F.Halzen: IceCube

VIA Lecture by Prof. Francis Halzen "IceCube and the Discovery of High-Energy Cosmic Neutrinos" was given on
24.04.2015.
The following questions were put and comments made during it.
Shantanu: Just a clarification. You mean fireball model of GRBs is ruled out?
Shantanu: Maybe you mentioned this, but is Anita sensitive to the flux of these Tev neutrinos detected by Icecube?
Shantanu: I presume there is no contamination/background from charm neutrinos?
You are welcome to continue discussion of this exciting problem in replies to this post.
24.04.2015.
The following questions were put and comments made during it.
Shantanu: Just a clarification. You mean fireball model of GRBs is ruled out?
Shantanu: Maybe you mentioned this, but is Anita sensitive to the flux of these Tev neutrinos detected by Icecube?
Shantanu: I presume there is no contamination/background from charm neutrinos?
You are welcome to continue discussion of this exciting problem in replies to this post.