The Origin of Mass - Exploring the Higgs Sector at the Large Hadron Collider with ATLAS Markus Schumacher, Universität Bonn Particle Physics Seminar, HU.
Discordant Estimates of Mass-Loss Rates for O-Type Stars Alex Fullerton STScI /HIA Derck Massa (STScI/SGT) & Raman Prinja (UCL)
Spectroscopic Transits. The Rossiter-McClaughlin Effect 1 1 0 +v –v 2 3 4 2 3 4 The R-M effect occurs in eclipsing systems when the companion crosses.
Thomas Lohse Humboldt-Universität zu Berlin Thomas Lohse Humboldt-Universität zu Berlin Stuff and Glue Particles and Forces Experimental methods What is.
Mini-Unit: Light Day 1 - Notes. What is light? Light can be described as a ray, a wave, and a particle.
16-1 Energy in Earth’s Atmosphere (pages 542–545) 1. State in what form energy travels from the sun to the earth. 2. Explain what happens to the sun’s.
Inelastic Subproject Report B. Fultz, Caltech Scope of Science in WBS 10 Tasks and goals of the DANSE subproject Release Plans Risks and Challenges.
Short pulses in optical microscopy Ivan Scheblykin, Chemical Physics, LU Outline: Introduction to traditional optical microscopy based on single photon.
March 25, 2015 “Wavestown” sheet 1.Label the 7 types of EM waves 2.Try to list as many uses or locations for EM radiation in the picture 3.Take out notes.
REMINDERS Exam II next Thursday, April 14! Practice exam will be posted on website - Same format as first exam – Multiple Choice & Short Answer Review.
Ultra High Speed InP Heterojunction Bipolar Transistors Mattias Dahlström Trouble is my business, (Raymond Chandler)
Tunneling in Complex Systems: From Semiclassical Methods to Monte Carlo simulations Joachim Ankerhold Theoretical condensed matter physics University of.