Overview of Thermodynamics Principles

Oct 7, 2024

Thermodynamics Lecture Notes

Introduction to Thermodynamics

  • Definition: Study of heat flow (thermo = heat, dynamics = motion of heat)
  • Developed in the 1800s during the Industrial Revolution.
  • Associated with the use of fossil fuels and the beginning of climate change awareness (first calculations on CO2 impact by Arrhenius).

Historical Context

  • Arrhenius (late 1800s) calculated the impact of CO2 on climate, predicting trouble for humanity in 2000 years due to emissions.
  • Exponential growth in CO2 since then has accelerated the timeline for climate issues.

Universal Application of Thermodynamics

  • Thermodynamics applies to various systems:
    • Biological (energy from food)
    • Mechanical (cars, boats)
    • Astrophysical (stars, black holes)
    • Economic systems (non-equilibrium thermodynamics)
  • Initially, it was based on macroscopic properties, now also incorporates microscopic (atomic/molecular) properties.

Laws of Thermodynamics

  1. Zeroth Law: Defines temperature.
    • Common-sense law: Heat flows from hot to cold.
  2. First Law: Defines energy conservation (U).
    • "You can break even" law: Energy cannot be created or destroyed; it can only be transformed.
  3. Second Law: Defines entropy.
    • Direction of time; entropy increases over time.
    • "You can break even at absolute zero" law: Perfect efficiency possible only at 0 K.
  4. Third Law: Numerical value of entropy.
    • "You can't get to zero degrees" law: Absolute zero is unattainable.

Importance of Definitions

  • Understanding definitions is crucial for solving thermodynamic problems:
    • System: Part of the universe being studied.
    • Surroundings: Everything outside the system.
    • Boundary: Division between system and surroundings (can be real or imaginary).

Types of Systems

  • Open System: Mass and energy can flow across the boundary.
  • Closed System: Energy can flow, but mass cannot.
  • Isolated System: Neither mass nor energy can flow.

Describing the System

  • Essential macroscopic properties:
    • Pressure, temperature, volume, number of moles, mass.
  • Homogeneous vs Heterogeneous systems:
    • Homogeneous: Uniform composition (e.g., milk coffee).
    • Heterogeneous: Different phases (e.g., ice water).
  • Equilibrium systems: Properties do not change over time or space.
  • State Variables: Describe equilibrium states (independent of how the state was reached).

Properties of Systems

  • Extensive Properties: Depend on the size of the system (e.g., mass, volume).
  • Intensive Properties: Independent of system size (e.g., temperature).
  • Can derive intensive properties from extensive ones (e.g., molar volume).

Transition Between States

  • Describes how to go from one equilibrium state to another using paths.
    • Reversible Path: System remains in equilibrium throughout the process.
    • Irreversible Path: System does not remain in equilibrium; requires energy to return to initial state.

Path Definition and Importance

  • Paths can be described using terms such as:
    • Adiabatic: No heat transfer.
    • Isobaric: Constant pressure.
    • Isothermal: Constant temperature.

Zeroth Law of Thermodynamics

  • Definition: If two systems are in thermal equilibrium with a third system, then they are in thermal equilibrium with each other.
  • Basis for defining temperature and thermometers.

Thermometer Basics

  • Must have a substance that changes properties based on temperature (e.g., volume, resistivity).
  • Need reference points for temperature scales (e.g., freezing and boiling points of water).
  • Overview of historical temperature scales (Celsius, Fahrenheit).

Conclusion

  • Next session will cover the ideal gas thermometer and the Kelvin scale.