1 Gibbs Free Energy and Spontaneity and the meaning of the universe…

Slides:



Advertisements
Similar presentations
CHEMICAL THERMODYNAMICS
Advertisements

Chapter 16 Spontaneous processes –Occur without assistance –Fast or slow –Thermodynamics predicts if reactions will occur but only focuses on the initial.
Spontaneity, Entropy, and Free Energy
Entropy and Free Energy Chapter 19. Laws of Thermodynamics First Law – Energy is conserved in chemical processes neither created nor destroyed converted.
Thermodynamics:Entropy, Free Energy, and Equilibrium
Spontaneous Processes
1 Entropy, Free Energy, and Equilibrium Chapter 18 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Chapter The Austrian physicist Ludwig Boltzmann introduced a model to relate the total number of microstates (the multiplicity, W) to entropy (S).
A spontaneous reaction (or favourable change) is a change that has a natural tendency to happen under certain conditions. Eg. The oxidation of iron (rust)
Entropy and Free Energy How to predict if a reaction can occur, given enough time? THERMODYNAMICS How to predict if a reaction can occur at a reasonable.
Chapter 19. Overview Spontaneous Processes Entropy Second Law of Thermo. Standard Molar Entropy Gibbs Free Energy Free Energy & Temp. & Equil. Const.
Thermodynamics Chapter 19 Liquid benzene Production of quicklime Solid benzene ⇅ CaCO 3 (s) ⇌ CaO + CO 2.
Prentice-Hall © 2007 General Chemistry: Chapter 19 Slide 1 of 44 CHEMISTRY Ninth Edition GENERAL Principles and Modern Applications Petrucci Harwood Herring.
Thermodynamics: Spontaneity, Entropy and Free Energy.
Chemical Thermodynamics: Entropy, Free Energy and Equilibrium Chapter
Copyright McGraw-Hill 2009 Chapter 18 Entropy, Free Energy and Equilibrium.
Chapter 17 THERMODYNAMICS. What is Thermodynamics? Thermodynamics is the study of energy changes that accompany physical and chemical processes. Word.
Rates of Reaction & Equilibrium. Part 1: Rates of Reaction.
Entropy, The Universe and Free Energy
Chemical Thermodynamics The chemistry that deals with the energy and entropy changes and the spontaneity of a chemical process.
Energy Changes in Chemical Reactions -- Chapter First Law of Thermodynamics (Conservation of energy)  E = q + w where, q = heat absorbed by system.
Daniel L. Reger Scott R. Goode David W. Ball Chapter 17 Chemical Thermodynamics.
Chemical Thermodynamics the study of Reaction Feasibility.
Ch. 19: Chemical Thermodynamics (Thermochemistry II) Chemical thermodynamics is concerned with energy relationships in chemical reactions. - We consider.
Chapter 19 Chemical Thermodynamics. First Law of Thermodynamics Energy cannot be created nor destroyed. Therefore, the total energy of the universe is.
Thermodynamics Chapter 18.
THERMODYNAMICS!!!! Nick Fox Dan Voicu.
A.P. Chemistry Spontaneity, Entropy, and Free Energy.
Chapter 19 Chemical Thermodynamics HW:
http:\\asadipour.kmu.ac.ir...46 slides. Thermodynamics http:\\asadipour.kmu.ac.ir...46 slides.
THERMODYNAMICS: ENTROPY, FREE ENERGY, AND EQUILIBRIUM Chapter 17.
Chapter 6. = the capacity to do work or to produce heat Kinetic energy = the energy due to motion depends on mass & velocity Potential Energy = energy.
Ch. 16: Spontaneity, Entropy, and Free Energy 16.1 Spontaneous Processes and Entropy.
Entropy, Free Energy, and Equilibrium Chapter 18 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Entropy, Free Energy, and Equilibrium Chapter 19 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
First Law of Thermodynamics – Basically the law of conservation of energy energy can be neither created nor destroyed i.e., the energy of the universe.
Thermodynamics Brown, LeMay Ch 19 AP Chemistry Monta Vista High School To properly view this presentation on the web, use the navigation arrows below and.
Chapter 19 Chemical Thermodynamics Lecture Presentation John D. Bookstaver St. Charles Community College Cottleville, MO © 2012 Pearson Education, Inc.
Chemical Thermodynamics Chapter 17 Chemical Thermodynamics.
http:\\asadipour.kmu.ac.ir...43 slides. Thermodynamics http:\\asadipour.kmu.ac.ir...43 slides.
Chapter 19 Spontaneity, entropy and free energy (rev. 11/09/08)
Entropy SS. Spontaneity  Spontaneous reactions occur by themselves. Ice melting above 32 o F Water falling over a waterfall Iron rusting  Most spontaneous.
11 © 2006 Brooks/Cole - Thomson Chemistry and Chemical Reactivity 6th Edition John C. Kotz Paul M. Treichel Gabriela C. Weaver CHAPTER 19 Principles of.
Chemistry 100 Chapter 19 Spontaneity of Chemical and Physical Processes: Thermodynamics.
Thermodynamics. study of energy changes that accompany physical and chemical processes. Thermochemistry is one component of thermodynamics which focuses.
Entropy and Free Energy (Kotz Ch 20) - Lecture #2
Entropy, Free Energy, and Equilibrium
CHE 116 No. 1 Chapter Nineteen Copyright © Tyna L. Meeks All Rights Reserved.
 I can identify and describe the five factors that affect reaction rates.
Free energy and Thermodynamics suroviec Spring 2014
Entropy, Free Energy, and Equilibrium Chapter 18 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display. PowerPoint.
Gibbs Free Energy Gibbs Free Energy The method used to determine spontaneity involves both ∆ S sys + ∆ S surr Gibbs deals with only the system,
Entropy, Free Energy, and Equilibrium Chapter 18 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Entropy, Free Energy, and Equilibrium Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Entropy, Free Energy, and Equilibrium Chapter 18 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
1 Entropy, Free Energy, and Equilibrium Chapter 18 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
20-1 Due: CH 20 Connect - Take out Notes/POGIL Today: Solving Problems for Thermodynamics HW: Test on Wednesday Potluck Thursday.
Free Energy and Thermodynamics By Emily Entner.
Chapter 19: Thermodynamics First Law of Thermodynamics: energy cannot be created or destroyed -total energy of the universe cannot change -you can transfer.
Chemical Thermodynamics First Law of Thermodynamics You will recall from earlier this year that energy cannot be created nor destroyed. Therefore, the.
Energy Changes in Chemical Reactions -- Chapter First Law of Thermodynamics (Conservation of energy)  E = q + w where, q = heat absorbed by system.
http:\\academicstaff.kmu.ac.ir\alia sadipour...43 slides.
Chapter 19 Spontaneity, entropy and free energy (rev. 11/09/08)
Chapter 17: Free Energy & Thermodynamics CHE 124: General Chemistry II Dr. Jerome Williams, Ph.D. Saint Leo University.
Entropy, Free Energy, and Equilibrium Chapter 18 Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display.
Ch. 19: Spontaneity (“Thermodynamically Favored”), Entropy and Free Energy.
Chapter 17 Lesson 2 Free Energy and Thermodynamics.
SPONTANEOUS REACTIONS. Spontaneity 1 st Law of Thermodynamics- energy of the universe is ________. Spontaneous Rxns occur without any outside intervention.
Rates of Reaction and Equilibrium
Presentation transcript:

1 Gibbs Free Energy and Spontaneity and the meaning of the universe…

2 Relationship Between  S surr & H Water  S Surr q(system)   S surr affected by heat transfer into or out of closed system Entropy of the surroundings will be affected only by the heat transferred into or out of any closed system. Heat added to surroundings: K.E. surr increases; Molecules are moving faster. K.E. surr increases; Molecules are moving faster. Disorder increases since there is more randomness Disorder increases since there is more randomness Entropy increases. Entropy increases. Note: q p = -  H sys   S surr

3 Heat flow; Temperature Dependent Remember that heat transfer is temperature dependent. Heat will transfer more efficiently with changes at low temperature than at high temperature. i.e., 100€ to an International College student is worth more than to High temperature, molecules are already moving fast, an extra 10°C will not increase their velocities as much as molecules at very low temperature. -  H sys =  S surr units: J. Tmol K Therefore since:  S univ =  S sys +  S surr  S univ =  S sys -  H sys T

4  S univ and Spontaneity Criteria for Spontaneity in terms of the system:  S univ =  S sys +  S surr  S univ =  S sys -  H sys T  S univ  H sys (-)  S univ  H sys (-) (+) Spontaneous  S sys (+) (+) Spontaneous  S sys (+) Spontaneous

5 Spontaneity in terms of T  S univ Criteria for Spontaneity in terms of the system:  S sys +  S surr =  S univ (1)  S sys -  H sys =  S univ (2) T Note rearranging eqn. 2 -T  S sys +  H sys = -T  S univ -T  S sys +  H sys = -T  S univ J. Willard Gibbs realized that -T  S univ can be defined as a new function provided that  T = 0

6 J. Willard Gibbs The Free Energy change (  G) is a measure of spontaneity of a process and of the useful energy available from such a process. J. Willard Gibbs ( ) was not particularly well known in his day, nor is his name widely recognized today, yet he is considered by some to be among the greatest scientists ever born in America. He was awarded th first doctorate in engineering granted in the United States, by Yale University. Gibbs became a professor of mathematical physics at Yale when he was 32 years old and began to publish a series of papers related to thermodynamics and equilibrium. Perhaps because his work was so theoretical, it was largely unappreciated at the time, though its great value was recognized by James Clerk Maxwell. Gibb’s work, if not his name, remains current and vital to this day.

7  G and Spontaneity Defining a new State function  G: -T  S univ  -T  S univ  =   T,  P= 0 Consider  G = - T  S univ  G 0  G = equilibrium  S univ = 0  G > 0nonspontaneous  S univ 0nonspontaneous  S univ < 0 (rev is spontaneous)

8  G: Pictorial View  H sys  S sys Gibbs’ Free Energy can be defined in terms of the enthalpy of the system (  H sys ) and the entropy of the system (  S sys ) -T  S univ =  H sys - T  S sys =  G  G =  H - T  S  G < 0  G > 0  G = equilb Forward reaction occur Spontaneous in forward direction Reverse reaction occur nonspontaneous in forward direction  G < 0  G > 0 See later that :  G  Keq or Q

9  G: Equations of Free Energy Gibbs’ Free Energy can be used to determine the Standard free energy (°) of formation  G =  H - T  S  G° f =  H° f - T  S° f ° Standard State f -formation from elements If data is not for formation process, then equation is slightly adjusted according to:  G° =  H° - T  S° Or from tabulated thermodynamic data:  G° rxn =  n  G° f (prod) -  n  G° f (react)

1010  G: Evaluation of Free Energy Consider the calculation for the following reaction: CH 3 OH (g) + O 2 (g)  CO 2 (g) + H 2 O (g) Determine  G°rxn 2 CH 3 OH (g) + 3 O 2 (g)  2 CO 2 (g) + 4 H 2 O (g)  H° rxn   S° rxn   G° rxn  Evaluate by:  G° rxn =  H° rxn - T  S° rxn  X° rxn =  n  X° f (prod) -  n  X° f (react) Or  G° rxn =  n  G° f (prod) -  n  G° f (react)

1 Effect of temperature on Free Energy Temperature influence on Free Energy and Spontaneity both  H,  S (+)  G =  H-T  S both  H,  S (+) (1000) (1) lg. # sm. # What is the sign of  G ? Temperature will dictate outcome of  G. T low : Temperature small  H-T  S   G (+) dominates negligiblenonspontaneous T high : Temperature large  H-T  S   G (-) negligible dominatesspontaneous

1212 Temperature Relationship and  G Consider Temperature affect on thermodynamic parameters  H-T  ST  G Spontaneity + a - +all -spon: T not impt - b + -all +nonspon: T not impt - c - -low -spon:  H impt - d - -high +nonspon :  S impt + e + +low +nonspon :  H impt + f + +high -spon:  S impt From this table, a spontaneous process can be made nonspontaneous i.e., c & d by increasing Temperature. i.e., c & d by increasing Temperature.

1313 Spontaneity: Example Example : (c) N 2 F 4(g)  2NF 2 (g)  H° - T  S°  G° (c) N 2 F 4(g)  2NF 2 (g)  H° - T  S°  G° 85 kJ 198 T Low  H° dominates  G° (+)  T High  S° dominates  G° (-)  Spontaneous Example : (c) What temp will spontaneity switch for the reaction: (c) What temp will spontaneity switch for the reaction: N 2 (g) + 3H 2(g)  2NH 3 (g)  H° - T  S°  G° N 2 (g) + 3H 2(g)  2NH 3 (g)  H° - T  S°  G° - 92 kJ J/K - 92 kJ T Low  H° dominates  G° (-)  T High  S° dominates  G° (+)  Nonspontaneous To go from spontaneous to nonspontaneous,  G° = 0 … T = - 92kJ = K below spontaneous kJ / K above, nonspontaneous kJ / K above, nonspontaneous

1414 Phase Change Process What determines the spontaneity of a phase change?  H:s l g  S:s l g Two factors competing: Which dominates will determine phase change. Note: In a phase change: s  l is at equilib. or  G° = 0 or  G° = 0 0 =  H° - T  S°  H° = T  S° With signs for  H &  S are the same T =  H°  S°  S° Endo  H(+) Exo  H(-)  S(+)  S(-)  S(+)

1515 Free Energy and work Science and Technology use physical and or chemical processes because these can do work. Economics: To make money €, the work to be preformed must be a possibility and efficient.  G provides information on spontaneity:  G (+) or (-) provides information on the spontaneity of the  P,  T = 0 Wasting time:  G is useful because it prevents the wasted effort on process with no inherent tendency to occur.  G isn’t whole story, Kinetics also important: Note that thermodynamically favorable process may still not occur to any appreciable extent because of the Kinetics. - It makes sense to find a catalyst to speed up the reaction. - It makes sense to find a catalyst to speed up the reaction. - Prevents wasting time and resource of seeking a catalyst on a reaction that won’t even work. - Prevents wasting time and resource of seeking a catalyst on a reaction that won’t even work.

1616  G Equations  G°  n  G° prod -  n  G° reaction  H° -   S° - RT ln K eq  G - RT ln Q