|COOKIES: By using this website you agree that we can place Google Analytics Cookies on your device for performance monitoring.|
Supernova Remnants and Cosmic Rays: An update on recent progress
If you have a question about this talk, please contact David Titterington.
*** Note unusual time ***
Supernovae are some of the most spectacular explosions in the Universe and their shocks produce the most energetic particles detected on Earth. Supernova remnant (SNR) shocks interact with their surrounding medium, heating and compressing it, as well as accelerating particles to cosmic ray (CR) energies, radio, infrared and X-ray observations of these objects make some of the most beautiful images in astrophysics. However, SNRs do not just make pretty pictures, they play crucial roles in the chemical evolution and structure of galaxies, as well as being ideal laboratories for detailed studies of strong shock physics, particle acceleration and magnetic field amplification mechanisms. In this talk I will discuss our studies of X-ray and gamma-ray emission from SNRs, which have allowed us to gain insight into the nature of particle acceleration as well as the interaction of strong shocks with dense media such as molecular clouds. I will present our most recent results on these topics and outline what we want to look into in the future.
This talk is part of the Cavendish Astrophysics Seminars series.
This talk is included in these lists:
Note that ex-directory lists are not shown.
Other listsDying Planet, Living Faith: Religious Contributions to Environmentalism DAMTP Information Theory Seminar The Real Me:
Other talksGlauber Gluons and Multiple Parton Interactions TBC The Prospects for Global Financial Stability Endogenous risk and price-mediated contagion Development and the cell cycle Are there limits to evolution? (Conference 25 & 26 September 2014)