21.2: Nuclear Equations
By the end of this section, you will be able to:
- Identify common particles and energies involved in nuclear reactions
- Write and balance nuclear equations
Changes of nuclei that result in changes in their atomic numbers, mass numbers, or energy states are nuclear reactions . To describe a nuclear reaction, we use an equation that identifies the nuclides involved in the reaction, their mass numbers and atomic numbers, and the other particles involved in the reaction.
Types of Particles in Nuclear Reactions
Many entities can be involved in nuclear reactions. The most common are protons, neutrons, alpha particles, beta particles, positrons, and gamma rays, as shown in Figure \(\PageIndex{1}\). Protons (\(\ce{^1_1p}\), also represented by the symbol \(\ce{^1_1H}\)) and neutrons (\(\ce{_0^1n}\)) are the constituents of atomic nuclei, and have been described previously. Alpha particles (\(\ce{_2^4He}\), also represented by the symbol \(\ce{_2^4\alpha}\)) are high-energy helium nuclei. Beta particles (\(\ce{_{−1}^0β}\), also represented by the symbol \(\ce{_1^0e}\)) are high-energy electrons, and gamma rays are photons of very high-energy electromagnetic radiation. Positrons (\(\ce{_{+1}^0e}\), also represented by the symbol \(\ce{_1^0β}\)) are positively charged electrons (“anti-electrons”). The subscripts and superscripts are necessary for balancing nuclear equations, but are usually optional in other circumstances. For example, an alpha particle is a helium nucleus (\(\ce{He}\)) with a charge of +2 and a mass number of 4, so it is symbolized \(\ce{_2^4He}\). This works because, in general, the ion charge is not important in the balancing of nuclear equations.
Note that positrons are exactly like electrons, except they have the opposite charge. They are the most common example of antimatter , particles with the same mass but the opposite state of another property (for example, charge) than ordinary matter. When antimatter encounters ordinary matter, both are annihilated and their mass is converted into energy in the form of gamma rays (\(\gamma\)) —and other much smaller subnuclear particles, which are beyond the scope of this chapter—according to the mass-energy equivalence equation \(E = mc^2\), seen in the preceding section. For example, when a positron and an electron collide, both are annihilated and two gamma ray photons are created:
\[\ce{_{-1}^0 e +_{+1}^0 e -> \gamma+\gamma} \nonumber \]
As seen in the chapter discussing light and electromagnetic radiation, gamma rays compose short wavelength, high-energy electromagnetic radiation and are (much) more energetic than better-known X-rays that can behave as particles in the wave-particle duality sense. Gamma rays are a type of high energy electromagnetic radiation produced when a nucleus undergoes a transition from a higher to a lower energy state, similar to how a photon is produced by an electronic transition from a higher to a lower energy level. Due to the much larger energy differences between nuclear energy shells, gamma rays emanating from a nucleus have energies that are typically millions of times larger than electromagnetic radiation emanating from electronic transitions.
Balancing Nuclear Reactions
A balanced chemical reaction equation reflects the fact that during a chemical reaction, bonds break and form, and atoms are rearranged, but the total numbers of atoms of each element are conserved and do not change. A balanced nuclear reaction equation indicates that there is a rearrangement during a nuclear reaction, but of nucleons (subatomic particles within the atoms’ nuclei) rather than atoms. Nuclear reactions also follow conservation laws, and they are balanced in two ways:
- The sum of the mass numbers of the reactants equals the sum of the mass numbers of the products.
- The sum of the charges of the reactants equals the sum of the charges of the products.
If the atomic number and the mass number of all but one of the particles in a nuclear reaction are known, we can identify the particle by balancing the reaction. For instance, we could determine that \(\ce{^{17}_8O}\) is a product of the nuclear reaction of \(\ce{^{14}_7N}\) and \(\ce{^4_2He}\) if we knew that a proton, \(\ce{^1_1H}\), were one of the two products.
The reaction of an \(α\) particle with magnesium-25 (\(\ce{_{12}^{25}Mg}\)) produces a proton and a nuclide of another element. Identify the new nuclide produced.
Solution
The nuclear reaction can be written as:
\[\ce{_{12}^{25}Mg +_2^4He ->_1^1H +_{Z}^{A}X} \nonumber \]
where \(A\) is the mass number and \(Z\) is the atomic number of the new nuclide, \(X\). Because the sum of the mass numbers of the reactants must equal the sum of the mass numbers of the products:
\[25+4= A +1 \nonumber \]
or \(A =28\).
Similarly, the charges must balance, so:
\[12+2= Z +1 \nonumber \]
and \(Z =13\).
Check the periodic table: The element with nuclear charge = +13 is aluminum. Thus, the product is \(\ce{_{13}^{28}Al}\)
The nuclide \(\ce{_{53}^{125}I}\) combines with an electron and produces a new nucleus and no other massive particles. What is the equation for this reaction?
- Answer
-
\[\ce{_{53}^{125}I +_{−1}^{0}e ->_{52}^{125}Te} \nonumber \]
Following are the equations of several nuclear reactions that have important roles in the history of nuclear chemistry:
- The first naturally occurring unstable element that was isolated, polonium, was discovered by the Polish scientist Marie Curie and her husband Pierre in 1898. It decays, emitting α particles: \[\ce{^{212}_{84}Po ->^{208}_{82}Pb +^{4}_{2}He} \nonumber \]
- The first nuclide to be prepared by artificial means was an isotope of oxygen, 17 O. It was made by Ernest Rutherford in 1919 by bombarding nitrogen atoms with α particles: \[\ce{^{14}_7N +^{4}_{2}He ->^{17}_8O +^{1}_{1}H} \nonumber \]
- James Chadwick discovered the neutron in 1932, as a previously unknown neutral particle produced along with 12 C by the nuclear reaction between 9 Be and 4 He: \[\ce{^{9}_4Be +^{4}_2He ->^{12}_6C +^{1}_0n} \nonumber \]
- The first element to be prepared that does not occur naturally on the earth, technetium, was created by bombardment of molybdenum by deuterons (heavy hydrogen, \(\ce{^{2}_1H}\)), by Emilio Segre and Carlo Perrier in 1937: \[\ce{^{2}_1H +^{97}_{42}Mo -> 2^{1}_0n +^{97}_{43}Tc} \nonumber \]
- The first controlled nuclear chain reaction was carried out in a reactor at the University of Chicago in 1942. One of the many reactions involved was: \[\ce{^{235}_{92}U +^{1}_{0} n ->^{87}_{35}Br +^{146}_{57}La + 3^{1}_{0}n} \nonumber \]