The process in which a large nucleus is forced to split into at least two approximately equal-sized fragments with the release of neutrons and a large amount of energy
Nuclear fission
1. Used in the production of electricity in a nuclear reactor
2. Used in nuclear weapons
Most daughter nuclei of fission reactions are radioactive and will decay at a slower rate
Most common fission reaction
Single slow moving neutron bombards uranium-235 to produce uranium-236 which breaks apart into at least two similar sized nuclei, a few neutrons and a large amount of energy
The energy released by nuclear fission is calculated the same way as decay reactions
The amount of energy produced in nuclear fission is often more than 100 times that produced in natural radioactive decay
Fission reaction
Uranium-235 nucleus bombarded with a single neutron fragments into three neutrons, caesium-137 and rubidium-96
The energy released in the fission reaction of a uranium-235 nucleus bombarded with a single neutron is 172.6 MeV
Chain reaction in nuclear fission
Production of extra neutrons which can go on to react with other fissile nuclei to trigger more fission reactions
Exponential cascade of more neutrons initiating more fission reactions
The amount of material needed to sustain a chain reaction is known as the critical mass
Nuclear fusion
The process whereby two smaller nuclei join, or fuse, together to create a larger nucleus with the creation of energy
Fusion reactions, specifically the reaction of two protons joining to make helium, are by far the most common type of nuclear or chemical reaction in the universe
Conditions for nuclear fusion
The small nuclei must be travelling very fast (usually achieved through high temperatures - approximately 10 million degrees)
There need to be enough nuclei available to sustain a reaction (occurs under very high pressure)
Common fusion reaction
Reaction of deuterium and proton to form helium-3
The amount of energy released in the fusion reaction of deuterium and proton to form helium-3 is 4.98 MeV
The energy per mass of reactants is much higher in nuclear fusion compared to nuclear fission
Atom
The basic building block of all matter
Nucleus of an atom
Consists of positively charged protons and neutral neutrons, surrounded by much lighter negatively charged electrons
Protons
Have a positive charge and a mass almost 2000 times the mass of an electron. The number of protons in the nucleus of the atom determines the element.
Neutrons
Have no charge hence they are neutral
Electrons
Have a negative charge and are significantly smaller than protons and neutrons
Properties of the 3 major particles found in atoms
Particle
Location
Symbol
Charge (C)
Mass (kg)
Mass (u)
Nucleons
Protons and neutrons that comprise the nucleus
Nuclide
The nucleus made up of protons and neutrons
Atomic number (Z)
The number of protons in a nucleus
Mass number (A)
The sum of the number of protons and neutrons in a nucleus
Nuclear notation
1. X<sub>Z</sub><sup>A</sup>
2. Element symbol
3. Atomic number
4. Mass number
There are 250 stable nuclei that exist in nature. Pb-208 is the heaviest naturally occurring stable nuclide.
Stable nucleus
A nucleus that does not gain or lose any protons, neutrons or energy over time
The periodic table indicates, in yellow, all elements that have no stable isotopes.
Radioactive
An unstable nucleus that changes over time, or has an excess of energy
Radioisotope
A radioactive isotope
Radionuclide
An unstable nucleus
Coulomb/Electrostatic force
The force acting on charged particles that causes them to move
In a nucleus, there is no Coulomb force between 2 neutrons or between a neutron and a proton because neutrons have no charge.
Strong nuclear force (SNF)
The force that overcomes the repulsive electrostatic forces to hold the nucleus together
The strong nuclear force is one of the four fundamental forces that exist in the universe, the others being electromagnetic, gravity and weak nuclear force.
Strong nuclear force
Mainly attractive, acts only in the nucleus on protons and neutrons, and acts at only very short distances
If more protons are added to a nucleus
More neutrons must be added for the SNF to balance the Coulomb force
Radioactive nuclides occur where
There are either too many protons relative to the number of neutrons (resulting in β+ decay) or there are too many neutrons relative to the number of protons (resulting in β- decay)