Answers to Selected Problems

Total Page:16

File Type:pdf, Size:1020Kb

Answers to Selected Problems Answers to Selected Problems Chapter 1 1.2. 0.55 A 1.3. +-y-.z- ++ y+, z+ t-t-y+,~+ -!-!y+.z+ *x+ lx+ t-x+ *s -ls i- s- 1- s+ -l s+ t- s+ BeO triplet CO singlet NO doublet 1.5. "Ionic bonds" using 6p electrons are stronger than those using 6s electrons (Pb2+2Br- p Pb4 +4Br-). "Covalent bonds" with 6s electrons are stronger than those with 6p electrons (PbMe4 > PbMe2)' The energy gap between 6p and 6s orbitals is larger than that for 2p and 2s orbitals. 1.6. SOl = Cda + b + c + d + e + f) S02 = C2(a + b - c - d + e +f) S03 = C3(a - b + c - d + e + f) 541 542 Answers to Selected Problems S04 = C4 (a + b + c + d - e +f) SOs = Cs(a + b - c - d - e +f) SOb = C6 (a - b - c + d - e + f) 1.9. B. c. D d. 0 1.10. There is no vibrational distortion of a homonuclear diatomic that can lower its symmetry. Chapter 2 2.2. Charge density qi = 1; n-bond order Pii = I. 2.3. Il.E = 1l.E,. + IlE,; 1l.E, = 2(1 - i 12) {J. 2.4. Second-order perturbations are not additive. In double union of even AHs, the second­ order terms are large and cannot be ignored. Chapter 3 3.1. 4 J -jill jm Answers to Selected Problems 543 3.2. a. Ii) I1E n = 2-=( 2 + --3) {J = 0.92{J " ,,/17.7 j17.7 I1Enp = 2 ( --~- + 1 ) {J = 1.28{J j17.7 )17.7 (ii) I1En, = 2 ( -~= + ~-- ) {J = 0.84{J )20.7 fti0 (iii) I1Enp = 2( -- 6- + -~){J = 1.47{J ,,/17.7 v17.7 (iv) I1En, = 2 ( -/ + 2 ) {J = 1.35{J ..;20.7 )20.7 Thus (iii) > (ii) > Ii): (iv) > (ii). b. Ii) (ii) (iii) (iv) (i) > (ii) > (iv):> (iii). ;- 3.4. I1E n values: (i) :2 (I - 3 v 17) fJ = 0.54{J. (ii) 2 (I :1, 20) {J = 0.66{J. (iii) 4.20fi + 2(1 - 3/" 20){J = 0.86{J. 544 Answers to Selected Problems (iv) 4/17/3 + 2(1 - 3/)17)/3 = 0.78/3. (v) 4;20/3 + 2(1 - 3;,/20)/3 = 0.86/3. (vi) 1 17/3 + 2(1 - 3/v 17) /3 = 0.60/3. 3.5. a. > b. < c. > d. < 3.6. x = 0.471 /3 = 0.471 /3 x = 0.638 TsX -t;x -x ' fs-x f '-LI"X x = 0.484 NorrD-- rrx "hx x = 0.433 3.7. For example. ratio of numbers of classical structures: NBMO coefficient, cc6 2:(2/)42) Answers to Selected Problems 545 l l/j4I) ~ ~ . cCO~ ~ ~ I o:x) 1:(1/)42) However, 3.8. -p ~ ~ > I > ~ ~ ct:o~ # # cSM. = (8/7) P 0 Chapter 4 4.2. They are stabilized by mutual conjugation. 4.3. CHr-OH CHz E01 6 + 2H zSO. ~ 6 + H30+ + 2HSO.- H 0 EO, 0+ 02S0• ~ G+DSO,- EE 20 ~-- D=o Br Li+ I 6 + BuLi ~ o +B~Br 546 Answers to Selected Problems 4.4. a. tlErr{ionization) (i) 2(1 - 3/Jl7) Ii = 0.541i CH20H (ii) ~I 2{1 - 5/}46) Ii = 0.531i cB/" ~ I § (iii) 2(1-5/fo)Ii=0.60Ii (iv) 2(1 - 4/}34) Ii = 0.63tJ (V) 2(1 - 3/fo) Ii = 0.691i (vi) 2(1 - 3/,,118) Ii = 0.591i Thus the order of equilibrium constants is (vi> (iv) > (iii) '> (vi) > (i) '> (ii) b. The anionic equilibrium constants should follow the same order because in the ab­ sence of heteroatoms, the change in 1t energy for anions, cations, and radicals should be the same. 'R 4.5. a. S' -GI Ill, / (i) All bond lengths are in units of the standard bond length (1.40 AI. Iii) The field effect Fs is obtained on the assumption that the substituent acts as a dipole with charge 4 at atom i and charge - 0.94 one standard bond length from i along the bond to the substituent. The magnitude of the charge is accounted for by the Fs parameter. Thus Answers to Selected Problems 547 for p-F, 0- ¢ F FF = 4.85, F F = 4.85 ( ! _ Q2) = 0.525 rim 3 4 (iii) q'.m is the formal negative charge at the reaction site when the substituent is replaced by CH2 -; for the p-F this is 1/7. Thus, (iv) The q's in the term for the mesomeric field effect are obtained in the same way. :r\\ 2.65 .tmd.ro bood 1m,"" 1. ~ ~ ,.x 0~ 7X F MFF L ;i' = -0.577(~ +~) = -0.062 .. m km 2.65 2.65 a F 1.4 = 0.525 - 0.30 - 0.062 = 0.16 a l ,4: Br = 0.23, CH3 = -0.11 a l .3 : CI = 0.50, CH30 = 0.12 b.1og(KF IKH ) = pa (- pK F ) - (- pK H ) = 1.74(0.16) = 0.27 pK r = 12.80 - 0.27 = 12.53 (calc) = 12.82 (obs). 4.6. These will follow the reactivity numbers, with appropriate statistical corrections: N, = 2(ao, + (/0,)' 4.7. This is a long exercise. The structure of the dimer is not known. 4.8. Increasing as should increase the half-wave potential in a linear way. The reactive center should be the center of the ring. 4.9. This is an OE, reaction; the change in It energy is given by /'iE. = 2(1 - ao,) p. 548 Answers to Selected Problems Chapter 5 5.1. This reversal illustrates the conflict between the -/ effect of alkyl groups and polarization stabilization of charge. For carbanions. the two effects oppose each other in the gas phase: for cations. they are in the same direction. In solution. the polarizability effects on relative stability are much less important because the medium is highly polarizable, and access of the solvent to the charged center is more important than charge polarization within the molecule. 5.3. Product B would be favored by increasing the solvation power of the medium. 5.3. This question involves the effect of charge delocalization in the transition state on relative solvent effects. The Elcb transition state has much more carbanionic character than that for the E2 reaction. Increasing solvation will favor Elcb reactions. 5.4. Since the BEP principle holds for these reactions. this can be answered in the context of Problems 4.4 and 3.4: H E E ../27 Nt = 4/.... 7 = LSI Nt = 12/ .... 127 = 2.31 N, = 12/.j5i = 1.68 Thus the relative rates are > 4 > 2; for nitration in acetic anhydride. the 1 isomer is formed fastest. Nt = 1.67 Reaction is fastest at the 2 position. 5.6. a. See Problem 4.9; the same principle applies since this is a BEP process. b. The least reactive molecule in the series will show the largest difference between Sv I and SN2 rates. Me0 2C 5.7. a. C02 Me I C ill ~CO'M' III C ~ I HU C02Me Answers to Selected Problems 549 b. d ~, N-N c. +- j/'~ LEi rI ~ /,,,.~ ··-=eN Ph X Ph I CH, CH, , -·-N Ph + N2 d. dJllH D 550 Answers to Selected Problems EE; e. ~< --. ~~ :XY yeO, yD, ""CD, EO! DE! ~~]D'I - ~ <==! + f. C AD, DD Y' D, 'CD, 2 "CH 2 Br Br Br y~/ H! (lJ (pJJr- g. ~ +l Br Br~ ',,-/ = ~ H Br Et:! -, ~-.::::::! m (\ A ~y Br CM" H Br Br o~ o~ EE; EE; ~ <===± h. Ht) \. j ~~~ \, H ~H -/'\ ]I nt '~ n! ~ H H ~ 1 H H~r H ~d a~ H OLL ~~ f50 Answers to Selected Problems 551 CF3 CF3 CF3 CF J I i. EE+ C 1 + ~ + III EE+ ~ I ~ ;6":t / C ~ 0 I I CF3 CF3 CF3 CF3 C02CH3 I ()JJ(CO,CH, C j. M! CH 2 I + III Ii I ~H2 I I (()~ ~ C ~ I C02CH3 C02CH 3 aC02CH3 m + 0> ~ C02CH3 5.S. a. NH z CI Br OH H b. H 20 -- ---> d ---H d Cis 5.12. Cl 5.14. Consider the 1,4 localization energies in the starting material and the intermediate. Chapter 6 6.1. The easiest way to examine the stabilities of open-chain and cyclic excited states using the PMO method is to compare the two by intramolecular union. llE. = 2p"/J,, 552 Answers to Selected Problems The problem is to determine the sign of Prs in the first excited state. The pairing theorem (p. 75) provides a direct basis for doing this. The AO coefficients in open-chain polymers are determined by symmetry and the magnitude of the coefficients on the terminal atoms increases as one approaches a. Thus for butadiene in its first excited state, the orbital occupation and symmetry are A--- S -+--LUMO A-+-1-HOMO S-*-ll- In this state, the 1,4 antibondingness of the singly occupied HOMO is exactly cancelled by the 1,4 bondingness of the singly occupied LUMO since the AO coefficients in these two orbitals are the same by the pairing theorem. The only remaining contribution to PIA is a positive one from the doubly occupied symmetric orbital. This will be the case in all 4n-polyene excited states because the magnitude of the terminal coefficients in­ creases on approaching a, so the symmetric (positive) contributions to P.-w will always be largest. Since P is negative, terminal intramolecular union will always decrease the energies of these systems, i.e., the cyclic systems are aromatic when compared to the excited states of their open-chain analog. 6.3. (See Ref. 22): o m leid+ 6.4.
Recommended publications
  • Transition State Theory. I
    MIT OpenCourseWare http://ocw.mit.edu 5.62 Physical Chemistry II Spring 2008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. 5.62 Spring 2007 Lecture #33 Page 1 Transition State Theory. I. Transition State Theory = Activated Complex Theory = Absolute Rate Theory ‡ k H2 + F "! [H2F] !!" HF + H Assume equilibrium between reactants H2 + F and the transition state. [H F]‡ K‡ = 2 [H2 ][F] Treat the transition state as a molecule with structure that decays unimolecularly with rate constant k. d[HF] ‡ ‡ = k[H2F] = kK [H2 ][F] dt k has units of sec–1 (unimolecular decay). The motion along the reaction coordinate looks ‡ like an antisymmetric vibration of H2F , one-half cycle of this vibration. Therefore k can be approximated by the frequency of the antisymmetric vibration ν[sec–1] k ≈ ν ≡ frequency of antisymmetric vibration (bond formation and cleavage looks like antisymmetric vibration) d[HF] = νK‡ [H2] [F] dt ! ‡* $ d[HF] (q / N) 'E‡ /kT [ ] = ν # *H F &e [H2 ] F dt "#(q 2 N)(q / N)%& ! ‡ $ ‡ ‡* ‡ (q / N) ' q *' q *' g * ‡ K‡ = # trans &) rot ,) vib ,) 0 ,e-E kT H2 qH2 ) q*H2 , gH2 gF "# (qtrans N) %&( rot +( vib +( 0 0 + ‡ Reaction coordinate is antisymmetric vibrational mode of H2F . This vibration is fully excited (high T limit) because it leads to the cleavage of the H–H bond and the formation of the H–F bond. For a fully excited vibration hν kT The vibrational partition function for the antisymmetric mode is revised 4/24/08 3:50 PM 5.62 Spring 2007 Lecture #33 Page 2 1 kT q*asym = ' since e–hν/kT ≈ 1 – hν/kT vib 1! e!h" kT h! Note that this is an incredibly important simplification.
    [Show full text]
  • Eyring Equation
    Search Buy/Sell Used Reactors Glass microreactors Hydrogenation Reactor Buy Or Sell Used Reactors Here. Save Time Microreactors made of glass and lab High performance reactor technology Safe And Money Through IPPE! systems for chemical synthesis scale-up. Worldwide supply www.IPPE.com www.mikroglas.com www.biazzi.com Reactors & Calorimeters Induction Heating Reacting Flow Simulation Steam Calculator For Process R&D Laboratories Check Out Induction Heating Software & Mechanisms for Excel steam table add-in for water Automated & Manual Solutions From A Trusted Source. Chemical, Combustion & Materials and steam properties www.helgroup.com myewoss.biz Processes www.chemgoodies.com www.reactiondesign.com Eyring Equation Peter Keusch, University of Regensburg German version "If the Lord Almighty had consulted me before embarking upon the Creation, I should have recommended something simpler." Alphonso X, the Wise of Spain (1223-1284) "Everything should be made as simple as possible, but not simpler." Albert Einstein Both the Arrhenius and the Eyring equation describe the temperature dependence of reaction rate. Strictly speaking, the Arrhenius equation can be applied only to the kinetics of gas reactions. The Eyring equation is also used in the study of solution reactions and mixed phase reactions - all places where the simple collision model is not very helpful. The Arrhenius equation is founded on the empirical observation that rates of reactions increase with temperature. The Eyring equation is a theoretical construct, based on transition state model. The bimolecular reaction is considered by 'transition state theory'. According to the transition state model, the reactants are getting over into an unsteady intermediate state on the reaction pathway.
    [Show full text]
  • Bimolecular Reaction Rate Coefficients in the Last Lecture, We Learned Qualitatively the Reaction Mechanisms of Hydrocarbon Combustion
    Combustion Chemistry Hai Wang Stanford University 2015 Princeton-CEFRC Summer School On Combustion Course Length: 3 hrs June 22 – 26, 2015 Copyright ©2015 by Hai Wang This material is not to be sold, reproduced or distributed without prior written permission of the owner, Hai Wang. Lecture 4 4. Bimolecular Reaction Rate Coefficients In the last lecture, we learned qualitatively the reaction mechanisms of hydrocarbon combustion. To make this description quantitative, we will need to have a basic knowledge of reaction rate theories. While the rate coefficients of a large number of combustion reactions are experimentally measured, reaction rate theories are often necessary to interpret the experimental data. We shall focus our discussion here to bimolecular reactions of the type A + B → C + D and leave the discussion for unimolecular reactions to a later time. 4.1 Hard Sphere Collision We discussed earlier that an elementary chemical reaction requires molecular collision. The rate coefficient of a bimolecular reaction is essentially the product of reaction probability of two reactants (A and B) upon collision at a given temperature γ(T) and the frequency of collision ZAB, k(T) [A][B] = γ(T) ZAB (4.1) Here we assume that molecules may be described by rigid spheres. Figure 4.1 shows several scenarios of molecular encounter. Starting from the head-on collision, an offset of the two axes of molecular motion leads to off-center collision. Suppose the diameter of A and B are σA and σB, respectively. The limiting off-center collision would have a spacing equal to (σA+σB)/2 between the two axes of molecular motions.
    [Show full text]
  • Reaction Mechanism of Transition Metal Complexes
    CHAPTER 3 Reaction Mechanism of Transition Metal Complexes – I: Inert and Labile Complexes The metal complexes in which the rate of ligand displacement reactions is very fast and hence show high reactivity are called as labile Complexes and this property is termed as lability. On the other hand, the metal complexes in which the rate of ligand displacement reactions is very slow and hence show less reactivity are called as inert complexes and this property is termed as inertness. Thermodynamic stability is the measure of the extent to which the complex will form or will be transformed into another complex when the system has reached equilibrium while kinetic stability refers to the speeds at which these transformations take place. The thermodynamic stability depends upon the energy difference of the reactant and product if the product has less energy than that of the reactant, it will be more stable than the reactant. The thermodynamic stability of metal complexes is calculated by the overall formation constant. If the value of log β is more than 8, the complex is considered as thermodynamically stable. Figure 1. The general reaction coordinates diagram. The kinetic stability of the complex depends upon the activation energy of the reaction. If the activation energy barrier is low, the reaction will take place at a higher speed. These types of complexes are also called as kinetically unstable. If the activation energy barrier is high, the substance will react slowly and will be called as kinetically stabilized or inert. There is no correlation between thermodynamic and kinetic stability. Thermodynamically stable products may labile or inert and the vice versa is also true.
    [Show full text]
  • Visualizing the Transition State and Reaction Coordinate”
    Teacher’s Guide to “Visualizing the Transition State and Reaction Coordinate” Jeffrey E. Fieberg, Ph.D. Chemistry Program Centre College Danville, KY 40422 [email protected] 859-238-5875 CHEMICAL CONCEPTS This demonstration can be used when teaching chemical kinetics in a General Chemistry course or in a Physical Chemistry course. Chemical Kinetics • Activation energy • Modeling chemical reactions, particularly isomerization reactions • Lindemann mechanism for unimolecular reactions • Dependence of reaction yield on particular partition of energy into internal modes of motion (vibrational, rotational) Transition State Theory (Activated Complex Theory) • Structure of the transition state • Inherent instability of the transition state • Observation of the reaction coordinate (reaction progress) HOW THE DEMONSTRATION ADDRESSES THE CHEMICAL CONCEPTS Transition state theory (TST), also called activated complex theory, is often introduced in general chemistry courses when discussing kinetics. A reaction energy diagram is used to follow the progress of the reaction from reactants through a transition state to products (see figure 1). The reaction energy diagram plots the system’s potential energy versus reaction coordinate (or reaction progress) and shows that reactant molecules must overcome an activation energy barrier to pass through the transition state (activated complex) to form products. This demonstration takes the very abstract concepts of transition state, activation energy, and reaction coordinate and makes them more concrete and accessible. The demonstration uses a child’s toy (Hoberman Switch Pitch) to model a chemical reaction that follows a reactant through a transition state before making a product. The reaction coordinate, activation energy, and specific geometry of the transition state are discussed as part of a question and answer dialogue.
    [Show full text]
  • Introduction to the Transition State Theory 29
    DOI: 10.5772/intechopen.78705 ProvisionalChapter chapter 2 Introduction toto thethe TransitionTransition StateState TheoryTheory Petr PtáPtáček,ček, FrantiFrantišekšek ŠŠoukaloukal andand TomáTomášš OpravilOpravil Additional information isis availableavailable atat thethe endend ofof thethe chapterchapter http://dx.doi.org/10.5772/intechopen.78705 Abstract The transition state theory (TST), which is also known as theory of absolute reaction rates (ART) and the theory of activated state (complex), is essentially a refined version of crude collision theory, which treats the reacting molecules as the rigid spheres without any internal degree of freedom. The theory explains the rate of chemical reaction assuming a special type of chemical equilibrium (quasi-equilibrium) between the reactants and acti- vated state (transition state complex). This special molecule decomposes to form the products of reaction. The rate of this reaction is then equal to the rate of decomposition of activated complex. This chapter also explains the limitation of TST theory and deals with the kinetics isotope effect. Keywords: transition state theory, theory of absolute reaction rates, activated complex, equilibrium constant, reaction rate, kinetics, activation energy, frequency factor, partition function, thermodynamics of activated state, kinetics isotope effect 1. Introduction “Two major findings have, however, stood the test of time. First, there was the unmistakable evidence that molecular collisions play the all-important role in communicating the activation energy to the molecules which are to be transformed and, second, there was the recognition of the activation energy (derivable for the Arrhenius Law of the temperature dependence) as a dominant, though by no means the sole, factor determining reactivity in general.”—C.N.
    [Show full text]
  • Transition State Theory. Atkins & Depaula: 7.6-7.7
    University of Washington Department of Chemistry Chemistry 453 Winter Quarter 2015 Lecture 22: Transition State Theory. Atkins & DePaula: 7.6-7.7 A. Activated Kinetics Kinetic rate equations are governed by several principles. The first is the Law of Mass Action. It state that for a chemical reaction k f ABAB P (22.1) the rate of formation of product i.e. d[P]/dt is dependent of the reaction concentrations: dP AB kA B (22.2) dt f However, the explicit dependence of stoichiometric coefficients is not general and rigorously only applies to elementary reactions. Deviations may occur for multiple steps involving reaction intermediates. The Principle of Detailed Balance states the relationship of kinetic constants k at equilibrium. For a reversible reaction: ABf at equilibrium the kr forward and reverse reactions are equal: rateforward rate reverse kA kB (22.3) freq eq k B K feq kA r eq Equation 22.3 means the kinetic constants kf and kr are not independent. Their ratio is the equilibrium constant. In equilibrium thermodynamics the van’t Hoff equation gives the temperature dependence of the enthalpy: dKln H (22.4) dT RT 2 Arrhenius proposed an analogous relationship for the temperature dependence of the kinetic constant dkln E f a (22.5) dT RT 2 The assumption of the Arrhenius equation 22.5 is that the reaction rate is determined by the activation barrier Ea at which point on the reaction coordinate molecules are in a high energy ‘activated state” or “transition-state”. The diagram below schematizes the activation barrier Ea. A chemical or physical process whose rate follows equation 22.5 is called an activated process.
    [Show full text]
  • Activated Complex Theory
    CHAPTER 3 Chemical Dynamics – I 143 Activated Complex Theory In 1935, an American chemist Henry Eyring; alongside two British chemists, Meredith Gwynne Evans and Michael Polanyi; proposed a new theory to rationalize the rate of different chemical reactions which was based upon the formation of an activated intermediate complex. This theory is also known as the "transition state theory", "theory of absolute reaction rates”, and "absolute-rate theory". The activated complex theory states that the rates of various elementary chemical reactions can be explained by assuming a special type of chemical equilibria (quasi-equilibrium) between reactants and activated complexes. Before the development of activated complex theory, the Arrhenius rate law was popularly used to determine energies for the potential barrier. However, the Arrhenius equation was based on empirical observations rather than mechanistic investigations as if one or more intermediates are involved in the conversion or not. For that reason, more development was essential to know the two factors present in the Arrhenius equation, the activation energy (Ea) and the pre-exponential factor (A). The Eyring equation from transition state theory successfully addresses these two issues and therefore contributed significantly to the conceptual understanding of reaction kinetics. Figure 11. The variation of free energy as the reaction proceeds. To explore the concept mathematically, consider a reaction between reactant A and B forming a product P via the activated complex X* as: ∗ 퐾 푘 (178) 퐴 + 퐵 ⇌ 푋∗ → 푃 The equilibrium constant for reactants to activated complex conversion is [푋∗] (179) 퐾∗ = [퐴][퐵] Copyright © Mandeep Dalal 144 A Textbook of Physical Chemistry – Volume I Henry Eyring showed that the rate constant for a chemical reaction with any order or molecularity can be given by the following relation.
    [Show full text]
  • The Basic Theorem of Temperature-Dependent Processes
    Review The Basic Theorem of Temperature-Dependent Processes Valentin N. Sapunov 1,* , Eugene A. Saveljev 1, Mikhail S. Voronov 1, Markus Valtiner 2,* and Wolfgang Linert 2,* 1 Department of Chemical Technology of Basic Organic and Petrochemical Synthesis, Mendeleev University of Chemical Technology of Russia, Miusskaya sq. 9, 125047 Moscow, Russia; [email protected] (E.A.S.); [email protected] (M.S.V.) 2 Department of Applied Physics, Vienna University of Technology, Wiedner Hauptstrasse 8-10/134-AIP, 1040 Vienna, Austria * Correspondence: [email protected] (V.N.S.); [email protected] (M.V.); [email protected] (W.L.) Abstract: The basic theorem of isokinetic relationships is formulated as “if there exists a linear correlation “structure∼properties” at two temperatures, the point of their intersection will be a common point for the same correlation at other temperatures, until the Arrhenius law is violated”. The theorem is valid in various regions of thermally activated processes, in which only one parameter changes. A detailed examination of the consequences of this theorem showed that it is easy to formulate a number of empirical regularities known as the “kinetic compensation effect”, the well- known formula of the Meyer–Neldel rule, or the so-called concept of “multi-excitation entropy”. In a series of similar processes, we examined the effect of different variable parameters of the process on the free energy of activation, and we discuss possible applications. Keywords: isokinetic relationship; Meyer–Neldel; multi-excitation entropy; free energy of activation Citation: Sapunov, V.N.; Saveljev, E.A.; Voronov, M.S.; Valtiner, M.; Linert, W.
    [Show full text]
  • Reaction Kinetics and Mechanisms in Coordination Compounds
    Reaction kinetics and mechanisms in coordination compounds The kinetics of inorganic reaction mechanism The mechanism of a chemical reaction is understood from transition state theory. The course of a chemical reaction involves collision of reactants sufficiently energetic to form the activated complex or transition state. Along the path from reactants to products kinetic energy is converted into potential energy by bond stretching, partial bond formation, angular distortions etc. The transition state is the species of maximum potential energy resulting from these motions. All energetically unfavourable processes have occurred by the time a transition state is reached. Activation energy: The energy required for the reactant to reach the transition state from ground state is called the activation energy. After the transition state, the collection of atoms rearranges toward more stable species: old bonds are fully broken, new bonds are fully made, and geometric rearrangement toward a more stable configuration (Relaxation) occurs. In multistep reactions a new transition state is reached for each distinguishable step. Plots can be made of the energy of a reacting system as a function of relative atomic positions. Consider the reaction, H2 + F → HF + H When all reactants are confined to a straight line, the distances between atoms are rH-H and rH-F describes relative atomic positions. The path which involves changes in both rH-H and rH-F is called reaction coordinate. A plot of energy verses two variable is three dimensional. Principle of microscopic reversibility Whether any reaction proceeds forward or backward, it follows the reaction coordinate. Atomic positions simply reverse themselves as the reaction is reversed, like a film shown backwards.
    [Show full text]
  • Unit 9A: Kinetics and Energy Changes
    Unit 9: Kinetics, Thermodynamics, & Equilibrium-Lecture Regents Chemistry ’14-‘15 Mr. Murdoch Unit 9a: Kinetics and Energy Changes 1. Student Name: _______________________________________ Class Period: ________ Unit 9a (Kinetics & Energy Changes) Page 1 of 43 Unit 9: Kinetics, Thermodynamics, & Equilibrium-Lecture Regents Chemistry ’14-‘15 Mr. Murdoch Page intentionally blank Unit 9a (Kinetics & Energy Changes) Page 2 of 43 Unit 9: Kinetics, Thermodynamics, & Equilibrium-Lecture Regents Chemistry ’14-‘15 Mr. Murdoch Unit 9 Vocabulary: 1. Activated Complex: The species that are formed and decomposed during the mechanism; also called the intermediate. 2. Activation Energy: The energy that must be added to allow the reactants to start the reaction and form the activated complex. 3. Catalyst: A chemical that is added to a reaction to eliminate steps in the mechanism, increase the reaction rate, and decrease the activation energy without itself being consumed by the reaction. 4. Effective Collision: A collision between reactant particles that results in a chemical reaction taking place. 5. Enthalpy: The total amount of potential energy stored in a substance. 6. Endothermic: A reaction that absorbs and stores energy from the surrounding environment. 7. Entropy: A system’s state of disorder. Entropy increases as temperature increases. Entropy increases as a substance goes from solid to liquid to gas. 8. Equilibrium: A system where the rate of forward change is equal to the rate of reverse change. At equilibrium there is no net change. 9. Exothermic: A reaction that releases stored energy into the surrounding environment. 10. Favored: A change in a thermodynamic property that contributes towards the reaction being spontaneous.
    [Show full text]
  • Chemical Kinetics
    Chemical Kinetics Lecture notes edited by John Reif from PPT lectures by: Chung (Peter) Chieh, University of Waterloo Hana El-Samad, UCSB John D. Bookstaver, St. Charles Community College Dan Reid, Champaign CHS Slides revised by Xin Song for Spring 2020 Term What are Chemical Kinetics? Chemical Kinetics Kinetics – how fast does a reaction proceed? Thermodynamics – does a reaction take place? Reaction speed: measured by the change in concentration with time. Important factors which affect rates of reactions: – reactant concentration – temperature – action of catalysts – surface area – pressure of gaseous reactants or products Dan Reid Champaign CHS Kinetics • Studies the rate at which a chemical process occurs. • Besides information about the speed at which reactions occur, kinetics also sheds light on the reaction mechanism (exactly how the reaction occurs). • John D. Bookstaver • St. Charles Community College Outline: Kinetics Reaction Rates How we measure rates. How the rate depends on amounts Rate Laws of reactants. How to calculate amount left or Integrated Rate Laws time to reach a given amount. How long it takes to react 50% of Half-life reactants. How rate constant changes with Arrhenius Equation temporature. Link between rate and molecular Mechanisms scale processes. • John D. Bookstaver • St. Charles Community College Reaction Rates Reaction Rates Rates of reactions can be determined by monitoring the change in concentration of either reactants or products as a function of time t. [A] = concentration of reactant A • John D. Boo kstaver • St. Charles Community College Reaction Rate • For the reaction A à B there are two ways of measuring rate: (1) the speed at which the reactants disappear (2) the speed at which the products appear • Reversible reactions: as products accumulates, they can begin to turn back into reactants.
    [Show full text]