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Gianluca Gregori

Professor of Physics

Research theme

  • Lasers and high energy density science
  • Plasma physics

Sub department

  • Atomic and Laser Physics

Research groups

  • Laboratory astroparticle physics
  • Oxford Centre for High Energy Density Science (OxCHEDS)
Gianluca.Gregori@physics.ox.ac.uk
Telephone: 01865 (2)82639
Clarendon Laboratory, room 029.8
  • About
  • Publications

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.
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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
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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.
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Achievement of target gain larger than unity in an inertial fusion experiment

Physical Review Letters American Physical Society 132:6 (2024) 065102

Authors:

H Abu-Shawareb, R Acree, P Adams, J Adams, B Addis, R Aden, P Adrian, Bb Afeyan, M Aggleton, L Aghaian, A Aguirre, D Aikens, J Akre, F Albert, M Albrecht, Bj Albright, J Albritton, J Alcala, C Alday, Da Alessi, N Alexander, J Alfonso, N Alfonso, E Alger, Sj Ali, Za Ali, A Allen, We Alley, P Amala, Pa Amendt, P Amick, S Ammula, C Amorin, Dj Ampleford, Rw Anderson, T Anklam, N Antipa, B Appelbe, C Aracne-Ruddle, E Araya, Tn Archuleta, M Arend, P Arnold, T Arnold, A Arsenlis, J Asay, Lj Atherton, D Atkinson, R Atkinson, Jm Auerbach

Abstract:

On December 5, 2022, an indirect drive fusion implosion on the National Ignition Facility (NIF) achieved a target gain G_{target} of 1.5. This is the first laboratory demonstration of exceeding "scientific breakeven" (or G_{target}>1) where 2.05 MJ of 351 nm laser light produced 3.1 MJ of total fusion yield, a result which significantly exceeds the Lawson criterion for fusion ignition as reported in a previous NIF implosion [H. Abu-Shawareb et al. (Indirect Drive ICF Collaboration), Phys. Rev. Lett. 129, 075001 (2022)PRLTAO0031-900710.1103/PhysRevLett.129.075001]. This achievement is the culmination of more than five decades of research and gives proof that laboratory fusion, based on fundamental physics principles, is possible. This Letter reports on the target, laser, design, and experimental advancements that led to this result.
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Classical Larmor formula through the Unruh effect for uniformly accelerated electrons

Physical Review D: Particles, Fields, Gravitation and Cosmology American Physical Society 109 (2024) 024044

Abstract:

We investigate the connection between the classical Larmor formula and the quantum Unruh effect by computing the emitted power by a uniformly accelerated charged particle and its angular distribution in the co-accelerated frame. We consider a classical particle accelerated with non-zero charge only for a finite period and then take the infinite-time limit after removing the effects due to the initial charging and final discharging processes. We show that the result found for the interaction rates agrees with previous studies in which the period of acceleration with non-zero charge was taken to be infinite from the beginning. We also show that the power and angular distribution of emission, which is attributed either to the emission or absorption of a Rindler photon in the co-accelerated frame, is given by the Larmor formula, confirming that, at tree level, it is necessary to take into account the Unruh effect in order to reproduce the classical Larmor radiation formula in the coaccelerated frame.
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