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Course: M 125, Fall 2009
School: Washington
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Energy Losses and Gravitational RadiationEnergy loss processes Now, we need to consider energy loss processes. Ask class: what are ways in which high-energy particles can lose energy? Generically, can lose energy by interacting with photons or other
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X-ray bursts Last time we talked about one of the major differences between NS and BH: NS have strong magnetic fields. That means that "hot spots" can be produced near the magnetic poles, leading to pulsations (this general statement is true for both
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Low-Energy Cosmic Rays Cosmic rays, broadly defined, are charged particles from outside the solar system. These can be electrons, protons, or ions; the latter two dominate the number observed. They are called cosmic "rays" because initially it was th
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Frontiers: Ultra High Energy Cosmic Rays We now focus on cosmic rays with almost unimaginable energies: 1019 eV and beyond. The very highest energy cosmic rays have energies in excess of 50 Joules(!), which is comparable to a tennis ball hit at 150 k
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Hydrogen exchange in proteins and nucleic acidsReading assignment: Raschke TM, Marqusee S. "Hydrogen exchange studies of protein structure" Curr Opin Biotechnol. 1998 Feb;9(1):80-6. Review. Englander SW, Sosnick TR, Englander JJ, Mayne L. "Mechanism
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