Nuclear Physics Flashcards
Atom
Particle made of protons, (neutrons) and electrons.
Element
Type of atom with a specific number of protons.
Nucleus
Core of an atom, consisting of protons and neutrons held together by the strong force.
Nucleon
Particle in the nucleus i.e. protons and neutrons.
Proton
Particle with 1 mass and 1 charge.
Neutron
Particle with 1 mass and 0 charge.
Electron
Particle with approximately 0 mass and -1 charge.
Atomic Number
Z, number of protons in the nucleus of a specific atom.
Atomic Mass
A, number of nucleons in the nucleus of a specific atom.
Isotope
Type of atom, with specific numbers of protons and neutrons. Isotopes of an element have the same chemical properties due to having the same number of protons but have different physical properties due to differing numbers of neutrons.
Nuclide
Specific nucleus, with certain numbers of protons and neutrons.
Nuclear reaction
Any process causing changes to a nucleus. Mass number and charge must be conserved.
Stable Nuclide
Specific nucleus that will remain the same indefinitely. Strong force is enough to overcome electrostatic repulsion between protons. For light elements (Z<21), require 1:1 ratio of protons to neutrons. For medium elements, require slightly more neutrons than protons. Heavy elements (Z>82) cannot be stable – size of nucleus is too great for the very short ranged strong force to hold it together.
Stable isotope
Specific atom with a nucleus that will remain the same indefinitely.
Unstable nuclide
Specific nucleus that will spontaneously change to become more stable.
Radioisotope/unstable isotope
Specific atom with a nucleus that will spontaneously change to become more stable.
Radioactive
Material containing unstable nuclei.
Nuclear decay
Emission of particles (or energy) from a nucleus to become more stable.
Activity
Number of decay events per second for a radioactive substance
Half life
Measure of exponential decay rate for a nuclide. Time for half of the remaining particles to decay.
Transmutation
Changing of one nuclide into another through nuclear decay.
Daughter nuclide/isotope
Product nucleus of nuclear decay.
Decay series
A sequence of nuclear decays through multiple unstable nuclides to an eventual stable nuclide.
Nuclear radiation
Particle or energy emitted from a nucleus.
Alpha decay
Emission of an alpha particle from a nucleus that is too large to be stable.
Beta minus decay
Emission of a beta (minus) particle from a nucleus that has too many neutrons as a neutron becomes a proton.
Beta plus decay
Emission of a beta plus particle from a nucleus that has too few neutrons as a proton becomes a neutron.
Gamma decay
Emission of a gamma ray from a nucleus that has too much energy to be stable. Commonly occurs after an alpha or beta decay.
Ionising radiation
Radiation capable of adding electron to or removing electrons from atoms, turning them into ions. Alpha, beta and gamma radiation.
Alpha particle/radiation
He-4 nucleus (2 protons, 2 neutrons). 2+ charge, travels at 0.1c, highly ionising, weakly penetrating.
Beta minus particle radiation
Electron. -1 charge, travels at 0.9c, moderately ionizing, moderately penetrating.
Beta plus particle radiation
Antielectron/positron. +1 charge, travels at 0.9c, moderately ionising, moderately penetrating. If it collides with an electron they will mutually annihilate emitting gamma radiation.
Gamma ray/radiation
High energy photon of light. 0 charge, travels at c, weakly ionising, highly penetrating.
Neutron radiation
Neutron. Not ionizing but can be absorbed by a nucleus, potentially transforming it into an unstable nuclide.
Mass defect
The difference in mass between a number of free nucleons and that many nucleons as a nucleus. Mass of the binding energy.
Binding energy
The energy lost by free nucleons in order to bond together as a nucleus. The energy required to separate all the nucleons in a nucleus into free particles.
Binding energy per nucleon
The average energy lost by each nucleon in a nucleus. Measure of stability of the nucleus. Higher binding energy per nucleon – more stable nuclide. Peaks at Fe-56.
Nuclear fusion
Joining of light nuclei to form heavier nuclei. Releases energy if the binding energy per nucleon increases, i.e. if moving towards Fe-56.
Fusion reactor
Machine maintain stable fusion reaction to generate heat to generate electricity. Requires enormous temperatures and pressures to cause collisions between nuclei, overcoming the electrostatic repulsion. Currently consumes more energy than is produced – developing technology.
Nuclear fission
Splitting of heavy nuclei into multiple lighter nuclei (and free neutrons). Releases energy if the binding energy per nucleon increases, i.e. if moving towards Fe-56. Can be spontaneous or triggered by absorption of free neutron.
Fissile
Nuclides that will readily undergo fission reactions.
Fission reactor
Machine maintaining stable fission reaction, typically to generate heat to generate electricity. Relies on stable chain reaction, fission can be triggered by neutrons and it emits neutrons.
Fuel rods
Fuel must be enriched to contain a higher proportion of fissile material.
Control rods
Material that absorbs free neutrons to control reaction rate in reactor. Control rods inserted if reaction rate too high.
Moderator
Slows neutrons so that they can be more easily absorbed by nuclei to trigger further fission reactions.
Shielding
Fission reaction and radioactive fission products emit radiation dangerous to workers. Reaction chamber must be shielded by metres of lead and concrete to absorb radiation, protecting plant workers.
Nuclear waste
Fuel lasts a long time but produces waste that remains radioactive for extremely long timespans – must be stored safely.
Critical mass
The minimum mass of fuel required to sustain a fission chain reaction. Shape dependent, sphere is most efficient.