Large scale structure, the Warm-Hot IGM and giant radio galaxies

Mathematics – Logic

Scientific paper

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Active Galactic Nuclei / Quasars, Atca

Scientific paper

One of the key challenges today is to account for nearly half of the baryons in the present day universe that are missing. These missing baryons are thought to pervade the moderate over-density filaments (with fractional overdensity ~ 10 to 100) of the large-scale structure as a Warm-Hot intergalactic medium (WHIM) of 10^5 to 10^7 K gas. The state of the gas is a consequence of the hydrodynamic infall heating and, more importantly, the astrophysical feedbacks on the environment from galaxy formation and evolution. We propose to use a sample of giant radio galaxies embedded in the filaments, with radio jets that interact with the gas beyond and outside of their host galaxy, as a probe of the WHIM. Modeling the jet-WHIM interaction and the evolution of the radio synchrotron plasma lobes in the gas and gravitational field of the surrounding large-scale structure constitutes a novel method of constraining the physical parameters and cosmological evolution of the WHIM gas, and thereby assessing the importance of feedback from galaxy evolution on the state of this gas.

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