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© copyright 2011 William A. Goddard III, all rights reserved Ch120a-Goddard-L19 Ch120a- Goddard- 1 Nature of the Chemical Bond with applications to catalysis, materials science, nanotechnology, surface science, bioinorganic chemistry, and energy William A. Goddard, III, [email protected] 316 Beckman Institute, x3093 Charles and Mary Ferkel Professor of Chemistry, Materials Science, and Applied Physics, California Institute of Technology Teaching Assistants: Caitlin Scott < [email protected] > Hai Xiao [email protected] ; Fan Liu Lecture 13 February 1, 2011 Pd and Pt, MH + bonding, metathesis Course number: Ch120a Hours: 2-3pm Monday, Wednesday, Friday
Transcript

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 Ch120a-Goddard-

L01

1

Nature of the Chemical Bond with applications to catalysis, materials

science, nanotechnology, surface science, bioinorganic chemistry, and energy

William A. Goddard, III, [email protected] Beckman Institute, x3093

Charles and Mary Ferkel Professor of Chemistry, Materials Science, and Applied Physics,

California Institute of Technology

Teaching Assistants: Caitlin Scott <[email protected]>Hai Xiao [email protected]; Fan Liu <[email protected]>

Lecture 13 February 1, 2011

Pd and Pt, MH+ bonding, metathesis

Course number: Ch120aHours: 2-3pm Monday, Wednesday, Friday

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

Last time

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

Compare chemistry of column 10

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 4

Ground state of group 10 column

Pt: (5d)9(6s)1 3D ground statePt: (5d)10(6s)0 1S excited state at 11.0 kcal/molPt: (5d)8(6s)2 3F excited state at 14.7 kcal/mol

Pd: (5d)10(6s)0 1S ground statePd: (5d)9(6s)1 3D excited state at 21.9 kcal/molPd: (5d)8(6s)2 3F excited state at 77.9 kcal/mol

Ni: (5d)8(6s)2 3F ground stateNi: (5d)9(6s)1 3D excited state at 0.7 kcal/molNi: (5d)10(6s)0 1S excited state at 40.0 kcal/mol

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 5

Salient differences between Ni, Pd, Pt

Ni Pd 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 d10

4d similar size to 5s (orthog to 3d,4s

Differential shielding favors n=4 over n=5,

stabilize 4d over 5s d10

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

Relativistic effects of 1s huge decreased KE contraction stabilize and contract all ns destabilize and expand nd

© 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?

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 7

Step 1: examine GVB orbitals for (PH3)2Pt(CH3)

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 8

Analysis of GVB wavefunction

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 9

Alternative models for Pt centers

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

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 11

energetics

Not agree with experiment

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 12

Possible explanation: kinetics

© 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 barrierCC large barrier

© 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 barrierCC large barrier

© 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

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 16

How estimate the size of barriers (without calculations)

© 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

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 18

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 resonance stabilization of TS high barier

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 19

Examine CH coupling at transition state

H can overlap both CH3 and Pd

sd hybrid simultaneously but CH3 cannot

thus get ~ ½ resonance

stabilization of TS

© 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

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

new

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 22

Pt goes from s1d9 to d10 upon reductive eliminationthus product stability is DECREASED by 12 kcal/mol

Using numbers from QM

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 23

Ground state configurations for column 10

Ni Pd Pt

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 24

Pd goes from s1d9 to d10 upon reductive eliminationthus product stability is INCREASED by 20 kcal/mol

Using numbers from QM

Pd and Pt would be ~ same

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 25

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

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 26

Summary energetics

Conclusion the atomic character of the metal can

control the chemistry

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 27

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

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 28

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+ (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

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 29

Bond energies MH+

Cr

Mo

Re

Ag

Cu

Au

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 30

Exchange energies:

Get 6*5/2=15 exchange terms5Ksd + 10 KddResponsible for Hund’s rule

Ksd KddMn+ 4.8 19.8 Tc+ 8.3 15.3Re+ 11.9 14.1

kcal/mol

Form bond to H, must lose half the exchange stabilization for the orbital bonded to the H

A[(d1a)(d2a)(d3a)(d4a)(d5a)(sa)]

Mn+: s1d5

For high spin (S=3)

A{(d1a)(d2a)(d3a)(d4a)(sdba)[(sdb)H+H(sdb)]( -ab ba)}

sdb is a half the time and b half the time

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 31

Ground state of M+ metals

Mostly s1dn-1Exceptions:1st row: V, Cr-Cu2nd row: Nb-Mo, Ru-Ag3rd row: La, Pt, Au

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 32

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

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

Charge transfer in MH+ bonds

electropositive

electronegative

1st row all electropositive

2nd row: Ru,Rh,Pd

electronegative3rd row:

Pt, Au, Hg electronegative

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

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

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

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

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

1st row

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

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

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

Steigerwald

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

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

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

2nd row

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

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

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

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

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

3rd row

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

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

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 54

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

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© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 64

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

Bonding2 elect

nonbonding1 elect

antibonding0 elect

Have 3 electrons, 3 MO’s

Have 1 bond. Next consider 4th atom, can we get 2 bonds?

To be allowed must have 2 bonds at TSHow assess number of bonds at the TS. What do the dots mean? Consider first the fragment

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 65

Can we have 2s + 2s reactions for transition metals?

2s + 2s forbidden for organics

X

Cl2Ti Cl2Ti Cl2Ti? ?

2s + 2s forbidden for organometallics?

Cl2Ti Cl2Ti Cl2TiMe

Me

Me

Me

Me

Me

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 66

Physics behind Woodward-Hoffman Rules

Bonding2 elect

nonbonding1 elect

antibonding0 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

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 67

Now consider a TM case: Cl2TiH+ + D2

Orbitals of reactants

GVB orbitals of TiH bond for Cl2TiH+

GVB orbitals of D2

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 68

Is Cl2TiH+ + D2 Cl2TiD+ + HD allowed?

Bonding2 elect

nonbonding1 elect

antibonding0 elect

when add Ti 4th 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

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 69

GVB orbitals at the TS for Cl2TiH+ + D2 Cl2TiD+ + HD

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 70

GVB orbitals for the Cl2TiD+ + HD product

Note get phase change for both orbitals

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 71

Follow the D2 bond as it

evolves into the HD bond

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 72

Follow the TiH bond as it

evolves into the TiD bond

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 73

Barriers small, thus allowed

Increased d character in bond smaller barrier

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 74

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 HBut 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

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

Thus ClMn-H bond is sp-like

ClMnH

Mn (4s)2(3d)5

The Cl pulls off 1 e from Mn, leaving a d5s1 configurationH bonds to 4s because of exchange stabilization of d5

Mn-H bond character0.07 Mnd+0.71Mnsp+1.20H

This cannot overlap the antisymmetric orbital delocalized over the three H atoms in the TSAs a result at the Transition state the MnH bond has the character of H3

- with both electrons on the H3.

This leads to a high barrier, ~45 kcal/mol

© copyright 2011 William A. Goddard III, all rights reservedCh120a-Goddard-L19 76

Show reaction for ClMnH + D2

Show example reactions

© copyright 2010 William A. Goddard III, all rights reservedCh120a-Goddard-L21 77

Olefin Metathesis

Diego Benitez, Ekaterina Tkatchouk, Sheng Ding

2+2 metal-carbocycle reactions

© copyright 2010 William A. Goddard III, all rights reservedCh120a-Goddard-L21 78

Mechanism: actual catalyst is a metal-alkylidene

R1 R1 R2 R2+

R1 R22

M

R2

R1 R3

M

R2

R1 R3

M

R2

R1 R3

Catalytically make and break double bonds!

OLEFIN METATHESIS

© copyright 2010 William A. Goddard III, all rights reservedCh120a-Goddard-L21 79

Ru Olefin Metathesis Basics

© copyright 2010 William A. Goddard III, all rights reservedCh120a-Goddard-L21 80

Common Olefin Metathesis Catalysts

© copyright 2010 William A. Goddard III, all rights reservedCh120a-Goddard-L21 81

Applications of the olefin metathesis reaction

Acc. Chem. Res. 2001, 34, 18-29

http://www.pslc.ws/macrog/pdcpd.htmbulletproof resin

Small scale synthesisto industrial polymers

© copyright 2010 William A. Goddard III, all rights reservedCh120a-Goddard-L21 82

History of Olefin Metathesis Catalysts

Ch120-L20 13/11/02GODDARD 83

Well-defined metathesis catalysts

Ru

PCy3

Ph

Cl

ClNN MesMes

Ru

PCy3

Ph

Cl

ClNN MesMes

R R

R=H, Ph, or -CH2-(CH2)2-CH2-

R R

R=H, Cl

NMo

PhCH3

CH3(F3C)2MeCO

(F3C)2MeCO

iPr iPrRuPCy3

PCy3

Ph

Cl

Cl

1 2 3 4Schrock 1991alkoxy imido molybdenum complexa

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 complexb

Grubbs 19991,3-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

© copyright 2010 William A. Goddard III, all rights reservedCh120a-Goddard-L21 84

Examples of Common Second Generation Grubbs-typeMetathesis Catalysts and Mechanism Overview

Ru

NNMes MesCl

Cl PhPCy3

Ru

NNMes MesCl

Cl PhPy

Ru

NNMes MesCl

ClO

i-Pr

slow initiating catalyst ultra-fast-initiating catalystfast-initiating catalyst

Ru

Cl

IMesCl

RLPh

IMes

Ru

LCl

Cl

Initiation

Ru

Cl

IMesCl

Cl

IMesClR

R2

Ru

R3

Ru

Cl

IMesCl

R1

PropagationR2R3

R3

R2

R1

+

Examples 2nd Generation Grubbs Metathesis Catalysts

General mechanism of Metathesis

© copyright 2010 William A. Goddard III, all rights reservedCh120a-Goddard-L21 85

Schrock and Grubbs catalysts make olefin metathesis practical

Schrock catalyst –very active, but destroysmany functional groups

Grubbs catalyst –very stable, high functionalgroup tolerance, but not asreactive as Schrock

Catalysts contain many years of evolutionary improvements


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