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VERSION:2.0
PRODID:-//Heidelberg University//HePhySTO//EN
CALSCALE:GREGORIAN
BEGIN:VEVENT
DTEND:20261201T163000Z
UID:6b23dd2dc13c8e9ca30f1a325d90423b@physik.uni-heidelberg.de
DTSTAMP:20260814T215213Z
LOCATION:
DESCRIPTION:Theories of galaxy formation\, structure\, and evolution increa
 singly include the effects of cosmic  rays on gas dynamics and energy balan
 ce. This is usually done by treating the cosmic rays as a fluid that is cou
 pled to the thermal gas by magnetic fields on global scales and electromagn
 etic fluctuations on kinetic scales. I will discuss the foundations and ass
 umptions of the fluid model\, assess whether it is correct and complete\,  
 where it can be improved\, and how it can be tested. To arrange a visit wit
 h the speaker during the visit\, please contact their host: Max Gronke\n\nI
 mported from https://www.physik.uni-heidelberg.de/hephysto/ (no warranty fo
 r accuracy).
URL;VALUE=URI:https://www.physik.uni-heidelberg.de/hephysto/index.php?s=tal
 k&id=12902
SUMMARY:Heidelberg Joint Astronomical Colloquium: Ellen Zweibel   - Resetti
 ng Cosmic Ray Propagation Theory
DTSTART:20261201T153000Z
END:VEVENT
END:VCALENDAR