SSL Colloquium: Christoph Weniger

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Christoph Weniger (Max-Planck-Institut für Physik, Germany) will present the SSL colloquium on May 3rd: `Recently, we identified a tentative gamma-ray line in the Galactic center
observations of the Fermi LAT, which would be an unequivocal smoking-gun
signature for dark matter annihilation in the Universe. One year after
discovery, the signature is still as ambiguous as it could be. I discuss
recent experimental and theoretical developments and show how the situation
could be clarified until end of next year.’

Clusters of Galaxies And The Constituents of Material In And Around Clusters of Galaxies

Richard Lieu, Dept. of Physics, University of Alabama in Huntsville

SSL Addition Conference Room at 3pm Tuesday December 18th

Since the mid 1990’s it has been increasingly apparent that material in and around clusters of  galaxies is multi-phased, consisting of dark matter and hot, virialized X-ray emitting gas, and also cooler gases and possibly non-thermal particles. The early evidence for the latter two components was from  EUV and soft X-ray observations from which it was inferred that a warm gas component lies predominantly at the outskirts of the cluster while relativistic particles may exist in the inner parts. Continue reading