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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 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] WCU Professor at EEWS-KAIST and

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

California Institute of Technology

Course number: KAIST EEWS 80.502 Room E11-101 Hours: 0900-1030 Tuesday and Thursday

Senior Assistant: Dr. Hyungjun Kim: [email protected] Teaching Assistant: Ms. Ga In Lee: [email protected]

Lecture 4, September 10, 2009

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2

Last time: The nodal Theorem

E00 < E10 < E20< E21 and E00 < E01 < E11 < E21

but nodal argument does not indicate the relative energies of E10 and E20 versus E01

+

Φ00 Φ10 Φ01 Φ20 +-

+ -

+ -

+ - Φ11

+

+- + - +

+

- -

Φ21

The nodal Theorem sometimes orders excited states in 2D, 3D The ground state of a system is nodeless (more properly, the ground state never changes sign). Useful in reasoning about

wavefunctions. Implies that ground state wavefunctions for H2+ are g not u)

For one dimensional finite systems, we can order all eigenstates by the number of nodes E0 < E1 < E2 .... En < En+1

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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 3

4

th

postulate of QM

Consider the exact eigenstate of a system HΦ = EΦ

and multiply the Schrödinger equation by some

CONSTANT phase factor (independent of position and time)

exp(ia) = eia

eia HΦ = H (eia Φ) = E (eia Φ)

Thus Φ and (eia Φ) lead to identical properties and we consider them to describe exactly the same state.

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4

The Hamiltonian for H

2+

For H atom the Hamiltonian is Ĥ = - (Ћ2/2me)2 – e2/r or

Ĥ = - ½ 2 – 1/r (in atomic units)

r

Coordinates of H atom

Coordinates of H2+

For H2+ molecule the Hamiltonian (in atomic units) is Ĥ = - ½ 2 + V(r) where

1 1 1

We will rewrite this as

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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 5

The Schrödinger Equation for H

2+

The exact (electronic wavefunction of H2+ is obtained by solving Here we can ignore the 1/R term (not

depend on electron coordinates) to write where e is the electronic energy

Then the total energy E becomes

E= e + 1/R R

Since v(r) depends on R, the wavefunction φ depends on R.

Thus for each R we solve for φ and e and add to 1/R to get the total energy E(R)

E(R)

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6

Inversion Symmetry

The operation of inversion (denoted as ) through the origin of a coordinate system changes the coordinates as

x ➔ -x y ➔ -y z ➔ -z

Taking the origin of the coordinate system as the bond midpoint, inversion changes the electronic coordinates as illustrated.

I^

The identity or do-nothing operator, is called einheit. e^

Applying the inversion twice, leads to the identity

x ➔ -x ➔ x; y ➔ -y ➔ y z ➔ -z ➔ z Nothing changes!

^I

^I

^I e^

= ( )2 =

Thus The inversion operator is of order 2

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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 7

Symmetry Theorem

If h(r) is invariant under inversion: h(-r) = h(r) Then for all eigenfunctions φ(r) of h

h(r)φ(r) = eφ(r) I^

I^

φg(r) = + φg(r) φu(r) = - φu(r)

g for gerade or even u for ungerade or odd

φg(r) φu(r)

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8

Now consider symmetry for H

2

molecule

For H2 the Hamiltonian is

1/r12 interaction between 2 electrons

all terms depending only on electron i For multielectron systems, inversion, , inverts all electron

coordinates simultaneously

I^

H(1,2)Φ(1,2) = E Φ(1,2) If H(1,2) is invariant under inversion:

H(-r1,-r2) = H(r1,r2)

Then for all eigenfunctionsΦ(1,2) of H

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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 9

inversion symmetry for H

2

wavefunctions

g

g

u u

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10

Permutation Symmetry

Transposing the two electrons in H(1,2) must leave the Hamiltonian invariant since the electrons are identical

H(2,1) = h(2) + h(1) + 1/r12 + 1/R = H(1,2)

We denote transposition as t where tΦ(1,2) = Φ(2,1) Applying t twice leads to the identity t2 = e,

t2Φ(1,2) = Φ(1,2)

Thus the previous arguments on inversion apply equally to transposition

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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 11

permutational symmetry for H

2

wavefunctions

symmetric

antisymmetric

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12

Electron spin

Consider application of a magnetic field

Our hamiltonian has not no terms dependent on the magnetic field.

Hence no effect.

But experimentally there is a huge effect. Namely The ground state of H atom splits into two states

This leads to the 5th postulate of QM

In addition to the 3 spatial coordinates x,y,z each electron has

internal or spin coordinates which leads to a magnetic dipole that is either aligned with the external magnetic field or it is opposite.

We label these as a for spin up and b for spin down. Thus the ground states of H atom are φ(xyz)a(spin) and φ(xyz)b(spin)

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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 13

Spin states for 1 electron systems

Our Hamiltonian does not involve any terms dependent on the spin, so without a magnetic field we have 2 degenerate states for H atom.

φ(r)a, with up-spin, ms = +1/2 φ(r)b, with down-spin, ms = -1/2

The electron is said to have a spin anglular momentum of S=1/2 with projections along a polar axis (say the external magnetic moment) of +1/2 (spin up) or -1/2 (down spin). This explains the observed splitting of the H atom into two states in a magnetic field

Similarly for H2+ the ground state becomes φg(r)a and φg(r)b

While the excited state becomes φu(r)a and φu(r)b

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Electron spin

+½ or a or up-spin and -½ or b or down-spin

But the only external manifestation is that this spin leads to a magnetic moment that interacts with an external magnetic field to splt into two states, one more stable and the other less

stable by an equal amount.

B=0 Increasing B

a b

Now the wavefunction of an atom is written as ψ(r,s)

where r refers to the vector of 3 spatial coordinates, x,y,z while s to the internal spin coordinates

So far we have considered the electron as a point particle with mass, me, and charge, -e.

In fact the electron has internal coordinates, that we refer to as spin, with two possible angular momenta.

DE = -gBzsz

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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 15

Spinorbitals

The Hamiltonian does not depend on spin the spatial and spin coordinates are independent. Hence the wavefunction can be written as a product of

a spatial wavefunction, φ(s), called an orbital, and a spin function, х(s) = a or b.

ψ(r,s) = φ(s) х(s)

where r refers to the vector of 3 spatial coordinates, x,y,z while s to the internal spin coordinates.

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spinorbitals for two-electron systems

Thus for a two-electron system with independent electrons, the wavefunction becomes

Ψ(1,2) = Ψ(r1,s1,r2,s2) = ψa(r1,s1) ψb(r2,s2)

= φa(r1) хa(s1) φb(r2) хb(s2)

=[φa(r1) φb(r2)][хa(s1) хb(s2)]

Where the last term factors the total wavefunction into space and spin parts

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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 17

Spin states for 2-electron systems

Since each electron can have up or down spin, any two-electron system, such as H2 molecule will lead to 4 possible spin states each with the same energy

Φ(1,2) a(1) a(2) Φ(1,2) a(1) b(2) Φ(1,2) b(1) a(2) Φ(1,2) b(1) b(2)

This immediately raises an issue with permutational symmetry Since the Hamiltonian is invariant under interchange of the spin for electron 1 and the spin for electron 2, the two-electron spin functions must be symmetric or antisymmetric with respect to interchange of the spin coordinates, s1 and s2

Neither symmetric nor antisymmetric Symmetric spin

Symmetric spin

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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 18

Spin states for 2 electron systems

Combining the two-electron spin functions to form symmetric and antisymmetric combinations leads to

Φ(1,2) a(1) a(2)

Φ(1,2) [a(1) b(2) + b(1) a(2)]

Φ(1,2) b(1) b(2)

Φ(1,2) [a(1) b(2) - b(1) a(2)]

Adding the spin quantum numbers, ms, to obtain the total spin projection, MS = ms1 + ms2 leads to the numbers above.

The three symmetric spin states are considered to have spin S=1 with components +1.0,-1, which are referred to as a triplet state (since it leads to 3 levels in a magnetic field)

The antisymmetric state is considered to have spin S=0 with just one component, 0. It is called a singlet state.

Antisymmetric spin Symmetric spin

MS +1 0 -1 0

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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 19

Permutational symmetry

Our Hamiltonian for H2,

H(1,2) =h(1) + h(2) + 1/r12 + 1/R Does not involve spin

This it is invariant under 3 kinds of permutaions Space only: r1 ➔ r2

Spin only: s1 ➔ s2

Space and spin simultaneously: (r1,s1) ➔ (r2,s2)

Since doing any of these interchanges twice leads to the identity, we know from previous arguments that

Ψ(2,1) =  Ψ(1,2) symmetry for transposing spin and space coord Φ(2,1) =  Φ(1,2) symmetry for transposing space coord

Χ(2,1) =  Χ(1,2) symmetry for transposing spin coord

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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 20

Permutational symmetries for H

2

and He

H2

He

the only states observed are

those for which the wavefunction changes sign

upon

transposing all coordinates of electron 1 and

2

Leads to the 6th postulate of

QM

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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 21

The 6

th

postulate of QM: the Pauli Principle

For every state of an electronic system

H(1,2,…i…j…N)Ψ(1,2,…i…j…N) = EΨ(1,2,…i…j…N) The electronic wavefunction Ψ(1,2,…i…j…N) changes sign upon transposing the total (space and spin)

coordinates of any two electrons

Ψ(1,2,…j…i…N) = - Ψ(1,2,…i…j…N) We can write this as

t

ij

Ψ = - Ψ for all I and j

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Implications of the Pauli Principle

Consider two independent electrons, 1 on the earth described by ψe(1)

and 2 on the moon described by ψm(2)

Ψ(1,2)=

ψe(1) ψm(2)

And test whether this satisfies the Pauli Principle

Ψ(2,1)=

ψm(1) ψe(2) ≠ - ψe(1) ψm(2)

Thus the Pauli Principle does NOT allow the simple product wavefunction for two independent electrons

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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 23

Quick fix to satisfy the Pauli Principle

Combine the product wavefunctions to form a symmetric combination

Ψ

s

(1,2)=

ψe(1) ψm(2) + ψm(1) ψe(2)

And an antisymmetric combination

Ψ

a

(1,2)=

ψe(1) ψm(2) - ψm(1) ψe(2) We see that

t12

Ψ

s

(1,2) = Ψ

s

(2,1) = Ψ

s

(1,2) (boson symmetry)

t12

Ψ

a

(1,2) = Ψ

a

(2,1) = -Ψ

a

(1,2) (Fermion symmetry)

Thus the Pauli Principle only allows the antisymmetric combination for two independent electrons

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24

Consider some simple cases: identical spinorbitals Ψ(1,2)=

ψe(1) ψm(2) - ψm(1) ψe(2)

Identical spinorbitals: assume that ψm = ψe Then

Ψ(1,2)=

ψe(1) ψe(2) - ψe(1) ψe(2) = 0

Thus two electrons cannot be in identical spinorbitals Note that if ψm = eia ψe where a is a constant phase factor, we still get zero

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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 25

Consider some simple cases: orthogonality

Consider the wavefuntion

Ψ

old

(1,2)=

ψe(1) ψm(2) - ψm(1) ψe(2)

where the spinorbitals ψm and ψe are orthogonal hence <ψme> = 0

Define a new spinorbital θm = ψm + l ψe (ignore normalization) That is not orthogonal to ψe. Then

Ψ

new

(1,2)=

ψe(1) θm(2) - θm(1) ψe(2) =

ψe(1) θm(2) + l ψe(1) ψe(2) - θm(1) ψe(2) - l ψe(1) ψe(2)

= ψe(1) ψm(2) - ψm(1) ψe(2)

old

(1,2)

Thus the Pauli Principle leads to orthogonality of

spinorbitals for different electrons, <ψij> = dij = 1 if i=j

=0 if i≠j

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26

Consider some simple cases: nonuniqueness

Starting with the wavefuntion

Ψ

old

(1,2)=

ψe(1) ψm(2) - ψm(1) ψe(2)

Consider the new spinorbitals θm and θe where θm = (cosa) ψm + (sina) ψe

θe = (cosa) ψe - (sina) ψm Note that <θij> = dij Then

Ψ

new

(1,2)=

θe(1) θm(2) - θm(1) θe(2) =

+(cosa)2 ψe(1)ψm(2) +(cosa)(sina) ψe(1)ψe(2) -(sina)(cosa) ψm(1) ψm(2) - (sina)2 ψm(1) ψe(2) -(cosa)2 ψm(1) ψe(2) +(cosa)(sina) ψm(1) ψm(2) -(sina)(cosa) ψe(1) ψe(2) +(sina)2 ψe(1) ψm(2)

[(cosa)2+(sina)2] [ψe(1)ψm(2) - ψm(1) ψe(2)]

old

(1,2)

Thus linear combinations of the spinorbitals do not change Ψ(1,2)

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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 27

Determinants

The determinant of a matrix is defined as

The determinant is zero if any two columns (or rows) are identical

Adding some amount of any one column to any other column leaves the determinant unchanged.

Thus each column can be made orthogonal to all other columns.(and the same for rows)

The above properities are just those of the Pauli Principle Thus we will take determinants of our wavefunctions.

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The antisymmetrized wavefunction

Where the antisymmetrizer can be thought of as the determinant operator.

Similarly starting with the 3!=6 product wavefunctions of the form Now put the spinorbitals into the matrix and take the deteminant

The only combination satisfying the Pauil Principle is

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© copyright 2009 William A. Goddard III, all rights reserved

EEWS-90.502-Goddard-L04 29

Example:

From the properties of determinants we know that interchanging any two columns (or rows) that is interchanging any two

spinorbitals, merely changes the sign of the wavefunction Interchanging electrons 1 and 3 leads to

Guaranteeing that the Pauli Principle is always satisfied

Referensi

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