Formulas
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Unit 1 Motion, forces and energy
1.1 Physical quantities and measurement techniques
Period from many oscillations
T = (time for n oscillations) ÷ n
T = period, the time for one complete oscillation (s); n = number of complete oscillations timed
Resultant of two vectors at right anglesExtended
resultant = √(a2 + b2)
a, b = sizes of two forces (N) or two velocities (m/s) that act at right angles to each other; the direction is found from tan θ = b / a, where θ is the angle between the resultant and a
1.2 Motion
Speed
v = s / t
v = speed (m/s); s = distance travelled (m); t = time taken (s)
Average speed
average speed = total distance travelled ÷ total time taken
distance in m, time in s, average speed in m/s
Distance from a speed–time graph
distance travelled = area under the speed–time graph
constant speed: area of a rectangle = speed × time; constant acceleration: split the area into a rectangle and a triangle where needed; area of a triangle = ½ × base × height
AccelerationExtended
a = Δv / Δt
a = acceleration (m/s2); Δv = change in velocity (m/s); Δt = time taken for the change (s)
1.3 Mass and weight
Gravitational field strength
g = W / m
g = gravitational field strength (N/kg); W = weight (N); m = mass (kg)
1.4 Density
Density
ρ = m / V
ρ = density (kg/m3 or g/cm3); m = mass (kg or g); V = volume (m3 or cm3)
1.5 Forces
Spring constantExtended
k = F / x
k = spring constant (N/m or N/cm); F = force, the load on the spring (N); x = extension (m or cm)
Resultant force and accelerationExtended
F = ma
F = resultant force (N); m = mass (kg); a = acceleration (m/s2), in the same direction as F
Moment of a force
moment = force × perpendicular distance from the pivot
force in N; perpendicular distance from the pivot to the line of the force in m; moment in N m
Principle of moments
total clockwise moment = total anticlockwise moment
for an object in equilibrium; all moments taken about the same pivot, in N m
1.6 Momentum
MomentumExtended
p = mv
p = momentum (kg m/s); m = mass (kg); v = velocity (m/s)
ImpulseExtended
impulse = FΔt = Δ(mv)
F = force (N); Δt = time for which the force acts (s); Δ(mv) = change in momentum (kg m/s); impulse in N s
Resultant force and momentumExtended
F = Δp / Δt
F = resultant force (N); Δp = change in momentum (kg m/s); Δt = time taken for the change (s)
Conservation of momentumExtended
total momentum before = total momentum after
applies when no resultant external force acts on the objects; momentum in kg m/s, with a sign for direction
1.7 Energy, work and power
Kinetic energyExtended
Ek = ½mv2
Ek = kinetic energy (J); m = mass (kg); v = speed (m/s)
Change in gravitational potential energyExtended
ΔEp = mgΔh
ΔEp = change in gravitational potential energy (J); m = mass (kg); g = gravitational field strength (9.8 N/kg near the Earth's surface); Δh = change in height (m)
Work done
W = Fd = ΔE
W = work done (J); F = force (N); d = distance moved in the direction of the force (m); ΔE = energy transferred (J)
Efficiency (energy)Extended
(%) efficiency = (useful energy output) / (total energy input) (× 100%)
both energies in the same unit (J); multiply by 100% to give a percentage
Efficiency (power)Extended
(%) efficiency = (useful power output) / (total power input) (× 100%)
both powers in the same unit (W); multiply by 100% to give a percentage
Power from work done
P = W / t
P = power (W); W = work done (J); t = time taken (s)
Power from energy transferred
P = ΔE / t
P = power (W); ΔE = energy transferred (J); t = time taken (s)
1.8 Pressure
Pressure
p = F / A
p = pressure (N/m2 or N/cm2; Pa in Extended); F = force acting at right angles to the surface (N); A = area (m2 or cm2)
Change in pressure beneath the surface of a liquidExtended
Δp = ρgΔh
Δp = change in pressure (Pa); ρ = density of the liquid (kg/m3); g = gravitational field strength (9.8 N/kg); Δh = change in depth (m)
Unit 2 Thermal physics
2.1 Kinetic particle model of matter
Kelvin and Celsius
T (in K) = θ (in °C) + 273
T = temperature in kelvin (K); θ = temperature in degrees Celsius (°C)
Gas at constant temperatureExtended
pV = constant
p = pressure of the gas (Pa); V = volume of the gas (m3); true for a fixed mass of gas at constant temperature, so p1V1 = p2V2
2.2 Thermal properties and temperature
Specific heat capacityExtended
c = ΔE / (mΔθ)
c = specific heat capacity (J/(kg °C)); ΔE = energy transferred to the object (J); m = mass (kg); Δθ = rise in temperature (°C). Rearranged: ΔE = mcΔθ
Unit 3 Waves
3.1 General properties of waves
Wave speed
v = fλ
v = wave speed (m/s); f = frequency (Hz); λ = wavelength (m)
3.2 Light
Law of reflection
angle of incidence = angle of reflection
i = angle of incidence (°); r = angle of reflection (°); both measured from the normal, so i = r
Refractive index from speedsExtended
n = speed of light in a vacuum ÷ speed of light in the material
n = refractive index of the material (no unit). In general n = speed in region 1 ÷ speed in region 2; here region 1 is a vacuum. The speed of light in air is almost the same as in a vacuum.
Refractive index from anglesExtended
n = sin i / sin r
n = refractive index (no unit); i = angle of incidence in air (°); r = angle of refraction in the material (°)
Critical angleExtended
n = 1 / sin c
n = refractive index of the material (no unit); c = critical angle (°)
3.3 Electromagnetic spectrum
Speed of electromagnetic wavesExtended
speed in a vacuum = 3.0 × 108 m/s
the same for every region of the spectrum; approximately the same in air; use it in v = fλ (see 3.1)
3.4 Sound
Speed of sound
v = s / t
v = speed of sound (m/s); s = distance the sound travels (m); t = time taken (s). For an echo, s is twice the distance to the reflecting surface.
Depth or distance from an echoExtended
depth = v × t ÷ 2
v = speed of sound in the material (m/s); t = time from sending the pulse to receiving the echo (s); divide by 2 because the pulse travels there and back
Unit 4 Electricity and magnetism
4.2 Electrical quantities
CurrentExtended
I = Q / t
I = current (A); Q = charge (C); t = time (s)
Electromotive forceExtended
E = W / Q
E = e.m.f. (V); W = work done by the source (J); Q = charge (C)
Potential differenceExtended
V = W / Q
V = p.d. (V); W = work done (J); Q = charge (C)
Resistance
R = V / I
R = resistance (Ω); V = p.d. (V); I = current (A)
Resistance of a metallic wireExtended
R ∝ l and R ∝ 1 / A
R = resistance (Ω); l = length of the wire (m); A = cross-sectional area of the wire (m2); same material at the same temperature
Electrical power
P = IV
P = power (W); I = current (A); V = p.d. (V)
Electrical energy
E = IVt
E = energy transferred (J); I = current (A); V = p.d. (V); t = time (s)
Cost of electricity
cost = energy used in kW h × price of 1 kW h
energy in kW h = power (kW) × time (h); 1 kW h = 3.6 × 106 J
4.3 Electric circuits
Sources in series
E = E1 + E2 + E3 + …
E = combined e.m.f. (V); E1, E2, E3 = e.m.f. of each source (V); all sources connected the same way round
Resistors in series
R = R1 + R2 + R3 + …
R = combined resistance (Ω); R1, R2, R3 = resistance of each resistor (Ω)
Two resistors in parallelExtended
R = R1R2 / (R1 + R2)
R = combined resistance (Ω); R1, R2 = resistance of each resistor (Ω); the same as 1 / R = 1 / R1 + 1 / R2
Currents at a junctionExtended
sum of currents into a junction = sum of currents out of the junction
for a supply current I that splits into two branches: I = I1 + I2 (A)
P.d.s in seriesExtended
V = V1 + V2 + …
V = total p.d. across the series components (V); V1, V2 = p.d. across each component (V)
P.d. across parallel branchesExtended
V = V1 = V2
V = p.d. across the parallel arrangement (V); V1, V2 = p.d. across each branch (V)
Potential dividerExtended
R1 / R2 = V1 / V2
R1, R2 = the two resistors in series (Ω); V1, V2 = p.d. across each of them (V)
4.4 Electrical safety
Current taken by an appliance
I = P / V
I = current (A); P = power of the appliance (W); V = supply p.d. (V); this is P = IV from 4.2.5, rearranged
4.5 Electromagnetic effects
Transformer equation
Vp / Vs = Np / Ns
V = voltage (V); N = number of turns; p = primary coil, s = secondary coil
Transformer at 100% efficiencyExtended
IpVp = IsVs
I = current (A); V = voltage (V); p = primary coil, s = secondary coil
Power loss in cablesExtended
P = I2R
P = power lost as thermal energy in the cables (W); I = current in the cables (A); R = resistance of the cables (Ω)
Unit 5 Nuclear physics
5.1 The nuclear model of the atom
Number of neutrons
number of neutrons = A − Z
A = nucleon number (mass number), Z = proton number (atomic number)
Balancing a nuclide equationExtended
total A before = total A after; total Z before = total Z after
A = nucleon number (top number), Z = proton number (bottom number)
5.2 Radioactivity
Corrected count rateExtended
corrected count rate = measured count rate − background count rate
count rates in counts/s or counts/minute
Amount left after n half-lives
amount left = starting amount ÷ 2n
amount = number of undecayed nuclei, or the count rate due to the source; n = number of half-lives that have passed
Alpha decayExtended
AZX → A−4Z−2Y + 42He
A = nucleon number, Z = proton number; X = parent nucleus, Y = new nucleus; 42He = α-particle
Beta decayExtended
AZX → AZ+1Y + 0−1e
A = nucleon number, Z = proton number; X = parent nucleus, Y = new nucleus; 0−1e = β-particle
Gamma emissionExtended
AZX → AZX + 00γ
A = nucleon number, Z = proton number; γ = gamma radiation
Unit 6 Space physics
6.1 The Earth and the Solar System
Average orbital speedExtended
v = 2πr / T
v = average orbital speed (m/s), r = average radius of the orbit (m), T = orbital period (s)
Time for light to travel a distance
t = d / c
t = time (s), d = distance (m), c = speed of light in a vacuum = 3.0 × 108 m/s
6.2 Stars and the Universe
One light-yearExtended
1 light-year = 9.5 × 1015 m
one light-year = the distance light travels in a vacuum in one year
Hubble constantExtended
H0 = v / d
H0 = Hubble constant (s−1), current estimate 2.2 × 10−18 per second; v = speed at which the galaxy is moving away from the Earth (m/s); d = distance of the galaxy from the Earth (m)
Age of the UniverseExtended
d / v = 1 / H0
d / v = estimate of the age of the Universe (s); H0 = Hubble constant (s−1)