All Study Guides Physical Chemistry I Unit 1
🧤 Physical Chemistry I Unit 1 – Intro to Physical Chem & ThermodynamicsPhysical 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)
Process functions depend on the path taken to reach the final state (heat, work)
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 Δ U = Q + W \Delta U = Q + W Δ U = Q + W
Δ U \Delta U Δ U is the change in internal energy
Q Q Q is the heat added to the system
W W W is the work done on the system
Second Law states that the entropy of the universe always increases in a spontaneous process
Expressed as Δ S u n i v e r s e > 0 \Delta S_{universe} > 0 Δ S u ni v erse > 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 P V = n R T PV = nRT P V = n RT
P P P is the pressure
V V V is the volume
n n n is the number of moles
R R R is the ideal gas constant
T T T 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
Work done by a gas during expansion is expressed as W = − P Δ V W = -P\Delta V W = − P Δ 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 + P V H = U + PV H = U + P V
U U U is the internal energy
P P P is the pressure
V V V is the volume
Change in enthalpy is equal to the heat absorbed or released at constant pressure
Expressed as Δ H = Q p \Delta H = Q_p Δ H = Q p
Heat capacity at constant pressure (C p C_p C p ) is greater than heat capacity at constant volume (C v C_v C 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 = k ln W S = k \ln W S = k ln W
k k k is the Boltzmann constant
W W W 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 (Δ G \Delta G Δ G ) determines the spontaneity of a process at constant temperature and pressure
Δ G < 0 \Delta G < 0 Δ G < 0 indicates a spontaneous process
Δ G > 0 \Delta G > 0 Δ G > 0 indicates a non-spontaneous process
Δ G = 0 \Delta G = 0 Δ 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 = H − T S G = H - TS G = H − TS
H H H is the enthalpy
T T T is the absolute temperature
S S S is the entropy
Change in Gibbs free energy determines the spontaneity of a process
Expressed as Δ G = Δ H − T Δ S \Delta G = \Delta H - T\Delta S Δ G = Δ H − T Δ S
Chemical equilibrium is reached when the forward and reverse reactions occur at the same rate
Equilibrium constant (K K K ) is related to the standard Gibbs free energy change (Δ G ∘ \Delta G^\circ Δ G ∘ )
Expressed as Δ G ∘ = − R T ln K \Delta G^\circ = -RT \ln K Δ G ∘ = − 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