Eduqas Definitions Doc 2
Eduqas Definitions Doc 2
TERMS, DEFINITIONS
&
UNITS
May 2015
This document is issued by WJEC Eduqas to assist teachers with the preparation of
candidates for the GCE examination in PHYSICS. It consists of the definitions of terms from
the current AS/A specification.
The definitions were produced by the Principal Examining team. It is acknowledged that
there will always be disagreement on precise definitions, but the aim has been to produce
wording which is accessible to students while preserving a fair level of rigour.
The rationale for the production of this document is to help learners towards an
understanding of the basic vocabulary of Physics, without which clear explanations are
impossible. It will also of course aid the learners in revision, as knowledge of terms,
definitions and units is examined in every paper.
Helen Francis
Domain Leader - Mathematics and Science
Subject Officer - Physics and Electronics
helen.francis@eduqas.co.uk
A level COMPONENT 1
1.5 (d) Angular For an object describing a circle at uniform speed, the
velocity, ω angular velocity ω is equal to the angle θ swept out by
∆θ
the radius in time ∆t divided by t (ω = )
∆t
UNIT: rad s-1
1.6 (a) Simple harmonic Shm occurs when an object moves such that its
motion (shm) acceleration is always directed toward a fixed point
and is proportional to its distance from the fixed point.
(a = – ω 2x)
Alternative definition:
The motion of a point whose displacement x changes
with time t according to x = A cos (ω t + ε), where A, ω
and ε are constants. [Variations of this kind are said to
be sinusoidal.]
1.6 (e) Period, T for an The time taken for one complete cycle.
oscillating body
Amplitude, A of an The maximum value of the object’s displacement (from
oscillating object its equilibrium position).
Phase The phase of an oscillation is the angle (ωt + ε) in the
equation x = A cos (ω t + ε). [ε is called the phase
constant.]
UNIT: rad
Frequency, f The number of oscillations per second. UNIT: Hz
1.6 (l) Free oscillations Free oscillations occur when an oscillatory system
[Natural oscillations] (such as a mass on a spring, or a pendulum) is
displaced and released.
[The frequency of the free oscillations is called the
system’s natural frequency.]
Damping Damping is the dying away, due to resistive forces, of
the amplitude of free oscillations.
1.6 (n) Critical damping Critical damping is the case when the resistive forces
on the system are just large enough to prevent
oscillations occurring at all when the system is
displaced and released.
1.6 (o) Forced oscillations These occur when a sinusoidally varying ‘driving’ force
is applied to an oscillatory system, causing it to
oscillate with the frequency of the applied force.
Resonance If, in forced vibrations, the frequency of the applied
force is equal to the natural frequency of the system
(e.g. mass on spring), the amplitude of the resulting
oscillations is large. This is resonance.
1.7 (a) Ideal gas An ideal gas strictly obeys the equation of state
pV = nRT, in which n is the number of moles, T is the
kelvin temperature and R is the molar gas constant.
R = 8.31 J mol-1 K-1. With the exception of very high
densities a real gas approximates well to an ideal gas.
1.7 (d) The mole The mole is the S.I. unit of an ‘amount of substance’. It
is the amount containing as many particles (e.g.
molecules) as there are atoms in 12 g of carbon-12.
Avogadro constant, This is the number of particles per mole.
NA (NA = 6.02 × 1023 mol-1)
1.8 (a) Internal energy, U, of This is the sum of the kinetic and potential energies of
a system the particles of a system.
1.8 (d) Heat, Q This is energy flow from a region at higher temperature
to a region at lower temperature, due to the
temperature difference. In thermodynamics we deal
with heat going into or out of a system. It makes no
sense to speak of heat in a system.
1.8 (f) Work, W If the system is a gas, in a cylinder fitted with a piston,
the gas does work of amount p∆V when it exerts a
pressure p and pushes the piston out a small way, so
the gas volume increases by ∆V. Work, like heat, is
energy in transit from (or to) the system.
1.8 (i) First law of The increase, ∆U, in internal energy of a system is
thermodynamics ∆U = Q – W in which Q is the heat entering the system
and W is the work done by the system. Any of the
terms in the equation can be positive or negative, e.g.
if 100 J of heat is lost from a system Q = –100 J.
1.8 (k) Specific heat The heat required, per kilogram, per degree celsius or
capacity, c kelvin, to raise the temperature of a substance.
UNIT: J kg-1 K-1 or J kg-1 °C-1
A level COMPONENT 2
Unit: none
2.2 (a) Potential The pd between two points is the energy converted from
difference (pd), V electrical potential energy to some other form per coulomb of
charge flowing from one point to the other. Unit: V [= J C-1]
2.2 (d) Ohm’s law The current in a metal wire at constant temperature is
proportional to the pd across it.
2.2 (e) Electrical The resistance of a conductor is the pd (V) placed across it
resistance, R divided by the resulting current (I) through it.
V
R= Unit: Ω [= V A-1]
I
2.2 (h) Resistivity, ρ The resistance, R, of a metal wire of length L and cross-
ρL
sectional area A is given by R = , in which ρ the
A
resistivity, is a constant (at constant temperature) for the
material of the wire. Unit: Ω m
2.2 (k) Superconducting The temperature at which a material, when cooled, loses all
transition its electrical resistance, and becomes super-conducting.
temperature, Tc Some materials (e.g. copper) never become superconducting
however low the temperature becomes.
2.3 (a) The law of Electric charge cannot be created or destroyed, (though
conservation of positive and negative charges can neutralise each other).
charge Charge cannot pile up at a point in a circuit.
2.3 (g) Emf, E The emf of a source is the energy converted from some other
form (e.g. chemical) to electrical potential energy per
coulomb of charge flowing through the source.
Unit: V
2.4 (a) Capacitor A capacitor is a pair of conducting plates separated by an
insulator. If a potential difference is placed across the plates,
they acquire equal and opposite charges.
2.4 (c) Capacitance, C, chargeon either plate
of a capacitor capacitance =
pdbetweenplates
Unit: F [= C V-1]
2.4 (e) Dielectric Insulator between the plates of a capacitor, also serving to
make the capacitance larger than if there were just empty
space.
2.5 (a) Hooke’s law The tension in a spring or wire is proportional to its extension
from its natural length, provided the extension is not too
great.
Spring constant, The spring constant is the force per unit extension.
k Unit: N m-1
2.5 (b) Stress, σ Stress is the force per unit cross-sectional area when equal
opposing forces act on a body.
Unit Pa or N m-2
Strain, ε Strain is defined as the extension per unit length due to an
applied stress. Unit: none
Young modulus, tensilestress
Young modulus E =
E
tensilestrain
Unless otherwise indicated this is defined for the Hooke’s law
region. Unit: Pa or N m-2
2.5 (d) Crystal Solid in which atoms are arranged in a regular array. There is
a long range order within crystal structures.
Crystalline solid Solid consisting of a crystal, or of many crystals, usually
arranged randomly. The latter is strictly a polycrystalline
solid. Metals are polycrystalline.
Amorphous solid A truly amorphous solid would have atoms arranged quite
randomly. Examples are rare. In practice we include solids
such as glass or brick in which there is no long range order in
the way atoms are arranged, though there may be ordered
clusters of atoms.
Polymeric solid A solid which is made up of chain-like molecules.
2.5 (e) Ductile material A material which can be drawn out into a wire. This implies
that plastic strain occurs under enough stress.
Elastic strain This is strain that disappears when the stress is removed,
that is the specimen returns to its original size and shape.
Plastic (or This is strain that decreases only slightly when the stress is
inelastic) strain removed. In a metal it arises from the movement of
dislocations within the crystal structure.
Elastic limit This is the point at which deformation ceases to be elastic.
For a specimen it is usually measured by the maximum
force, and for a material, by the maximum stress, before the
strain ceases to be elastic.
Dislocations in Certain faults in crystals which (if there are not too many)
crystals reduce the stress needed for planes of atoms to slide. The
easiest dislocation to picture is an edge dislocation: the edge
of an intrusive, incomplete plane of atoms.
Grain boundaries The boundaries between crystals (grains) in a polycrystalline
material.
Ductile fracture The characteristic fracture process in a ductile material. The
(necking) fracture of a rod or wire is preceded by local thinning which
increases the stress.
2.5 (f) Brittle material Material with no region of plastic flow, which, under tension,
fails by brittle fracture.
Brittle fracture This is the fracture under tension of brittle materials by
means of crack propagation.
2.5 (g) Elastic hysteresis When a material such as rubber is put under stress and the
stress is then relaxed, the stress-strain graphs for increasing
and decreasing stress do not coincide, but form a loop. This
is hysteresis.
2.6 (a) Newton’s law of The gravitational force between two particles is proportional
gravitation to the product of their masses, m1 and m2, and inversely
proportional to their separation squared, r2.
Gm1m2
F= in which G is the gravitational constant.
r2
G = 6.67 × 10-11N m2 kg-2.
Coulomb’s law The electrostatic force, F, between two small bodies is
proportional to the product of their charges, Q1 and Q2, and
inversely proportional to their separation squared, r2.
Q1Q2
F= in which ε is 0the permittivity of free space = 8.85
4πε 0 r 2
× 10-12 F m-1
Electric field The force experienced per unit charge by a small positive
strength, E charge placed in the field. Unit: V m-1 or N C-1
Gravitational field The force experienced per unit mass by a mass placed in the
strength, g field. Unit: m s-2 or N kg-1
Electric potential, Electric potential at a point is the work done per unit charge
VE in bringing a positive charge from infinity to that point.
Unit: V or JC-1
Gravitational Gravitational potential at a point is the work done per unit
potential, Vg mass in bringing a mass from infinity to that point.
Unit: J kg-1.
2.7 (b) Black body A black body is a body (or surface) which absorbs all the
electromagnetic radiation that falls upon it. No body is a
better emitter of radiation at any wavelength than a black
body at the same temperature.
2.7 (d) Wien’s The wavelength of peak emission from a black body is
displacement law inversely proportional to the absolute (kelvin) temperature of
the body.
λmax = W
T [W = the Wien constant = 2.90 × 10-3 m K]
Absolute or The temperature, T in kelvin (K) is related to the
kelvin temperature, θ, in celsius (°C) by:
temperature T / K= θ / °C + 273.15
At 0 K (-273.15°C) the energy of particles in a body is the
lowest it can possibly be.
Stefan’s law The total electromagnetic radiation energy emitted per unit
[The Stefan- time by a black body is given by power = A σT4 in which A is
Boltzmann law] the body’s surface area and σ is a constant called the Stefan
constant. [σ = 5.67 × 10-8 W m-2 K-4]
Luminosity of a The luminosity of a star is the total energy it emits per unit
star time in the form of electromagnetic radiation. UNIT: W
[Thus we could have written luminosity instead of power in
Stefan’s law (above).]
Intensity The intensity of radiation at a distance R from a source is
P
given by I = UNIT: W m-2
4πR 2
2.8 (a) Kepler’s laws of Each planet moves in an ellipse with the Sun at one focus.
planetary motion:
1
Kepler’s laws of The line joining a planet to the centre of the Sun sweeps out
planetary motion: equal areas in equal times.
2
Kepler’s laws of T2, the square of the period of the planet’s motion, is
planetary motion: proportional to r3, in which r is the semi-major axis of its
3 ellipse. [For orbits which are nearly circular, r may be taken
as the mean distance of the planet from the Sun.]
2.8 (e) Dark matter Matter which we can’t see, or detect by any sort of radiation,
but whose existence we infer from its gravitational effects.
2.8 (i) Radial velocity of This is the component of a star’s velocity along the line
a star [in the joining it and an observer on the Earth.
context of
Doppler shift]
2.8 (k) Galactic radial This is the mean component of a galaxy's velocity along the
velocity line joining it and an observer on Earth.
A level COMPONENT 3