The lecture on nuclear reactions is presented in two parts. Nuclear reaction notation is introduced. The role of energetics in nuclear reactions is discussed and evaluated, including Q value, reaction barriers, and threshold energy. Center of mass and laboratory frames are discussed. The different processes involved in the formation of isotopes is provided including photonuclear processes. Reaction energetics, mechanisms and types are described. Nuclear reaction cross sections are described, with a presentation on values and limits given. This includes role of angular momentum in cross section values. The stellar production of elements is presented in terms of nuclear reactions. These provide the basis for understanding the formation of isotopes in stars. Part one is 27 minutes, part 2 is 36 minutes. The lecture is assigned on Monday 30 January 2017 and due Saturday 4 February 2017.
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DeleteI am confused about question 2. What explains the the large cross section?
ReplyDeleteI correlated it to the de Broglie wavelength of thermal neutrons but I'm not sure if that is correct!
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