Nuclear fission is the process in which a heavy nucleus splits into two or more lighter nuclei, accompanied by the release of neutrons and a large amount of energy.
An important example is the fission of 92U235 induced by a slow (thermal) neutron:

Energy released per fission ≈ 200 MeV = 3.2 × 10⁻¹¹ J. This energy arises from the mass defect between the initial nucleus plus incident neutron and the final products; the difference appears as kinetic energy of the fragments and the emitted neutrons, and as gamma radiation. The quantitative energy (Q-value) of a nuclear reaction is given by the mass difference multiplied by c2:
Q = (Initial mass - final mass) c²
OR

Key numbers to remember:
Nuclear chain reaction occurs when one fission event produces neutrons that go on to induce further fissions, thereby sustaining a sequence (chain) of reactions.
Key points and terminology:
Chain reactions may be of two types:

A nuclear reactor is an engineered device in which a controlled nuclear chain reaction is maintained to produce heat for electricity generation or for other purposes (research, propulsion, isotope production).
The main parts and their functions:
In power reactors the heat produced by fission is used to generate steam that drives turbines; precise control and heat removal are essential for safety. An atom bomb works on the principle of an uncontrolled chain reaction, where fissile material is rapidly brought to a supercritical configuration.
Nuclear fusion is the process in which two light nuclei combine to form a heavier nucleus, with a net release of energy when the binding energy per nucleon of the product is greater than that of the reactants.
Common fusion reactions of interest:
Some textbook presentations give a simplified net reaction in which three deuterons combine to form an alpha particle (2He4) with an overall release of energy (a commonly quoted value is ~21.6 MeV for a particular net process). Actual fusion proceeds via intermediary steps (D-D and D-T channels) as shown above.
Fusion releases very large amounts of energy per unit mass of fuel compared with chemical reactions.
Conditions Required for Fusion
Nuclear fusion requires extremely high temperatures and pressures to overcome the Coulomb repulsion between positively charged nuclei:
Applications and devices:
Thermonuclear energy is the energy released in nuclear fusion reactions. Fusion reactions involve light nuclei (often isotopes of hydrogen such as deuterium and tritium) while fission reactions are typically initiated and sustained by neutrons interacting with heavy nuclei.

Q1. In a nuclear reactor, what is the function of the moderator?
Solution: The moderator (heavy water D₂O, graphite) slows down fast neutrons to thermal energies so they can be efficiently absorbed by U-235 to cause further fission.
Q2. In a nuclear fission reaction of U-235, energy released per fission is 200 MeV. How many fissions per second are needed to produce a power of 1 MW?
Solution: Power = 1 MW = 10⁶ W = 10⁶ J/s
Energy per fission = 200 MeV = 200 × 1.6 × 10⁻¹³ J = 3.2 × 10⁻¹¹ J
Number of fissions = 10⁶ / 3.2 × 10⁻¹¹ = 3.125 × 1016 fissions/s
Q3. The multiplication factor k in a nuclear reactor is maintained at:
Solution: In a nuclear reactor, k = 1, k is kept equal to 1 for a steady and controlled chain reaction. k < 1 means chain dies out. k > 1 means uncontrolled explosion (atom bomb principle).
Q4.The D-T fusion reaction releases 17.6 MeV of energy. The energy released per nucleon is:
Solution: D has mass number 2, T has mass number 3 Total nucleons = 2 + 3 = 5
Energy per nucleon = 17.6/5 = 3.52 MeV
| 1. What is nuclear fission? | ![]() |
| 2. How does a nuclear reactor work? | ![]() |
| 3. What are the advantages of nuclear energy? | ![]() |
| 4. What are the risks associated with nuclear energy? | ![]() |
| 5. How does nuclear energy compare to other sources of energy? | ![]() |