PHENIX OVERVIEW W.A. Zajc Columbia University for the PHENIX Collaboration Special thanks to J. Mitchell (BNL) for animations * Outline Why Nuclear Physics? Why RHIC? Why…

TeV Gamma-Ray Results and Links to mm-Surveys Gavin Rowell (University of Adelaide) (H.E.S.S. results - for the H.E.S.S. collab.) (Future TeV plans - for the Adelaide group)…

The buoyant force on an object totally submerged in a fluid depends on Fission: Heavy Elements can reduce energy (i.e. increase binding energy per nucleon) by splitting roughly…

Nuclear Astrophysics Working Group Nuclear Astrophysics Working Group Discussion Schedule 6:00 â 6:15 Philippe Collon (p-process: AMS) 6:15 â 6:30 Alan Chen (Classical…

The Power in Sean's Palm By Mark Foster Evening blows across the sky, early stars stretching out like cotton, soft and deep. This is June in Colorado, just past dusk:…

Probing the High-z Universe with Galaxy Counts from Ultra Deep Surveys and the Cosmic Near Infrared Background Eiichiro Komatsu (Univ. of Texas, Austin) Astrophysics Seminar@UCSB…