Dynamics of rising magnetized cavities and UHECR acceleration in clusters of galaxies

Details Dynamics of rising magnetized cavities and UHECR acceleration in clusters of galaxies Dynamics of rising magnetized cavities and UHECR acceleration in clusters of galaxies

2011-05-30

arxiv.org/abs/1105.6092v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

9 pages

Scientific paper

We study the expansion of low density cavities produced by Active Galactic Nuclei jets in clusters of galaxies. The long term stability of these cavities requires the presence of linked magnetic fields. We find solutions describing the self-similar expansion of structures containing large-scale electromagnetic fields. Unlike the force-free spheromak-like configurations, these solutions have no surface currents and, thus, are less susceptible to resistive decay. The cavities are internally confined by external pressure, with zero gradient at the surface. If the adiabatic index of the plasma within the cavity is $\Gamma>4/3$, the expansion ultimately leads to the formation of large-scale current sheets. The resulting dissipation of the magnetic field can only partially offset the adiabatic and radiative losses of radio emitting electrons. We demonstrate that if the formation of large-scale current sheets is accompanied by explosive reconnection of the magnetic field, the resulting reconnection layer can accelerate cosmic rays to ultra high energies. We speculate that the enhanced flux of UHECRs towards Centaurus A originates at the cavities due to magnetic reconnection.

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