All Study Guides Thermodynamics Unit 18
🥵 Thermodynamics Unit 18 – Thermodynamics in Materials ScienceThermodynamics in materials science explores how energy and matter interact, shaping the behavior of materials. It covers key concepts like the laws of thermodynamics, energy transfer, and phase equilibria, which are crucial for understanding material properties and processes.
This field helps engineers and scientists design better materials, optimize manufacturing processes, and predict material behavior in various conditions. From selecting the right alloy for an engine to developing efficient energy storage systems, thermodynamics plays a vital role in materials science applications.
Got a Unit Test this week? we crunched the numbers and here's the most likely topics on your next test Key Concepts and Definitions
Thermodynamics studies the relationships between heat, work, energy, and matter
System refers to the specific material or region under study (metal alloy)
Surroundings include everything outside the system that can interact with it (furnace)
State variables describe the current condition of a system (temperature, pressure, volume)
Intensive variables are independent of the system size (density)
Extensive variables depend on the size of the system (mass, volume)
Equilibrium occurs when a system's state variables remain constant over time
Thermal equilibrium exists when the system and surroundings have the same temperature
Mechanical equilibrium exists when the system and surroundings have the same pressure
Process describes the path a system takes from one state to another (heating, cooling)
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
First Law states that energy cannot be created or destroyed, only converted from one form to another
Mathematically expressed as Δ U = Q − W \Delta U = Q - W Δ U = Q − W , where Δ U \Delta U Δ U is the change in internal energy, Q Q Q is heat added, and W W W is work done by the system
Second Law states that the total entropy of an isolated system always increases over time
Entropy is a measure of the disorder or randomness of a system
Spontaneous processes occur naturally and increase the entropy of the universe
Third Law states that the entropy of a perfect crystal at absolute zero is zero
Absolute zero (0 K or -273.15°C) is the lowest possible temperature
Unattainable in practice due to the infinite steps required to reach it
Energy and Enthalpy
Internal energy (U U U ) is the sum of the kinetic and potential energies of a system's particles
Depends on the system's temperature, volume, and composition
Heat (Q Q Q ) is the transfer of thermal energy between a system and its surroundings
Positive when heat is added to the system, negative when heat is removed
Work (W W W ) is the energy transfer due to a force acting over a distance
Positive when work is done by the system, negative when work is done on the system
Enthalpy (H H H ) is the sum of a system's internal energy and the product of its pressure and volume
Mathematically expressed as H = U + P V H = U + PV H = U + P V
Useful for processes occurring at constant pressure (most chemical reactions)
Specific heat capacity (c c c ) is the amount of heat required to raise the temperature of one unit mass of a substance by one degree
Varies with temperature and pressure
Higher values indicate a greater ability to store thermal energy (water vs. metal)
Entropy and Free Energy
Entropy (S S S ) is a measure of the disorder or randomness of a system
Increases with increasing temperature, volume, or number of particles
Mathematically expressed as Δ S = ∫ d Q T \Delta S = \int \frac{dQ}{T} Δ S = ∫ T d Q , where d Q dQ d Q is the heat added reversibly and T T T is the absolute temperature
Gibbs free energy (G G G ) is the maximum amount of non-expansion work that can be extracted from a system
Mathematically expressed as G = H − T S G = H - TS G = H − TS , where H H H is enthalpy, T T T is absolute temperature, and S S S is entropy
Spontaneous processes have a negative change in Gibbs free energy (Δ G < 0 \Delta G < 0 Δ G < 0 )
Helmholtz free energy (A A A ) is similar to Gibbs free energy but applies to processes at constant volume
Mathematically expressed as A = U − T S A = U - TS A = U − TS , where U U U is internal energy, T T T is absolute temperature, and S S S is entropy
Maxwell relations are a set of equations that relate the partial derivatives of thermodynamic potentials (U U U , H H H , A A A , G G G )
Useful for deriving other thermodynamic properties and equations
Phase Equilibria and Diagrams
Phase refers to a physically distinct and homogeneous portion of a system (solid, liquid, gas)
Phase transition occurs when a substance changes from one phase to another (melting, boiling)
Accompanied by changes in properties such as density, enthalpy, and entropy
Phase diagram is a graphical representation of the conditions at which different phases are stable
Pressure-temperature (P P P -T T T ) diagrams are common for single-component systems (water)
Temperature-composition (T T T -x x x ) diagrams are used for binary systems (alloys)
Gibbs phase rule relates the number of components (C C C ), phases (P P P ), and degrees of freedom (F F F ) in a system
Mathematically expressed as F = C − P + 2 F = C - P + 2 F = C − P + 2
Degrees of freedom are the number of independent variables that can be changed without altering the number of phases
Lever rule is used to determine the relative amounts of phases present in a two-phase region of a phase diagram
Based on the distances between the overall composition and the phase boundaries
Thermodynamic Properties of Materials
Molar volume (V m V_m V m ) is the volume occupied by one mole of a substance
Varies with temperature and pressure
Used to calculate density and other properties
Thermal expansion coefficient (α \alpha α ) is the fractional change in length or volume per unit change in temperature
Positive for most materials, indicating expansion upon heating
Important for designing components that experience temperature changes (bridges, engines)
Compressibility (β \beta β ) is the fractional change in volume per unit change in pressure
Inverse of the bulk modulus, which measures a material's resistance to compression
Higher values indicate a more easily compressed material (gases vs. solids)
Thermal conductivity (k k k ) is the rate at which heat is conducted through a material
Varies with temperature, density, and composition
Higher values indicate a better ability to transfer heat (metals vs. insulators)
Electrical conductivity (σ \sigma σ ) is the ability of a material to conduct electric current
Depends on the number of free electrons and their mobility
Metals have high electrical conductivity due to their delocalized electrons
Applications in Materials Science
Materials selection involves choosing the best material for a given application based on its properties and performance requirements
Ashby charts plot material properties (strength vs. density) to aid in selection
Processing techniques are used to control the structure and properties of materials
Heat treatment can alter the microstructure and mechanical properties of alloys (annealing, quenching)
Sintering consolidates powdered materials into solid components (ceramics, metals)
Corrosion is the degradation of a material due to chemical reactions with its environment
Thermodynamics can predict the stability of materials in different environments (Pourbaix diagrams)
Corrosion prevention methods include coatings, cathodic protection, and alloying
Energy materials convert between different forms of energy (solar cells, batteries)
Efficiency is limited by thermodynamic factors such as the Carnot efficiency and the Shockley-Queisser limit
Materials design can optimize properties such as band gap, conductivity, and stability
Problem-Solving Techniques
Identify the system and surroundings, specifying the boundary and any transfers of energy or matter
Determine the initial and final states of the system, noting any changes in temperature, pressure, volume, or composition
Apply the relevant laws and equations of thermodynamics, such as the First Law (Δ U = Q − W \Delta U = Q - W Δ U = Q − W ) or the Gibbs free energy equation (Δ G = Δ H − T Δ S \Delta G = \Delta H - T\Delta S Δ G = Δ H − T Δ S )
Use appropriate sign conventions for heat (Q Q Q ) and work (W W W )
Consider any assumptions or approximations, such as constant pressure or reversibility
Solve for the desired quantity, checking units and reasonableness of the answer
Use tabulated data for properties such as enthalpy of formation, entropy, or heat capacity
Interpolate or extrapolate data if necessary, using appropriate techniques (linear interpolation)
Interpret the results in the context of the problem, discussing any implications or limitations
Relate the answer to the problem statement and any real-world applications
Consider sources of error or uncertainty, such as measurement limitations or approximations