29 June 2026 to 3 July 2026
EICC, Edinburgh
Europe/London timezone

Kinetic Instabilities in Extreme Plasma Physics: Laboratory and Astrophysical Dynamics

Not scheduled
20m
EICC, Edinburgh

EICC, Edinburgh

150 Morrison St, Edinburgh EH3 8EE
Plenary and Invited Presentation Fundamental Plasma Physics - Theory (BSAP)

Description

Extreme plasma physics concerns regimes in which strong electromagnetic fields, intense radiation, and matter–antimatter pair production fundamentally alter kinetic plasma behaviour. Such conditions arise in pulsar and black-hole magnetospheres, relativistic shocks, and are increasingly accessible in laboratory experiments. This thesis addresses two central components of this field: radiative plasma kinetics and electron–positron pair-plasma dynamics.
A kinetic model for radiatively dominated plasmas is developed using analytical theory and large-scale particle-in-cell simulations. Synchrotron cooling in strongly magnetized collisionless plasmas is shown to drive phase-space bunching, generically producing anisotropic ring-shaped momentum distributions with population inversion, i.e., ∂ f /∂ p⊥ > 0. These non-equilibrium states are unstable to the electron cyclotron maser instability (ECMI). Radiation reaction sustains the phase-space bunching, maintaining coherent emission beyond classical saturation. An analogous radiation-reaction–driven mechanism also arises in plasma wakefield accelerators, where betatron cooling induces amplitude bunching and ring-like phase-space structures in relativistic beams, enabling coherent emission via the ion-channel laser instability.
The thesis further investigates the collective behaviour of relativistic electron–positron plasmas, with contributions to the first laboratory generation of high-density, quasi-neutral pair beams at CERN’s SPS and led three-dimensional kinetic simulations demonstrating that realistic energy spread and angular divergence suppress current-filamentation growth. Additional non-ideal effects, including charge imbalance and multi-species components, were also analysed. This improved understanding of pair-beam instabilities establishes experimental constraints relevant to γ-ray–induced pair cascades and limits on the intergalactic magnetic field.
Together, these studies advance a unified kinetic description of extreme plasmas encompassing both radiative effects and pair-plasma dynamics.

Author

Dr Pablo Bilbao (GoLP/Instituto de Plasmas e Fusão Nuclear, Instituto Superior Técnico, Universidade de Lisboa, 1049-001 Lisbon, Portugal)

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