activity
19972025
most citedFundamental differences between SPH and grid methods

623 citations · 5.7k across the 89 of their papers we have counts for

collaborators

89 papers

physics.plasm-ph2025

Measurement of ion acceleration and diffusion in a laser-driven magnetized plasma

J. T. Y. Chu, J. W. D. Halliday, C. Heaton +25

Here we present results from an experiment performed at the GSI Helmholtz Centre for Heavy Ion Research. A mono-energetic beam of chromium ions with initial energies of …

physics.plasm-ph2023★ 28 cited

Laboratory realization of relativistic pair-plasma beams

C. D. Arrowsmith, P. Simon, P. Bilbao +26

Relativistic electron-positron plasmas are ubiquitous in extreme astrophysical environments such as black holes and neutron star magnetospheres, where accretion-powered jets and pu…

physics.plasm-ph2021

Learning Transport Processes with Machine Intelligence

Francesco Miniati, Gianluca Gregori

We present a machine learning based approach to address the study of transport processes, ubiquitous in continuous mechanics, with particular attention to those phenomena ruled by…

physics.plasm-ph2021★ 30 cited

Strong suppression of heat conduction in a laboratory replica of galaxy-cluster turbulent plasmas

J. Meinecke, P. Tzeferacos, J. S. Ross +32

Galaxy clusters are filled with hot, diffuse X-ray emitting plasma, with a stochastically tangled magnetic field whose energy is close to equipartition with the energy of the turbu…

physics.plasm-ph2020★ 48 cited

Time-resolved fast turbulent dynamo in a laser plasma

A. F. A. Bott, P. Tzeferacos, L. Chen +25

Understanding magnetic-field generation and amplification in turbulent plasma is essential to account for observations of magnetic fields in the universe. A theoretical framework a…

physics.plasm-ph2018★ 1 cited

Transport of high-energy charged particles through spatially-intermittent turbulent magnetic fields

L. E. Chen, A. F. A. Bott, P. Tzeferacos +22

Identifying the sources of the highest energy cosmic rays requires understanding how they are deflected by the stochastic, spatially intermittent intergalactic magnetic field. Here…