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Flashcards · YPH11 · Topic 5
Thermodynamics, Radiation, Oscillations and Cosmology flashcards
41 cards on Topic 5, subtopics 5.3 to 5.6. Pick a subtopic or study them all.
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5.3 Thermodynamics
- Internal energy
- The sum of the randomly distributed kinetic and potential energies of the molecules in a system.
- Why does the temperature stay constant while a substance melts or boils?
- The energy supplied increases the potential energy of the molecules (their separation), not their kinetic energy, so the temperature does not change.
- Specific heat capacity and specific latent heat equations
- ΔE = mcΔθ: energy to raise 1 kg by 1 K is c. ΔE = LΔm: energy to change the state of 1 kg with no temperature change is L.
- Energy to turn 0.50 kg of water at 100 °C into steam? (L = 2.26 × 10⁶ J/kg)
- E = 2.26 × 10⁶ × 0.50 = 1.13 × 10⁶ J
- Absolute zero and the kelvin scale
- T(K) = θ(°C) + 273. At absolute zero the molecules have minimum internal energy, not zero energy.
- Ideal gas equations
- pV = nRT (R = 8.31 J mol⁻¹ K⁻¹) pV = NkT (k = 1.38 × 10⁻²³ J K⁻¹) T in kelvin.
- Kinetic theory: pressure, and mean molecular kinetic energy
- pV = ⅓Nm⟨c²⟩ ½m⟨c²⟩ = (3/2)kT: mean molecular kinetic energy depends only on absolute temperature.
- Assumptions of the kinetic model of an ideal gas
- Many molecules in random motion; molecular volume negligible; no forces between molecules except in collisions; collisions elastic; collision time negligible compared with time between collisions.
- Why is the internal energy of an ideal gas only kinetic?
- There are no intermolecular forces, so there is no molecular potential energy. The internal energy depends only on temperature.
- Core Practicals 12, 13 and 14
- 12: calibrate a thermistor in a potential divider as a thermostat. 13: determine a specific latent heat. 14: pressure and volume of a fixed mass of gas at constant temperature.
5.4 Nuclear Decay
- Alpha radiation
- A helium nucleus, charge +2. Stopped by paper. Strongly ionising.
- Beta-minus radiation
- An electron, charge −1. Stopped by about 3 mm of aluminium. Moderately ionising.
- Gamma radiation
- An electromagnetic photon, no charge. Reduced by thick lead. Weakly ionising.
- Why is alpha the least penetrating radiation?
- It is the most strongly ionising, so it loses its energy quickly and travels only a short distance.
- Mass deficit and binding energy
- Mass deficit: the mass of the separated nucleons minus the mass of the nucleus. The binding energy is ΔE = c²Δm. 1 u = 1.66 × 10⁻²⁷ kg.
- Why do both fission and fusion release energy?
- Binding energy per nucleon peaks around iron. Fusing light nuclei and splitting heavy nuclei both move towards higher binding energy per nucleon.
- Beta-minus and beta-plus decay in terms of nucleons
- β⁻: n → p + e⁻ + antineutrino (A same, Z + 1). β⁺: p → n + e⁺ + neutrino (A same, Z − 1).
- Activity and the decay constant
- A = λN (Bq). λ is the probability per unit time that a nucleus decays. N = N₀e^(−λt), and t½ = ln 2 / λ.
- How do you find λ from activity measurements?
- Subtract background, then plot ln A against t: a straight line of gradient −λ.
- Core Practical 15
- Investigate the absorption of gamma radiation by lead (count rate against absorber thickness, background subtracted).
5.5 Oscillations
- Definition of simple harmonic motion
- Acceleration is proportional to the displacement from the equilibrium position and always directed towards it: a = −ω²x. The restoring force F = −kx.
- Maximum speed and maximum acceleration in SHM
- v_max = ωA, at the equilibrium position. a_max = ω²A, at maximum displacement. ω = 2πf = 2π/T.
- Periods of a simple pendulum and of a mass on a spring
- Pendulum: T = 2π√(l/g) (small angles only). Mass–spring: T = 2π√(m/k). Neither depends on the amplitude.
- A 0.60 kg mass oscillates on a spring of k = 15 N/m. Period?
- T = 2π√(0.60/15) = 2π × 0.20 = 1.26 s
- Phase of velocity relative to displacement in SHM
- Velocity leads displacement by 90°: it is maximum at zero displacement and zero at maximum displacement.
- Phase of acceleration relative to displacement in SHM
- Acceleration is 180° out of phase with displacement: maximum and opposite at the extremes, zero at the centre.
- Light damping
- The amplitude decays gradually over many oscillations.
- Critical damping
- The fastest return to equilibrium without overshooting (used in car suspension). Heavy damping returns more slowly, also without oscillating.
- Free vs forced oscillation, and resonance
- Free: at the natural frequency with no driving force. Forced: driven by an external periodic force. Resonance: driving frequency = natural frequency, giving maximum amplitude.
- Effect of more damping on a resonance curve
- Lower peak amplitude, a broader curve, and the peak shifts slightly to a lower frequency.
5.6 Astrophysics and Cosmology
- Newton’s law of gravitation, and the field of a point mass
- F = Gm₁m₂/r² g = F/m = Gm/r²
- Gravitational potential of a point mass
- V = −Gm/r. Always negative, rising to zero at infinity (unlike electric potential, which can be positive).
- Luminosity vs radiant flux
- Luminosity L: total power emitted by a star. Radiant flux F: power received per unit area, F = L / (4πd²).
- Standard candle, with an example
- An object of known luminosity, so measuring its flux gives its distance. Type Ia supernovae have a consistent peak luminosity.
- Trigonometric parallax
- The apparent shift of a nearby star against distant background stars as the Earth orbits the Sun, used to find its distance.
- Wien’s law and the Stefan–Boltzmann law
- λmax T = 2.898 × 10⁻³ m K L = 4πr²σT⁴ Use Wien for temperature first, then Stefan for radius.
- A star has surface temperature 5800 K. Peak wavelength?
- λmax = 2.898 × 10⁻³ ÷ 5800 = 5.00 × 10⁻⁷ m (500 nm)
- Hertzsprung–Russell diagram: axes and regions
- Luminosity (up) against temperature (increasing to the left). Main sequence: diagonal band. Red giants: top right (cool, luminous, so large). White dwarfs: bottom left (hot, dim, so small).
- Evolution of a Sun-like star and of a massive star
- Sun-like: main sequence → red giant → planetary nebula → white dwarf. Massive: main sequence → red supergiant → supernova → neutron star or black hole.
- Doppler red-shift equation, and the age of the universe
- z = Δλ/λ ≈ v/c. Hubble’s law v = H₀d gives an age of about 1/H₀.
- Why is there controversy about the age and fate of the universe?
- The value of the Hubble constant is uncertain, and the possible existence of dark matter (from galactic rotation curves) and dark energy affects how the expansion changes.