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Angular velocity
angular displacement per unit time
Field line
Represents the path a mass would take when placed within the field
Gravitational field
Area where object with mass experiences an attractive force due to gravity
Gravitational potential
Work done in moving a unit mass from an infinite distance to that point
Newton’s law of gravitation
Force between two masses is proportional to the product of the masses involved and inversely proportional to the square of the separation of the masses
Synchronous orbit
An orbit with a time period of one day. Orbiting body will return to the same point in the sky each day
Specific heat capacity
Amount of energy required to increase the temperature of 1kg of a substance by 1 Kelvin without changing state
Specific latent heat
amount of energy required to change the state of a substance per kg without a change of temperature.
Fusion - solid to liquid
Vaporisation - liquid to gas
Internal energy
Sum of randomly distributed potential and kinetic energies of the particles in a substance.
(In an ideal gas, will just be the KE as we assume there to be no intermolecular forces so no potential energy between particles).
Critical damping
Damping that reduces displacement of an oscillating object to its equilibrium position in the quickest time possible, without further oscillation.
Damping
Occurs when a force opposes the system’s motion. Energy is dissipated from the oscillating system.
Natural frequency
a system naturally oscillates at this when there is no external force applied.
Overdamping
System is damped more than required to stop oscillations. It takes longer for the system to return to equilibrium than for critical damping
Simple Harmonic Motion
Acceleration is directly proportional to the acceleration of the object in the opposition direction
Underdamping
A type of damping where energy is gradually removed from the system. Amplitude slowly decreases.
Coulomb’s law
force that acts between two point charges is proportional to the product of their charges and inversely proportional to the square of their separation.
Attractive for opposite charges and repulsive for like charges.
Electric field strength
Force per unit positive charge
Electric potential
Work done per unit charge on a positive test charge in bringing it from infinity to a point in the field
Equipotential
Surface of constant potential. No work is done by the field when an object moves along an equipotential
Electric field lines
Lines demonstrating direction which a positive charge would follow
Capacitance
Charge stored per unit pd in a capacitor
What is a parallel plate capacitor
Two parallel conducting plates. With an insulator between them (dielectric)
Electromagnetic induction
An emf is induced in a wire when it is moved relative to a magnetic field
Faraday’s law
Induced E.M.F in a circuit is proportional to the rate of change of magnetic flux linkage through the circuit and acts in a direction that opposes the change producing it.
Lenz’s law
direction of an induced current is such that it opposes the current that created it
Magnetic flux density
Force per unit current per unit length on a current carrying wire placed perpendicular to the field. Measured in Tesla.
De Broglie hypothess
All particles have a wave-like natue and a particle-like nature.
Wavelength = h/momentum.
Intensity
Power transferred per unit area
Emission spectrum
When atom’s de-excite they move from one energy level to another, with a discrete energy gap between these levels. This creates a photon of that energy and the frequency of this photon make up the emission spectrum.
Absorption spectrum
Frequencies at which an element absorbs photons corresponds to the spacings between energy levels in the element’s atoms.
Photon
A discrete quanta of energy of electromagnetic radiation. E=hf.
Threshold frequency
Minimum frequency of light needed to cause electrons to be emitted from the surface of a metal. (Sometimes energy required will be higher than threshold as energy needed to get electrons to surface).
Can also be thought of as MAX wavelength.
Work function
Minimum energy required to remove an electron from a metal’s surface.
Activity
rate of decay of radioactive nuclei in an isotope.
(A = N x decay constant)
Measured in Becquerels
Binding energy
Energy required to split a nucleus into its individual nucleons to infinity.
(The greater the binding energy per nucleon, the more stable the nucleus is).
Decay constant
Constant probability of a nuclear decay occurring per unit time
Mass-energy equivalence
The energy equivalent of a given mass is equal to the product of the mass and the speed of light squared
Mass defect
Difference in mass between a nucleus and the sum of the masses of its constituent nucleons
Random nature of decay
Cannot predict when a nucleus will decay
Spontaneous nature of decay
Decay is independent of physical factors such as temperature
Acoustic impedance
Product of the speed of sound through a given medium and the density of the medium
Attenuation of X-Rays
Reduction of the intensity of X-rays when they pass through matter. Decay of this intensity is exponential.
Briefly outline Computerised Axial Tomography Scanning
produces a cross section of the body by rotating a monochromatic x-ray beam around it in combination with a series of detectors
How do piezoelectric crystals work
When a potential difference is applied, crystals deform. When the crystal is deformed, a potential difference is produced
What type of wave is ultrasound, and what frequency do they sit above
They are sound waves. Higher than audible frequency (20,000 Hz)
Hubble’s law
Speed of a galaxy moving away from ours is proportional to its distance away from us.
Constant of proportionality is Hubble’s constant.
Luminosity
Total power radiated by a star.
Given by Stefan-Botlzmann Law: L = 4 x pi x R² x sigma x T4
What is red shift
Shifting of an object’s wavelength towards the longer wavelength end of the spectrum due to the object moving away from the Earth. Doppler effect. Red shift is evidence for the expansion of the universe.
Standard candle
Object of known luminosity, used as a reference to measure other stars and the distance to them.
Wien’s displacement law
The peak wavelength of emitted radiation is inversely proportional to its absolute temperature.
wavelength x T = constant.
State the order of the electromagnetic spectrum from largest wavelength to smallest.
Radio
Microwave
Infrared
Visible (ROYGBIV)
Ultraviolet
X-Ray
Gamma Ray