Download presentation
Presentation is loading. Please wait.
1
THERMODYNAMICS thermo – heat dynamics – changes
Laws of Thermodynamics: 0th, 1st, 2nd, 3rd
2
Note: Thermodynamics ……..
· is not concerned about rate of changes (kinetics) but the states before and after the change · does not deal with time
3
Classical Thermodynamics
Marcoscopic observables T, P, V, … Statistical Thermodynamics Microscopic details dipole moment, molecular size, shape
4
Joule’s experiment T mgh adiabatic wall (adiabatic process)
T mgh adiabatic wall (adiabatic process) U (energy change) = W (work) = mgh Thermometer w h
5
Conclusion: work and heat has the same effect
Page 59 w T time interval of heating U = q (heat) Conclusion: work and heat has the same effect to system (internal energy change) * FIRST LAW: U = q + W
6
U: internal energy is a state function [ = Kinetic Energy (K.E.)
+ Potential Energy (P.E.) ] q: energy transfer by temp gradient W: force distance E-potential charge surface tension distance pressure volume First Law: The internal energy of an isolated system is constant
7
Convention: Positive: heat flows into system work done onto system Negative: heat flows out of system work done by system Pressure-volume Work P1 = P2 V2 V1 M
8
If weight unknown, but only properties of system
are measured, how can we evaluate work? M M V2 P P V1 Assume the process is slow and steady, Pint = Pext
9
Free Expansion: Free expansion occurs when the external pressure
is zero, i.e. there is no opposing force
10
Quasi equilibrium process:
Reversible change: a change that can be reversed by an infinitesimal modification of a variable. Quasi equilibrium process: Pint = Pext + dP (takes a long time to complete) infinitesimal at any time quasi equilibrium process
11
what we have consider was isobaric expansion
Page 64-66 P V Example: P1 = 200kPa = P2 V1 = 0.04m3 V2 = 0.1m3 * what we have consider was isobaric expansion (constant pressure) other types of reversible expansion of a gas: isothermal, adiabatic
12
Isothermal expansion remove sand slowly at the same time
Page 65-66 Isothermal expansion remove sand slowly at the same time maintain temperature by heating slowly * P T V1 V2 V area under curve
13
Ex. V1 = 0.04m3 P1 = 200kPa V2 = 0.1m3
14
Adiabatic Reversible Expansion
For this process PV = constant for ideal gas (proved later) V1 P T1 (slightly larger than 1) V2 P T2
15
|Wa|>|Wb|>|Wc|>|Wd|
Ex. V1 = 0.04m3, P1 = 200kPa, V2 = 0.1m3, = 1.3 200kPa const a d b V P d: pressure drop without volume change |Wa|>|Wb|>|Wc|>|Wd| isothermal adibatic
16
State Function Vs Path Function
State function: depends only on position in the x,y plane e.g.: height (elevation) 300 1 B 2 200 100m Y X A
17
Path Function: depends on which path is taken to reach destination
from 1 2, difference of 300m (state function) but path A will require more effort. Internal energy is a state function, heat and work are path functions P 3 2 481.13K 192.45K 1 200kPa 0.04 0.1 V/m3
18
5 moles of monoatomic gas
19
Joule’s second experiment
Energy UU(V,T) ??? thermometer V2 V1 adiabatic wall At time zero, open valve
20
After time zero, V1 V1+V2 T=0 Q=0 W=0 no Pext U=0 thermometer
No temperature change adiabatic wall After time zero, V1 V1+V2 T= Q=0 W=0 no Pext U=0
21
U=U(T) Energy is only a function of temperature for ideal gas
* 0 (for ideal gas) CV is constant volume heat capacity
22
*Enthalpy Define H = U + PV state function intensive variables
state function intensive variables locating the state Enthalpy is also a state function H = U + PV + VP
23
H = QP constant pressure heating
At constant pressure H = U+PV = U - W = Q H = QP constant pressure heating H is expressed as a functional of T and P for ideal gases
24
Thermochemistry Heat transferred at constant volume qV = U Heat transferred at constant pessure qP = H Exothermic H = - Endothermic H = +
25
Standard states, standard conditions
do not measure energies and enthalpies absolutely but only the differences, U or H The choice of standard state is purely a matter of convenience
26
What is the standard state ?
The standard states of a substance at a specified temperature is its pure form at 1 atmosphere
27
25oC, 1 atmosphere: the most stable forms of elements assign “zero enthalpy” Ho298 = 0 used for chemical reactions
28
Standard enthalpy of formation
Standard enthalpy change for the formation of the compound from its elements in their reference states. Reference state of an element is its most stable state at the specified temperature & 1 atmosphere C (s) + 2H2 (g) CH4 (g) Hfo = -75 kJ 289K, 1 atm From the definition, Hfo for elements 0
29
Hess’s Law The standard enthalpy of an overall reaction is the sum of the standard enthalpies of the individual reactions into which a reaction may be divided. Standard reaction enthalpy is the change in enthalpy when the reactants in their standard states change to products in their standard states.
30
Hess’ Law H1 H1 = H2 + H3 + H4 state function
Hess’s law is a simple application of the first law of thermodynamics
31
e.g. C (s) + 2H2 (g) CH4 (g) H1o = ?
298K, 1 atm C (s,graphite) + O2 (g) CO2 (g) Ho = kJ H2 (g) + ½O2(g) H2O (l) Ho = kJ CH4 (g) + 2O2 (g) CO2 (g) + 2H2O (l) Ho = kJ H1o = (-285.8) - (-890.4) = -75 kJ/mole
32
Heat of Reaction (Enthalpy of Reaction)
Enthalpy change in a reaction, which may be obtained from Hfo of products and reactants Reactants Products I stoichiometric coefficient, + products, - reactants E.g. CH4 (g) + Cl2 (g) CH3Cl (g) + HCl (g)
33
Hfo/ kJ CH3Cl HCl Cl CH Hro = ( ) - ( ) = kJ Reactants Products elements elements
34
* Page 83 2A + B 3C + D 0 = 3C + D - 2A - B Generally, 0 = J J J
J denotes substances, J are the stoichiometric numbers *
35
Bond energy (enthalpy)
Assumption – the strength of the bond is independent of the molecular environment in which the atom pair may occur. C (s,graphite) + 2H2 (g) CH4(g)Ho = kJ H2 (g) 2H (g) Ho = kJ C (s,graphite) C (g) Ho= kJ C (s,graphite) + 2H2 (g) C (g) + 4H (g) Ho = 2(435.3) = kJ C (g) + 4H (g) CH4 (g) H = = kJ CH Bond enthalpy = /4 kJ = kJ
36
Temperature dependence of Hr
HrT CP,P R Hro CP,R T
37
H2 = Ho + CP(T2-T1) assume CP,i constant wrt T
What is the enthalpy change for vaporization (enthalpy of vaporization) of water at 0oC? H2O (l) H2O (g) Ho = (-286.1) = kJmol-1 H2 = Ho + CP(T2-T1) assume CP,i constant wrt T H (273) = Ho(298) + CP(H2O,g) - CP (H2O,l)( ) = ( )(-25) = 43.0 kJ/mole
38
Reversible vs Irreversible
Non-spontaneous changes vs Spontaneous changes Reversibility vs Spontaneity First law does not predict direction of changes, cannot tell which process is spontaneous. Only U = Q + W
39
Second Law of Thermodynamics
Origin of the driving force of physical and chemical change The driving force: Entropy Application of Entropy: Heat Engines & Refrigerators Spontaneous Chemical Reactions Free Energy
40
Second Law of Thermodynamics
No process is possible in which the sole result is the absorption of heat from a reservoir and its complete conversion into work Hot Reservoir q w Engine
41
Direction of Spontaneous Change
More Chaotic !!!
42
Entropy (S) is a measurement of the randomness
Spontaneous change is usually accompanied by a dispersal of energy into a disorder form, and its consequence is equivalent to heating Entropy (S) is a measurement of the randomness of the system, and is a state function! S Q S 1 / T
43
Page 122 Entropy S For a reversible process, the change of entropy is defined as (thermodynamic definition of the entropy) * Another expression of the Second Law: The entropy of an isolated systems increases in the course of a spontaneous change: Stot > 0 where Stot is the total entropy of the isolated system
44
Entropy S The entropy of an isolated systems increases in the course of a reversible change: Stot = 0 where Stot is the total entropy of the isolated system
45
Carnot’s Theoretical Heat Engine
Heat flows from a high temperature reservoir to a low temperature body. The heat can be utilized to generate work. e.g. steam engine.
46
The efficiencies of heat engines
Hot Reservoir q w Engine DS = - |q|/Th < not possible! contrary to the second law
47
The Nernst Theorem The entropy change accompanying any physical or
chemical transformation approaches zero as the temperature approaches zero. DS 0 as T0
48
Third Law of Thermodynamics If the entropy of each element in its most
state is taken as zero at the absolute zero of temperature, every substance has a positive entropy. But at 0K, the entropy of substance may equals to 0, and does become zero in perfect crystalline solids. Implication: all perfect materials have the same entropy (S=0) at absolute zero temperature Crystalline form: complete ordered, minimum entropy
49
Statistical Interpretation of S
S = 0 at 0K for perfect crystals S = k ln Boltzmann number of arrangements postulate of entropy Boltzmann constant
50
Entropy Change of Mixing
one distinguish arrangement number of arrangement increased
51
In general mixing NA, NB Entropy change of mixing Stirling’s approximation: ln N! N ln N + 0(N) for large N
52
Extensions of 2nd Law TdS dq Clausius Inequality For adiabatic process, Entropy will always attain maximum in adiabatic processes. A similar function for other processes?
53
Define Helmholtz free energy
A = U - TS Thermodynamic State Function dA = dU - TdS - SdT Substitute into Clausius Inequality for isothermal, isochoric (constant volume) process,
54
change in Helmholtz free energy = maximum isothermal work
Example of isothermal, isochoric process: combustion in a bomb calorimeter O2 + fuel Temp. bath O2, CO2, H2O Higher P heat given out
55
Gibbs Free Energy Define Gibbs free energy G = H - TS Thermodynamic state function = U + PV -TS dG = dU +PdV + VdP -TdS -SdT
56
constant pressure, constant temperature
G will tend to a minimum value equilibrium spontaneous change More applications since most processes are isothermal, isobaric chemical reactions at constant T, P Reactants Products endothermic H is positive exothermic H is negative
57
Change of Gibbs free energy with temperature
(constant pressure)
58
In P 1/T
59
Example: What is the change in the boiling
point of water at 100oC per torr change in atmospheric pressure? Hvap = 9725 cal mol-1 Vliq = l mol-1 Vvap = l mol-1
Similar presentations
© 2024 SlidePlayer.com. Inc.
All rights reserved.