ESS End-to-End Optics and Layout Integration Håkan Danared European Spallation Source Catania, 6 July 2011.
Colloquium, UC Riverside, J. Brau, October 31, 2002 1 The Next Linear Collider and the Origin of Electroweak Physics Jim Brau UC Riverside October 31,
P. Grannis – Snowmass Workshop July 1, 2001 Any major new accelerator facility should address the big questions of particle physics research for the next.
What can an e + e - Linear Collider teach us ? P. Grannis/PHENO 2001 May 7, 2001 Understanding the source of electroweak symmetry breaking is the most.
P. Grannis; Oct. 27, 2000 1.Physics capability at ~ 500 GeV -- highlights 2.Special operating conditions 3.What energy/luminosity will we ultimately need?
The Case for a 500 GeV Linear Collider P. Grannis HEPAP subpanel meeting SLAC, May 23, 2001 Understanding the source of electroweak symmetry breaking.
P. Grannis; Oct. 27, 2000
P. Grannis – Snowmass Workshop July 1, 2001
