🧤Physical Chemistry I Unit 1 – Intro to Physical Chem & Thermodynamics

Physical Chemistry I introduces fundamental thermodynamic concepts, exploring energy, heat, and work in chemical systems. This unit covers the laws of thermodynamics, states of matter, and equations of state, providing a foundation for understanding molecular behavior and energy transformations. The course delves into enthalpy, entropy, and free energy, connecting these concepts to chemical equilibrium and spontaneity. Students learn to apply thermodynamic principles to real-world systems, from heat engines to biological processes, bridging theory with practical applications.

Key Concepts and Definitions

  • Thermodynamics studies the relationships between heat, work, and energy in a system
  • System refers to the specific part of the universe under study (can be open, closed, or isolated)
  • Surroundings include everything outside the system
  • State functions depend only on the current state of the system (pressure, temperature, volume)
    • Path independent
  • Process functions depend on the path taken to reach the final state (heat, work)
    • Path dependent
  • Extensive properties depend on the amount of matter in the system (volume, mass)
  • Intensive properties are independent of the amount of matter (density, temperature)

Fundamental Laws of Thermodynamics

  • Zeroth Law states that if two systems are in thermal equilibrium with a third system, they are in thermal equilibrium with each other
    • Allows for the definition of temperature
  • First Law states that energy cannot be created or destroyed, only converted from one form to another
    • Expressed as ΔU=Q+W\Delta U = Q + W
      • ΔU\Delta U is the change in internal energy
      • QQ is the heat added to the system
      • WW is the work done on the system
  • Second Law states that the entropy of the universe always increases in a spontaneous process
    • Expressed as ΔSuniverse>0\Delta S_{universe} > 0
  • Third Law states that the entropy of a perfect crystal at absolute zero is zero
    • Provides a reference point for entropy calculations

States of Matter and Phase Transitions

  • Matter exists in three main states solid, liquid, and gas
    • Plasma is sometimes considered a fourth state
  • Solid has a fixed shape and volume due to strong intermolecular forces
  • Liquid has a fixed volume but takes the shape of its container due to moderate intermolecular forces
  • Gas has no fixed shape or volume due to weak intermolecular forces
  • Phase transitions occur when a substance changes from one state to another
    • Melting solid to liquid
    • Vaporization liquid to gas
    • Sublimation solid to gas
    • Condensation gas to liquid
    • Freezing liquid to solid
    • Deposition gas to solid

Equations of State and Ideal Gas Law

  • Equation of state relates the state variables (pressure, volume, temperature) of a system
  • Ideal Gas Law is a specific equation of state for ideal gases
    • Expressed as PV=nRTPV = nRT
      • PP is the pressure
      • VV is the volume
      • nn is the number of moles
      • RR is the ideal gas constant
      • TT is the absolute temperature
  • Real gases deviate from ideal behavior at high pressures and low temperatures
    • Van der Waals equation accounts for these deviations
  • Dalton's Law states that the total pressure of a mixture of ideal gases is the sum of the partial pressures of each gas

Energy, Heat, and Work

  • Energy is the capacity to do work or transfer heat
    • Kinetic energy is associated with motion
    • Potential energy is associated with position or configuration
  • Heat is the transfer of energy due to a temperature difference
    • Measured in joules (J) or calories (cal)
  • Work is the transfer of energy due to a force acting over a distance
    • Measured in joules (J)
  • Work done by a gas during expansion is expressed as W=PΔVW = -P\Delta V
    • Negative sign indicates work is done by the system
  • Heat capacity is the amount of heat required to raise the temperature of a substance by one degree
    • Specific heat capacity is the heat capacity per unit mass

Enthalpy and Heat Capacity

  • Enthalpy is a state function that represents the total heat content of a system
    • Expressed as H=U+PVH = U + PV
      • UU is the internal energy
      • PP is the pressure
      • VV is the volume
  • Change in enthalpy is equal to the heat absorbed or released at constant pressure
    • Expressed as ΔH=Qp\Delta H = Q_p
  • Heat capacity at constant pressure (CpC_p) is greater than heat capacity at constant volume (CvC_v)
    • Difference is due to the work done during expansion
  • Hess's Law states that the enthalpy change of a reaction is independent of the pathway
    • Allows for the calculation of enthalpy changes using standard enthalpies of formation

Entropy and Spontaneity

  • Entropy is a measure of the disorder or randomness of a system
    • Expressed as S=klnWS = k \ln W
      • kk is the Boltzmann constant
      • WW is the number of microstates
  • Second Law of Thermodynamics states that the entropy of the universe always increases in a spontaneous process
  • Spontaneous processes occur without external intervention
    • Gibbs free energy (ΔG\Delta G) determines the spontaneity of a process at constant temperature and pressure
      • ΔG<0\Delta G < 0 indicates a spontaneous process
      • ΔG>0\Delta G > 0 indicates a non-spontaneous process
      • ΔG=0\Delta G = 0 indicates a system at equilibrium
  • Entropy of mixing always increases when two substances are combined

Free Energy and Chemical Equilibrium

  • Gibbs free energy is a state function that combines enthalpy and entropy
    • Expressed as G=HTSG = H - TS
      • HH is the enthalpy
      • TT is the absolute temperature
      • SS is the entropy
  • Change in Gibbs free energy determines the spontaneity of a process
    • Expressed as ΔG=ΔHTΔS\Delta G = \Delta H - T\Delta S
  • Chemical equilibrium is reached when the forward and reverse reactions occur at the same rate
    • Equilibrium constant (KK) is related to the standard Gibbs free energy change (ΔG\Delta G^\circ)
      • Expressed as ΔG=RTlnK\Delta G^\circ = -RT \ln K
  • Le Chatelier's Principle states that a system at equilibrium will shift to counteract any external stress
    • Changes in concentration, pressure, volume, or temperature can shift the equilibrium position

Applications in Real-World Systems

  • Thermodynamics plays a crucial role in understanding and optimizing real-world systems
  • Heat engines convert heat into mechanical work (internal combustion engines, steam turbines)
    • Efficiency is limited by the Second Law of Thermodynamics
  • Refrigerators and heat pumps transfer heat from a cold reservoir to a hot reservoir
    • Coefficient of performance (COP) measures the efficiency
  • Phase diagrams show the conditions at which different phases of a substance are stable
    • Used in materials science and engineering (alloys, ceramics)
  • Gibbs free energy is used to predict the feasibility of chemical reactions
    • Important in chemical synthesis and industrial processes (Haber-Bosch process for ammonia production)
  • Biological systems rely on thermodynamic principles (energy transduction in cells, protein folding)
  • Environmental science uses thermodynamics to study climate change and global energy balance


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© 2024 Fiveable Inc. All rights reserved.
AP® and SAT® are trademarks registered by the College Board, which is not affiliated with, and does not endorse this website.