• 1963 Daresbury selected

HEI driving force: Liverpool/Manchester/Glasgow/Sheffield/ (Lancaster)

Page 28: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Daresbury Laboratory - 1964

Page 29: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Construction of NINA - 1964

Page 30: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

A Bad Day at the Office !

Page 31: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Grand Opening of NINA - 1967

Page 32: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

The NINA Synchrotron

Page 33: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Chadwick’s 75th Birthday – Daresbury Event

Page 34: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

NINA Closure

• UK joined SPS at CERN on condition domestic programme terminated (NINA AND NIMROD)

• NINA switched off in 1977

• Alternative major facilities already sought - and found:

• NSF (discussed)

• ISIS and SRS (part 2 next week)

Page 35: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

EM Radiation from Accelerating Charge

Non-relativistic charge source

Page 36: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Fundamentals of Radiation Emission

• Any charge that is accelerated emits radiation

• Properties calculated since 1897 (Larmor)

Lienard and Schott studied relativistic particles on circular trajectories:

P E4/R2

• So this applies to accelerated beams of charged particles in a ring (synchrotron)

SYNCHROTRON RADIATION

=> Severe losses and energy restrictions eg NINA

Page 37: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Relativistic Emission

Relativistic Emission Cone

Electron rest frame

Laboratory frame

Transforming between frames

tan = -1sin (1 + cos ) -1

if = 90

then: = -1

Page 38: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Emission from Bends

First observed 1947GE Synchrotron

Electron

Cone angle = 1/Acceleration

= E/m0c2

Page 39: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Synchrotron Radiation Spectrum

R

1/

1/ R1/

Observer

e-

33

4

c

R Pulse Length

(electron transit arc - photon transit chord)

For 2 GeV, 1.2 T:

R ~ 5.5 m, ~ 4000

Wavelength ~ 0.1 nm33

R4

Typical wavelength

Page 40: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Universal Synchrotron Radiation Curve

1E+05

1E+06

1E+07

1E+08

1E+09

1E+10

1E+11

1E+12

1E+13

0.0001 0.001 0.01 0.1 1 10 100w/wc

Sp

ectr

al P

hot

on F

lux

(ph

oton

s/s/

mra

d/0

.1%

ban

dw

idth

/GeV

/100

mA

)

ww

ww

c/

3/5c

b13 du)u(KEI10x46.2N

In units of photons/s/mrad/0.1% bandwidth

Page 41: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Accelerators in Space

Crab Nebula

Page 42: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Synchrotron Radiation –New Particle Accelerator Applications

Accelerating charged particles emit electromagnetic radiation– very inconvenient for circular electron accelerators !

• 1972 Scientific use started at Daresbury by Manchester group

• 1974 SRS Design Study (NINA replacement – 2nd Generation)

• 1980 SRS commissioning (world’s first dedicated x-ray source)

• 1987 High brightness upgrade

• Many pioneering additions: – superconducting wigglers undulators precision beam steering high currents

• 2008 Project termination

Page 43: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Daresbury SRS

• Design studies completed 1975 – anticipate NINA end

• Based on an electron storage ring

• World’s first dedicated x-ray source

• First user programme 1981

• Major UK success story for 27 years

• Pioneering developments and upgrades

Page 44: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Daresbury SRS Concept

Storage RingBooster

Linac

Beamlines

80 keV

12 MeV 600

MeV

World’s first dedicated x-ray source

2 GeV

Page 45: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Daresbury Laboratory

Page 46: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

SRS Storage Ring Parameters

Electron Energy 2 GeV

Operating Current 300 mA

Total Circumference 96 m

Revolution Frequency 3.1 MHz

Pressure in Beam Tube 10-12 atm

Number of Dipoles 16

Dipole Current at 2 GeV 1,420 A

Dipole Field 1.2 T

RF Power Input to Beam 250 kW

Stored Beam Lifetime 30 hours

Page 47: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

SRS Components - High Technology

Page 48: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

A Synchrotron as an Injector

SRS Booster

600 MeV

Page 49: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

SRS Lifetime (Example)

Operating mode is fill storage ring every morning24/7 running (6000 hours annual)

Page 50: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Real Synchrotron Radiation

Beam port

Page 51: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Synchrotron Radiation Spectrum

1E+05

1E+06

1E+07

1E+08

1E+09

1E+10

1E+11

1E+12

1E+13

0.0001 0.001 0.01 0.1 1 10 100w/wc

Sp

ectr

al P

hot

on F

lux

(ph

oton

s/s/

mra

d/0

.1%

ban

dw

idth

/GeV

/100

mA

)

Broad band source

Covers huge spectral range

Range set by electron energy and bending field strength

Flux/power far exceeds previous sources

Page 52: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

From Source to Detector

• Light from source can be split for more than one experiment

• Light focused using mirrors

• Narrow range of wavelengths selected by monochromator

• Light illuminates crystal sample and is diffracted

• Diffraction pattern observed with detector

Page 53: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Wide Range of Applications

FMV Virus Structure (1990) Light Harvesting Complex(photosynthesis)

Protein Crystallography

LIGA

Materials science

Page 54: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

The Nobel Prize: F1 ATPase structure

• Sir John Walker shared 1997 Nobel Prize for Chemistry - structure of the F1 ATPase enzyme, using the SRS

Page 55: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

High Field Insertion Devices

1.0E+10

1.0E+11

1.0E+12

1.0E+13

1.0E+14

1.0 10.0 100.0 1000.0 10000.0 100000.0

Photon Energy (eV)Sp

ectr

al P

hoto

n F

lux

(pho

tons

/s/m

rad/

0.1%

ban

dwid

th)

1.2 T Magnet6.0 T Magnet

Normal Straight

With Insertion Device

SRS Superconducting Wavelength Shifter6.0 Tesla

Page 56: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Alternative Compact Light Source

Designed at DaresburySold by Oxford Instruments to IBM in 1990 - lithographyOperated successfully for 10 years

700 MeV

4.5 T

Page 57: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Big Accelerators - CERN

Page 58: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Types of Accelerator

• Linear Accelerators (Linacs)• Multi-cell concepts TW and SW

• Cyclotrons• Low energy limit

• Synchrocyclotrons• RF variation compensates mass change – extends energy reach

• Betatrons• Beam is ‘secondary’ of a transformer - magnetic field limit

• Synchrotrons and Storage Rings• Ramped magnetic field matches energy – annular design

• Other variants• Microtron RFQ FFAG ???

Page 59: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Accelerator Physics Challenges

• Classical electrodynamics - Maxwell (mainly !)• Lorentz forces: Deflection and acceleration

• Single particle dynamics• transport, stability, nonlinear dynamics - tracking & differential algebra

• Multi-particle dynamics• collective effects, wake fields, space charge, coherent instabilities

Production Transport Injection Acceleration Extraction Manipulation Delivery

Analytic modelling + Computer simulation (Start-to-End)

(Major code development)

Experimental verification (Commissioning !)

fs nm

Page 60: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Accelerator Technologies

Sources - electron guns photoinjectors, ion sources, ……..

Magnets - EM / SCM / PM DC / AC / PulsedHarmonic / Periodic Power supplies

RF System - structures power sources

Vacuum - UHV modelling diagnostics pumping

Diagnostics - fast high precision non-interactive

Geodesics - alignment feedback

Radiation - losses shielding personnel safety

Dumps - spallation targets collimators

Engineering - mechanical electrical civil

Controls - advanced process control

NB Multi-disciplinary teams. Resource issues - construction/operation.

Page 61: Cockcroft Education Lectures 2009M W Poole Introduction to Accelerators Part 1 M W Poole Director, ASTeC

Cockcroft Education Lectures 2009 M W Poole

Concluding Remarks

• Origins of particle accelerators discussed

• Reason for Daresbury Lab (and CI) existence explained

• Applications beyond particle physics highlighted

• Additional concepts mentioned

• Next week: surveys of various advanced applications