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Yoan Rappaz

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Magnetic fields in the weakly collisional plasma of galaxy clusters: from amplification mechanisms to observables

Yoan Rappaz

Magnetic fields are ubiquitous in the Universe and observed in various astrophysical systems, with different amplitudes. In galaxy clusters, they are typically on the order of a few

\mu\mathrm{G}

. Comparing this value with the amplitude of magnetic seed ...

EPFL2024

Yoan Rappaz

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Magnetic fields in the weakly collisional plasma of galaxy clusters: from amplification mechanisms to observables

The effect of pressure-anisotropy-driven kinetic instabilities on magnetic field amplification in galaxy clusters

Cosmic evolution of the Faraday rotation measure in the intracluster medium of galaxy clusters

The effect of pressure-anisotropy-driven kinetic instabilities on magnetic field amplification in galaxy clusters

Cosmic evolution of the Faraday rotation measure in the intracluster medium of galaxy clusters

Magnetic fields in the weakly collisional plasma of galaxy clusters: from amplification mechanisms to observables