A2 Physics Terms Flashcards
Absolute scale (Thermal)
Temperature scale in Kelvins defined in terms of absolute zero, 0K, and the triple point of water, 273.16 K, which is the temperature at which ice, water and water vapour are in thermal equilibrium.
Absolute zero
- The lowest possible temperature;
2. The temperature at which an object has minimum internal energy.
Absolute temperature T
in kelvin = temperature in degrees Celsius + 273(.15)
activity A
of a radioactive isotope, is the number of nuclei of the isotope that disintegrate per second.
Unit: Becquerel (Bq) - 1 disintegration per second.
Alpha decay
change in an unstable nucleus when it emits an alpha particle, which is a particle consisting of 2 protons and 2 neutrons (a helium nucleus).
Alpha radiation (Composition, Emission circumstances, Absorption, Range, Comparison of Ionisation ability)
- Particles composed of 2 p + 2n
- Alpha particle is emitted by a heavy, unstable nucleus, which is then less unstable as a result.
- Alpha radiation easily absorbed by paper,
- Range of no more than a few centimetres.
- More ionising than Beta or Gamma radiation.
Amplitude
the maximum displacement from equilibrium of an oscillating object
Angular displacement
The angle an object in circular motion turns through.
If its time period is T and its frequency f, its angular displacement in time t, in radians is = 2 PI f t = 2 PI t/T
Angular speed, w
the rate of change of angular displacement of an object in circular (or orbital or spinning) motion.
Angular frequency, w
for an object oscillating at frequency f in simple harmonic motion its angular frequency = 2 PI f
Atomic mass unit u
correctly referred to as the unified atomic mass contestant,
- Equals 1/12 th of the mass of at atom of the carbon isotope 12,6 C = 1.661 x 10^-27 kg
Atomic number Z
of an atom of an element is the number of protons in the nucleus of the atom. It is also the order number of the element in the periodic table.
Avogadro Constant, N(a)
The number of atoms in 12g of th carbon isotope 12,6 C.
- N(a) is used to define the mole
- Its value is 6.02 x 10^23 1/mol
back emf
emf induced in the spinning coil of an electric motor or in any coil in which the current is changing
eg. the primary coli in a transformer
A back emf acts against the applied pd.
Background radiation
radiation due to naturally occurring radioactive substances in the environment (e.g. in the ground or in building materials or elsewhere in the environment).
Background radiation is also caused by cosmic rays.
Beta decay
- Change in nucleus when a neutron changes in a proton and a beta minus particle and an antineutrino are emitted if the nucleus is neutron-rich.
- OR a proton changes to a neutron, and a beta plus particle and a neutrino are emitted if the nucleus is proton rich.
Beta minus radiation
electrons (beta particles) emitted by unstable neutron rich nuclei (e.g. nuclei with a neutron/proton ratio greater than for stable nuclei).
- B minus radiation is easily absorbed by paper,
- Has a range in air of no more than a few centimetres,
- Is less ionising than alpha radiation, and but more ionising than gamma radiation.
Beta plus radiation
Positrons emitted by unstable proton rich nuclei (i.e. nuclei with a neutron/proton ratio smaller than for stable nuclei).
Positrons emitted in solids or liquids travel no further than about 2 mm before they are annihilated.
Binding energy of a nucleus
The work that must be done to separate a nucleus into its constituent neutrons and protons.
Binding energy = mass defect x c^2
Binding energy in MeV = mass defect in (u) x 931.3
Binding energy per nucleon
- The average work done per nucleon, to separate a nucleus into its constituent parts.
- The binding energy per nucleon of a nucleus = binding energy of a nucleus / mass number A.
- The binding energy per nucleon is greatest for iron nuclei of mass number about 56.
- The binding energy curve is a graph of binding energy per nucleon against mass number A.
Boiling point
The temperature at which a pure liquid at atmospheric pressure boils.
Boyle’s law
For a fixed mass of gas at constant temperature, its pressure x volume is constant.
A gas that obeys Boyle’s law is said to be an ideal gas.
BL: pV = k, constant m, T
Boltzmann Constant, k
the molar gas constant divided by the Avogadro number = R/N(a).
See KE of molecules of an ideal gas
Brownian motion
The random and unpredictable motion of a particle such as smoke, caused by molecules of the surrounding substance colliding at random with the particle.