23
James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys University of Oxford, Oxfordshire, UK Central Laser Facility, Rutherford Appleton Laboratory, UK Bright Radiation Source based on Plasma-micro-bunched Diamond Beam

James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

Embed Size (px)

DESCRIPTION

Image Source: Synchrotron Facilities Europe

Citation preview

Page 1: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

James HollowayUniversity College London, London, UK

PhD Supervisors:

Professor Matthew WingUniversity College London, London, UK

Professor Peter NorreysUniversity of Oxford, Oxfordshire, UK

Central Laser Facility, Rutherford Appleton Laboratory, UK

Bright Radiation Source based on

Plasma-micro-bunched Diamond Beam

Page 2: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

Image Source: http://www.veqter.co.uk/residual-stress-measurement/synchrotron-diffraction

Synchrotron Facilities Worldwide

Page 3: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

Image Source: http://www.veqter.co.uk/residual-stress-measurement/synchrotron-diffraction

Synchrotron Facilities Europe

Page 4: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

Image Source: http://www.veqter.co.uk/residual-stress-measurement/synchrotron-diffraction

Synchrotron Facilities Europe

330 mm

26 mm

14.6 mm

120 mm

52 mm

5.4 mm

2.4 mm

13.2 mm PETRA III

Electron beam lengthProton beam length

Page 5: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

• Use existing facilities’ beams to drive PWA• Accelerate higher energy beams using PWA• Generate harder X-rays from 3rd generation light sources

The Goal

σideal = λp / (π√2)

Need beam lengths of:

σz < 1 mm

• These beams are too long to drive effective wakefields

• Existing beam lines have limited space• Longitudinal compression via magnetic

chicanes takes considerable space and expense

The Problem

• Micro-bunch beams to make them an effective wakefield driver

The Solution

Page 6: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

• Strong transverse kick from laser wakefield

• Propagate beam through vacuum

• Pass micro-bunches into second plasma stage when on-axis number density maximised

Micro-Bunching Via Wakefield Kick and Drift Space

Long electron beamLed by laser

Neutral plasma

+

++

+

+

+---

+

Vacuum

Micro-bunched driver beam.

Secondplasma

cell

Page 7: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

Beam number density. 51 mm of propagation

• E = 300 MeV • εp = 0• σz = 0.6 cm • σr = √2 / kp

• Q = 0.1 nC

Electron beam

• ne = 2.84e22 m-3

• λp = 200 um• Er = 1 GVm-1

The Plasma

Page 8: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

3.5 x 1019

3.1 x1019 m-3

On axis number density

enhanced by ~ an order of magnitude

Beam number density. 51 mm of propagation

Page 9: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys
Page 10: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

Diamond Booster Param• E = 300 MeV • εp = 0• σz = 0.6 cm • σr = √2 / kp

• Q = 0.1 nC

Electron beam

2 31

First Plasma Cell (3.5 mm)

Vacuum(48.5 mm) Second Plasma Cell

(> 100 mm)

1) The long beam given transverse momentum by strong wakefield.

2) Micro-bunches form as half e- defocused, other half focused

3) At the moment the beam has achieved best micro-bunching*, pass into the second plasma cell.

The ‘Drift Space’ Design

• First plasma cell analogous to lens

• Longer first cell results in a stronger focus and shorter vacuum needed

• However strong focus results in higher emittance micro-bunches

• ne = 2.84e22 m-3

• λp = 200 um• Er = 1 GVm-1

The Plasma

Page 11: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

Run♯ Cell Length (mm)

Vacuum Length(mm)

Peak Nd @ 2 m (e19 m-3)

5 2.5 65.5 4.09

6 3.0 57.0 4.00

7 3.5 48.5 3.90

8 4.0 42.0 3.73

9 4.5 37.5 3.80

10 5.0 32.0 3.64

No vacuum ∞ 0.0 0.13

Effects of First Cell length

200

200 mm

Single cell design. Electrons focused too hard and lost

from micro-bunch

Two-Stage design results in stable micro-bunches

Page 12: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys
Page 13: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

The Diamond light source at RAL uses a 3 GeV electron beam to generate soft x-rays.

Beam length: σz = 26 mm

Too long to effectively drive a wakefield! (λp ~ 100um).

A proof of principle experiment has been proposed to micro-bunch the beam using a laser-driven wakefield. The beam can then drive a PWA to:

• Create a higher energy electron beam• Create a poor mans FEL using betatron oscillations within the wake

• E = 3 GeV • ε = 140 nm rad • σz = 26 mm • Q = 2 nC

Diamond Booster Beam

The Diamond Light Source

Page 14: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

Linac

Pictures by Michael Bloom, Imperial College.

90 KeV

Page 15: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

Booster

Pictures by Michael Bloom, Imperial College.

158m circumference

Page 16: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

The Diamond ExperimentServeral slides of tour of Diamond!

Transfer Line

Pictures by Michael Bloom, Imperial College.

Page 17: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

Diamond Booster Param• E = 300 MeV • εp = 0• σz = 0.6 cm • σr = √2 / kp

• Q = 2 nC

Electron beam

1) The long beam given transverse momentum by high amplitude wakefield.

2) Micro-bunches form as half e- defocused, other half focused.

3) At the moment the beam has achieved micro-bunching*, pass into the second plasma cell.

The ‘Drift Space’ Design

• ne = 1.11e22 m-3

• λp = 300 um• Er = 1 GVm-1

The Plasma

Page 18: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys
Page 19: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

A B

Page 20: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys
Page 21: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys
Page 22: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

Acknowledgements

Professor Matthew WingUniversity College London, London, UK

Professor Peter NorreysUniversity of Oxford, Oxfordshire, UK

Central Laser Facility, Rutherford Appleton Laboratory, UK

Professor Robert BinghamUniversity of Strathclyde, Glasgow, UK

Central Laser Facility, Rutherford Appleton Laboratory, UK

Doctor Raoul TrinesCentral Laser Facility, Rutherford Appleton Laboratory, UK

Computing resources provided by STFC’s e-Science facility, SCARF and DiRAC.

Page 23: James Holloway University College London, London, UK PhD Supervisors: Professor Matthew Wing University College London, London, UK Professor Peter Norreys

• Many existing particle beam facilities • Can treat these beams and make them

suitable to drive PWA• Two-stage drift-space design achieves

this over short distances• PWA can generate higher energy

electrons and in turn generate harder X-rays form existing infrastructure

• PWA can generate X-rays directly from micro-bunch oscillations

• Ion motion can be a problem!

Thank you for listening

Concluding