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© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 1 Nature of the Chemical Bond with applications to catalysis, materials.

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Presentation on theme: "© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 1 Nature of the Chemical Bond with applications to catalysis, materials."— Presentation transcript:

1 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 1 Nature of the Chemical Bond with applications to catalysis, materials science, nanotechnology, surface science, bioinorganic chemistry, and energy Lecture 19 February 16, 2011 Transition metals:Pd and Pt William A. Goddard, III, wag@wag.caltech.eduwag@wag.caltech.edu 316 Beckman Institute, x3093 Charles and Mary Ferkel Professor of Chemistry, Materials Science, and Applied Physics, California Institute of Technology Teaching Assistants: Wei-Guang Liu wgliu@wag.caltech.edu Caitlin Scott

2 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 2 Last time

3 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 3 Compare chemistry of column 10

4 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 4 Ground state of group 10 column Pt: (5d) 9 (6s) 1 3 D ground state Pt: (5d) 10 (6s) 0 1 S excited state at 11.0 kcal/mol Pt: (5d) 8 (6s) 2 3 F excited state at 14.7 kcal/mol Pd: (5d) 10 (6s) 0 1 S ground state Pd: (5d) 9 (6s) 1 3 D excited state at 21.9 kcal/mol Pd: (5d) 8 (6s) 2 3 F excited state at 77.9 kcal/mol Ni: (5d) 8 (6s) 2 3 F ground state Ni: (5d) 9 (6s) 1 3 D excited state at 0.7 kcal/mol Ni: (5d) 10 (6s) 0 1 S excited state at 40.0 kcal/mol

5 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 5 Salient differences between Ni, Pd, Pt NiPd Pt 4s more stable than 3d 5s much less stable than 4d 6s, 5d similar stability 3d much smaller than 4s (No 3d Pauli orthogonality) Huge e-e repulsion for d 10 4d similar size to 5s (orthog to 3d,4s Differential shielding favors n=4 over n=5, stabilize 4d over 5s  d 10 2 nd row (Pd): 4d much more stable than 5s  Pd d 10 ground state 3 rd row (Pt): 5d and 6s comparable stability  Pt d 9 s 1 ground state Relativistic effects of 1s huge  decreased KE  contraction  stabilize and contract all ns  destabilize and expand nd

6 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 6 Mysteries from experiments on oxidative addition and reductive elimination of CH and CC bonds on Pd and Pt Why is CC coupling so much harder than CH coupling?

7 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 7 Step 1: examine GVB orbitals for (PH 3 ) 2 Pt(CH 3 )

8 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 8 Analysis of GVB wavefunction

9 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 9 Alternative models for Pt centers

10 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 10

11 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 11 energetics Not agree with experiment

12 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 12 Possible explanation: kinetics

13 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 13 Consider reductive elimination of HH, CH and CC from Pd Conclusion: HH no barrier CH modest barrier CC large barrier

14 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 14 Consider oxidative addition of HH, CH, and CC to Pt Conclusion: HH no barrier CH modest barrier CC large barrier

15 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 15 Summary of barriers But why? This explains why CC coupling not occur for Pt while CH and HHcoupling is fast

16 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 16 How estimate the size of barriers (without calculations)

17 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 17 Examine HH coupling at transition state Can simultaneously get good overlap of H with Pd sd hybrid and with the other H Thus get resonance stabilization of TS  low barrier

18 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 18 Examine CC coupling at transition state Can orient the CH 3 to obtain good overlap with Pd sd hybrid OR can orient the CH 3 to obtain get good overlap with the other CH 3 But CANNOT DO BOTH SIMULTANEOUSLY, thus do NOT get resonance stabilization of TS  high barier

19 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 19 Examine CH coupling at transition state H can overlap both CH 3 and Pd sd hybrid simultaneously but CH 3 cannot thus get ~ ½ resonance stabilization of TS

20 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 20 Now we understand Pt chemistry But what about Pd? Why are Pt and Pd so dramatically different

21 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 21 new

22 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 22 Pt goes from s 1 d 9 to d 10 upon reductive elimination thus product stability is DECREASED by 12 kcal/mol Using numbers from QM

23 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 23 Pd goes from s 1 d 9 to d 10 upon reductive elimination thus product stability is INCREASED by 20 kcal/mol Using numbers from QM Pd and Pt would be ~ same

24 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 24 Thus reductive elimination from Pd is stabilized by an extra 32 kcal/mol than for Pt due to the ATOMIC nature of the states The dramatic stabilization of the product by 35 kcal/mol reduces the barrier from ~ 41 (Pt) to ~ 10 (Pd) This converts a forbidden reaction to allowed

25 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 25 Summary energetics Conclusion the atomic character of the metal can control the chemistry

26 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 26 Examine bonding to all three rows of transition metals Use MH+ as model because a positive metal is more representative of organometallic and inorganic complexes M0 usually has two electrons in ns orbitals or else one M+ generally has one electron in ns orbitals or else zero M2+ never has electrons in ns orbitals

27 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 27 Ground states of neutral atoms Sc(4s)2(3d) Ti(4s)2(3d)2 V(4s)2(3d)3 Cr(4s)1(3d)5 Mn(4s)2(3d)5 Fe(4s)2(3d)6 Co(4s)2(3d)7 Ni(4s)2(3d)8 Cu(4s)1(3d)10 Sc ++ (3d)1 Ti ++ (3d)2 V ++ (3d)3 Cr ++ (3d)4 Mn ++ (3d)5 Fe ++ (3d)6 Co ++ (3d)7 Ni ++ (3d)8 Cu ++ (3d)10 Sc + (4s)1(3d)1 Ti + (4s)1(3d)2 V+V+ (4s)0(3d)3 Cr + (4s)0(3d)5 Mn + (4s)1(3d)5 Fe + (4s)1(3d)6 Co + (4s)0(3d)7 Ni + (4s)0(3d)8 Cu + (4s)0(3d)10

28 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 28 Bond energies MH+ Cr Mo Re Ag Cu Au

29 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 29 Exchange energies: Get 6*5/2=15 exchange terms 5Ksd + 10 Kdd Responsible for Hund’s rule Ksd Kdd Mn+4.819.8 Tc+8.315.3 Re+11.914.1 kcal/mol Form bond to H, must lose half the exchange stabilization for the orbital bonded to the H A [(d 1  )(d 2  )(d 3  )(d 4  )(d 5  )(s  )] Mn+: s 1 d 5 For high spin (S=3) A {(d 1  )(d 2  )(d 3  )(d 4  )(sd b  )[(sd b )H+H(sd b )](  )} sd b is  half the time and  half the time

30 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 30 Ground state of M + metals Mostly s1dn-1 Exceptions: 1 st row: V, Cr-Cu 2 nd row: Nb-Mo, Ru-Ag 3 rd row: La, Pt, Au

31 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 31 Size of atomic orbitals, M + Valence s similar for all three rows, 5s biggest Big decrease from La(an 57) to Hf(an 72 Valence d very small for 3d

32 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 32 Charge transfer in MH + bonds electropositive electronegative 1 st row all electropositive 2 nd row: Ru,Rh,Pd electronegative 3 rd row: Pt, Au, Hg electronegative

33 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 33

34 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 34

35 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 35

36 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 36

37 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 37 1 st row

38 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 38

39 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 39 Schilling

40 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 40 Steigerwald

41 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 41

42 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 42

43 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 43 2 nd row

44 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 44

45 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 45

46 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 46

47 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 47

48 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 48

49 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 49

50 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 50 3 rd row

51 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 51

52 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 52

53 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 53

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55 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 55

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57 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 57

58 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 58

59 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 59

60 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 60

61 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 61

62 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 62

63 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 63 Physics behind Woodward-Hoffman Rules For a reaction to be allowed, the number of bonds must be conserved. Consider H 2 + D 2 2 bondsTS ? bonds2 bonds Bonding 2 elect nonbonding 1 elect antibonding 0 elect Have 3 electrons, 3 MO’s Have 1 bond. Next consider 4 th atom, can we get 2 bonds? To be allowed must have 2 bonds at TS How assess number of bonds at the TS. What do the dots mean? Consider first the fragment

64 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 64 Can we have 2s + 2s reactions for transition metals? 2s + 2s forbidden for organics X Cl 2 Ti ?? 2s + 2s forbidden for organometallics? Cl 2 Ti Me

65 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 65 Physics behind Woodward-Hoffman Rules Bonding 2 elect nonbonding 1 elect antibonding 0 elect Have 1 bond. Question, when add 4 th atom, can we get 2 bonds? Can it bond to the nonbonding orbital? Answer: NO. The two orbitals are orthogonal in the TS, thus the reaction is forbidden

66 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 66 Now consider a TM case: Cl 2 TiH + + D 2 Orbitals of reactants GVB orbitals of TiH bond for Cl 2 TiH + GVB orbitals of D 2

67 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 67 Is Cl 2 TiH + + D 2  Cl 2 TiD + + HD allowed? Bonding 2 elect nonbonding 1 elect antibonding 0 elect when add Ti 4 th atom, can we get 2 bonds? Answer: YES. The two orbitals can have high overlap at the TS orthogonal in the TS, thus the reaction is allowed Now the bonding orbital on Ti is d-like. Thus at TS have

68 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 68 GVB orbitals at the TS for Cl 2 TiH + + D 2  Cl 2 TiD + + HD

69 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 69 GVB orbitals for the Cl 2 TiD + + HD product Note get phase change for both orbitals

70 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 70 Follow the D2 bond as it evolves into the HD bond

71 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 71 Follow the TiH bond as it evolves into the TiD bond

72 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 72 Barriers small, thus allowed Increased d character in bond  smaller barrier

73 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 73 Are all MH reactions with D2 allowed? No Example: ClMn-H + D2 Here the Mn-Cl bond is very polar Mn(4s-4p z ) lobe orbital with Cl:3pz This leaves the Mn: (3d) 5 (4s+4pz), S=3 state to bond to the H But spin pairing to a d orbital would lose 4*K dd /2+K sd /2= (40+2.5) = 42.5 kcal/mol whereas bonding to the (4s+4pz) orbital loses 5*K sd /2 = 12.5 kcal/mol As a result the H bonds to (4s+4pz), leaving a high spin d5. Now the exchange reaction is forbidden

74 © copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 74 Show reaction for ClMnH + D2 Show example reactions

75 © copyright 2010 William A. Goddard III, all rights reservedCh120a-Goddard-L21 75 Olefin Metathesis Diego Benitez, Ekaterina Tkatchouk, Sheng Ding 2+2 metal-carbocycle reactions

76 © copyright 2010 William A. Goddard III, all rights reservedCh120a-Goddard-L21 76 Mechanism: actual catalyst is a metal-alkylidene Catalytically make and break double bonds! OLEFIN METATHESIS

77 © copyright 2010 William A. Goddard III, all rights reservedCh120a-Goddard-L21 77 Ru Olefin Metathesis Basics

78 © copyright 2010 William A. Goddard III, all rights reservedCh120a-Goddard-L21 78 Common Olefin Metathesis Catalysts

79 © copyright 2010 William A. Goddard III, all rights reservedCh120a-Goddard-L21 79 Applications of the olefin metathesis reaction Acc. Chem. Res. 2001, 34, 18-29 http://www.pslc.ws/macrog/pdcpd.htm bulletproof resin Small scale synthesis to industrial polymers

80 © copyright 2010 William A. Goddard III, all rights reservedCh120a-Goddard-L21 80 History of Olefin Metathesis Catalysts

81 Ch120-L20 13/11/02 GODDARD 81 Well-defined metathesis catalysts Schrock 1991 alkoxy imido molybdenum complex a Bazan, G. C.; Oskam, J. H.; Cho, H. N.; Park, L. Y.; Schrock, R. R. J. Am. Chem. Soc. 1991, 113, 6899-6907 Grubbs 1991 ruthenium benzylidene complex b Grubbs 1999 1,3-dimesityl-imidazole-2-ylidenes P(Cy) 3 mixed ligand system” c Scholl, M.; Trnka, T. M.; Morgan, J. P.; Grubbs, R. H. Tetrahedron Lett. 1999, 40, 2247-2250. Wagener, K. B.; Boncella, J. M.; Nel, J. G. Macromolecules 1991, 24, 2649-2657

82 © copyright 2010 William A. Goddard III, all rights reservedCh120a-Goddard-L21 82 Examples 2 nd Generation Grubbs Metathesis Catalysts General mechanism of Metathesis

83 © copyright 2010 William A. Goddard III, all rights reservedCh120a-Goddard-L21 83 Schrock and Grubbs catalysts make olefin metathesis practical Schrock catalyst – very active, but destroys many functional groups Grubbs catalyst – very stable, high functional group tolerance, but not as reactive as Schrock Catalysts contain many years of evolutionary improvements


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