PhysicsQ&A by dot point

Apply the concepts of gravitational potential energy and kinetic energy to determine the total energy of a planet or satellite in its orbit, and the energy changes that occur when satellites move between orbits

Derive and apply the concept of gravitational potential energy in a radial gravitational field, U = -G M m / r, including the concept of escape velocity

Investigate the relationship of Kepler's Laws of Planetary Motion to the forces acting on, and the total energy of, planets in circular and non-circular orbits using v = 2 pi r / T and T^2 / r^3 = 4 pi^2 / (G M)

Apply qualitatively and quantitatively Newton's Law of Universal Gravitation, F = G m_1 m_2 / r^2, to determine the magnitude of force, gravitational field strength g = G M / r^2, and acceleration due to gravity at different points in a radial gravitational field

Investigate the relationship between the forces acting on objects in non-uniform circular motion (banked tracks, conical pendulums, vertical circles) and apply the relationship tau = r F sin theta for torque

Predict quantitatively the orbital properties of planets and artificial satellites in a variety of situations, including near-Earth and geostationary orbits, using the relationship between orbital speed, radius, and period

Analyse the motion of projectiles by resolving the motion into horizontal and vertical components, making the following assumptions: a constant vertical acceleration due to gravity, zero air resistance

Conduct investigations to explain and evaluate, for objects executing uniform circular motion, the relationships that exist between centripetal force, mass, speed and radius, and solve problems using the relationships a_c = v^2 / r, v = 2 pi r / T, F_c = m v^2 / r and omega = delta theta / delta t

Investigate and quantitatively derive and analyse the interaction between charged particles and uniform electric fields, including: electric field between parallel charged plates E = V/d, acceleration of charged particles by the electric field F_net = ma, F = qE, work done on the charge W = qV, W = qEd, K = (1/2)mv^2

Analyse the interaction between charged particles and uniform magnetic fields, including: acceleration, perpendicular to velocity F = qv x B, circular motion of a charged particle moving perpendicular to a uniform magnetic field

Investigate quantitatively and analyse the interaction between current-carrying conductors and uniform magnetic fields F/l = I B sin theta, including parallel current-carrying wires F/l = mu_0 I_1 I_2 / (2 pi r)

Analyse the operation of DC and AC motors, including the torque on a current loop tau = n B I A cos theta, the role of the commutator, back EMF, and the AC induction motor principle

Model qualitatively and quantitatively the electric field, including direction and shape, produced between parallel charged plates and the potential difference, using E = V/d

Describe and quantitatively analyse electromagnetic induction using Faraday's law (induced EMF = - N dPhi/dt) and Lenz's law, including motional EMF, eddy currents and the induction coil

Describe how magnetic flux can be sensed by the changing alignment of a magnet on a compass needle and quantitatively analyse the concept of magnetic flux density B and flux Phi = B A cos theta in a magnetic field

Analyse the operation of ideal and real transformers, including the turns ratios V_s/V_p = N_s/N_p and I_p/I_s = N_s/N_p, energy losses, and the role of step-up and step-down transformers in AC power transmission

Describe the electromagnetic spectrum in terms of frequency, wavelength and photon energy, and outline how Maxwell's equations conceptually predict electromagnetic waves travelling at the speed of light

Investigate experimental and observational evidence for special relativity, including atmospheric and accelerator muon decay, GPS clock corrections, and the routine use of relativistic mechanics in particle physics

Analyse the Michelson-Morley experiment, state Einstein's two postulates of special relativity, and apply the consequences of time dilation, length contraction and relativity of simultaneity

Derive and apply the mass-energy equivalence E = mc^2, including the calculation of mass defect and binding energy in nuclear reactions

Analyse the photoelectric effect, including Einstein's photon equation hf = phi + KE_max, the role of Planck's constant, and the inability of the wave model to explain the threshold frequency and the kinetic-energy results

Compare classical and relativistic momentum, derive p = gamma m v, and analyse the role of relativistic momentum in particle accelerators

Investigate emission and absorption spectra, distinguish continuous, line emission and line absorption spectra, and analyse stellar spectra to identify chemical composition, surface temperature and motion

Analyse the wave model of light using Young's double-slit experiment, single-slit diffraction and polarisation, and apply Malus's law I = I_0 cos^2 theta to polarised light

Investigate the line emission spectra to examine the Balmer-Rydberg equation 1/lambda = R(1/n_f^2 - 1/n_i^2), and assess the limitations of the Bohr model of the hydrogen atom

Investigate, assess and model the experimental evidence supporting the existence and properties of the electron, including cathode ray tube experiments and Thomson's determination of the charge-to-mass ratio of the electron

Investigate de Broglie's matter waves, and the experimental evidence that confirms their existence including the Davisson-Germer experiment, and how matter waves explain the stability of Bohr orbits

Account for the energy released in nuclear fission and fusion in terms of mass defect and binding energy, using E = mc^2 and the binding energy curve

Investigate, assess and model Millikan's oil drop experiment to determine the elementary charge and the quantisation of electric charge

Investigate the evidence for the Big Bang theory and the early evolution of the universe, including cosmic microwave background radiation, abundance of light elements, and Hubble's law v = H_0 d

Examine the radioactive decay of atomic nuclei (alpha, beta, gamma) and represent these decays as nuclear equations; use the decay law N = N_0 e^(-lambda t) and the concept of half-life T_1/2

Investigate and analyse the Geiger-Marsden (Rutherford) gold foil experiment and Rutherford's nuclear model of the atom, and Chadwick's discovery of the neutron

Investigate the contribution of Schrodinger to the current model of the atom, including the probabilistic interpretation of the wavefunction and the concept of atomic orbitals replacing Bohr's fixed orbits

Investigate the Standard Model of matter, including quarks, leptons and the fundamental forces, and the role of particle accelerators in confirming the existence of these particles

Account for the production of emission and absorption spectra and compare these with a continuous black body spectrum; investigate stellar evolution using the Hertzsprung-Russell diagram and account for the synthesis of elements heavier than iron in supernovae