Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force...

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Thermodynamics Free E and Phase D J.D. Price

Transcript of Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force...

Page 1: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

ThermodynamicsFree E and Phase D

J.D. Price

Page 2: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

•Force - the acceleration of matter (N, kg m/sForce - the acceleration of matter (N, kg m/s22))

•Pressure (Pressure (PP) - a force applied over an area ) - a force applied over an area (N/m(N/m22))

•Work (W) - force multiplied by distance (kg Work (W) - force multiplied by distance (kg mm22/s/s22, Joule), Joule)

•Energy - enables work (J)Energy - enables work (J)

•Temperature (Temperature (TT) - a measurement relating to the ) - a measurement relating to the kinetic (movement) energy of the system (units kinetic (movement) energy of the system (units ºC or K)ºC or K)

•Heat (Q) - an energy form relatable to Heat (Q) - an energy form relatable to temperature (J, but also calories: 1 g water 1 K,)temperature (J, but also calories: 1 g water 1 K,)

Page 3: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

E.B. Watson

Page 4: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

step 1: heat ice (-20oC - 0oC)Q1 = (100g)(0.50 cal/goC)(20oC) = 1.0 kcal

step 2: melt ice at 0oCQ2 = (100g)(80 cal/g) = 8.0 kcal

step 3: heat water (0oC - 100oC)Q3 = (100g)(1.0 cal/goC)(100oC) = 10.0 kcal

step 4: boil water at 100oCQ4 = (100g)(540 cal/g) = 54.0 kcal

step 5: heat vapor to 120oCQ5 = (100g)(0.48 cal/goC)(20oC) = 0.96 kcal

Example calculation: How much energy is required to heat 100 g of ice at -20oC to water vapor at 120oC.

Page 5: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

The difference between Q and W is always the same.

It is the difference in internal energy (U) between the 2 states. So

U2 - U1 = Q - Wor

U = Q - WE.B. Watson

Page 6: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Ideally, in a heat engine, if heat is put into the system to move from state 1 to state 2 and the engine then returns to state 1, the change in internal energy of the system is zero, so

Qin = Wout

E.B. Watson

E.B. Watson

Page 7: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

The First LawThe First Law

Energy may be converted from one form to another, but Energy may be converted from one form to another, but the total amount of energy is the same. the total amount of energy is the same.

U = -Utherm - Umech

Isolated systemQ - heat gained by the systemW - work done on the system

U = Q - W

Thermodynamics – relating heat, work, and energy

Page 8: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

An expression of work can be made using P and V (the steam engine).

Thermal energy (H)

H = U + PV

Page 9: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Q - system heat transfer Q = Cp (T2 - T1)Where Cp is heat capacity

W - work done on the system W = P (V2 - V1)

H - Enthalpy, a variable that covers internal energy and the work term U + PV

U = U2 - U1 = Q - WU2 - U1 = Q - P (V2 - V1)U2 - U1 + P (V2 - V1) = QU2 - U1 + PV2 - PV1 = Q

(U2 + PV2 ) - ( U1 + PV1 ) = Q

(H2 - H1) = Cp (T2 - T1)

Page 10: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

dH = dU + PdV +VdP

if P is constant

dH = dU + PdV

Page 11: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Reactions

A change in phase(s)

Phases A and B react to make phase C

A + B = C

Reversibility - a slight change causes the reaction to proceed, and the opposite change reverses it.

Page 12: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

P is constant

Reaction: A + B = C + D

HA = UA + PVA

HB = UB + PVB

HPr = UPr +PVPr

HRe = URe +PVRe

Page 13: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Products - Reactants

HPr - HRe = H = U +PV

H is the latent heat

Positive is exothermic

Negative is endothermic

What of H2Osolid = H2Oliquid?

Page 14: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.
Page 15: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

U = 0 = Q – W

Okay, but could you go backwards?

E.B. Watson

Page 16: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

The Second LawThe Second Law

Heat flows from warmer to cooler bodies. To go Heat flows from warmer to cooler bodies. To go backwards requires energy or work.backwards requires energy or work.

The second law is also stated: Mechanical Mechanical energy can be converted 100% into heat, but energy can be converted 100% into heat, but heat cannot be converted 100% into mechanical heat cannot be converted 100% into mechanical energy.energy.

"You can't break even.""You can't break even."

Thermodynamics – relating heat, work, and energy

Page 17: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Heat cannot be converted 100% into Heat cannot be converted 100% into mechanical energymechanical energy

Some of the heat is lost, because it creates disorder in the system.

Entropy

Thermodynamics – relating heat, work, and energy

SU = dQ / T (rev) = 0

Page 18: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Entropy - the possible ways to combine the properties of individual particles to produce the observable properties of the whole system.

Solids - low S, Liquids - higher S

S = dq/T (rev)

U = TS - PV or dU = TdS - PdV

Page 19: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Plausible conclusion: the total entropy of the entire universe is continually increasing.

The "heat death of the universe." At some point, the universe may run out of heat.

E.B. Watson

Page 20: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

The Third Law

The entropy of a perfect crystal at 0 K is zero.

The "Zeroth" Law

Two systems in thermal equilibrium with the same third system are in thermal equilibrium with each another.

Thermodynamics – relating heat, work, and energy

Page 21: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Total Energy = bound energy + free energy

Gibbs Free Energy (G)

G = H - TS -or-

G = U + PV -TS

dG = dU +PdV + VdP - TdS - SdT

Page 22: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

G = H - TS

Provided all terms are at the same conditions!

Since the earth includes a wide range of T and P (easily measured), and H, S, and V are often difficult to measure, we would like to calculate G at different P and T using steps of H, S, and V.

G = Hfo - TSo + PVo

Page 23: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Isothermal and Isobaric

dG = dU +PdV - TdS

dG = 0 if reversible

dU = TdS - PdV

dG < 0 if irreversible

dU < TdS - PdV

Page 24: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

CaCO3Al2SiO5

Page 25: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Some substituting

Reversible

dG = dU+PdV + VdP - TdS - SdT

dU = TdS - PdV

dGRe = VRedP - SRedT and dGPr = VPrdP - SPrdT

dGRe - dGPr = VRedP - SRedT - VPrdP + SPrdT

dG = VdP - SdT

ddG = G = VVddP P - - SSddTT

Page 26: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

dG = VdP - SdT

At equilibrium, dG = 0

dP/dT = S/ V = H/ (TV)

Clausius-Clapeyron equation - the slope of a reaction boundary in P-T

space!!!

Page 27: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

BombReaction VesselCalorimeter

BombReaction VesselCalorimeter

The vessel is strong such that there is constant P

With a known heat capacity (Cp) for all of the calorimeter parts, we can determine the energy of reaction.

Erxn = -Cp x T Univ. of Maine

Page 28: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Graphite - Diamond298 K Ho

( /Kcal )mole

So ( /cal

)mole K

Go ( /Kcal

)mole

Vo (cm3/

)mole Graphite 0 1.372 0 5.2982

Diamond 0.453 0.568 0.693 3.4166

Reaction is Cgraphite= Cdiamond

Hfo

di Hfo

gr = 453 - 0 = 453 (cal/mole)

S = Sodi - So

gr = 0.568 - 1.372 = -0.804 (cal/mole K)

V = Vodi - Vo

gr = 3.4166 - 5.2982 = -1.881 (cm3/mole)

-1.881 / 41.8 = -0.0450 (cal/mole)

41.8 bar cm3 = 1 calorie

Page 29: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Graphite becomes diamond, G = 0

G = 0 = Ho -TSo + PVo

G = 0 = 453 (cal/mole) - -0.804 (cal/mole K) T - -0.045 (cal/mole bar) P

P = (Ho -TSo) / -Vo

P = (453 (cal/mole) + -0.804 (cal/mole K) T ) / 0.045 (cal/mole bar)

T = 298.15 K {note: this is 25oC}

P = (453 - -0.804(298))/ 0.045 = 15,389 bars

Page 30: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

dP/dT = S/ V

-0.804 cal/mole K

-1.881 cm3/mole X 41.8 bar cm3/cal

= 17.9 bar/K

{Line: y = mx + b} P = 17.9 T + b

15,389 bars - 17.9 (298.15 K) = b

b = 1.006 kb

Page 31: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Which phase is stable at 1 bar and 25 oC?

G = Hfo -TSo + PVo

Ggr = 0 - 298.15 K x (1.372 (cal/mole K) ) + 1 bar (5.2982 / 41.8) (cal/mole bar)

= -408.9 (cal/mole)

Gdi = 453 (cal/mole) - 298.15 K x (0.568 (cal/mole) ) + 1 bar (3.4166 / 41.8) (cal/mole bar)

= 283.7 (cal/mole)

Page 32: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Which phase is stable at 20 kbar and 25 oC?

G = Hfo -TSo + PVo

Ggr = 0 - 298.15 K x (1.372 (cal/mole K) ) + 20000 bar (5.2982 / 41.8) (cal/mole bar)

= 2126.0 (cal/mole)

Gdi = 453 (cal/mole) - 298.15 K x (0.568 (cal/mole) ) + 20000 bar (3.4166 / 41.8) (cal/mole bar)

= 1918.4 (cal/mole)

Page 33: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Phase Diagram

Recall that as you go into the Earth, both P and T increase

These two variables control phase stability of compositions in the earth.

On the left is a map for phases of carbon

Page 34: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Why the discrepancy between the three curves?

Page 35: Thermodynamics Free E and Phase D J.D. Price. Force - the acceleration of matter (N, kg m/s 2 )Force - the acceleration of matter (N, kg m/s 2 ) Pressure.

Phase stability

G = Hfo - TSo + PVo

G = Ho - TSo + PVo

dP/dT = S/ V