Chapter: Chapter 43
Learning Objectives
LO 43.1.0 Solve problems related to nuclear fission.
LO 43.1.1 Distinguish atomic and nuclear burning, noting that in both processes energy is
produced because of a reduction of mass.
LO 43.1.2 Define the fission process.
LO 43.1.3 Describe the process of a thermal neutron causing a 235U to undergo fission, and
explain the role of the intermediate compound nucleus.
LO 43.1.4 For the absorption of a thermal neutron, calculate the change in the system’s mass and
the energy put into the resulting oscillation of the intermediate compound nucleus.
LO 43.1.5 For a given fission process, calculate the Q value in terms of the binding energy per
nucleon.
LO 43.1.6 Explain the Bohr–Wheeler model for nuclear fission, including the energy barrier.
LO 43.1.7 Explain why thermal neutrons cannot cause 238U to undergo fission.
LO 43.1.8 Identify the approximate amount of energy (MeV) in the fission of any high-mass
nuclide to two middle-mass nuclei.
LO 43.1.9 Relate the rate at which nuclei fission and the rate at which energy is released.
LO 43.2.0 Solve problems related to the nuclear reactor.
LO 43.2.1 Define chain reaction.
LO 43.2.2 Explain the neutron leakage problem, the neutron energy problem, and the neutron
capture problem.
LO 43.2.3 Identify the multiplication factor and apply it to relate the number of neutrons and
power output after a given during of cycles to the initial number of neutrons and power output.
LO 43.2.4 Distinguish subcritical, critical, and supercritical.
LO 43.2.5 Describe the control over the response time.
LO 43.2.6 Give a general description of a complete generation.
LO 43.3.0 Solve problems related to a natural nuclear reactor.
LO 43.3.1 Describe the evidence that a natural nuclear reactor operated in Gabon, West Africa,
about 2 billion years ago.
LO 43.3.2 Explain why a deposit of uranium ore could go critical in the past but not today.
LO 43.4.0 Solve problems related to thermonuclear fusion: the basic process.
LO 43.4.1 Define thermonuclear fusion, explaining why the nuclei must be at a high temperature
to fuse.
LO 43.4.2 For nuclei, apply the relationship between their kinetic energy and their temperature.
LO 43.4.3 Explain the two reasons why fusion of two nuclei can occur even when the kinetic
energy associated with their most probable speed is insufficient to overcome their energy barrier.
LO 43.5.0 Solve problems related to thermonuclear fusion in the sun and other stars.
LO 43.5.1 Explain the proton–proton cycle for the Sun.
LO 43.5.2 Explain the stages after the Sun has consumed its hydrogen.
LO 43.5.3 Explain the probable source of the elements that are more massive than hydrogen and