The Physics and Cosmology of TeV Blazars

«   »
Su Mo Tu We Th Fr Sa
30 31 1 2 3 4 5
6 7 8 9 10 11 12
13 14 15 16 17 18 19
20 21 22 23 24 25 26
27 28 29 30 1 2 3
Date/Time:Monday, 21 Oct 2013 from 4:10 pm to 5:00 pm
Location:Physics 0003
Actions:Download iCal/vCal | Email Reminder
Philip Chang (University of Wisconsin-Milwaukee)

The universe is teeming with very high energy gamma ray sources (> 100 GeV), but it is generally thought that their impact on the universe is minor at best. On energetic grounds, this assumption seems well-founded because the energy density in TeV photons is 0.2% of that of ionizing photons from quasars. However, as I hope to show in this talk, this is not the case. Rather, the greater efficiency by which TeV photons can be converted to heating in the intergalactic medium (IGM) allows TeV blazars dominate the heating of the IGM at low redshift. I will discuss the nature of this conversion via beam instabilities. I will then discuss how the resultant heating from these TeV sources makes dramatic differences in the formation of structure in the universe. In particular, I will discuss how it gives rise to the inverted temperature-density profile of the IGM, the bimodality of galaxy clusters, and the paucity of dwarf galaxies in galactic halos and voids.

For more information, please visit

Philip Chang is an assistant professor of Physics at the University of Wisconsin-Milwaukee studying aspects of theoretical astrophysics and cosmology. He is interested in supernovae, compact objects, disk dynamics, plasma astrophysics, and turbulent star formation. He is originally from New York and earned his Ph.D. in Physics in 2005 from UCSB under the direction of Professor Lars Bildsten (Director and Permanent Member of the KITP). He then moved on to the Department of Astronomy at UC Berkeley as a Miller and TAC Fellow from 2005-2009. From 2009-2011, he was a postdoctoral fellow at CITA. From 2011 onward, he has been a member of the faculty at the University of Wisconsin-Milwaukee.