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Ti:sapphire laser

Professor Simon Hooker

Professor of Atomic & Laser Physics

Research theme

  • Accelerator physics
  • Lasers and high energy density science
  • Plasma physics

Sub department

  • Atomic and Laser Physics

Research groups

  • Laser-plasma accelerator group
  • Oxford Centre for High Energy Density Science (OxCHEDS)
Simon.Hooker@physics.ox.ac.uk
  • About
  • Publications

Inverse free electron lasers and laser wakefield acceleration driven by CO2 lasers

Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 364:1840 (2006) 611-622

Authors:

WD Kimura, NE Andreev, M Babzien, I Ben-Zvi, DB Cline, CE Dilley, SC Gottschalk, SM Hooker, KP Kusche, SV Kuznetsov, IV Pavlishin, IV Pogorelsky, AA Pogosova, LC Steinhauer, A Ting, V Yakimenko, A Zigler, F Zhou

Abstract:

The staged electron laser acceleration (STELLA) experiment demonstrated staging between two laser-driven devices, high trapping efficiency of microbunches within the accelerating field and narrow energy spread during laser acceleration. These are important for practical laser-driven accelerators. STELLA used inverse free electron lasers, which were chosen primarily for convenience. Nevertheless, the STELLA approach can be applied to other laser acceleration methods, in particular, laser-driven plasma accelerators. STELLA is now conducting experiments on laser wakefield acceleration (LWFA). Two novel LWFA approaches are being investigated. In the first one, called pseudo-resonant LWFA, a laser pulse enters a low-density plasma where nonlinear laser/plasma interactions cause the laser pulse shape to steepen, thereby creating strong wakefields. A witness e-beam pulse probes the wakefields. The second one, called seeded self-modulated LWFA, involves sending a seed e-beam pulse into the plasma to initiate wakefield formation. These wakefields are amplified by a laser pulse following shortly after the seed pulse. A second e-beam pulse (witness) follows the seed pulse to probe the wakefields. These LWFA experiments will also be the first ones driven by a CO2 laser beam. © 2006 The Royal Society.
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GeV laser-plasma electron acceleration in a cm-scale capillary waveguide

Optics InfoBase Conference Papers (2006)

Authors:

K Nakamura, C Tóth, B Nagler, CGR Geddes, CB Schroeder, E Esarey, WP Leemans, AJ Gonsalves, SM Hooker

Abstract:

33 mm plasma channels produced in a gas-filled capillary discharge and 40 TW, 40 fs laser pulses were used to produce GeV electron beams in a multi-table-top setup. © 2006 Optical Society of America.

GeV laser-plasma electron acceleration in a cm-scale capillary waveguide

Optics InfoBase Conference Papers (2006)

Authors:

K Nakamura, C Tóth, B Nagler, CGR Geddes, CB Schroeder, E Esarey, WP Leemans, AJ Gonsalves, SM Hooker

Abstract:

33 mm plasma channels produced in a gas-filled capillary discharge and 40 TW, 40 fs laser pulses were used to produce GeV electron beams in a multi-table-top setup. ©2006 Optical Society of America.

GeV laser-plasma electron acceleration in a cm-scale capillary waveguide

Optics InfoBase Conference Papers (2006)

Authors:

K Nakamura, C Tóth, B Nagler, CGR Geddes, CB Schroeder, E Esarey, WP Leemans, AJ Gonsalves, SM Hooker

Abstract:

33 mm plasma channels produced in a gas-filled capillary discharge and 40 TW, 40 fs laser pulses were used to produce GeV electron beams in a multi-table-top setup. © 2006 Optical Society of America.

GeV laser-plasma electron acceleration in a cm-scale capillary waveguide

Optics InfoBase Conference Papers (2006)

Authors:

K Nakamura, C Tóth, B Nagler, CGR Geddes, CB Schroeder, E Esarey, WP Leemans, AJ Gonsalves, SM Hooker

Abstract:

33 mm plasma channels produced in a gas-filled capillary discharge and 40 TW, 40 fs laser pulses were used to produce GeV electron beams in a multi-table-top setup. © 2006 Optical Society of America.
More details from the publisher

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