What Is Nuclear Potential Energy and Where Does It Come From?

Energy is the capacity to do work, and potential energy is the form stored within a system, dependent on the configuration or position of its components. Nuclear potential energy is the specialized energy locked within the nucleus of an atom. This reservoir is related to the powerful forces that hold the subatomic particles together, representing the energy required to separate the nucleus into its individual components.

The Source: Binding Energy and Mass Defect

The energy stored within the nucleus originates from the strong nuclear force, the most powerful of nature’s four fundamental forces. Although this force acts only over very short distances, its strength overcomes the electrostatic repulsion between the positively charged protons packed closely together. The energy associated with this force, which holds the protons and neutrons (nucleons) together, is quantified as nuclear binding energy.

Binding energy is defined as the energy required to completely disassemble a nucleus into its constituent protons and neutrons. Paradoxically, the mass of a stable nucleus is always measurably less than the sum of the masses of its individual, separated protons and neutrons. This phenomenon is known as the mass defect.

This missing mass was converted into the energy that binds the nucleus together when the nucleons combined. This conversion follows Albert Einstein’s mass-energy equivalence equation, \(E=mc^2\). The change in mass multiplied by the speed of light squared equals the energy released during the formation of the nucleus. The mass defect, therefore, is the direct measurement of the stored nuclear potential energy, which is released as binding energy upon formation.

Fission and Fusion: How Nuclear Potential Energy is Released

The stored nuclear potential energy is accessed through two primary types of nuclear reactions: fission and fusion. Both processes involve changing the arrangement of nucleons to form a more stable configuration, thereby releasing the excess binding energy. The fundamental driver for energy release in both cases is the difference in the binding energy per nucleon between the initial and final nuclei.

Nuclear fission involves the splitting of a heavy, unstable nucleus, such as Uranium-235, into two or more smaller, lighter nuclei. When a neutron strikes the nucleus, it fragments, releasing substantial energy and more neutrons that can continue the chain reaction. The resulting smaller nuclei have a greater binding energy per nucleon than the original heavy nucleus, and this increase in stability corresponds to the energy released.

Nuclear fusion is the opposite process, where two light atomic nuclei combine to form a single, heavier nucleus. This process, which powers the sun and other stars, typically involves isotopes of hydrogen, like deuterium and tritium, combining to form helium. The resulting nucleus possesses a significantly higher binding energy per nucleon than the original light nuclei. The energy released is a direct result of the mass converted to energy in forming the tightly bound product.

Magnitude: Comparing Nuclear Energy to Chemical Energy

To appreciate the scale of nuclear potential energy, it is often compared to chemical energy, which is the energy released by burning fuels like wood or gasoline. Chemical energy involves the rearrangement of electrons as atoms form or break molecular bonds. These interactions are governed by the electromagnetic force, which is much weaker than the strong nuclear force.

A typical chemical reaction, such as the combustion of a carbon atom, releases energy on the order of a few electron volts (eV) per atom. A single nuclear fission event, such as the splitting of a Uranium-235 nucleus, releases approximately 200 million electron volts (MeV) of energy. Nuclear reactions are millions of times more energetic per unit of mass than chemical reactions.

The difference in magnitude stems from the fundamental forces at play. Chemical reactions only involve the outer electron shells of an atom, while nuclear reactions involve restructuring the dense, tightly bound core. This energy difference explains why a tiny amount of nuclear fuel can power a city for months, a capability unmatched by chemical fuel. Harnessing this energy is the basis for nuclear power generation.