Fission & fusion
- Nuclear fission & fusion are nuclear reactions that change the nucleus of an atom to produce high amounts of energy from the energy stored in the nucleus of an atom
Nuclear fission
- Nuclear fission is defined as:
The splitting of a large, unstable nucleus into two smaller nuclei
- During fission:
- A neutron collides with an unstable nucleus
- The neutron and the nucleus are the reactants
- The nucleus splits into two smaller nuclei (called daughter nuclei) and two or three neutrons
- The daughter nuclei and the neutrons are the products of the reaction
- Gamma rays are also emitted
- A neutron collides with an unstable nucleus
Nuclear fission process
A neutron is fired into the target nucleus, causing it to split
Nuclear fission nuclide equations
- An example of a nuclide equation for the fission of uranium-235 is:
- Where:
- is an unstable isotope of uranium
- is a neutron
- is an unstable isotope of krypton
- is an unstable isotope of barium
Nuclear fission of uranium-235
Large nuclei can decay by fission to produce smaller nuclei and neutrons with a lot of kinetic energy
Nuclear fission mass and energy values
- Energy is conserved in a nuclear fission reaction
- In the example:
- The sum of the nucleon (top) numbers of the reactants (left-hand side) is equal to the sum of the nucleon numbers of the products (right-hand side):
- The same is true for the proton (bottom) numbers:
- The products of fission move away very quickly
- During a fission reaction, energy is transferred from nuclear energy store of the parent nucleus to the kinetic energy store of the reactants
- The mass of the products is less than the mass of the original nucleus
- This is because the remaining mass has been converted into energy, which is released during the fission process
- Large isotopes with a large nucleon number, such as uranium and plutonium, both undergo fission and are used as fuels in nuclear power stations
Nuclear fusion
- Nuclear fusion is defined as:
When two light nuclei join to form a heavier nucleus
- Stars use nuclear fusion to produce energy
- In most stars, hydrogen nuclei (light nuclei) are fused together to form a helium nucleus (heavier nucleus) and massive amounts of energy is produced
Nuclear fusion of hydrogen
Two hydrogen nuclei fuse to form a helium nucleus
- Nuclear fusion requires extremely high temperature and pressure
- So fusion is very hard to reproduce on Earth
Nuclear fusion nuclide equations
- An example of a nuclide equation for fusion is:
- Where:
- is deuterium (isotope of hydrogen with 1 proton and 1 neutron)
- is hydrogen (with one proton)
- is an isotope of helium (with two protons and one neutron)
Nuclear fusion mass and energy values
- The energy produced during nuclear fusion comes from a very small amount of a particle’s mass converted into energy
- Therefore, the mass of the product (fused nucleus) is less than the mass of the two original nuclei (reactants)
- The remaining mass has been converted into the energy released when the nuclei fuse
- The amount of energy released during nuclear fusion is huge:
- The energy from 1 kg of hydrogen that undergoes fusion is equivalent to the energy from burning about 10 million kilograms of coal
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Worked example
A nuclide equation for nuclear fission is stated as:
Calculate the number of neutrons, N emitted in this reaction.
Answer:
Step 1: Calculate the sum of the nucleon numbers of the reactants
- The reactants are on the left-hand side of the equation
- The nucleon numbers are the top numbers in the nuclide notation
235 + 1 = 236
Step 2: Calculate the sum of the nucleon numbers of the products
- The products are on the right-hand side of the equation
96 + 137 + (N × 1) = 233 + N
Step 3: Equate the total nucleons of the reactants and products
236 = 233 + N
Step 4: Rearrange for the number of neutrons, N
N = 236 – 233 = 3