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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

Quantum Effects on Dynamic Structure Factors in Dense Magnetized Plasmas

(2023)

Authors:

Tushar Mondal, Gianluca Gregori

De Bernardo Stempel, Patrizia (2022). Die sprachliche Analyse der niedergermanischen Votivformulare und Dedikantennamen (Corpus F.E.R.C.AN., II/1). Forschungen zur antiken Religion, 1. Wien: Verlag der 脰sterreichischen Akademie der Wissenschaften

ARYS Antig眉edad Religiones y Sociedades Universidad Carlos III de Madrid (2023) 520-523

Classical Larmor formula through the Unruh effect for uniformly accelerated electrons

(2023)

Authors:

Georgios Vacalis, Atsushi Higuchi, Robert Bingham, Gianluca Gregori

Multi-Messenger Measurements of the Static Structure of Shock-Compressed Liquid Silicon at 100 GPa

(2023)

Authors:

H Poole, MK Ginnane, M Millot, GW Collins, SX Hu, D Polsin, R Saha, J Topp-Mugglestone, TG White, DA Chapman, JR Rygg, SP Regan, G Gregori

Searching for wave-like dark matter with QSHS

SciPost Physics Proceedings SciPost 12 (2023)

Authors:

Ian Bailey, Bhaswati Chakraborty, Gemma Chapman, Edward J Daw, John Gallop, Gianluca Gregori, Edward Hardy, Ling Hao, Edward Laird, Peter Leek, John March-Russell, Phil Meeson, Sea谩rbhan 脫 Peat谩in, Yuri Pashkin, Mitchell G Perry, Michele Piscitelli, Edward Romans, Subir Sarkar, Paul J Smith, Ningqiang Song, Mahesh Soni, Boon Kok Tan, Stephen West, Stafford Withington

Abstract:

In 2021 the Quantum Sensors for the Hidden Sector (QSHS) collaboration was founded in the UK and received funding to develop and demonstrate quantum devices with the potential to detect hidden sector particles in the 渭eV to 100 渭eV mass window. The collaboration has been developing a range of devices. It is building a high-field, low-temperature facility at the University of Sheffield to characterise and test the devices in a haloscope geometry. This paper introduces the collaboration's motivation, aims, and progress.

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