B. Walton
Imperial College London
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Featured researches published by B. Walton.
Nature | 2004
S. P. D. Mangles; C. D. Murphy; Z. Najmudin; A. G. R. Thomas; John Collier; A. E. Dangor; E. J. Divall; P. S. Foster; J. G. Gallacher; C. J. Hooker; D. A. Jaroszynski; A. J. Langley; W. B. Mori; P.A. Norreys; F. S. Tsung; R. Viskup; B. Walton; K. Krushelnick
High-power lasers that fit into a university-scale laboratory can now reach focused intensities of more than 1019 W cm-2 at high repetition rates. Such lasers are capable of producing beams of energetic electrons, protons and γ-rays. Relativistic electrons are generated through the breaking of large-amplitude relativistic plasma waves created in the wake of the laser pulse as it propagates through a plasma, or through a direct interaction between the laser field and the electrons in the plasma. However, the electron beams produced from previous laser–plasma experiments have a large energy spread, limiting their use for potential applications. Here we report high-resolution energy measurements of the electron beams produced from intense laser–plasma interactions, showing that—under particular plasma conditions—it is possible to generate beams of relativistic electrons with low divergence and a small energy spread (less than three per cent). The monoenergetic features were observed in the electron energy spectrum for plasma densities just above a threshold required for breaking of the plasma wave. These features were observed consistently in the electron spectrum, although the energy of the beam was observed to vary from shot to shot. If the issue of energy reproducibility can be addressed, it should be possible to generate ultrashort monoenergetic electron bunches of tunable energy, holding great promise for the future development of ‘table-top’ particle accelerators.
Physics of Plasmas | 2001
Victor Malka; Jérôme Faure; J.R. Marques; F. Amiranoff; Jean-Philippe Rousseau; S. Ranc; Jean-Paul Chambaret; Z. Najmudin; B. Walton; P. Mora; A. Solodov
Detailed measurements of electron spectra and charges from the interaction of 10 Hz, 600 mJ laser pulses in the relativistic regime with a gas jet have been done over a wide range of intensities (1018–2×1019 W/cm2) and electron densities (1.5×1018–1.5×1020 cm−3), from the “classical laser wakefield regime” to the “self-modulated laser wakefield” regime. In the best case the maximum electron energy reaches 70 MeV. It increases at lower electron densities and higher laser intensities. A total charge of 8 nC was measured. The presented simulation results indicate that the electrons are accelerated mainly by relativistic plasma waves, and, to some extent, by direct laser acceleration.
Laser and Particle Beams | 2006
S. P. D. Mangles; B. Walton; Z. Najmudin; A. E. Dangor; K. Krushelnick; Victor Malka; M. Manclossi; N. Lopes; C. Carias; G. Mendes; F. Dorchies
A “table-top” high power laser has been used to generate beams of accelerated electrons up to energy of 20 MeV from interactions with underdense plasmas. The energy spectrum of these beams was measured using a magnetic spectrometer and proof-of-principle experiments were performed to evaluate the suitability of these beams for electron radiography applications.
Physics of Plasmas | 2003
Z. Najmudin; K. Krushelnick; E.L. Clark; S. P. D. Mangles; B. Walton; A. E. Dangor; S. Fritzler; Victor Malka; E. Lefebvre; Daniel Gordon; Frank Tsung; C. Joshi
The interaction of intense laser pulses (power>30 TW) with underdense plasmas has been studied. In the regime where the pulse length is much longer than the plasma period (τl≫2πωp−1), the laser pulse is found to be self-modulated at the plasma frequency by the forward Raman scattering instability. Wavebreaking of the resulting plasma wave results in energetic electrons being accelerated to more than 100 MeV. Reducing the pulse length so that τl∼2πωp−1, but retaining the same power, also leads to wavebreaking. This is a direct result of a combination of laser beam self-focusing, front-edge laser pulse steepening and relativistic lengthening of the plasma wave wavelength, which can result in a forced growth of the wakefield plasma wave, even for initially nonresonant laser pulses (τl≠πωp−1). Since, in this forced laser wakefield regime, the interaction of the plasma wave and the bunch of accelerated electrons with the laser pulse is reduced, this can result in higher energy gain (to beyond 200 MeV) and bett...
Physics of Plasmas | 2005
K. Krushelnick; Z. Najmudin; S. P. D. Mangles; A. G. R. Thomas; M.S. Wei; B. Walton; A. Gopal; E.L. Clark; A. E. Dangor; S. Fritzler; C. D. Murphy; P.A. Norreys; W. B. Mori; J. G. Gallacher; D. A. Jaroszynski; R. Viskup
The interaction of high intensity laser pulses with underdense plasma is investigated experimentally using a range of laser parameters and energetic electron production mechanisms are compared. It is clear that the physics of these interactions changes significantly depending not only on the interaction intensity but also on the laser pulse length. For high intensity laser interactions in the picosecond pulse duration regime the production of energetic electrons is highly correlated with the production of plasma waves. However as intensities are increased the peak electron acceleration increases beyond that which can be produced from single stage plasma wave acceleration and direct laser acceleration mechanisms must be invoked. If, alternatively, the pulse length is reduced such that it approaches the plasma period of a relativistic electron plasma wave, high power interactions can be shown to enable the generation of quasimonoenergetic beams of relativistic electrons.
Philosophical Transactions of the Royal Society A | 2006
S. P. D. Mangles; K. Krushelnick; Z. Najmudin; M.S. Wei; B. Walton; A. Gopal; A. E. Dangor; S. Fritzler; C. D. Murphy; A. G. R. Thomas; W. B. Mori; J. G. Gallacher; D. A. Jaroszynski; P.A. Norreys; R. Viskup
The physics of the interaction of high-intensity laser pulses with underdense plasma depends not only on the interaction intensity but also on the laser pulse length. We show experimentally that as intensities are increased beyond 1020 W cm−2 the peak electron acceleration increases beyond that which can be produced from single stage plasma wave acceleration and it is likely that direct laser acceleration mechanisms begin to play an important role. If, alternatively, the pulse length is reduced such that it approaches the plasma period of a relativistic electron plasma wave, high-power interactions at much lower intensity enable the generation of quasi-mono-energetic beams of relativistic electrons.
Optics Letters | 2002
B. Walton; Z. Najmudin; M.S. Wei; C. Marle; R. J. Kingham; K. Krushelnick; A. E. Dangor; R. J. Clarke; M. J. Poulter; Cristina Hernandez-Gomez; S. Hawkes; D. Neely; John Collier; C. Danson; S. Fritzler; Victor Malka
A short-pulse laser beat wave scheme for advanced particle accelerator applications is examined. A short, intense (3-ps, >10(18)-W cm(-2)) two-frequency laser pulse is produced by use of a modified chirped-pulse amplification scheme and is shown to produce relativistic plasma waves during interactions with low-density plasmas. The generation of plasma waves was observed by measurement of forward Raman scattering. Resonance was found to occur at an electron density many times that expected, owing to ponderomotive displacement of plasma within the focal region.
Physics of Plasmas | 2006
B. Walton; S. P. D. Mangles; Z. Najmudin; M. Tatarakis; M.S. Wei; A. Gopal; C. Marle; A. E. Dangor; K. Krushelnick; S. Fritzler; Victor Malka; R. J. Clarke; Cristina Hernandez-Gomez
Two experiments studying the interaction of high intensity laser pulses (1×1019–5×1020W∕cm2) with underdense plasma are compared. The experiments used lasers that differed in power and focused intensity but had similar pulse duration (∼1ps). Spectroscopic measurements of the forward scattered light (sidebands) near the fundamental laser frequency produced by the self-modulation instability were performed and the energies of electrons accelerated in the interaction are measured and compared. It is found that at high intensities the sideband intensities and the electron energies were not directly correlated, implying that relativistic plasma wave generation is not the most important mechanism for electron acceleration in the ultrahigh intensity regime. Simulation results for the forward scattered spectrum agree well with experimental results.
Physics of Plasmas | 2006
B. Walton; Z. Najmudin; M.S. Wei; C. Marle; R. J. Kingham; K. Krushelnick; A. E. Dangor; R. J. Clarke; M. J. Poulter; Cristina Hernandez-Gomez; S. Hawkes; D. Neely; John Collier; C. Danson; S. Fritzler; Victor Malka
Experiments to examine the generation of relativistic plasma waves via a high-intensity short-pulse beat-wave scheme are described in detail. The pulse stretcher of the Vulcan chirped-pulse amplification (CPA) laser system was modified to produce two frequency, 3ps pulses focusable to intensities up to 1018Wcm−2. Short high-intensity pulses were used to avoid limitations to the plasma-wave amplitude due to the modulational instability. Two experiments were undertaken, at 3 and 10TW, with the generation of plasma waves diagnosed by measuring the sidebands produced in the spectrum of the forward scattered beam. A resonance in the sideband signal was observed for an initial plasma density higher than expected for the given beat frequency. This resonance shift can be attributed to transverse ponderomotive expulsion of plasma electrons from the laser focal region. A monotonically increasing background was also observed, which was due to nonresonant cross-phase modulation.
SUPERSTRONG FIELDS IN PLASMAS: Third International Conference on Superstrong Fields in Plasmas | 2006
Z. Najmudin; B. Walton; S. P. D. Mangles; A. E. Dangor; S. Fritzler; Victor Malka; Jérôme Faure; M. Tatarakis; K. Krushelnick
Measurements have been made of the magnetic field generated by the passage of high intensity short laser pulses through underdense plasmas. For a 30 fs, 1 J, 800 nm linearly‐polarised laser pulse, an azimuthal magnetic field is observed at a radial extent of approximately 200 μm. The field is found to exceed 2.8 MG. For a 1 ps, 40 J, 1054 nm circularly‐polarised laser pulse, a solenoidal field is observed that can exceed 7 MG. This solenoidal field is absent with linear polarised light, and hence can be considered as an Inverse Faraday effect. Both types of field are found to decay on the picosecond timescale. For both the azimuthal and solenoidal fields produced by such intense lasers, the production of energetic electrons by the interaction is thought to be vital for magnetic field generation.