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Minnesota Institute for Astrophysics

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Presentation on theme: "Minnesota Institute for Astrophysics"— Presentation transcript:

1 Minnesota Institute for Astrophysics
N Langer PDF Minnesota Institute for Astrophysics

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Georges Lemaître Came up with a theory of the expansion of the universe, based on Einstein’s GR. "the Cosmic Egg exploding at the moment of the creation" Minnesota Institute for Astrophysics

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Ylem, the hot cosmic soup at the beginning George Gamow Fred Hoyle Minnesota Institute for Astrophysics

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Alas, Gamov could not get past the ‘barrier’ at mass 5. Mr. Tomkins leaps the mass 5 gap! Minnesota Institute for Astrophysics

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Burbidge, Burbidge, Fowler and Hoyle Minnesota Institute for Astrophysics

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Nuclear Shell Model Minnesota Institute for Astrophysics

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Solar Neutrnio Experiment Minnesota Institute for Astrophysics

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The pp-chain reactions starts at temperatures around 4×106 K making it the dominant energy source in smaller stars. A self-maintaining CNO chain starts at approximately 15×106 K, but its energy output rises much more rapidly with increasing temperatures. At approximately 17×106 K, the CNO cycle starts becoming the dominant source of energy. The Sun has a core temperature of around 15.7×106 K, and only 1.7% of 4He nuclei produced in the Sun are born in the CNO cycle. Minnesota Institute for Astrophysics

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Book eqs. 6.25, 6.26 Minnesota Institute for Astrophysics

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The half-life of 5Li is 3.7×10−22 s and that of 8Be is 6.7×10−17 s Need a RESONANCE to up the reaction rate. The beryllium-8 ground state has almost exactly the energy of two alpha particles. In the second step, 8Be + 4He has almost exactly the energy of an excited state of 12C. Minnesota Institute for Astrophysics

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