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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

Contribution of ALEGRO to the Update of the European Strategy on Particle Physics

(2025)

Authors:

B Cros, P Muggli, L Corner, J Farmer, M Ferarrio, S Gessner, L Gizzi, E Gschwendtner, M Hogan, S Hooker, W Leemans, C Lindstrøm, J List, A Maier, J Osterhoff, P Piot, J Power, I Pogorelsky, M Turner, J-L Vay, J Wood

On the localization of the high-intensity region of simultaneous space-time foci

Optics Express Optica Publishing Group 33:4 (2025) 7645-7645

Authors:

Emily Archer, Bangshan Sun, Roman Walczak, Martin Booth, Simon Hooker

Abstract:

<jats:p>Simultaneous space-time focusing (SSTF) is sometimes claimed to reduce the longitudinal extent of the high-intensity region near the focus, in contradiction to the original work on this topic. Here we seek to address this confusion by using numerical and analytical methods to investigate the degree of localization of the spatio-temporal intensity of an SSTF pulse. The analytical method is found to be in excellent agreement with numerical calculations and yields, for bi-Gaussian input pulses, expressions for the three-dimensional spatio-temporal intensity profile of the SSTF pulse, and for the on-axis bandwidth, pulse duration, and pulse-front tilt (PFT) of the SSTF pulse. To provide further insight, we propose a method for determining the transverse input profile of a non-SSTF pulse with equivalent spatial focusing. We find that the longitudinal variations of the peak axial intensities of the SSTF and spatially equivalent (SE) pulses are the same, apart from a constant factor, and hence that SSTF does not constrain the region of high intensity more than a non-SSTF pulse with equivalent focusing. We demonstrate that a simplistic method for calculating the pulse intensity exaggerates the degree of intensity localization, unless the spatio-temporal couplings inherent to SSTF pulses are accounted for.</jats:p>
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On the localisation of the high-intensity region of simultaneous space-time foci

(2024)

Authors:

Emily Archer, Bangshan Sun, Roman Walczak, Martin Booth, Simon Hooker
More details from the publisher
Details from ArXiV

Report on the Advanced Linear Collider Study Group (ALEGRO) Workshop 2024

ArXiv 2408.03968 (2024)

Authors:

J Vieira, B Cros, P Muggli, IA Andriyash, O Apsimon, M Backhouse, C Benedetti, SS Bulanov, A Caldwell, Min Chen, V Cilento, S Corde, R D'Arcy, S Diederichs, E Ericson, E Esarey, J Farmer, L Fedeli, A Formenti, B Foster, M Garten, CGR Geddes, T Grismayer, MJ Hogan, S Hooker, A Huebl, S Jalas, M Kirchen, R Lehe, W Leemans, Boyuan Li, CA Lindström, R Losito, CE Mitchell, WB Mori, P Piot, D Terzani, M Thévenet, M Turner, J-L Vay, J Vieira, D Völker, Jie Zhang, W Zhang
Details from ArXiV

Resonant excitation of plasma waves in a plasma channel

Physical Review Research American Physical Society 6:2 (2024) L022001

Authors:

Aimee Ross, James Chappell, John Van De Wetering, James Cowley, Emily Archer, Nicolas Bourgeois, L Corner, Dr Emerson, Linus Feder, Xj Gu, Oscar Jakobsson, H Jones, Alexander Picksley, L Reid, Wei-Ting Wang, Roman Walczak, Simon Hooker

Abstract:

We demonstrate resonant excitation of a plasma wave by a train of short laser pulses guided in a preformed plasma channel, for parameters relevant to a plasma-modulated plasma accelerator (P-MoPA). We show experimentally that a train of N≈10 short pulses, of total energy ∼1J, can be guided through 110mm long plasma channels with on-axis densities in the range 1017-1018cm-3. The spectrum of the transmitted train is found to be strongly red shifted when the plasma period is tuned to the intratrain pulse spacing. Numerical simulations are found to be in excellent agreement with the measurements and indicate that the resonantly excited plasma waves have an amplitude in the range 3-10GVm-1, corresponding to an accelerator stage energy gain of order 1GeV.
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