Emission of pairs of Minkowski photons through the lens of the Unruh effect

Physical Review D American Physical Society (APS) (2025)

Steady state rotational dynamics of a weakly ionised hydrogen plasma under cross-field configuration

Physics of Plasmas American Institute of Physics 32:12 (2025) 123505

Authors:

H Muir, N Eschbach, G Rodway-Gant, I Vankov, A Chen, B Wrixon, Z Li, A Gunn, Gianluca Gregori

Abstract:

We study a novel device for generating a high speed rotating plasma. The device weakly ionises and accelerates a hydrogen gas in a co-axial cylindrical chamber via the perpendicular configuration of electrodes with a magnetic field generated by a superconducting magnetic. It has been hypothesised that extreme velocities and plasma particle compression could be achieved under this configuration1 . This work develops a rigorous theoretical model of the bulk plasma dynamics under steady state centrifugal operation. By exploiting the axisymmetry of the system, and from application of problem-specific governing assumptions, a steady state 1D model for the rotational dynamics of the bulk plasma is derived. From here, we present fully analytical solutions for the radial profiles of the MHD model: [azimuthal velocity, particle densities, pressure] and a semi-analytical solution for electric potential. Tables of selfconsistent plasma parameters are computed to provide a comprehensive characterisation of the bulk plasma state. The model is able to determine the peak velocities and plasma compression, and permits parametric studies to elucidate the complex and non-linear relationships between operational device settings and the achieved steady state plasma state condition. The new theoretical solutions therefore provide necessary insights into the viability of the novel device for high energy-density plasma applications.

Multi-messenger dynamic imaging of laser-driven shocks in water using a plasma wakefield accelerator.

Nature communications 17:1 (2025) 529

Authors:

Mario D Balcazar, Hai-En Tsai, Tobias M Ostermayr, Paul Campbell, Matthew R Trantham, Félicie Albert, Qiang Chen, Cary Colgan, Gilliss M Dyer, Zachary Eisentraut, Eric Esarey, Elizabeth S Grace, Benjamin Greenwood, Anthony J Gonsalves, Sahel Hakimi, Robert Jacob, Brendan Kettle, Paul King, Karl Krushelnick, Nuno Lemos, Eva E Los, Yong Ma, Stuart PD Mangles, John Nees, Isabella M Pagano, Carl B Schroeder, Raspberry A Simpson, Anthony V Vazquez, Jeroen van Tilborg, Cameron GR Geddes, Alexander GR Thomas, Carolyn C Kuranz

Abstract:

Understanding dense matter hydrodynamics is critical for predicting plasma behavior in environments relevant to laser-driven inertial confinement fusion. Traditional diagnostic sources face limitations in brightness, spatiotemporal resolution, and in their ability to detect relevant electromagnetic fields. In this work, we present a dual-probe, multi-messenger laser wakefield accelerator platform combining ultrafast X-rays and relativistic electron beams at 1 Hz, to interrogate a free-flowing water target in vacuum, heated by an intense 200 ps laser pulse. This scheme enables high-repetition-rate tracking the evolution of the interaction using both particle types. Betatron X-rays reveal a cylindrically symmetric shock compression morphology assisted by low-density vapor, resembling foam-layer-assisted fusion targets. The synchronized electron beam detects time-evolving electromagnetic fields, uncovering charge separation and ion species differentiation during plasma expansion - phenomena not captured by photons or hydrodynamic simulations. We show that combining both probes provides complementary insights spanning kinetic to hydrodynamic regimes, highlighting the need for hybrid physics models to accurately predict fusion-relevant plasma behavior.

Structural evolution of iron oxides melts at Earth's outer-core pressures

(2025)

Authors:

Cà line Crépisson, Mila Fitzgerald, Domenic Peake, Patrick 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, Zuzana KonôpkovÃ, 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

Suppression of pair beam instabilities in a laboratory analogue of blazar pair cascades

Proceedings of the National Academy of Sciences National Academy of Sciences 122:45 (2025) e2513365122

Authors:

Charles Arrowsmith, Francesco Miniati, Pablo J Bilbao, Pascal Simon, Archie Bott, Stephane Burger, Hui Chen, Filipe D Cruz, Tristan Davenne, Anthony Dyson, Ilias Efthymiopoulos, Dustin H Froula, Alice Goillot, Jon T Gudmundsson, Dan Haberberger, Jack WD Halliday, Thomas Hodge, Brian T Huffman, Sam Iaquinta, G Marshall, Brian Reville, Subir Sarkar, Alexander Schekochihin, Luis O Silva, Raspberry Simpson, Vasiliki Stergiou, Raoul MGM Trines, Thibault Vieu, Nikolaos Charitonidis, Robert Bingham, Gianluca Gregori

Abstract:

The generation of dense electron-positron pair beams in the laboratory can enable direct tests of theoretical models of γ-ray bursts and active galactic nuclei. We have successfully achieved this using ultrarelativistic protons accelerated by the Super Proton Synchrotron at (CERN). In the first application of this experimental platform, the stability of the pair beam is studied as it propagates through a meter-length plasma, analogous to TeV γ-ray-induced pair cascades in the intergalactic medium. It has been argued that pair beam instabilities disrupt the cascade, thus accounting for the observed lack of reprocessed GeV emission from TeV blazars. If true, this would remove the need for a moderate strength intergalactic magnetic field to explain the observations. We find that the pair beam instability is suppressed if the beam is not perfectly collimated or monochromatic, hence the lower limit to the intergalactic magnetic field inferred from γ-ray observations of blazars is robust.