Phase Transitions and Third Law Flashcards
Thermodynamic Potentials and States of Matter
-free energy seeks a minimum (most negative) at equilibrium
G = U - TS + PV
-fix P, change T and leave V free
-U is determined by the strength of intermolecular interactions (more negative means they are stronger)
-at low temperatures, U wins and you get solid
-at high temperatures, S wins and you get gases
Phase Diagrams
- summarises the conditions of temperature and pressure under which a substance exists in different phases e.g. solids/liquids/gases
- boundaries between the regions show values at pressure and temperature at which the two phases coexist in equilibrium
Triple Point
-temperature and pressure at which the solid, liquid and vapour phases coexist
Critical Temperature
- liquid/vapour boundary ends
- at temperatures greater than the critical temperature you cannot compress a vapour to form a gas
First Order Phase Transitions
- associated with a latent heat, L
- most common transitions are first order e.g. melting, boiling
- during a first order transitions, heat supplied to the system doesn’t increase temperature, but is absorbed in converting the substance from one phase to another
- this implies that there is a discontinuous change in the entropy and therefore a singularity (e.g. an infinite!) heat capacity at the transition
Entropy Change During Transition
Equation
ΔStrans = ΔHtrans/Ttrans = Ltrans/Ttrans
Entropy Change During Transition
Derivation
ΔStrans = ΔQtrans/Ttrans -generally changes such as melting/boiling occur at fixed pressure since: H = U + PV dH = dQ + dW + PdV + VdP dH = dQ - PdV + PdV +VdP dH = dQ + VdP -at constant pressure: dH = dQ -therefore: ΔQtrans = ΔHtrans = Ltrans -so change in entropy is given by: ΔStrans = ΔHtrans/Ttrans = Ltrans/Ttrans
Chemical Potential
Definition
-the chemical potential is the Gibb’s free energy per particle for a homogeneous one-component system
Chemical Potential
Derivation
-for phase transitions we need to generalise the thermodynamic potentials to include situations where N can change
-for phase transitions, its most common to work in terms of T and P as G is extensive
G(T,P,N) = N * g(T,P)
μ = g(T,P)
dG = -SdT + VdP = Ndg = dμ
Clapeyron Equation
Description
- describes the phase equilibrium curve
- describes how transition temperature changes with pressure
- derived by setting the chemical potential to be the same for both phases
Clapeyron Equation
Derivation
-consider an infinitesimal change in P and T that occurs in such a way that phases A and B remain in equilibrium dμa = dμb -for each phase separately: dGi = Nidgi = dμi = -SidT + VidP -setting dμ for each phase equal: -SadT + VadP = -SbdT + VbdP -rearrange for dP/dT (Vb - Va) dP = (Sb - Sa) dT dP/dT = (Sb - Sa) / (Vb - Va) dP / dT = ΔS / ΔV -and since ΔS = ΔQ/T = Lab/T = ΔHtrans/T -therefore: dP/dT = Lab/TΔV = ΔHtrans/TΔV
Clapeyron Equation
Equation
dP/dT = Lab/TΔV = ΔHtrans/TΔV
Clapeyron Equation
Solid-Liquid Boundary
dP/dT = ΔHfus / TΔVfus
-enthalpy of melting is almost always positive
-volume change is positive but small
=> the slope dP/dT is steep and usually positive
(water is an exception as it contracts on melting)
Solid to Liquid Transition - The Effect of Volume
- when a solid melts into a liquid, if there is an increase in volume (ΔV>0) then when pressure is increased (dP>0), melting temperature increases (dT>0)
- if there is a decease in molar volume on melting then increasing pressure (dP>0), then melting temperature will decrease (dT<0)
Clapeyron Equation
Liquid-Vapour Boundary
dP/dT = ΔHvap / TΔVvap
- enthalpy change on vaporisation is positive
- change in volume is always positive (and large) as gas volume > liquid volume
- dP/dT is always positive, but smaller than for the solid/liquid boundary since ΔV is greater