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Credit: hdwallpaperim.com/

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

Statistical theory of electronic degrees of freedom in wave packet molecular dynamics

Physical Review E American Physical Society (APS) 114:1 (2026) 15219

Authors:

Daniel Plummer, Pontus Svensson, Wiktor Jasniak, Patrick Hollebon, Sam M Vinko, Gianluca Gregori

Abstract:

<jats:p>We derive statistical distributions for the degrees of freedom in wave packet molecular dynamics models. Specifically, a theory is developed for the width distributions of Gaussian wave packets in both isotropic and anisotropic formulations. The resulting distribution functions show good agreement with molecular dynamics data under warm dense matter conditions, providing practical guidance for constraining the confining potential, an empirical parameter in the model. We also discuss how these distributions influence the resulting effective Coulomb interactions.</jats:p>
More details from the publisher

Roadmap for warm dense matter physics

Plasma Physics and Controlled Fusion 68:7 (2026)

Authors:

Jan Vorberger, Frank Graziani, David Riley, Andrew D Baczewski, Isabelle Baraffe, Mandy Bethkenhagen, Simon Blouin, Maximilian P Böhme, Michael Bonitz, Michael Bussmann, Alexis Casner, Witold Cayzac, Peter Celliers, Gilles Chabrier, Nicolas Chamel, Dave Chapman, Mohan Chen, Jean Clérouin, Gilbert Collins, Federica Coppari, Tilo Döppner, Tobias Dornheim, Luke B Fletcher, Dirk O Gericke, Siegfried Glenzer, Alexander F Goncharov, Gianluca Gregori, Sebastien Hamel, Stephanie B Hansen, Nicholas J Hartley, Suxing Hu, Omar A Hurricane, Valentin V Karasiev, Joshua J Kas, Brendan Kettle, Thomas Kluge, Marcus D Knudson, Alina Kononov, Zuzana Konôpková, Dominik Kraus, Andrea Kritcher, Sophia Malko, Gérard Massacrier, Burkhard Militzer, Zhandos A Moldabekov, Michael S Murillo, Bob Nagler, Nadine Nettelmann, Paul Neumayer, Benjamin K Ofori-Okai

Abstract:

This roadmap presents the state-of-the-art, current challenges and near future developments anticipated in the thriving field of warm dense matter (WDM) physics. Originating from strongly coupled plasma physics, high pressure physics and high energy density science, the WDM physics community has recently taken a giant leap forward. This is due to spectacular developments in laser technology, diagnostic capabilities, and computer simulation techniques. Only in the last decade has it become possible to perform accurate enough simulations & experiments to truly verify theoretical results as well as to reliably design experiments based on predictions. Consequently, this roadmap discusses recent developments of and contemporary challenges for theoretical methods and experimental techniques needed to describe, create and diagnose WDM. A large part of this roadmap is dedicated to specific WDM systems and applications in astrophysics, inertial confinement fusion and novel material synthesis.
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Structural evolution of iron oxides melts at Earth’s outer-core pressures

Nature Communications Springer Nature (2026)

Authors:

Céline Crépisson, Mila Fitzgerald, Domenic Peake, Patrick G Heighway, Thomas Stevens, Adrien Descamps, David McGonegle, Alexis Amouretti, Karim K Alaa El-Din, Michal Andrzejewski, Sam Azadi, Erik Brambrink, Carolina Camarda, David A Chin, Samuele Di Dio Cafiso, Ana Coutinho Dutra, Hauke Höppner, Kohdai Yamamoto, Phani S Karamched, Zuzana Konôpková, Motoaki Nakatsutsumi, Norimasa Ozaki, Danae N Polsin, Jan-Patrick Schwinkendorf, Georgiy Shoulga, Cornelius Strohm, Minxue Tang, Harry Taylor, Monika Toncian, Yizhen Wang, Jin Yao, Gianluca Gregori, Justin S Wark, Karen Appel, Marion Harmand, Sam M Vinko

Abstract:

Oxygen and other light elements comprise up to 5 wt% of the Earth’s outer-core, and may significantly influence its physical properties and the operation of the geodynamo. Here we report in situ X-ray diffraction measurements of Fe, Fe + 4.5 FeO (atomic proportion), and Fe2O3 melts at 177-440 GPa, achieved using laser-driven shock compression at an x-ray free-electron laser. The melts exhibit Fe-O coordination numbers between 4.0(0.4) and 4.5(0.4), indicating predominantly four-fold coordination environments. These coordination states are significantly smaller than those of Fe-bearing lower-mantle phases such as bridgmanite and ferropericlase. Shorter Fe-Fe interatomic distances in compressed iron oxide melts drive the denser packing relative to ambient melts, while the structural differences between Fe + 4.5 FeO and Fe2O3 melts under shock indicate that the oxidation state modulates oxygen solubility in liquid Fe. At 177 GPa ( ~ 380 km below the core-mantle boundary) and 3800 K, Fe2O3 melts exhibit higher Fe-O coordination, suggesting that local variations in oxygen content could contribute to the stratification in the uppermost outer-core inferred from seismological and geomagnetic observations.
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Photon accelerator in magnetized electron–ion plasma

New Journal of Physics IOP Publishing 28:6 (2026) 064302

Authors:

SV Bulanov, SS Bulanov, TZ Esirkepov, G Gregori, GM Grittani, M Lamač, BK Russell, AGR Thomas, P Valenta

Abstract:

Strong magnetic fields and plasmas are intrinsically linked in both terrestrial laboratory experiments and in space phenomena. One of the most profound consequences of that is the change in relationship between the frequency and the wave number of electromagnetic waves propagating in plasma in the presence of such magnetic fields when compared to the case without these fields. Furthermore, magnetic fields alter electromagnetic wave interaction with relativistic plasma waves, resulting in different outcomes for particle and radiation generation. For a relativistic plasma wave-based photon acceleration this leads to an increased frequency gain and, thus, potentially to higher efficiency. The influence of a magnetic field leads to quantitative and qualitative change in the properties of photon acceleration, amplifying the increase in the electromagnetic wave frequency.
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Details from ORA

Electron-ion equilibration in superheated gold

Nature Communications (2026)

Authors:

Travis D Griffin, Dirk O Gericke, Daniel Haden, Hae Ja Lee, Eric Galtier, Eric Cunningham, Dimitri Khaghani, Michael Larsen, Lennart Wollenweber, Ben Armentrout, Carson Convery, Karen Appel, Gilliss Dyer, Luke B Fletcher, Sebastian Göde, JB Hastings, Jeremy Iratcabal, Emma E McBride, Jacob Molina, Giulio Monaco, Landon Morrison, Hunter Stramel, Sameen Yunus, Ulf Zastrau, Siegfried H Glenzer, Gianluca Gregori, Bob Nagler, Thomas G White

Abstract:

Electron-ion equilibration dynamics in samples driven into superheated states with multi-eV electron temperatures represent a fundamental process in nonequilibrium physics. A clear picture of the evolving ion temperature is essential for understanding the strength of the electron-ion coupling. However, direct, model-independent measurements of the ion temperature in laser-irradiated samples have remained experimentally elusive. Using inelastic X-ray scattering with meV-resolution in gold samples, the ion response to ultrafast heating by the hot electrons can be resolved, quantifying the electron-ion equilibration dynamics. We report measurements revealing a strongly enhanced energy transfer rate compared to that in weakly excited gold. Moreover, we obtain a quasi-constant electron-ion coupling at the highly elevated electron temperatures. These results place new constraints on electron-ion energy transfer in warm dense matter and establish a path toward quantitative benchmarking of models for nonequilibrium dynamics.
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