Ch.17 Flashcards
The Second Law of Thermodynamics - Entropy
The second law of thermodynamics tells us that spontaneous processes are those that raise the “entropy” of the universe.
• for any spontaneous process, the entropy of the universe increases (∆Suniv >0)
• Entropy is a state function so we normally concern ourselves with the change in entropy, ∆S = Sfinal- Sinitial
∆Suniv = ∆Ssys + ∆Ssurr > 0
• Processes which have ∆Ssys < 0 are not impossible, but must be coupled to some other process for which ∆S > 0 so that ∆Suniverse > 0
• Processes which have ∆Ssys > 0 may be non-spontaneous if they are coupled to other processes for which ∆S < 0 so that ∆Suniverse < 0
Entropy
• Entropy is often (over)simplified as a quantitative measure of “disorder”
• More correctly, entropy measures how dispersed the energy of the universe or a part of the universe is
• In other words, a state that requires a very specific arrangement of atoms (concentrated energy) is low entropy, while a state that allows for considerable variation (dispersed energy) is high entropy
• Entropy depends on how many different microstates can produce identical macrostates
Macro vs. Microstates
• Macrostate - describes the properties of the bulk system
– measurement parameters include things like pressure and temperature
— The container of gas has a specific volume, temperature and pressure
• Microstate - describes the properties of the individual molecules that make up the bulk system
– For example, the identity, orientation and velocity of every molecule in a sample of matter.
—At any given moment the gas molecules each have a velocity; va,vb,vc…
— Many combinations of velocities can satisfy the observed macrostate
Macro vs. Microstates – Phase Changes
- A sample of gas can have many different combinations of molecule positions and velocities that correspond to a given temperature, pressure and volume
- Condensing that gas into a liquid requires (nearly) all of the gas molecules to occupy a small portion of the container, giving fewer arrangements that correspond to the observed state functions
- Crystallizing the liquid into a solid further restricts the number of positions and orientations of molecules (microstates) that are consistent with the macrostate.
- The solid thus has a lower entropy than the liquid, and the liquid has a lower entropy than the gas.
Microstates & Entropy
• The more microstates that can describe a system, the higher the entropy of the system
• Opening the valve between the flasks of gas equalizes the pressure, because there are more ways of arranging the gas molecules across both flasks
Quantifying Entropy
• The Boltzmann equation describes the entropy of a system based on the number of microstates
S = k ln W
k = Boltzmann constant, R/NA
units are JK-1
W = # microstates
• The entropy of a state increases with the number of energetically equivalent ways to arrange the components of the system
• The state with the highest entropy also has the greatest dispersal of energy
• A state in which a given amount of energy is more highly dispersed has more entropy that a state in which the same energy is more highly concentrated.
• This allows us to define a state of zero entropy, when there is only one possible microstate
• A perfect crystal allows no deviations in the positions of the atoms or molecules, and zero temperature means none of the particles are moving.
Processes with ∆S > 0
• Melting, vapourization, sublimation
– Or reactions that turn solid starting materials into gaseous products
• Increase in temperature at a constant V
• Increase in the volume of a gas at constant P
• Increase in the number of moles of gas in a reaction
– Or any other process that increases the number of particles
Heat Transfer and Changes in Entropy
• Changes in enthalpy provide a means by which chemical reactions can be coupled to the rest of the universe
• Consider a process where entropy decreases, such as freezing of water
• We know that ∆Suniv must not decrease, so we must consider the entropy change of the system and
surroundings, ∆Ssys and ∆Ssurr
• ∆Suniv = ∆Ssys + ∆Ssurr
• Transfer of heat from a warmer place (the water) to a cooler place (the portion of the universe surrounding the water) results in an increase in entropy, which offsets the decrease in entropy resulting from the phase change
• Generally, exothermic processes increase Ssurroundings, while endothermic processes decrease Ssurroundings
– Hotter conditions = more possible combinations of individual molecular velocities (more microstates)
Temperature Dependence of ∆Ssurr
• The dispersal of energy to the surroundings and ∆Ssurr is temperature dependent
– The greater the temperature, the smaller the increase in entropy for a given amount of energy dispersed to the surroundings
– Adding heat to something very cold results in a larger increase in entropy than adding the same amount of heat to something warmer
Entropy is a measure of energy dispersal (joules) per unit temperature (kelvin)
Units: J/K
Quantifying ∆Ssurroundings
• A process that emits heat into the surroundings (qsys negative), increases the entropy of the surroundings (positive ∆Ssurr), exothermic reactions
• A process that absorbs heat from the surroundings (qsys postitive), decreases the entropy of the surroundings (negative ∆Ssurr), endothermic reactions
• The magnitude of the change in entropy of the surroundings is proportional to the magnitude of qsys and inversely proportional to temperature
∆Ssurr = qsurr/T = -qsys/T
• For a process occurring at constant temperature and pressure, the entropy change of the surroundings is equal to the energy dispersed into the surroundings (-∆Hsys) divided by the temperature of the surroundings in kelvin
∆Ssurr = -∆Hsys/T
• Note that this is not accounting for any work done on or by the system
Entropy of Phase Transitions
Consider a system that consists of a mixture of solid and liquid, or liquid and gas, that is at the phase change temperature and pressure
– The system is at equilibrium under these conditions
– At equilibrium, ∆Suniverse = 0, as the process is freely reversible
• A change to the lower entropy phase is exothermic
• A change to the higher entropy phase is endothermic
- For ∆Suniverse = 0, ∆Ssystem = - ∆Ssurroundings
• ∆Ssurr= -∆Hsys/T, and ∆Ssys = - ∆Ssurr,
• So ∆Sfusion = ∆Hfusion/Tm.p. and ∆Svaporization = ∆Hvaporization/Tb.p.
Calculating ∆S°rxn
• We’ve already seen the standard states for ∆H°
• Gas : 1 bar
• Liquid or Solid : pure substance at 1 bar and 25°C
• Substance in solution : concentration of 1 mol/L
• Standard entropy change for a reaction (∆S°rxn) is the change in entropy for a process in which all of the reactants and products are in their standard states
• We can use standard molar entropies (S°) to calculate ∆S°rxn
• ∆S°rxn = ∑nS°(products) - ∑nS°(reactants)
Standard Molar Entropies, S°
• There is a relative zero enthalpy, which was the standard enthalpy of formation for an element in its standard state
• There is no absolute zero for enthalpy
• Entropy has an absolute zero, so standard entropies for elements in their standard state is not zero
– Entropy can only be zero at 0K
• Standard molar entropies have the units JK-1mol-1
• Note that entropy (like enthalpy) is an extensive property and depends on the amount of the substance
Third Law of Thermodynamics
— The entropy of a perfect crystal at absolute zero (0K) is zero
• A perfect crystal at absolute zero has only 1 microstate (W=1), so the ln(W) term in the Boltzmann equation is zero and the entropy (S) is zero
S=k ln(W)
Entropy – Structure Relationships
Gaseous states of compounds have higher entropies than liquid or solid
• Entropy increases with increasing molar mass of elements in the same state
• Allotropes - materials with two or more forms (ie. graphite and diamond) can have different entropy values
• In a given state entropy usually increases with increasing molecular complexity
– N2(g) has more entropy than Ar(g) even though Ar(g) has a higher molecular mass
Gibbs Free Energy
• We have seen that ∆Ssurr = -∆Hsys/T
• We have also seen that ∆Suniv = ∆Ssys + ∆Ssurr
• Thus, ∆Suniv is related to both ∆Ssys and ∆Hsys
∆Suniv = ∆Ssys + ∆Ssurr
∆Suniv = ∆Ssys - ∆Hsys/T
-T∆Suniv = -T∆Ssys + T∆Hsys/T (multiply by -T)
-T∆Suniv = ∆H - T∆S (rearrange)
∆G = ∆H - T∆S (Gibbs energy)
∆G = -T∆Suniv
• If ∆G is negative then ∆Suniv is positive and the reaction is spontaneous