NSSCO Physics (6118) study materials
NSSCO Physics (6118) study resources

NSSCO Physics (6118) cheat sheet

NSSCO Physics (6118) · Keep the key ideas within reach.

Quick reference

Measurement and Units

  • SI base units: metre (m) length, kilogram (kg) mass, second (s) time, ampere (A) current, kelvin (K) temperature, mole (mol) amount of substance, candela (cd) luminous intensity.

  • Derived units: N = kg m s^-2; J = N m = kg m^2 s^-2; W = J s^-1; Pa = N m^-2; C = A s; V = J C^-1 = W A^-1; ohm = V A^-1.

  • Prefixes: nano 10^-9, micro 10^-6, milli 10^-3, centi 10^-2, kilo 10^3, mega 10^6, giga 10^9.

  • Density p = m/V in kg m^-3; regular solid volume from dimensions, irregular solid volume by displacement in a measuring cylinder.

  • Resolution of instruments: metre rule 1 mm, vernier calliper 0.1 mm, micrometer screw gauge 0.01 mm.

  • Reading uncertainty: analogue scale +/- half the smallest division; digital display +/- the last digit shown.

  • Random error is reduced by repeat readings and averaging; systematic error such as zero error shifts every reading the same way and must be subtracted, not averaged out.

  • Perpendicular vectors add by Pythagoras, magnitude sqrt(x^2 + y^2); non-perpendicular vectors add by scale drawing (nose-to-tail) or by resolving into components.

Quick reference

Kinematics and Dynamics: Motion, Forces and Momentum

  • Constant-acceleration equations: v = u + at; s = ut + 0.5at^2; v^2 = u^2 + 2as; s = 0.5(u + v)t.

  • Gradient of a displacement-time graph = velocity; gradient of a velocity-time graph = acceleration; area under a velocity-time graph = displacement.

  • Newton's first law: a body stays at rest or moves with constant velocity in a straight line unless a resultant external force acts on it.

  • Newton's second law: resultant force F = ma (F in N, m in kg, a in m s^-2); weight W = mg with g about 9.8 N kg^-1 near the Earth's surface.

  • Newton's third law: if A exerts a force on B, B exerts an equal and opposite force on A; the two forces act on different bodies and never cancel on one object.

  • Momentum p = mv is a vector in kg m s^-1; total momentum is conserved in collisions and explosions when no external resultant force acts.

  • Impulse = Ft = change in momentum = mv - mu; the area under a force-time graph equals the impulse.

  • Friction and drag oppose relative motion; terminal velocity is reached when drag equals weight, so the resultant force and acceleration are zero.

Quick reference

Work, Energy, Power and Pressure

  • Work W = Fd, where d is the distance moved along the direction of the force; 1 J = 1 N m.

  • Kinetic energy KE = 0.5mv^2; change in gravitational potential energy = mg(delta h).

  • Conservation of energy: energy is neither created nor destroyed, only transferred between stores; total energy in = total energy out.

  • Power P = W/t = E/t = Fv; 1 W = 1 J s^-1.

  • Efficiency = (useful energy output / total energy input) x 100%; friction, heating and sound always make efficiency less than 100%.

  • Pressure p = F/A in pascals (Pa = N m^-2); for the same force, a smaller contact area gives a larger pressure.

  • Pressure in a liquid p = rho g h; at a given depth it acts equally in all directions and does not depend on the shape or width of the container.

  • Pascal's principle: pressure applied to an enclosed fluid is transmitted undiminished, so F1/A1 = F2/A2 in a hydraulic system.

  • Upthrust equals the weight of fluid displaced (Archimedes' principle); a body floats when upthrust equals its weight and sinks when its weight is greater.

Quick reference

Thermal Physics

  • Temperature measures the average kinetic energy of particles; heat is energy in transit because of a temperature difference, so a body does not contain 'heat'.

  • Specific heat capacity c: Q = mc(delta theta); for water c is about 4200 J kg^-1 K^-1, so 4200 J raises 1 kg by 1 K.

  • Specific latent heat L: Q = mL, the energy to change state at constant temperature; for water the latent heat of vaporisation is about 2.26 x 10^6 J kg^-1.

  • Conduction in solids relies on particle vibration and free electrons; convection in fluids relies on density differences; radiation is infrared electromagnetic waves and needs no medium.

  • Dull black surfaces are good absorbers and emitters of infrared; shiny light surfaces are poor absorbers and good reflectors.

  • Gas laws for a fixed mass: Boyle p1V1 = p2V2 at constant T; pressure law p1/T1 = p2/T2 at constant V; Charles V1/T1 = V2/T2 at constant p; T must be in kelvin.

  • Kelvin temperature T = theta(degrees C) + 273; a temperature change of 1 K equals a change of 1 degree C.

  • Evaporation happens below the boiling point at the liquid surface; it speeds up with higher temperature, larger surface area, moving air and lower humidity, and it cools the remaining liquid.

Quick reference

Waves

  • A wave transfers energy without transferring matter; mechanical waves need a medium, electromagnetic waves travel through vacuum.

  • Transverse waves oscillate perpendicular to the direction of travel (light, water ripples); longitudinal waves oscillate parallel to travel, forming compressions and rarefactions (sound).

  • Wave quantities: amplitude = maximum displacement; wavelength lambda = crest to crest; frequency f = oscillations per second; period T = 1/f.

  • Wave equation v = f lambda; the speed in a given medium is fixed, so a higher frequency means a shorter wavelength.

  • At a boundary between media the frequency stays constant while speed and wavelength change, causing a change of direction (refraction).

  • Reflection: angle of incidence = angle of reflection. Diffraction: spreading of waves at a gap or edge. Interference: superposition of waves from two coherent sources.

  • Diffraction is greatest when the gap width is about equal to the wavelength, and is negligible when the gap is much wider.

  • Electromagnetic spectrum in order of increasing frequency: radio, microwave, infrared, visible, ultraviolet, X-rays, gamma rays; all travel at 3.0 x 10^8 m s^-1 in vacuum.

Quick reference

Sound and Light

  • Sound is a longitudinal wave that needs a medium; it travels at about 340 m s^-1 in air and faster in liquids and solids, but not through vacuum.

  • Audible range is about 20 Hz to 20 kHz; ultrasound is above 20 kHz and is used in sonar, medical imaging and cleaning.

  • Echo ranging: 2d = v t, so d = v t / 2, because the sound travels to the reflector and back.

  • Law of reflection: angle of incidence = angle of reflection, both measured from the normal; a plane mirror forms a virtual, upright, same-size, laterally inverted image.

  • Refraction: light bends towards the normal entering a denser medium (slower) and away from the normal entering a less dense medium (faster).

  • Refractive index n = sin i / sin r = speed in vacuum / speed in medium; the critical angle is given by sin c = 1/n.

  • Total internal reflection occurs for light travelling from a denser to a less dense medium when the angle of incidence exceeds the critical angle; used in optical fibres and prisms.

  • Converging lens: parallel rays meet at the principal focus, focal length f, power P = 1/f in dioptres (D). Real images are inverted and can be projected; virtual images are upright.

  • A prism disperses white light because the refractive index differs for each colour; red is deviated least and violet most.

Quick reference

Electricity and Magnetism

  • Current I = Q/t is the rate of flow of charge, measured with an ammeter in series; conventional current flows from positive to negative.

  • Potential difference V = W/Q is energy transferred per unit charge, measured with a voltmeter in parallel across the component.

  • Ohm's law: V = IR for a metallic conductor at constant temperature; resistance R = V/I in ohms and equals the gradient of a V-I graph.

  • Series: current is the same everywhere, voltage splits, R = R1 + R2 + ... Parallel: voltage is the same, current splits, 1/R = 1/R1 + 1/R2 + ...

  • Power P = VI = I^2R = V^2/R; energy E = Pt, with domestic energy measured in kilowatt-hours (1 kWh = 3.6 x 10^6 J).

  • Magnetic field lines run from north to south outside a magnet and never cross; a current-carrying solenoid behaves like a bar magnet and an iron core makes an electromagnet.

  • Motor effect: a conductor carrying current at right angles to a magnetic field feels a force F = BIl; the direction is given by Fleming's left-hand rule.

  • Electromagnetic induction: relative motion between a magnet and a coil, or a changing magnetic field, induces a voltage whose direction opposes the change (Lenz's law).

  • Transformer: Vp/Vs = Np/Ns; for an ideal transformer VpIp = VsIs, so a step-up transformer raises voltage and lowers current.

Quick reference

Atomic and Nuclear Physics

  • The atom has a small, dense, positively charged nucleus of protons and neutrons, surrounded by electrons; most of the atom is empty space.

  • Proton number Z = number of protons, which fixes the element; nucleon number A = protons + neutrons; isotopes have the same Z but different A.

  • Alpha decay: an alpha particle is a helium nucleus (2 protons, 2 neutrons), so A falls by 4 and Z by 2. Beta decay: a neutron becomes a proton and an electron, so Z rises by 1 and A is unchanged. Gamma emission changes neither A nor Z.

  • Penetration: alpha is stopped by paper or a few centimetres of air, beta by a few millimetres of aluminium, gamma is only reduced by thick lead or concrete; ionising power is in the reverse order.

  • Half-life is the time for half the nuclei in a sample to decay, so the activity also halves in each half-life.

  • Nuclear equations must balance nucleon numbers (top) and proton numbers (bottom) on both sides.

  • Fission: a heavy nucleus such as uranium-235 absorbs a neutron, splits into two lighter nuclei and releases energy plus more neutrons; used in power reactors.

  • Fusion: light nuclei such as hydrogen isotopes join to form a heavier nucleus, releasing energy; it needs very high temperature and powers stars.

  • Background radiation comes from cosmic rays, rocks, radon gas and medical or nuclear sources, and must be subtracted from counts when measuring a source's activity.