Speed of sound in methane under conditions of planetary interiors

Physical Review Research American Physical Society 6:2 (2024) l022029

Authors:

Thomas Whitehead, Hannah Poole, Emma E McBride, Matthew Oliver, Adrien Descamps, Luke B Fletcher, W Alex Angermeier, Cameron H Allen, Karen Appel, Florian P Condamine, Chandra B Curry, Francesco Dallari, Stefan Funk, Eric Galtier, Eliseo J Gamboa, Maxence Gauthier, Peter Graham, Sebastian Goede, Daniel Haden, Jongjin B Kim, Hae Ja Lee, Benjamin K Ofori-Okai, Scott Richardson, Alex Rigby, Christopher Schoenwaelder, Peihao Sun, Bastian L Witte, Thomas Tschentscher, Ulf Zastrau, Bob Nagler, Jb Hastings, Giulio Monaco, Dirk O Gericke, Siegfried H Glenzer, Gianluca Gregori

Abstract:

We present direct observations of acoustic waves in warm dense matter. We analyze wave-number- and energy-resolved x-ray spectra taken from warm dense methane created by laser heating a cryogenic liquid jet. X-ray diffraction and inelastic free-electron scattering yield sample conditions of 0.3±0.1 eV and 0.8±0.1 g/cm−3, corresponding to a pressure of ∼13 GPa. Inelastic x-ray scattering was used to observe the collective oscillations of the ions. With a highly improved energy resolution of ∼50 meV, we could clearly distinguish the Brillouin peaks from the quasielastic Rayleigh feature. Data at different wave numbers were utilized to derive a sound speed of 5.9±0.5 km/s, marking a high-temperature data point for methane and demonstrating consistency with Birch's law in this parameter regime.

Speed of sound in methane under conditions of planetary interiors

Physical Review Research 6, L022029 (2024)

Authors:

Thomas G White, Hannah Poole, Emma E McBride, Matthew Oliver, Adrien Descamps, Luke B Fletcher, W Alex Angermeier, Cameron H Allen, Karen Appel, Florian P Condamine, Chandra B Curry, Francesco Dallari, Stefan Funk, Eric Galtier, Eliseo J Gamboa, Maxence Gauthier, Peter Graham, Sebastian Goede, Daniel Haden, Jongjin B Kim, Hae Ja Lee, Benjamin K Ofori-Okai, Scott Richardson, Alex Rigby, Christopher Schoenwaelder, Peihao Sun, Bastian L Witte, Thomas Tschentscher, Ulf Zastrau, Bob Nagler, JB Hastings, Giulio Monaco, Dirk O Gericke, Siegfried H Glenzer, Gianluca Gregori

Abstract:

We present direct observations of acoustic waves in warm dense matter. We analyze wave-number- and energy-resolved x-ray spectra taken from warm dense methane created by laser heating a cryogenic liquid jet. X-ray diffraction and inelastic free-electron scattering yield sample conditions of 0.3 ± 0.1 eV and 0.8 ± 0.1 g/cm-3, corresponding to a pressure of ~13 GPa. Inelastic x-ray scattering was used to observe the collective oscillations of the ions. With a highly improved energy resolution of ~50 meV, we could clearly distinguish the Brillouin peaks from the quasielastic Rayleigh feature. Data at different wave numbers were utilized to derive a sound speed of 5.9 ± 0.5 km/s, marking a high-temperature data point for methane and demonstrating consistency with Birch's law in this parameter regime.

Bounds on heavy axions with an X-ray free electron laser

(2024)

Authors:

Jack WD Halliday, Giacomo Marocco, Konstantin A Beyer, Charles Heaton, Motoaki Nakatsutsumi, Thomas R Preston, Charles D Arrowsmith, Carsten Baehtz, Sebastian Goede, Oliver Humphries, Alejandro Laso Garcia, Richard Plackett, Pontus Svensson, Georgios Vacalis, Justin Wark, Daniel Wood, Ulf Zastrau, Robert Bingham, Ian Shipsey, Subir Sarkar, Gianluca Gregori

Electron-beam-based Compton scattering x-ray source for probing high-energy-density physics

Physical Review Accelerators and Beams American Physical Society 27:3 (2024) 034701

Authors:

Hans G Rinderknecht, G Bruhaug, G, Vlad Costin Musat, Gianluca Gregori, Hannah Poole, David Bishel, David A Chin, JR Rygg, GW Collins

Abstract:

The physics basis for an electron-beam-based Compton scattering (ECOS) x-ray source is investigated for single-shot experiments at major high energy density facilities such as the Omega Laser Facility, National Ignition Facility, and Z pulsed power facility. A source of monoenergetic (δϵ/ϵ<5%) 10- to 50-keV x rays can be produced by scattering of a short-pulse optical laser by a 23- to 53-MeV electron beam and collimating the scattered photons. The number and spectrum of scattered photons is calculated as a function of electron packet charge, electron and laser pulse duration, laser intensity, and collision geometry. A source with greater than 1010 photons in a 1-mm radius spot at the OMEGA target chamber center and 100-ps time resolution is plausible with the available electron gun and laser technology. Design requirements for diffraction, inelastic scattering and imaging experiments as well as opportunities for improved performance are discussed.

Narrow bandwidth, low-emittance positron beams from a laser-wakefield accelerator.

Scientific reports 14:1 (2024) 6001

Authors:

MJV Streeter, C Colgan, J Carderelli, Y Ma, N Cavanagh, EE Los, H Ahmed, AF Antoine, T Audet, MD Balcazar, L Calvin, B Kettle, SPD Mangles, Z Najmudin, PP Rajeev, DR Symes, AGR Thomas, G Sarri

Abstract:

The rapid progress that plasma wakefield accelerators are experiencing is now posing the question as to whether they could be included in the design of the next generation of high-energy electron-positron colliders. However, the typical structure of the accelerating wakefields presents challenging complications for positron acceleration. Despite seminal proof-of-principle experiments and theoretical proposals, experimental research in plasma-based acceleration of positrons is currently limited by the scarcity of positron beams suitable to seed a plasma accelerator. Here, we report on the first experimental demonstration of a laser-driven source of ultra-relativistic positrons with sufficient spectral and spatial quality to be injected in a plasma accelerator. Our results indicate, in agreement with numerical simulations, selection and transport of positron beamlets containing N e + ≥ 10 5 positrons in a 5% bandwidth around 600 MeV, with femtosecond-scale duration and micron-scale normalised emittance. Particle-in-cell simulations show that positron beams of this kind can be guided and accelerated in a laser-driven plasma accelerator, with favourable scalings to further increase overall charge and energy using PW-scale lasers. The results presented here demonstrate the possibility of performing experimental studies of positron acceleration in a laser-driven wakefield accelerator.