Positively charged nucleus (which contains neutrons and protons) surrounded by negatively charged electrons
Subatomic Particles
Proton
Neutron
Electron
Electron
Relative Mass: 0 (0.0005), Relative Charge: -1
Typical radius of an atom: 1 × 10−10 metres
Radius of the nucleus is 10 000 times smaller than the atom
Most (nearly all) the mass of the atom is concentrated at the nucleus
Electron Arrangement
Electrons lie at different distances from the nucleus (different energy levels)
The electron arrangements may change with the interaction with EM radiation
Isotopes
Atoms of the same element, but with different masses, which have the same number of protons but different number of neutrons
Elements
All atoms of the same element have the same number of protons
Neutral Atoms
Have the same number of electrons and protons
Atomic Notation
𝑍𝑍𝑋𝑋±𝑛𝑛𝐴𝐴 , where X is the letter of the element, A is the mass number, Z is the proton number, and N is the charge
Atoms and EM Radiation
1. When electrons move to a higher orbit (further from the nucleus), the atom has absorbed EM radiation
2. When the electrons falls to a lower orbit (closer to the nucleus), the atoms has emitted EM radiation
3. If an electron gains enough energy, it can leave the atom to form a positive ion
Dalton said everything was made of tiny spheres (atoms) that could not be divided
JJ Thomson discovered the electron
Rutherford realised most of the atom was empty space
Rutherford Model: Positive nucleus at the centre of the atom, and negative electrons existing in a cloud around the nucleus
Bohr produced the final model of the atom
Positive charge of nucleus could be subdivided into smaller particles, each with the same amount of charge – the proton
James Chadwick provided evidence to prove neutrons existed
Radioactive Decay
Unstable atomic nuclei give out radiation as they change to become more stable. This is a random process.
Activity
The rate at which a source of unstable nuclei decays, measured in Becquerel (Bq)
Count-rate
The number of decays recorded by a detector per second
Forms of Radioactive Decay
Alpha (α)
Beta Minus (β)
Gamma (γ)
Neutrons
Alpha Decay
Highly ionising, weakly penetrating (~5cm of air)
Beta Decay
Medium ionising, medium penetration (~50cm of air, sheet of paper)
Gamma Decay
Low ionising, highly penetrating (very far in air, few cm of lead)
Nuclear Equations
1. Alpha Decay: 𝑍𝑍𝑋𝑋𝐴𝐴 → 𝑍𝑍−2𝑌𝑌𝐴𝐴−4 + 𝐻𝐻𝑃𝑃24
2. Beta Decay: 𝑍𝑍𝑋𝑋𝐴𝐴 → 𝑍𝑍+1𝑌𝑌𝐴𝐴 + 𝑃𝑃−10
3. Gamma Decay: Does not cause the mass or charge to change
Half-Life
The time taken for half the nuclei in a sample to decay or the time taken for the activity or count rate of a sample to decay by half
Half-life cannot be predicted when any one nucleus will decay, but it enables the activity of a very large number of nuclei to be predicted during the decay
Short Half-Life
The source presents less of a risk, as it does not remain strongly radioactive
Long Half-Life
The source remains weakly radioactive for a long period of time
Net Decline
Calculate the ratio of net decline of radioactive nuclei after X half-lives
Contamination
Radioactive atoms are transferred to an object, lasting for a long period of time
Irradiation
Exposing an object to nuclear radiation, but does not make it radioactive, lasting only for a short period of time
Scientific reports on the effects of radiation on humans need to be peer reviewed
Background Radiation
Weak radiation that can be detected from natural / external sources
Radiation Dose
Measured in Sieverts (Sv)
Uses of Radioactivity
Tracers (e.g. Technetium)
Chemotherapy
Nuclear Fission
1. Splitting of a large and unstable nucleus (e.g. uranium or plutonium), releasing energy and neutrons
2. Spontaneous fission is rare, usually requires absorbing a neutron first
3. Chain reaction occurs as released neutrons cause further fissions
Nuclear Fusion
Two small nuclei fuse to form a heavier nucleus, releasing energy