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ChE 553 Lecture 29 Catalysis By Metals 1

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ChE 553 Lecture 29. Catalysis By Metals. Objective. Apply what we have learned to reactions on metal surfaces. Metals Work By Same Mechanisms As Other Catalysts. Metal catalysts can help initiate reactions Metal catalysts can stabilize the intermediates of a reaction - PowerPoint PPT Presentation

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Page 1: ChE 553 Lecture 29

ChE 553 Lecture 29Catalysis By Metals

1

Page 2: ChE 553 Lecture 29

Objective

• Apply what we have learned to reactions on metal surfaces

2

Page 3: ChE 553 Lecture 29

Metals Work By Same Mechanisms As Other Catalysts

• Metal catalysts can help initiate reactions• Metal catalysts can stabilize the intermediates of a

reaction• Metal catalysts can hold the reactants in close

proximity and in the right configuration to react• Metal catalysts can be designed to block side

reactions• Metal catalysts can stretch bonds and otherwise

make bonds easier to break• Metal catalysts can donate and accept electrons• Metal catalysts can act as efficient means for

energy transfer

3

Page 4: ChE 553 Lecture 29

Mechanisms Of Reactions On Metals

• Generally metal catalyzed reactions follow catalytic cycle with adsorbtion, reaction, desorption

• Form adsorbed radicals

• Radicals react

• Molecules desorb

4

Page 5: ChE 553 Lecture 29

Typical Reactions On Metals

• Simple molecular adsorption reactions

• Dissociative adsorption reactions

• Bond scission reactions

• Addition reactions

• Recombination reactions

• Desorption reactions

5

Page 6: ChE 553 Lecture 29

Adsorption On Metals

• Molecular Adsorption

CO + S COad

• Dissociative adsorption– oxidative addition

H2 + 2S 2Had

6

Page 7: ChE 553 Lecture 29

Molecular vs Dissociative Adsorption

7

2

2 2

DissociativeAdsorption

MolecularAdsorption

NoAdsorption

Molecular And

DissociativeAdsorption

ActivatedDissociativeAdsorption

LimitedData

PtIrOsRe

PdRhRu

NiCo

AuPt

AgPd

CuNi

Ir

Ni

AuPtIrOsRe

AgPdRhRu

CuNi

Sc Ti V Cr Mn Fe

Y Zr Nb Mo Tc

La Hf Ta W

CO300 K

Dissociated

Molecular

Sc Ti V Cr Mn Fe

Y Zr Nb Mo Tc

La Hf Ta W

N

Dissociated Molecular

Ti V Cr Mn Fe Co

Zr Nb Mo Tc Ru

Hf Ta W Re

NO300 K

Dissociated Molecular

Sc

Y

La

Rh

Os

Sc Ti V Cr Mn

Y Zr Nb Mo Tc

La Hf Ta W

NO100 K

Dissociated

Sc Ti V Cr Mn Fe

Y Zr Nb Mo Tc

La Hf Ta W

300 K

Dissociated Activated

Sc Ti V Cr Mn Fe Co Ni Cu

Y Zr Nb Mo Tc Ru Rh Pd Ag

La Hf Ta W Re Os Ir Pt

O

300 K

Dissociated

O

100 KAu

Key

AuPt

AgPd

Cu

IrOsRe

RhRu

Co

Fe Co

Molecular

Au

Ag

Cu

AuPtIrOsRe

Ag

CuNiCo

PdRhRu

Figure 5.12 The metals which dissociate CO, NO, H2, O2

and CO at various temperatures.

Page 8: ChE 553 Lecture 29

Bond Fragmentation Reactions

CH3CH2OH(ad) + S CH3CH2O(ad) +H(ad) CH3CH3O(ad) + S CH3CHO(ad) + H(ad) CH3CHO(ad) + S CH3CO(ad) + H(ad) CH3CO(ad) + S CO(ad) + CH3(ad)

(14.4)

CH3CH2CO(ad) + S CH3CH2(ad) + CO(ad) (14.5)

8

Page 9: ChE 553 Lecture 29

Association Reactions

CH3CH2(ad) + CO(ad) CH3CH2CO(ad) + S (14.6)

Combined displacement-association reactions

CO + CH3CH2(ad) + CO(ad) CO(ad) + CH3CH2CO(ad)

(14.7)

9

Page 10: ChE 553 Lecture 29

Reactions Continued Hydrogen migration

CH2CH2(ad) + H(ad) CH3CH2(ad) + S (14.8)

Molecular desorption:

CO(ad) CO + S (14.9)

10

Page 11: ChE 553 Lecture 29

Recombinative Desorption (Reductive Elimination)

CH3CH2(ad) + H(ad) CH3CH3 + 2S

(14.10)

2H(ad) H2 + 2S (14.11)

11

Page 12: ChE 553 Lecture 29

Displacement Reaction

CH3CH2(ad) + H2 CH3CH3 + H(ad) (14.12)

CO + 2 H(ad) H2 +CO(ad)

(14.13)

CO + CH2CH3(ad) + H(ad) CH3CH3 + CO(ad)

(14.14)

12

Page 13: ChE 553 Lecture 29

-scission

 

R2CDCH2(ad) R2C=CH2 + D(ad)

(14.15)

13

Page 14: ChE 553 Lecture 29

Example Catalytic Mechanisms: Olefin Hydrogenation

14

HH

H

H CC H

H

HH

H

C CH

H H

HH

HC

H

CHH

HH

HH

HH

HC

H

CHH

HH

C

H

CHH

HH

H

H

C C

HH H

Page 15: ChE 553 Lecture 29

Principles Of Catalytic Reaction

• Metals can help initiate reactions• Metals can stabilize the intermediates

of a reaction• Metals can hold the reactants in close

proximity and in the right configuration to react

• Metals can stretch bonds and otherwise make bonds easier to break

• Metals can donate and accept electrons

15

Page 16: ChE 553 Lecture 29

Mechanism On Surface Similar To Radical Reactions In Gas Phase – But Radicals Bound To Surface

16

X + H H X

X O 2O XO H OH H

H OH H O H

H O OH + O

X 2H H X

2

2

2

2 2

2

2

2

(5.152)

H S H

O 2S 2OO H OH H

2O H 2OH

O H OH

2OH H O O

H OH H O

H 2S 2H

2 (ad)

2 (ad)

(ad) 2 (ad) (ad)

(ad) 2 (ad)

(ad) (ad) (ad)

(ad) 2 (ad)

(ad) (ad) 2

2 (ad)

2

(5.153)

Page 17: ChE 553 Lecture 29

Electrons In Metals Solvate Radicals

• Metals are solvents for radicals. They lower the energy of radical species which allows initiation-propagation reactions to occur.

• Adsorbed radicals have lower energies than gas phase radicals which leads to higher concentrations.

• Intrinsic barriers of species adsorbed on metals similar to gas phase radicals.

17

Page 18: ChE 553 Lecture 29

Electrons In Metals Solvate Radicals

18

s

Distance normal to the surface (bohr)

Sca

led

Ele

ctro

n D

ensi

ty

0.0

-0.5

1.0

= 2 (Al)

-20 0-10 100.0

-0.5

1.0

Abs

olut

e E

lect

ron

Den

sity

-20 0-10 10

Distance normal to the surface (bohr)

r s = 5 (Cs)rKey: = Positive Charge

Figure 14.18 The electron density extending out from a metal surface. (Note 1 bohr =0.52Å)

Page 19: ChE 553 Lecture 29

Metals Stabilize Intermediates

19

C

H

CHH

C

H

CHH

H H H H H H H HC

H

CHH

HH

C

H

CH H

HH

C

H

CHH

H

Page 20: ChE 553 Lecture 29

Multiple Radicals

One key difference between gas phase and surface is that di & tri radicals are stable on metals

N Gives possibilities

for interesting chemistry

20

Page 21: ChE 553 Lecture 29

Metals Initiate Reactions

21

2

2 2

DissociativeAdsorption

MolecularAdsorption

NoAdsorption

Molecular And

DissociativeAdsorption

ActivatedDissociativeAdsorption

LimitedData

PtIrOsRe

PdRhRu

NiCo

AuPt

AgPd

CuNi

Ir

Ni

AuPtIrOsRe

AgPdRhRu

CuNi

Sc Ti V Cr Mn Fe

Y Zr Nb Mo Tc

La Hf Ta W

CO300 K

Dissociated

Molecular

Sc Ti V Cr Mn Fe

Y Zr Nb Mo Tc

La Hf Ta W

N

Dissociated Molecular

Ti V Cr Mn Fe Co

Zr Nb Mo Tc Ru

Hf Ta W Re

NO300 K

Dissociated Molecular

Sc

Y

La

Rh

Os

Sc Ti V Cr Mn

Y Zr Nb Mo Tc

La Hf Ta W

NO100 K

Dissociated

Sc Ti V Cr Mn Fe

Y Zr Nb Mo Tc

La Hf Ta W

300 K

Dissociated Activated

Sc Ti V Cr Mn Fe Co Ni Cu

Y Zr Nb Mo Tc Ru Rh Pd Ag

La Hf Ta W Re Os Ir Pt

O

300 K

Dissociated

O

100 KAu

Key

AuPt

AgPd

Cu

IrOsRe

RhRu

Co

Fe Co

Molecular

Au

Ag

Cu

AuPtIrOsRe

Ag

CuNiCo

PdRhRu

Figure 5.12 The metals which dissociate CO, NO, H2, O2

and CO at various temperatures.

Page 22: ChE 553 Lecture 29

D-bands Help Tear Bonds Apart

22

Figure 12.20 A diagram of the key interactions during the dissociation of hydrogen on platinum.

Page 23: ChE 553 Lecture 29

Activation Energy For H2 Dissociation

Metal Heat of dissociative adsorption of H2

Intrinsic barrier for dissociative adsorption of H2

Pt -13 kcal/mole <6 kcal/mole

Si -54 kcal/mole ~80 kcal/mole

Al ~-70 kcal/mole >90 kcal/mole

K ~-70 kcal/mole >90 kcal/mole 23

H SH - H/ \S - S

H H| |

S - S2 2

Page 24: ChE 553 Lecture 29

Redox Chemistry

24

Co + C H CH Co + H + C HHCH

3+6 5 3

2+ +6 5

(14.53)

C HHCH

O C HHCH

OO6 5 2 6 5

(14.54)

C HHCH

OO Co C HHC O Co OH6 5

26 5

3

(14.55)

OH H H O- +2

(14.56)

OH + H H O- +2

(14.57)

Page 25: ChE 553 Lecture 29

Metals Hold Reactants In Correct Configuration To React

25

CC O

H HH

HH

H

**

CC OH H

H

HH

H

**

A B

Figure 14.20 Balandin's suggested multiplet for the decomposition of ethanol a) to form ethylene b)to form acetyladehyde. The asterisks in the figures represent places on the surface where reaction can occur.

Page 26: ChE 553 Lecture 29

Metals Hold The Reactants In The Correct Configuration To React

26

C

C

C

C

CC

3C2H2 C6H6

Figure 12.15 The active site for reaction (12.91) on a palladium catalyst.

(12.91)

Page 27: ChE 553 Lecture 29

Structure Sensitive Reactants

27

1000

500

100 10

30

5010 -11

10 -9

10 -7

10 -5

10 -3

10 -1

10 1

10 3

10 5

10 7

10 9

Act

ivat

on E

nerg

y F

or N

O D

isso

ciat

ion

(kca

l/mol

e)

Dis

soci

atio

n T

empe

ratu

re (

íK)

% D

isso

ciat

ion

In T

PD

Cal

cula

ted

Orb

ital

Ava

ilab

ilit

y

Tur

nove

r N

umbe

r E

xtra

pola

ted

To

400í

K (

sec

-1)

(111

)

(110

)

(210

)

(410

)

(100

)

(111

)

Face

Orbital Availability

% Dissociation

Dissociation Temperature

EA For NO Dissociation

Rate Constant For NO Dissociation

2

1

100

50

Figure 14.22 The rate of nitric oxide dissociation on several of the faces of platinum along the principle zone axes of the stereographic triangle. Adapted from Masel[1983].

Page 28: ChE 553 Lecture 29

Structure Sensitive Reactions

28

140120100806040200

0.001

0.01

0.1

1

10

100

300

Particle Size,

Rat

e (m

olec

ules

/sit

e/se

c) o

A

Ao

  

Figure 14.21 The rate of the reaction

N2 + 3H2 2NH3

over an iron catalyst as a function of size of the iron particles in the catalyst. Data of Boudart et al [1975]

Page 29: ChE 553 Lecture 29

Different Reactions Show Different Structure Sensitivity

29

Reaction Largest variation in

rate with geometry observed prior to

1999

2CO+O2 2CO2 6

C2H4+H2 C2H6 12

CH3OH CH2(ad)+H2O >100

C2H6+H2 2CH4 104

N2+3H2 2NH3 105

2NO+2H2 N2+2H2O ~1021

Page 30: ChE 553 Lecture 29

Practical Catalysts Are Supported Structures With Multiple Exposed Faces

30

Figure 12.4 A picture of a supported metal catalyst.

step

kink

adatom

Page 31: ChE 553 Lecture 29

Summary

• Metals can help initiate reactions - in particular they facilitate bond scission processes

• Metals can stabilize the intermediates of a reaction particularly radical intermediates

• Metals can lower the intrinsic barriers to bond scission. The d-electrons promote bond scission and bond formation. The s-electrons promote redox chemistry.

• D’s convert forbidden reactions to allowed reactions. Produces tremendous rate enhancements.

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