Meter-scale conditioned hydrodynamic optical-field-ionized plasma channels

Physical Review E American Physical Society (APS) 102:5 (2020) 53201

Authors:

A Picksley, A Alejo, Rj Shalloo, C Arran, A von Boetticher, L Corner, Ja Holloway, J Jonnerby, O Jakobsson, C Thornton, R Walczak, Sm Hooker

Abstract:

We demonstrate through experiments and numerical simulations that low-density, low-loss, meter-scale plasma channels can be generated by employing a conditioning laser pulse to ionize the neutral gas collar surrounding a hydrodynamic optical-field-ionized (HOFI) plasma channel. We use particle-in-cell simulations to show that the leading edge of the conditioning pulse ionizes the neutral gas collar to generate a deep, low-loss plasma channel which guides the bulk of the conditioning pulse itself as well as any subsequently injected pulses. In proof-of-principle experiments we generate conditioned HOFI (CHOFI) waveguides with axial electron densities of $n_\mathrm{e0} \approx 1 \times 10^{17} \; \mathrm{cm^{-3}}$, and a matched spot size of $26 \; \mathrm{\mu m}$. The power attenuation length of these CHOFI channels is $L_\mathrm{att} = (21 \pm 3) \; \mathrm{m}$, more than two orders of magnitude longer than achieved by HOFI channels. Hydrodynamic and particle-in-cell simulations demonstrate that meter-scale CHOFI waveguides with attenuation lengths exceeding 1 m could be generated with a total laser pulse energy of only $1.2$ J per meter of channel. The properties of CHOFI channels are ideally suited to many applications in high-intensity light-matter interactions, including multi-GeV plasma accelerator stages operating at high pulse repetition rates.

Probing the Electronic Structure of Warm Dense Nickel via Resonant Inelastic X-Ray Scattering.

Physical review letters 125:19 (2020) 195001

Authors:

OS Humphries, RS Marjoribanks, QY van den Berg, EC Galtier, MF Kasim, HJ Lee, AJF Miscampbell, B Nagler, R Royle, JS Wark, SM Vinko

Abstract:

The development of bright free-electron lasers (FEL) has revolutionized our ability to create and study matter in the high-energy-density (HED) regime. Current diagnostic techniques have been successful in yielding information on fundamental thermodynamic plasma properties, but provide only limited or indirect information on the detailed quantum structure of these systems, and on how it is affected by ionization dynamics. Here we show how the valence electronic structure of solid-density nickel, heated to temperatures of around 10 of eV on femtosecond timescales, can be probed by single-shot resonant inelastic x-ray scattering (RIXS) at the Linac Coherent Light Source FEL. The RIXS spectrum provides a wealth of information on the HED system that goes well beyond what can be extracted from x-ray absorption or emission spectroscopy alone, and is particularly well suited to time-resolved studies of electronic-structure dynamics.

Observations of Pressure Anisotropy Effects within Semi-Collisional Magnetized-Plasma Bubbles

(2020)

Authors:

ER Tubman, AS Joglekar, AFA Bott, M Borghesi, B Coleman, G Cooper, CN Danson, P Durey, JM Foster, P Graham, G Gregori, ET Gumbrell, MP Hill T Hodge, S Kar, RJ Kingham, M Read, CP Ridgers, J Skidmore, C Spindloe, AGR Thomas, P Treadwell, S Wilson, L Willingale, NC Woolsey

Generation of photoionized plasmas in the laboratory: Analogues to astrophysical sources

Proceedings of the International Astronomical Union Cambridge University Press (CUP) 15:S350 (2020) 321-325

Authors:

S White, R Irwin, R Warwick, G Sarri, Gf Gribakin, Fp Keenan, E Hill, Sj Rose, Gj Ferland, F Wang, G Zhao, B Han, D Riley

Abstract:

Implementation of a novel experimental approach using a bright source of narrowband X-ray emission has enabled the production of a photoionized argon plasma of relevance to astrophysical modelling codes such as Cloudy. We present results showing that the photoionization parameter ζ = 4ÏF/ne generated using the VULCAN laser was ≈ 50 erg cm s-1, higher than those obtained previously with more powerful facilities. Comparison of our argon emission-line spectra in the 4.15-4.25 Å range at varying initial gas pressures with predictions from the Cloudy code and a simple time-dependent code are also presented. Finally we briefly discuss how this proof-of-principle experiment may be scaled to larger facilities such as ORION to produce the closest laboratory analogue to a photoionized plasma.

Modelling burning thermonuclear plasma

Philosophical Transactions A: Mathematical, Physical and Engineering Sciences Royal Society 378:2184 (2020) 20200014

Authors:

Steven J Rose, Peter Hatfield, Robbie HH Scott

Abstract:

Considerable progress towards the achievement of thermonuclear burn using inertial confinement fusion has been achieved at the National Ignition Facility in the USA in the last few years. Other drivers, such as the Z-machine at Sandia, are also making progress towards this goal. A burning thermonuclear plasma would provide a unique and extreme plasma environment; in this paper we discuss (a) different theoretical challenges involved in modelling burning plasmas not currently considered, (b) the use of novel machine learning-based methods that might help large facilities reach ignition, and (c) the connections that a burning plasma might have to fundamental physics, including quantum electrodynamics studies, and the replication and exploration of conditions that last occurred in the first few minutes after the Big Bang.