'Nuclear reaction rates' diaporamas de présentation

The Interior of Stars II

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Do your course evaluations. pa.uky

Do your course evaluations. http://www.pa.uky.edu I will add 5 points on your final exam if you complete the evaluation. C. Particles begin to form. At around 10 -6 seconds, particles begin to form. During this time quarks and anti-quarks where forming from radiant energy.

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Chapter 15: The Sun: A Nuclear Powerhouse

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Lecture 13

Lecture 13. Review: Static Stellar structure equations. Hydrostatic equilibrium:. Equation of state:. Mass conservation:. Energy generation:. Polytrope. or. Radiation. Convection. The Solar model. In this way we can build up a model of the interior structure of the Sun

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Stellar Structure

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Astrophysics with DRAGON: The 26g Al (p,?) 27 Si Reaction Heather Crawford a,1 for the DRAGON Collaborati

H 2. 27 Si. 26 Al. ?. Gas Target. 26 Si. 27 Si. 28 Si. ?. 25 Al. 26 Al. 27 Al. 24 Mg. 25 Mg. 26 Mg. The DRAGON Facility at ISAC-TRIUMF

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