Electrons absorb energy from collisions with free electrons, causing them to 'jump up' energy levels
Excited electrons are very unstable
De-excitation:
Excited electrons lose energy, causing them to fall back energy levels
This process results in the emission of photons
1897 - JJ Thompson discovered the electron
1904 - Plum pudding model:
Negatively charged 'plums' embedded into a positively charged 'pudding'
Electrons were thought to be mobile
1909 - Alpha particle scattering experiment:
Attempted to prove the plum puddingmodel
Some alpha particles deflecteddramatically, while others did not deflect at all
Led to the realization of an extremely dense positively charged matter in the centre of the atom (nucleus) by Rutherford
1911 - Rutherford proposed the nuclear model
1913 - Bohr atom:
Proposed that electrons were located in circular orbitals at specific distances from the nucleus
1932 - James Chadwick discovered the neutron
Stable isotopes remainthesame over time
Unstable isotopes decay into another type of atom, ionizing part of them, becoming more stable
Alpha radiation:
Helium nucleus
Relative mass of 4u, relative charge of 2+
Slow speed, high ionizing power
Weak penetrating power, can travel around 2cm in air
Absorbed by thin sheets of paper or skin, deflects towards the negative plate in an electric field
Beta radiation:
Electron emitted from the nucleus
Small relative mass of 1/1845u, relative charge of -1
Fast speed, moderate ionizing and penetrating power
Travels about 1m in air
Absorbed by an aluminum sheet, deflects towards the positive plate in an electric field
Gamma radiation:
High frequency electromagnetic wave from the nucleus
No mass or relative charge
Speed of light (3x10^8 m/s), weak ionizing power
High penetrating power, infinite range in air
Absorbed by thick lead or concrete, does not deflect in an electric field
As each nucleus decays, the number of atoms decreases, so the activity falls
The Geiger counter gives a count rate from the sample (counts per sec)
Radioactive decay is a spontaneous and random process, not influenced by environmental factors
Half-life is the time it takes for half of the unstable nuclei in a sample to decay
Isotopes with a short half-life have a high activity
Radiation is the emissions of energy as electromagnetic waves or as moving subatomic particles
Ionisation is the process of becoming ions
Ionising radiation can damage human cells and tissues, leading to cell death and potential tumor formation
Acute radiation exposure symptoms include: skin burns, reduction of white blood cells, and radiation sickness
Higher dose equals a higher risk of cancer or cell death
Risk can never be zero due to background radiation
Irradiation is the exposure of an object to ionising radiation, without making the object radioactive
Contamination is the unwanted presence of radioactive material on an object through physical contact
Precautions for handling radioactive material include: keeping sources shielded, wearing protective clothing, avoiding skin contact, wearing a mask, limiting exposure time, using tongs, and monitoring exposure
To measure radiation dose absorbed by the body, the sievert (Sv) is used
Background radiation is the low-level radiation always present from natural and man-made sources
Unstable atoms can become more stable by decaying and releasing ionising radiation
Binary Fission is when unstable nuclei break apart
Nuclear Fission is the process of splitting a large and unstable nucleus
Fissionable isotopes are isotopes that can be split via nuclear fission
Firing a neutron into the nucleus can make a fissionable isotope split
When a nucleus undergoes fission, it splits into two smaller daughter nuclei, some individual neutrons, and a small amount of matter converts into energy in the form of gamma rays
Daughter nuclei are extremely radioactive
A moderator can slow neutrons
Thermal neutrons have already been slowed down, increasing the chance of neutron absorption
Control rods control the rate of reaction
Superheating a gas causes the atoms to have so much energy that their electrons become excited and 'shed' off, ionizing the particles and allowing the gas to conduct electricity