Thermodynamics

1.1 Kinetic Theory of Pressure & Temperature

  • Focus Question: What causes pressure?

  • Kinetic Theory: A gas is described as small particles in constant, random motion.

  • Closed System: A system that does not exchange matter with the environment.

  • Pressure: Force exerted on a surface per unit area.- Pressure = \frac{F}{A}

    • Units: Pascals (Pa), 1 Pa = 1 \frac{N}{m^2}

  • Gas pressure in a closed container results from gas molecules colliding with the container.

  • Force is the rate of change in momentum (p = mv).

  • For one molecule hitting a piston:- F = \frac{\Delta p}{t} = \frac{mv - m(-v)}{t} = \frac{2mv}{t}

    • The change in velocity magnitude is 2v, accounting for direction.

  • For N molecules hitting the piston per unit time t:- F = \frac{2Nmv}{t}

    • Pressure \ P = \frac{F}{A} = \frac{2Nmv}{At}

  • Pressure measures how often gas molecules collide with the container.

Temperature and Kinetic Energy

  • Temperature: Measure of the average kinetic energy of individual molecules.- Higher temperature means faster molecular motion.

    • Solids: Particles vibrate.

    • Liquids: Particles move across each other.

    • Gases: Particles move freely.

  • Temperature and average kinetic energy:- K{avg} = \frac{3}{2} kB T

    • k_B: Boltzmann’s constant = 1.38 \times 10^{-23} \frac{J}{K}

    • T: Temperature in Kelvin.

  • Molecules move at different speeds; K_{avg} is based on the average speed.

  • At 0 K, molecules stop moving.

  • Root Mean-Square Speed (v_{rms}):

    • K = \frac{1}{2} m v{rms}^2 = \frac{3}{2} kB T

    • v{rms} = \sqrt{\frac{3kB T}{m}}

    • m: mass of one molecule.

  • Maxwell-Boltzmann distribution describes the speeds of molecules in a gas.

  • v_{rms} is slightly to the right of the peak of the distribution graph.

Thermal Expansion

  • Most substances expand when heated.

  • Increased particle vibration leads to increased particle distance.

  • Linear Expansion:

    • \Delta L = L_0 \alpha \Delta T

    • L = L_0(1 + \alpha \Delta T)

    • \alpha: coefficient of linear expansion (units: 1/°C).

  • Railroad tracks have “expansion joints”.

  • Constructing a Temperature Scale:

    • Use a substance with known thermal expansion (e.g., mercury).

    • Measure length at a lower temperature (e.g., freezing point of water).

    • Measure length at a higher temperature (e.g., melting point of water).

    • Write a linear equation: Temperature = slope \times length

  • Area Expansion:

    • Thermal expansion of 2D or 3D objects occurs outward.

    • Holes in objects also expand.

1.2 Thermal Energy Transfer

  • Focus Question: Is something with a higher temperature necessarily "hot"?

  • At high temperatures, particles vibrate faster.

  • Energy transfers from faster to slower particles during collisions.

  • Heat: Transfer of thermal energy between objects in thermal contact due to a temperature difference.- Heat flows from high to low temperature.

    • Variable: Q, Units: Joules (J).

    • 4.186 J = 1 \text{ cal}

Zeroth Law of Thermodynamics

  • Thermal Contact: Thermal energy can be exchanged between objects.

  • Thermal Equilibrium: No net energy exchange occurs between objects in thermal contact.

  • Zeroth Law: If A and B are both in thermal equilibrium with C, then A and B are in equilibrium with each other.

1.3 Gas Laws

  • Focus Question: How do pressure, volume, and temperature affect each other?

Ideal Gas Model Assumptions

  • Composition: Large amount of particles travel in random direction at various speeds.

  • Distance of Particles: Particles are far apart compared to their size.

  • Attractive Force: Particles interact only in collisions (no attractive forces).

  • Collisions: Collisions of particles with container wall are perfectly elastic.

Gas Laws

  • Relate temperature, pressure, and volume of a confined ideal gas.

  • Explained by kinetic theory.

  • Pressure:

    • Matter consists of small particles in motion.

    • Particles collide with the walls of the container (perfectly elastically) and bounce off, changing their direction and thus momentum.

    • A force acting over a time is required to change momentum, and this force causes pressure:

    • F = \frac{\Delta p}{\Delta t}

    • Pressure is force over area.

    • In thermodynamics, pressure is the average rate of change of momentum of particles hitting the container per unit area.

    • Higher pressure means more and faster collisions.

  • Boyle’s Law: Volume of a gas is inversely proportional to pressure (constant temperature).- P1V1 = P2V2

  • Charles’ Law: Volume of a gas is directly proportional to absolute temperature (constant pressure).- \frac{V1}{T1} = \frac{V2}{T2}

  • 3rd Law: Pressure is directly proportional to absolute temperature (constant volume).- \frac{P1}{T1} = \frac{P2}{T2}

1.4 The First Law of Thermodynamics

  • Focus Question: How does conservation of energy apply to thermodynamics processes?

Total Internal Energy

  • Temperature measures average kinetic energy.

  • Total internal energy is the combined energy of all molecules in the system.

  • Average kinetic energy of a molecule: \frac{3}{2} kB T or \frac{3}{2} \frac{nR}{NA}T

  • Internal Energy = U = N(\frac{3}{2} k_B T)

  • U = (nNA) (\frac{3}{2} \frac{R}{NA} T) \rightarrow U = \frac{3}{2} nRT

  • For ideal gas, T = \frac{PV}{nR}, so U = \frac{3}{2} PV

Work Done in Thermodynamics Processes

  • Work Done in Thermodynamics Processes:- The initial pressure of the gas is P and the cross-sectional area of the piston is A, then the force with which one must push is PA.

    • If the piston is compressed some distance\Delta x, the work done is: W = F \Delta x \rightarrow W = PA(-\Delta x)

    • A \Delta x is volume, so W = -P \Delta V

    • Work is the area under a Pressure vs. volume graph

    • Work is only done when volume changes

The First Law of Thermodynamics

  • Conservation of energy in thermal physics.

  • Internal energy can be changed by doing work or adding heat.- \Delta U = Q + W

    • \Delta U - change in internal energy

    • Q - heat added to system

    • W – work done on the system

  • Sign conventions:- \Delta U > 0: Temperature increases.

    • \Delta U < 0: Temperature decreases.

    • Q > 0: Heat enters the system.

    • Q < 0: Heat leaves the system.

    • W > 0: Work is done on the system; system is compressed.

    • W < 0: Work is done by the system, system expands.

Types of Processes

  • Isobaric Process: Constant pressure, \Delta P = 0.

    • W = P \Delta V

    • Requires heat addition for expansion and heat removal for contraction to maintain constant pressure with temperature changes.

  • Isothermal Process: Constant temperature, \Delta U = 0.

    • 0 = Q + W \rightarrow Q = -W

    • Adding heat causes expansion, removing heat causes contraction.

  • Isochoric Process: Constant volume, W = 0.

    • \Delta U = -Q

    • Adding heat increases molecular speed (temperature), removing heat slows molecules down.

  • Adiabatic Process: No heat enters or leaves the system, Q = 0.

    • \Delta U = W

    • Typically fast processes.

    • Adiabatic compression increases temperature, adiabatic expansion decreases temperature.

1.5 The Second Law of Thermodynamics

  • Focus Question: What is entropy?

  • Entropy: Measure of disorder in a system.

  • Change in entropy: \Delta S = \frac{Q}{T} at constant temperature.

  • 2nd Law of Thermodynamics: Entropy of the universe increases in all natural processes.

  • Work can decrease entropy.

  • Disorderly arrangements are more probable.

  • Consequences:- Impossible for thermal energy to flow from cold to hot without work.

    • Impossible to completely convert heat into mechanical work in a cyclic process.

1.6 Specific Heat & Conductivity

  • Focus Question: What factors affect the rate of thermal energy transfer?

Transfer of Energy

  • Conduction: Heat transfer between objects in contact with a temperature difference.- Heat flows from hot to cold.

  • Conduction occurs if there is a temperature difference between two parts of a conducting medium. The rate of heat transfer (power) through a conductor can be given by:- Q/t: rate of heat transfer

    • \frac{Q}{t} = \frac{kA(TH - TC)}{L} - k – thermal conductivity, a constant that depends on the type of material

      • The rate of thermal energy transfer is quicker for shorter lengths and larger temperature differences.

      • Materials that are good thermal conductors have a higher value of 𝑘. Good thermal conductors allow heat to easily flow through them.

  • Convention: Heat transfer by movement by molecules in a fluid.- Convention occurs because a substance’s density decreases when temperature increases

    • As air gets hotter, it gets less dense and rises, colder air takes its place.

  • Radiation: Heat transfer by electromagnetic waves.- Radiation is the only form of heat transfer that can occur in a vacuum since electromagnetic waves can travel in a vacuum.

  • Phase Changes- As heat is added to a solid: - As heat is added, particles in the solid vibrate faster. Heat added increases the internal energy which causes temperature to increase.

    • At the melting point, temperature will remain constant despite added heat. Instead, added heat works to overcome the attractive force between