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Slide 1Cosmology and extragalactic astronomy Mat Page Mullard Space Science Lab, UCL Particles in the hot, early Universe. Slide 2 Particles This lecture: Particles in the…
Slide 1Jaap Velthuis (University of Bristol)1 Radiation damage in silicon sensors Topics: –Damage due to protons and neutrons Radiation induced defects Annealing Donor…
Slide 1 Slide 2 Slide 3 Kirchhoff's laws,there are three types of spectra: continuum, emission line, and absorption line. High pressure, high temperature gas Low pressure,…
Sound & Light Chapter 15 Sound Sound waves are caused by vibrations, and carry energy through a medium. Sound waves are longitudinal waves. Speed of sound depends on…
Announcements 10/24/12 Prayer Slinkies: Please turn-in & cross out your name Lab 6 due tonight Exam 2 starts tomorrow, goes through Tuesday evening My office hours today:…
Ch. 6: The Sun Chemical energy? The Sunâs luminosity is about 4x1026 joules per second. Its mass is about 2x1030 kg. What is its energy source? Chemical energy? The Sunâs…