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Dissecting the Sequence of Reactions in Proton Fusion
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Classroom Contents
Why Stars Shine - Introduction to Astrophysics
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- 1 The Sun's Luminosity and Age Suggest an Energy Source
- 2 Kelvin´s Colleagues Reveal Solar Nuclear Fusion
- 3 Basic Nuclear Physics Shows Low Energy Binding
- 4 The Most Stable Possible Nuclei are Revealed
- 5 Positive Nuclei Result in Fusion, Fission, and Decay
- 6 Symmetry Energy Explains the Binding Energy Curve
- 7 Mostly Hydrogen, the Sun Fuses It to Helium to Shine
- 8 E=mc2 Reveals Exchange Rates for Energy and Mass
- 9 What the Energy Emission Rate Reveals
- 10 Dissecting the Sequence of Reactions in Proton Fusion
- 11 Quantum Theory Aids Protons in Fusing
- 12 Instability of Helium-2 Nucleus Solved
