Working Group 1: Radiative QED Plasmas

Leader: Marija Vranic

Co-Leader: Indrek Vurm

Research

This group focuses on plasmas where radiation and quantum processes—such as electron-positron pair production—strongly influence plasma dynamics in both astrophysical and laboratory environments.

Key Scientific Questions

  • How does radiation and pair production affect the physics of dissipation processes such as shocks, magnetic reconnection, and turbulence?
  • What are the observational signatures of radiative QED processes?
  • Can laboratory experiments probe these processes and validate underlying models?

Key Objectives / Main Tasks

  • Conduct a systematic comparison of numerical methods (e.g. PIC, MHD, Monte Carlo, radiative transfer), establish their domains of validity, and identify current gaps.
  • Map the parameter regimes where laboratory experiments can access astrophysically relevant conditions and benchmark simulations.
  • Coordinate the use of observational constraints to guide theoretical and numerical development, and use models to inform observational strategies.

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To learn more about WG1 research, please contact the working group leader. To join a working group, please apply via the COST website.

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