Chapter 11 · Introduction

Chapter 11 — Thermodynamics

Heat and work are two ways of moving energy into or out of a body. This chapter writes the energy account of a gas — the first law, $\Delta U=Q-W$ — follows a gas through its basic processes, and finds why no engine can turn all of its heat into work.

Pump up a bicycle tyre quickly and feel the barrel of the pump: it is warm, although nothing hot has touched it. Open a bottle of soda and a little cloud appears in the neck — the escaping gas has cooled itself below the dew point by pushing back the air. A pressure cooker whistles, a car engine burns fuel and drives the wheels, a refrigerator pumps heat out of a cold box into a warm kitchen. In every case energy is being moved about in two different ways: as heat, which flows because of a temperature difference, and as work, done when a force moves something — a piston, a pump handle, a turbine blade.

Thermodynamics is the bookkeeping of those two flows. You will start with the idea of thermal equilibrium and the zeroth law, which is what makes a thermometer meaningful. Then you will meet the energy stored inside a body, its internal energy, and the first law: heat in, minus work out, equals the increase of internal energy. Applied to an ideal gas, the first law explains why a gas needs more heat to warm it at constant pressure than at constant volume, and what happens to the pressure, volume and temperature in isothermal, adiabatic, isochoric and isobaric changes — all drawn on a $p$–$V$ diagram where work is an area. Finally the second law tells you what the first law cannot: which way heat flows on its own, why some processes can never be undone, and why even a perfect engine — the Carnot engine — must throw some heat away.

Thermal equilibrium→Zeroth law→$\Delta U=Q-W$→$C_p-C_v=R$→$W=$ area under $p$–$V$→$pV^\gamma=$ const→Second law→$\eta=1-\dfrac{T_2}{T_1}$
🎯 By the end of this chapter you can…
  • explain thermal equilibrium, state the zeroth law of thermodynamics and use it to explain why thermometers work;
  • distinguish heat, work and internal energy, and explain why internal energy is a property of the state while heat and work depend on the process;
  • state and apply the first law, $\Delta U=Q-W$, with the sign convention $W$ = work done by the system;
  • calculate the work done by a gas, $W=\int p\,dV$, as the area under a $p$–$V$ graph;
  • derive Mayer's relation $C_p-C_v=R$ for an ideal gas and use $\gamma=\dfrac{C_p}{C_v}$;
  • describe state variables and the equation of state, and analyse quasi-static isothermal, adiabatic ($pV^\gamma=$ const), isochoric, isobaric and cyclic processes;
  • state the second law in the Kelvin–Planck and Clausius forms, and tell reversible from irreversible processes;
  • describe the Carnot cycle and use $\eta=1-\dfrac{T_2}{T_1}$, with general heat engines, refrigerators and heat pumps as a JEE Advanced extension;
  • tackle Board, JEE Main, JEE Advanced and NEET-style problems on thermodynamics.
Teaser — Two Ways to Warm the Water

An insulated beaker holds $0.50\ \text{kg}$ of water ($c=4186\ \text{J kg}^{-1}\text{K}^{-1}$). A $20\ \text{kg}$ weight falling $2.0\ \text{m}$ turns a paddle wheel that churns the water; a burner underneath can also supply heat. Choose how many times the weight is dropped and how much heat the burner gives. Before you look: if the same total energy goes in, does it matter which route it takes?

100 J
work done on water $W_\text{on}$—
heat supplied $Q$—
gain in internal energy—
temperature rise $\Delta T$—

Sections in this chapter

✅ Before you start
You will need work done by a force and the work–energy theorem (Section 5.1), and the idea of conservation of energy (Section 5.2); the area under a graph as an integral (Section 2.2); and pressure as force per unit area (Section 9.1). From Class 11 Physics, Chapter 10 — Thermal Properties of Matter you need temperature on the kelvin scale, the ideal-gas equation $pV=nRT$ with $R=8.31\ \text{J mol}^{-1}\text{K}^{-1}$, and specific and molar specific heat capacity, $Q=mc\,\Delta T=nC\,\Delta T$. The molecular picture of internal energy (why $C_v=\tfrac32R$ for a monatomic gas) comes in Chapter 12 — Kinetic Theory; here those values are simply quoted. From mathematics you need logarithms and powers ($\ln$, $V^{\gamma}$) and significant figures (Section 1.2).