Revision Notes
Edexcel IAL Physics: Thermodynamics — Revision Notes
Condensed recall notes on internal energy, specific heat capacity, latent heat, the gas laws and kinetic theory for Edexcel International A Level Physics WPH15.
- Subject
- Physics
- Level
- A LEVELS
- Topic
- Unit 5: Thermodynamics, Radiation, Oscillations and Cosmology
- Author
- Iftikhar Azeemi
- Updated
Aligned to Pearson Edexcel A Level Physics (YPH11), Issue 3. Official specification .
Condensed for the final weeks. For the full explanation, use the Thermodynamics study guide.
Internal energy
The sum of the randomly distributed kinetic and potential energies of the molecules in a system — distinct from the macroscopic, ordered kinetic or potential energy of the object as a whole (e.g. a moving car’s bulk kinetic energy is not internal energy).
Both parts matter:
- The kinetic component depends on temperature.
- The potential component depends on separation, so it changes during a change of state.
This is why temperature stays constant while a substance melts or boils — the energy supplied increases the potential component only. That explanation is examined every series.
Heating equations
E = m c delta-theta specific heat capacity
E = m L specific latent heat
Specific heat capacity — energy to raise 1 kg by 1 K. Specific latent heat — energy to change the state of 1 kg with no temperature change.
Latent heat of vaporisation exceeds latent heat of fusion, because boiling must completely separate the molecules and do work pushing back the atmosphere, whereas melting only loosens them.
Worked example. 0.50 kg of water at 100 °C is converted entirely to steam at 100 °C (L of vaporisation = 2.26 × 10⁶ J/kg).
E = L m = 2.26x10^6 x 0.50 = 1.13x10^6 J (1.13 MJ)
CORE PRACTICAL 12 calibrates a thermistor in a potential divider circuit for use as a thermostat. CORE PRACTICAL 13 determines the specific latent heat of a phase change experimentally.
Temperature and absolute zero
T(K) = theta(C) + 273
Absolute zero is where molecules have minimum internal energy — not zero energy.
Temperature measures the mean kinetic energy of molecules, not the total thermal energy. A bath of warm water holds far more thermal energy than a cup of boiling water, despite being cooler — conflating the two is the commonest conceptual error.
Ideal gases
pV = nRT n in moles, R = 8.31 J mol^-1 K^-1
pV = NkT N molecules, k = 1.38 x 10^-23 J K^-1
pV = (1/3) N m <c^2>
(1/2) m <c^2> = (3/2) k T
The central result: mean molecular kinetic energy is proportional to absolute temperature only — not to pressure, volume, or the identity of the gas. Helium and xenon at the same temperature have equal mean molecular kinetic energy; the xenon simply moves more slowly because it is heavier.
T must always be in kelvin.
CORE PRACTICAL 14 investigates the relationship between pressure and volume of a fixed mass of gas at constant temperature (Boyle’s law).
Assumptions of the kinetic model: many molecules in random motion; molecular volume negligible; no intermolecular forces except during collisions; elastic collisions; collision time negligible compared with the time between collisions.
Real gases deviate most at high pressure and low temperature, because molecules are close together, so their own volume matters and attractions become significant — exactly the two assumptions that fail. This is why real gases are best approximated as ideal at low pressure and high temperature, where molecules are far apart and their own volume and mutual attractions become negligible by comparison.
Because an ideal gas has no intermolecular forces, it has no molecular potential energy, so its internal energy is entirely kinetic and depends only on temperature.
Exam traps
- Defining internal energy as kinetic energy only.
- Using E = mcΔθ during a change of state.
- Confusing temperature with thermal energy.
- Using °C in gas equations.
- Saying molecules stop at absolute zero.
- Saying heavier molecules have more kinetic energy at the same temperature.
- Forgetting which CORE PRACTICAL investigates which relationship — 12 is thermistor calibration, 13 is specific latent heat, 14 is Boyle’s law.
Self-test
- Define internal energy, covering both components.
- Why does temperature stay constant during boiling?
- Why is latent heat of vaporisation greater than latent heat of fusion?
- What is mean molecular kinetic energy proportional to?
- Under what conditions do real gases deviate most from ideal behaviour, and why?
- 0.50 kg of water at 100 °C is converted entirely to steam at 100 °C. Find the energy required (L of vaporisation = 2.26 × 10⁶ J/kg).
- What does CORE PRACTICAL 14 investigate?
- Distinguish internal energy from the macroscopic kinetic energy of a moving object.
Answers: 1. The sum of the randomly distributed kinetic and potential energies of the molecules; the kinetic part depends on temperature and the potential part on molecular separation. 2. The energy supplied increases the potential component by separating molecules rather than the kinetic component, so temperature does not rise. 3. Vaporisation must completely overcome the intermolecular forces and also do work against atmospheric pressure as the vapour expands; melting only loosens the forces. 4. The absolute temperature, and nothing else. 5. High pressure and low temperature, because molecules are close together so their own volume is no longer negligible and intermolecular attractions become significant. 6. E = Lm = 2.26×10⁶ × 0.50 = 1.13×10⁶ J (1.13 MJ). 7. The relationship between pressure and volume of a fixed mass of gas at constant temperature (Boyle’s law). 8. Internal energy is the random, disordered kinetic and potential energy of a substance’s individual particles; a moving object’s macroscopic kinetic energy is the ordered motion of the object as a whole and is a separate quantity entirely.
Related resources
-
Study Guides
Unit 5: Astrophysics and Cosmology
Gravitational fields, black body radiation, astronomical distance measurement, the Hertzsprung-Russell diagram, redshift and the Hubble constant for sub-topic 5.6 of Pearson Edexcel International A Level Physics (YPH11), Unit 5.
Physics · Pearson Edexcel · A LEVELS
-
Practice Questions
Edexcel IAL Physics: Astrophysics and Cosmology — Practice Questions
Original exam-style practice questions with full worked answers on luminosity, the HR diagram, stellar evolution and Hubble law for Edexcel IAL Physics.
Physics · Pearson Edexcel · A LEVELS
-
Revision Notes
Edexcel IAL Physics: Astrophysics and Cosmology — Revision Notes
Condensed recall notes on luminosity, Wien and Stefan laws, the HR diagram, stellar evolution and Hubble law for Edexcel International A Level Physics WPH15.
Physics · Pearson Edexcel · A LEVELS
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