Lecture 19 February 16, 2011 Transition metals:Pd and Pt Nature of the Chemical Bond with applications to catalysis, materials science, nanotechnology, surface science, bioinorganic chemistry, and energy William A. Goddard, III, wag@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 <cescott@caltech.edu> Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 1 Last time Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 2 Compare chemistry of column 10 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 3 Ground state of group 10 column Pt: (5d)9(6s)1 3D ground state Pt: (5d)10(6s)0 1S excited state at 11.0 kcal/mol Pt: (5d)8(6s)2 3F excited state at 14.7 kcal/mol Ni: (5d)8(6s)2 3F ground state Ni: (5d)9(6s)1 3D excited state at 0.7 kcal/mol Ni: (5d)10(6s)0 1S excited state at 40.0 kcal/mol Pd: (5d)10(6s)0 1S ground state Pd: (5d)9(6s)1 3D excited state at 21.9 kcal/mol Pd:Ch120a-Goddard-L19 (5d)8(6s)2 3F excited state atWilliam 77.9A. Goddard kcal/mol © copyright 2011 III, all rights reserved 4 Salient differences between Ni, Pd, Pt Ni Pd Pt 2nd row (Pd): 4d much more stable than 5s Pd d10 ground state 3rd row (Pt): 5d and 6s comparable stability Pt d9s1 ground state 5s much less stable than 4d 6s, 5d similar stability Differential shielding favors Relativistic effects of 1s 3d much smaller than 4s n=4 over n=5, (No 3d Pauli orthogonality) huge decreased KE 10 stabilize 4d over 5s d Huge e-e repulsion for d10 contraction stabilize 4d similar size to 5s and contract all ns 5 Ch120a-Goddard-L19 © copyright 2011 reservedand expand nd (orthog to William 3d,4s A. Goddard III, all rights destabilize 4s more stable than 3d 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? © copyright 2011 William A. Goddard III, all rights reserved Ch120a-Goddard-L19 6 Step 1: examine GVB orbitals for (PH3)2Pt(CH3) Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 7 Analysis of GVB wavefunction Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 8 Alternative models for Pt centers Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 9 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 10 energetics Ch120a-Goddard-L19 Not agree with experiment 11 © copyright 2011 William A. Goddard III, all rights reserved Possible explanation: kinetics Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 12 Consider reductive elimination of HH, CH and CC from Pd Conclusion: HH no barrier CH modest barrier CC large barrier Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 13 Consider oxidative addition of HH, CH, and CC to Pt Ch120a-Goddard-L19 Conclusion: HH no barrier CH modest barrier CCreserved large barrier 14 © copyright 2011 William A. Goddard III, all rights Summary of barriers This explains why CC coupling not occur for Pt while CH and HHcoupling is fast But why? Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 15 How estimate the size of barriers (without calculations) Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 16 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 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 17 Examine CC coupling at transition state Can orient the CH3 to obtain good overlap with Pd sd hybrid OR can orient the CH3 to obtain get good overlap with the other CH3 But CANNOT DO BOTH SIMULTANEOUSLY, thus do NOT get 18 resonance© stabilization ofA. TS III,high barier Ch120a-Goddard-L19 copyright 2011 William Goddard all rights reserved Examine CH coupling at transition state Ch120a-Goddard-L19 H can overlap both CH3 and Pd sd hybrid simultaneously but CH3 cannot thus get ~ ½ resonance stabilization of TS 19 © copyright 2011 William A. Goddard III, all rights reserved Now we understand Pt chemistry But what about Pd? Why are Pt and Pd so dramatically different Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 20 new Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 21 Pt goes from s1d9 to d10 upon reductive elimination thus product stability is DECREASED by 12 kcal/mol Using numbers from QM Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 22 Pd goes from s1d9 to d10 upon reductive elimination thus product stability is INCREASED by 20 kcal/mol Using numbers from QM Pd and Pt would be ~ same Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 23 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 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 24 Summary energetics Conclusion the atomic character of the metal can control the chemistry Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 25 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 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 26 Ground states of neutral atoms Sc (4s)2(3d) Sc+ (4s)1(3d)1 Ti (4s)2(3d)2 Ti+ (4s)1(3d)2 V (4s)2(3d)3 V+ (4s)0(3d)3 Cr (4s)1(3d)5 Cr+ (4s)0(3d)5 Mn (4s)2(3d)5 Mn+ (4s)1(3d)5 Fe (4s)2(3d)6 Fe+ (4s)1(3d)6 Co (4s)2(3d)7 Co+ (4s)0(3d)7 Ni (4s)2(3d)8 Ni+ (4s)0(3d)8 Cu (4s)1(3d)10 Cu+ Ch120a-Goddard-L19 (4s)0(3d)10 Sc++ Ti ++ V ++ Cr ++ Mn ++ Fe ++ Co ++ Ni ++ Cu++ © copyright 2011 William A. Goddard III, all rights reserved (3d)1 (3d)2 (3d)3 (3d)4 (3d)5 (3d)6 (3d)7 (3d)8 (3d)10 27 Bond energies MH+ Re Mo Au Cr Cu Ag Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 28 Exchange energies: Mn+: s1d5 For high spin (S=3) A[(d1a)(d2a)(d3a)(d4a)(d5a)(sa)] Get 6*5/2=15 exchange terms 5Ksd + 10 Kdd Responsible for Hund’s rule Ksd Kdd Mn+ 4.8 19.8 kcal/mol Tc+ 8.3 15.3 Re+ 11.9 14.1 Form bond to H, must lose half the exchange stabilization for the orbital bonded to the H A{(d1a)(d2a)(d3a)(d4a)(sdba)[(sdb)H+H(sdb)](ab-ba)} sdb is a half the time and b half the time Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 29 Ground state of M+ metals Mostly s1dn-1 Exceptions: 1st row: V, Cr-Cu 2nd row: Nb-Mo, Ru-Ag 3rd row: La, Pt, Au Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 30 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 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 31 Charge transfer in MH+ bonds electropositive 1st row all electropositive 2nd row: Ru,Rh,Pd electronegative 3rd row: Pt, Au, Hg electronegative electronegative Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 32 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 33 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 34 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 35 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 36 1st row Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 37 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 38 Schilling Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 39 Steigerwald Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 40 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 41 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 42 2nd row Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 43 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 44 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 45 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 46 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 47 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 48 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 49 3rd row Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 50 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 51 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 52 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 53 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 54 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 55 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 56 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 57 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 58 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 59 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 60 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 61 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 62 Physics behind Woodward-Hoffman Rules For a reaction to be allowed, the number of bonds must be conserved. Consider H2 + D2 2 bonds TS ? bonds 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 Have 3 electrons, 3 MO’s Have 1 bond. Next consider 4th atom, can nonbonding Bonding antibonding we Ch120a-Goddard-L19 get 2 bonds? 1 elect 2 2011 elect © copyright William A. Goddard III, all rights reserved 0 elect 63 Can we have 2s + 2s reactions for transition metals? 2s + 2s forbidden for organics X 2s + 2s forbidden for organometallics? ? Cl2Ti Cl2Ti Me Me Ch120a-Goddard-L19 Cl2Ti Cl2Ti Me ? Me Cl2Ti Cl2Ti Me © copyright 2011 William A. Goddard III, all rights reserved Me 64 Physics behind Woodward-Hoffman Rules Bonding 2 elect nonbonding 1 elect antibonding 0 elect Have 1 bond. Question, when add 4th 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 65 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved Now consider a TM case: Cl2TiH+ + D2 Orbitals of reactants GVB orbitals of TiH bond for Cl2TiH+ GVB orbitals of D2 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 66 Is Cl2TiH+ + D2 Cl2TiD+ + HD allowed? Bonding 2 elect nonbonding 1 elect antibonding 0 elect when add Ti 4th atom, can we get 2 bonds? Now the bonding orbital on Ti is d-like. Thus at TS have Answer: YES. The two orbitals can have high overlap at the TS orthogonal in the TS,©thus the reaction is allowed Ch120a-Goddard-L19 copyright 2011 William A. Goddard III, all rights reserved 67 GVB orbitals at the TS for Cl2TiH+ + D2 Cl2TiD+ + HD Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 68 GVB orbitals for the Cl2TiD+ + HD product Note get phase change for both orbitals Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 69 Follow the D2 bond as it evolves into the HD bond Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 70 Follow the TiH bond as it evolves into the TiD bond Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 71 Barriers small, thus allowed Increased d character in bond smaller barrier Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 72 Are all MH reactions with D2 allowed? No Example: ClMn-H + D2 Here the Mn-Cl bond is very polar Mn(4s-4pz) 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*Kdd/2+Ksd/2= (40+2.5) = 42.5 kcal/mol whereas bonding to the (4s+4pz) orbital loses 5*Ksd/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 Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 73 Show reaction for ClMnH + D2 Show example reactions Ch120a-Goddard-L19 © copyright 2011 William A. Goddard III, all rights reserved 74 Olefin Metathesis 2+2 metal-carbocycle reactions Diego Benitez, Ekaterina Tkatchouk, Sheng Ding Ch120a-Goddard-L21 © copyright 2010 William A. Goddard III, all rights reserved 75 OLEFIN METATHESIS Catalytically make and break double bonds! R1 R1 + R2 2 R2 R1 R2 Mechanism: actual catalyst is a metal-alkylidene R2 M R1 Ch120a-Goddard-L21 R2 R2 M M R3 R1 R3 R1 R3 © copyright 2010 William A. Goddard III, all rights reserved 76 Ru Olefin Metathesis Basics Ch120a-Goddard-L21 © copyright 2010 William A. Goddard III, all rights reserved 77 Common Olefin Metathesis Catalysts Ch120a-Goddard-L21 © copyright 2010 William A. Goddard III, all rights reserved 78 Applications of the olefin metathesis reaction Small scale synthesis to industrial polymers Acc. Chem. Res. 2001, 34, 18-29 Ch120a-Goddard-L21 bulletproof resin http://www.pslc.ws/macrog/pdcpd.htm 79 © copyright 2010 William A. Goddard III, all rights reserved History of Olefin Metathesis Catalysts Ch120a-Goddard-L21 © copyright 2010 William A. Goddard III, all rights reserved 80 Well-defined metathesis catalysts R iPr N (F3C)2MeCO Mo (F3C)2MeCO Cl PCy3 Ph Ru Cl PCy3 iPr Ph CH 3 CH 3 Bazan, G. C.; Oskam, J. H.; Cho, H. N.; Park, L. Y.; Schrock, R. R. J. Am. Chem. Soc. 1991, 113, 6899-6907 Cl Ru N Mes Ph PCy3 R=H, Cl 2 Grubbs 1991 ruthenium benzylidene complexb 1 Schrock 1991 alkoxy imido molybdenum complexa Mes N Cl R Wagener, K. B.; Boncella, J. M.; Nel, J. G. Macromolecules 1991, 24, 2649-2657 GODDARD 3 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. Ch120-L20 13/11/02 81 Examples of Common Second Generation Examples 2nd Generation Grubbs Metathesis Grubbs-type Catalysts Metathesis Catalysts and Mechanism Overview Mes N N Mes Cl Mes N Ru Cl PCy3 N Mes Cl Mes N Ru Cl Ph Ru O Cl i-Pr slow initiating catalyst N Mes Cl fast-initiating catalyst Py Ph ultra-fast-initiating catalyst General mechanism of Metathesis IMes Ru Cl Cl Ph L IMes Cl Ru Cl IMes Cl Ru R3 R1 L R2 Initiation R Cl IMes IMes Cl R Ru Cl R3 R2 Cl Propagation Ru Cl R3 + R1 R2 Ch120a-Goddard-L21 © copyright 2010 William A. Goddard III, all rights reserved 82 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 Ch120a-Goddard-L21 © copyright 2010 William A. Goddard III, all rights reserved 83