Skip to main content
Home
Department Of Physics text logo
  • Research
    • Our research
    • Our research groups
    • Our research in action
    • Research funding support
    • Summer internships for undergraduates
  • Study
    • Undergraduates
    • Postgraduates
  • Engage
    • For alumni
    • For business
    • For schools
    • For the public
Menu
Space and Planets (artistic image)
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

Measuring Unruh radiation from accelerated electrons

European Physical Journal C Springer 84:5 (2024) 475

Authors:

Gianluca Gregori, Giacomo Marocco, Subir Sarkar, R Bingham, C Wang

Abstract:

Detecting thermal Unruh radiation from accelerated electrons has presented a formidable challenge due not only to technical difficulties but also for lack of conceptual clarity about what is actually seen by a laboratory observer. We give a summary of the current interpretations along with a simpler heuristic description that draws on the analogy between the Unruh effect and radiation from a two-level atomic system. We propose an experiment to test whether there is emission of thermal photons from an accelerated electron.
More details from the publisher
Details from ORA
More details

Multimessenger measurements of the static structure of shock-compressed liquid silicon at 100 GPa

Physical Review Research American Physical Society 6:2 (2024) 023144

Authors:

H Poole, Mk Ginnane, M Millot, Hm Bellenbaum, Gw Collins, Sx Hu, D Polsin, R Saha, J Topp-Mugglestone, Tg White, Da Chapman, Jr Rygg, Sp Regan, G Gregori

Abstract:

The ionic structure of high-pressure, high-temperature fluids is a challenging theoretical problem with applications to planetary interiors and fusion capsules. Here we report a multimessenger platform using velocimetry and in situ angularly and spectrally resolved x-ray scattering to measure the thermodynamic conditions and ion structure factor of materials at extreme pressures. We document the pressure, density, and temperature of shocked silicon near 100GPa with uncertainties of 6%, 2%, and 20%, respectively. The measurements are sufficient to distinguish between and rule out some ion screening models.

More details from the publisher
Details from ORA
More details

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.
More details from the publisher
Details from ORA

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
More details from the publisher
Details from ArXiV

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.
More details from the publisher
Details from ORA
More details

Pagination

  • First page First
  • Previous page Prev
  • Page 1
  • Page 2
  • Page 3
  • Page 4
  • Current page 5
  • Page 6
  • Page 7
  • Page 8
  • Page 9
  • …
  • Next page Next
  • Last page Last

Footer Menu

  • Contact us
  • Giving to the Dept of Physics
  • Work with us
  • Media

User account menu

  • Log in

Follow us

FIND US

Clarendon Laboratory,

Parks Road,

Oxford,

OX1 3PU

CONTACT US

Tel: +44(0)1865272200

University of Oxfrod logo Department Of Physics text logo
IOP Juno Champion logo Athena Swan Silver Award logo

© University of Oxford - Department of Physics

Cookies | Privacy policy | Accessibility statement

Built by: Versantus

  • Home
  • Research
  • Study
  • Engage
  • Our people
  • News & Comment
  • Events
  • Our facilities & services
  • About us
  • Current students
  • Staff intranet