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The top documents tagged [photodisintegration]
X-RAY INTERACTION WITH MATTER. COLLIMATE OR NOT TO COLLIMATE?! SCATTER
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Stars & The Sun If you want to make an apple pie from scratch, you must first create the Universe- Carl Sagan
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The Collective Model Aard Keimpema. Contents Vibrational modes of nuclei Deformed nuclei Rotational modes of nuclei Coupling between rotational and vibrational
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1. accretion disk - flat disk of matter spiraling down onto the surface of a star. Often from a companion star
216 views
Simulation Parameters and Results We performed nine simulations to test the sensitivity of our results to resolution, viscous stress-to-pressure ratio
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The s-process Fe Co Ni Rb Ga Ge Zn Cu Se Br As Zr Y Sr Kr (n, ) ()() ()() r-process p-process 63 Ni, t 1/2 =100 a 64 Cu, t 1/2 =12 h, 40 % (
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Chapter 17: Evolution of High-Mass Stars. Massive stars have more hydrogen to start with but they burn it at a prodigious rate The overall reaction is
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Development of Giant Air Shower in Earth’s Atmosphere
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Lecture 2: Formation of the chemical elements Bengt Gustafsson: Current problems in Astrophysics Ångström Laboratory, Spring 2010
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AGASA results Anisotropy of EHE CR arrival direction distribution
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The Reactions The Main Sequence – The P – P Chain
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Study of high energy cosmic rays with the sparse very large air shower array ALTA/CZELTA
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