4–9 Dec 2015
International Conference Centre Geneva
Europe/Zurich timezone
THE REGISTRATION IS OPEN

Cosmic magnetic fields and ways of probing them

6 Dec 2015, 14:00
25m
Level 2, Room 13 (International Conference Centre Geneva)

Level 2, Room 13

International Conference Centre Geneva

17 Rue de Varembé, 1211 Geneva

Speaker

Prof. Philipp Kronberg (University of Toronto)

Description

In this talk I focus on magnetic probes and related discoveries of the physical state of space between stars and galaxies. It begins with the Milky Way disc, then clusters of galaxies, magnetic fields in the megaparsec scale filaments of Large Scale Structure (LSS), and cosmological voids. I discuss the energetics, some the physical, and gas dyamical basics, and the measurement techniques used to date – with the aim of communicating a sense of possibilities for future improvement. I discuss an emerging convergence between particle accelerators such as at CERN, Cosmic Rays, and astrophysical jets -- on scales of kpc – Mpc. I include observation – based estimates of the largest energy transfers in the extragalactic Universe. These appear largely electromagnetic, and involve recently estimated currents of $\sim 10^{18}$ Amperes. The jets feed into very large, magnetised CR clouds having accumulated energies of up to $10^{61}$ ergs. The jets are powered by supermassive black holes in galactic nuclei, and provide a measurable, and surprisingly efficient conversion of gravitational infall energy to electromagnetic and cosmic ray energy. Finally, I show how electric circuit models are helpful in understanding energy flows from galaxy nuclei into intergalactic space.

Author

Prof. Philipp Kronberg (University of Toronto)

Presentation materials

There are no materials yet.