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1

Zoltán Rolik

2018 fall

Zoltán Rolik Physical Chemistry and Structural Chemistry

(2)

Physical Chemistry

Physical Chemistry I - Equilibrium (phase equilibrium, chemical equilibrium)

Physical Chemistry II - Change (reaction kinetics, transport, electrochemistry)

Physical Chemistry III - Structure (molecular structure,

spectroscopy, materials science)

(3)

Curriculum

Introduction

The basics of quantum mechanics The structure of the hydrogen atom Structure of many-electron atoms Optical spectroscopy

Rotational spectroscopy Vibrational spectroscopy

Electronic structure of molecules

3

(4)

Curriculum

Photoelectron spectroscopy Lasers and laser spectroscopy Fundamentals of nuclear structure Nuclear magnetic resonance Mass spectrometry

X-ray diraction

(5)

The structure of atoms, molecules, and other particles is described by quantum mechanics.

The foundation of quantum mechanics was laid in the 1920´s.

Preliminaries: some experiments which contradict the principles of classical physics

5

(6)

Joseph Fraunhofer's experiment, 1815

The sunlight was dispersed by a grating.

Dark lines were observed in the continuous spectrum.

(7)

The spectrum of the sun

7

(8)

the sun emits continuous radiation

the particles of the gas surrounding the Earth and the Sun absorb only photons of particular wavelength/frequency particle A absorbs light of

A1

,

A2

, ... frequency particle B absorbs light of

B1

,

B2

, ... frequency, etc.

hence the energy of particle A can be changed by quanta of

E

A

= h

A1

, h

A2

, ... and the energy of particle B can be

changed by E

B

= h

B1

, h

B2

, ...

(9)
(10)
(11)

11

(12)

that is, the corresponding physical quantities have only discrete values.

This realization is reected by the term quantum mechanics

(13)

In the non-relativistic case the submicroscopic systems can be described by the Schrödinger equation

i ~ @

@ t (r; t ) = ~

2

2 m r

2

+ V (r; t )

(r; t )

Let's start from the beginning. What does i stand for?

13

(14)

complex numbersa

aP. Atkins, J. Paula, R. Friedman, Chapter 2

Natural numbers

negative numbers (Diophantus [200 - c.284 CE]: The solution of the 4 = 4 x + 20 equation is absurd.)

rational numbers (Pythagorean school: all phenomena in the universe can be reduced to whole numbers and their ratios)

but what is p

2?

(15)

complex numbers

Real numbers form a closed set for the a + b ; a b ; a b ; a = b ( a ; b 2 R) operations.

But what is p

1? (Cardano, 1545)

15

(16)

complex numbers

real line vs. complex plane 1D vs. 2D

( x ) ( x ; y )

x ; y 2 R (ordered pairs) ( x ; y ) 6= ( y ; x )

(17)

complex numbers

addition, (a;b) + (c;d) , (a+c;b+d) subtraction, (a;b) (c;d) , (a c;b d) multiplication, (a;b) (c;d) , (ac bd;ad+bc) real numbers have the form of (a; 0) they lie on the real axis:

(a; 0) + (c; 0) , (a+c; 0) (a; 0) (c; 0) , (a c; 0)

(a; 0) (c; 0) , (ac; 0)

17

(18)

complex numbers

imaginary numbers have the form of (0; b ) they lie on the imaginary axis:

z = (0; b ) z z = z

2

(0; b ) (0; b ) , ( b

2

; 0)

z

2

= b

2

z 2 C ; b 2 R

(0; 1) (0; 1) , ( 1; 0)

(19)

complex numbers

z = (0; 1) is special, it is denoted by i , and called the imaginary unit ( i

2

= 1) with its help z = ( a ; b ) = a + bi

complex conjugate of z = a + bi is denoted by a star superscript z

= a bi

z z

= (a + bi ) (a bi ) = a

2

+ b

2

= jzj

2

19

(20)

complex numbers

division by a complex number:

a + bi

c + di = a + bi

c + di c di c di

= (a + bi )(c di ) c

2

+ d

2

= (ac + bd )

c

2

+ d

2

+ (bc ad )

c

2

+ d

2

i

(21)

complex numbers

polar form of complex numbers

z = a + bi = r (cos ' + i sin ') r = p

a

2

+ b

2

tan ' = b a multiplication and division in polar form:

z

1

= r

1

(cos '

1

+ i sin '

1

) z

2

= r

2

(cos '

2

+ i sin '

2

) z

1

z

2

= r

1

r

2

(cos('

1

+ '

2

) + i sin('

1

+ '

2

))

z

1

z

2

= r

1

r

2

(cos('

1

'

2

) + i sin('

1

'

2

))

21

(22)

Taylor-series

if f (x) is innitely dierentiable at a real or complex number a then f (x) = f (a) + f

0

(a)(x a) + 1

2 f

00

(a)(x a)

2

+ 1

3 2 f

000

(a)(x a)

3

+ : : :

= X

1

n=0

f

(n)

( a )

n ! ( x a )

n

when a = 0 it is called a Mclaurin series

(23)

Taylor-series,a= 0

f ( x ) = exp( x ) = e

x

e

x

= e

0

+ ( e

0

)

0

( x 0) + 1

2 ( e

0

)

00

( x 0)

2

+ 1

3 2 ( e

0

)

000

( x 0)

3

+ : : :

= X

1

n=0

1 n ! x

n

23

(24)

Taylor-series,a= 0

f ( x ) = sin( x )

sin x = 0 + x + 0 1

3! x

3

+ 0 + 1

5! x

5

+ 0 1

7! x

7

+ : : :

= X

1

n=0

1

n

(2 n + 1)! x

2n+1

(25)

Taylor-series,a= 0

f ( x ) = cos( x )

cos x = 1 + 0 1

2! x

2

+ 0 + 1

4! x

4

+ 0 1

6! x

6

+ : : :

= X

1

n=0

1

n

(2 n )! x

2n

25

(26)

Euler's formula

i

0

= 1 i

1

= i

i

2

= 1 i

3

= i

recall that e

z

= 1 + z +

12

z

2

+

3!1

z

3

+ : : : if z = ix

e

ix

= 1 + ix + 1

2 i

2

x

2

+ 1

3! i

3

x

3

+ 1

4! i

4

x

4

+ 1

5! i

5

x

5

+ : : :

(27)

Euler's formula

e

ix

= 1 + ix + 1

2 i

2

x

2

+ 1

3! i

3

x

3

+ 1

4! i

4

x

4

+ 1

5! i

5

x

5

+ : : :

= 1 + ix 1

2 x

2

i 1

3! x

3

+ 1

4! x

4

+ i 1

5! x

5

+ : : :

= 1 1

2 x

2

+ 1

4! x

4

+ ix i 1

3! x

3

+ i 1

5! x

5

+ : : :

= (1 1

2 x

2

+ 1

4! x

4

+ : : : ) + i ( x 1

3! x

3

+ 1

5! x

5

+ : : : )

= cos x + i sin x

27

(28)

complex numbers

exponential form of complex numbers

z = a + bi = r (cos ' + i sin ') polar form e

i'

= cos ' + i sin '

z = r e

i'

exponential form

(29)

conserved properties

conservation laws

a

some measurable physical properties do not change

mass (m)

b

and energy ( E )

electric charge ( q ) linear momentum (p) angular momentum (l)

aThere is always a symmetry behind the conservation laws: conservation of energy is connected to the time-invariance of physical systems.

bconservation of mass is not exact: nuclear fusions

29

(30)

the ability to do work

the kinetic energy (E

kin

| K ) is due to motion; E

kin

= f (p) a moving object can do work

the potential energy ( E

pot

| V ) is due to position; E

pot

= g (r) stored energy of an object that can do work

E

tot

= E

kin

+ E

pot

or H = K + V

Hamilton function: E=H=H(p, q), where p; q are the

canonical coordinates.

(31)

simple manipulations

recall the scalar product of vectors: v v = jvj

2

= v

2

E

kin

= 1 2 mv

2

p = mv p

2

= m

2

v

2

E

kin

= p

2

2 m

31

(32)

Epot= 0

E

tot

= E

kin

= p

2

2 m p 2 mE

kin

= p = m dx

dt dx

dt =

r 2 E

kin

Z

x(t)

m

x(0)

dx =

r 2 E

kin

m

Z

t

0

dt

x ( t ) = x (0) +

r 2 E

kin

m t p ( t ) = mv ( t ) = m dx

dt = m

r 2E

kin

m p(t ) = p

2mE

kin

(33)

restoring force is proportional to the displacement from the equilibrium position

the spring stores the energy as V ( x ) = 1

2 kx

2

) F

x

= dV dx F = kx

m d

2

x

dt

2

= kx m

2

e

t

= ke

t

( m

2

+ k ) e

t

= 0

2

= k m = i

r k

m = i !

x ( t ) = c

1

e

i!t

+ c

2

e

i!t

= A sin(! t + ') p(t ) = m dx

dt = !Am cos(!t + ')

x(t) =et) dx

dt = et ) d2x

dt2 = 2et

33

(34)

uniform circular motion, centripetal force,Fcp, and angular momentum, `

Fcp=ma=mr!2=mv2 r

` =rp=rmv

s '=2r

2 ) s=r ' v=ds

dt = lim

t!0

s

t =r lim

t!0

' t

=r !

v '=2v

2 ) v=v ' a=dv

dt = lim

t!0

v

t =v lim

t!0

' t

=v ! =r !2

(35)

special case of rotational motion, r is xed

x ( t ) = A sin( 2

T t ) = A sin(! t ) v = r !

a = v ! = r!

2

F = mv

2

r

35

(36)

correspondences

linear momentum p angular momentum ` = r p = I ! velocity v angular velocity ! = r v

r

2

mass m moment of inertia I = mr

2

Kinetic energy p

2

2m

`

2

2I

(37)

modela

asee also in wikipedia, Wave equation, Hooke's law

elastic, homogeneous string stretched to a length of L endpoints are xed

is the mass of the string per unit length

u ( x ; t ) represents the displacement of the string at a point x at a time t from its equilibrium position

only vertical movements are allowed

37

(38)
(39)

derivation

T

1

cos = T

2

cos( + ) := T T

2

sin( + ) T

1

sin = m a = x @

2

u ( x ; t )

@ t

2

T

2

sin( + )

T

2

cos( + )

T

1

sin T

1

cos = 1

T x @

2

u ( x ; t )

@ t

2

tan( + ) tan = 1

T x @

2

u ( x ; t )

@t

2

@ u

x+x

@x

@ u

x

@x = 1

T x @

2

u ( x ; t )

@t

2

39

(40)

derivation

@ u

x+x

@ x

@ u

x

@ x = 1

T x @

2

u ( x ; t )

@ t

2

@ux+x

@x @ux

x

@x

= 1 T

@

2

u ( x ; t )

@ t

2

@

2

u ( x ; t )

@ x

2

= 1

T = @

2

u ( x ; t )

@ t

2

@

2

u ( x ; t )

@ x

2

= 1

c

2

@

2

u ( x ; t )

@ t

2

(41)
(42)

traveling, standing waves and interference

(x;t) =A sin(kx !t) sin + sin = 2 sin( +

2 ) cos(

2 )

(x;t)interference=A sin(kx !t) +A sin(kx !t+ ') = 2A sin(kx !t+' 2) cos('

2) (x;t)standing=A sin(kx !t) +A sin(kx+ !t) = 2A sin(kx) cos(!t)

(x;t)standing=A sin(kx !t) A sin(kx+ !t) = 2A cos(kx) sin(!t)

(43)
(44)

light

light is electromagnetic radiation: (x;t) =A sin(kx !t) =A sin(2(x ct)) amplitude,A, maximum displacement from the rest position

wavelength, , the distance between two successive maxima

(45)

(Einstein, 1905), heat capacity of low temperature isolator crystals (Debye, 1912): energy is quantized, E = h .

Diagram of the maximum kinetic energy as a

function of the frequency of light on zinc.

de Broglie (1924): all matter has wave properties, p =

h

= ~k

45

(46)

H emission spectrum

the experimental emission spectrum of the H-atom

(47)

H emission spectruma

awikipedia, Hydrogen spectral series

Balmer(n 3)

~ = 1096801 4

1 n2

cm 1 Rydberg(n2>n1)

~ = 109680 1

n21 1 n22

cm 1

Ritz combination rule: spectral lines include frequencies that are either the sum or the dierence of the frequencies of two other lines [the wavenumber (

~ = 1=) of any spectral line is the dierence between two terms

~ =term(i) term(j) ]

47

(48)

atomic emission spectra, characteristic for the atoms

(49)

Bohr's theory of the H-atom (1913)a

awikipedia

existence of stationary orbits (xed nucleus and circular orbit), no electromagnetic radiation

frequency condition: E =h(his the Planck constant, 6:626 10 34J s) angular momentum is quantized: ` =n~, ~ =h=2

49

(50)

Bohr's theory of the H-atom (1913)

Felectrostatic=Fcentripetal

e2

40r2 = mev2 r

` =n~ =rmev v= n~

rme

v2= n2~2 m2er2 e2

40r2 = memn22~2

er2

r r = n2~240

mee2

Bohr radius,a0= 0:529 Å, (n= 1)

vacuum permittivity 0= 8:854187817620::: 10 12A2s4kg 1m 3

(51)

Bohr's theory of the H-atom

Etot =Ekin+Epot

=1

2mev2 e2 40r

=1 2

e2 40r

e2

40r = 1 2

e2 40r

= 1

2 e2 40n2~240

mee2

= mee4 80h2

1 n2

e2

40r2 =mev2 r mev2= re2

40r2 r =n2~240

mee2

~2= h2 42

51

(52)

Bohr's theory of the H-atom

E =h =hc =hc~ E =En2 En1= mee4

80h2( 1 n12

1 n22)

~ = 1 hc

mee4 80h2( 1

n21 1 n22)

~ =RH( 1 n21

1 n22) RH= 1

hc mee4

80h2 = 109737cm 1 RH= 109638cm 1from experiment

(53)

Bohr's theory of the H-atom

Bohr(n2>n1) : ~ = hc1 8me0eh42(n12 1

1 n22)cm 1

Lyman(n1= 1) Balmer(n1= 2) Paschen(n1= 3) Brackett(n1= 4)

1

1On December 1, 2011, it was announced that Voyager 1 detected the rst Lyman-alpha radiation originating from the Milky Way galaxy. Lyman-alpha radiation had previously been detected from other galaxies, but due to interference from the Sun, the radiation from the Milky Way was not detectable.

(Wikipedia)

53

(54)

plausibility of Bohr's quantization condition, ` =n~

pphoton= h

(Einstein) pparticle= h

(de Broglie)

= h

pparticle 2r =n 2r =n h

pelectron

` =rp=n h 2

constructive, destructive interferences standing wave - stationary orbit

(55)

plausibility of Bohr's quantization condition, ` =n~

Wave-particle duality: "It seems as though we must use sometimes the one theory and sometimes the other, while at times we may use either.

We are faced with a new kind of diculty. We have two contradictory pictures of reality; separately neither of them fully explains the phenomena of light, but together they do." (Einstein)

c = E = h

55

(56)

some arguments for the Schrödinger equation

of course there is no proof of it, it is a postulate

Free particle waves: ( x ; t ) = e

i(kx !t)

! = E =~ (Planck)

@

@t ( x ; t ) = i

~ E ( x ; t ) i ~ @

@ t ( x ; t ) = E ( x ; t )

k = p =~ (De Broglie)

@

2

@x

2

( x ; t ) = ( i

~ )

2

p

2

( x ; t )

~

2

2m

@

2

@x

2

( x ; t ) = p

2

2m ( x ; t )

The energy is a classical free particle:

E = p

2

2 m

@ ~

2

@

2

(57)

particle in a force eld, time-independent Schrödinger equation

If the particle is not free (3D):

i ~ @

@t (r; t ) = ~

2

2m @

2

@x

2

+ @

2

@y

2

+ @

2

@z

2

+ V (r)

(r; t ) A particular solution of the time-dependent Schrödinger equation:

(r; t ) = (r) e

~iEt

i ~ @

@t (r) e

~iEt

= E (r) e

~iEt

Using the relations above we obtain the time-independent Schrödinger equation

~

2

2 m

@

2

@ x

2

+ @

2

@ y

2

+ @

2

@ z

2

+ V (r)

(r) = E (r)

57

(58)

Schrödinger equation for the particle in the 1D box modela

aAtkins, part II, chapter 8

~2 2m

d2 (x)

dx2 +V(x) (x) =E (x) Ekin+Epot=Etot

@2 (x)

@x2 = 2m(E V(x))

~2 (x) d2y

dx2 = k2y

y2 feikx; sin(kx); cos(kx)g

(59)

Schrödinger equation for the particle in the 1D box model

~2 2m

d2 (x)

dx2 +V(x) (x) =E (x)

No particle in the innit potential area! ( x ) = 0 if x < 0 or x > L .

@2 (x)

@x2 = 2mE

~2 (x) k=

r2mE

~2

(x) =Ccoskx+Dsinkx

(0) = 0 (L) = 0

) ()

(C= 0

D= 0 or sinkL= 0 kL=n n= (1; 2; )

(x) =Dsinn Lx

59

(60)

Schrödinger equation for the particle in the 1D box model

V(x) = 8>

><

>>

:

1; 1 <x 0 0; 0 <x<L 1; Lx< 1

k= r2mE

~2 =n

L k2=2mE

~2 =n22 L2

2mE

~2 = n22 L2 En= n2h2

8mL2

Born probability interpretation: R1

1 2(x)dx= 1

(61)

properties of the solutions

Born probability interpretationR11 2(x)dx=1

i.e., probability of nding the particle betweenx andx+dxis 2(x)dx

ifn" then E "

n= 1, zero-point energy

hasn 1 nodes in the 0 <x<Linterval ground and excited states

with increasing mass the energy gap between the levels,En+1 En, decreases

(r) = (r) (r) satises the continuity equation,@@t +divj = 0, where

j(r;t) =2mi~

(r ) r

is the probability current

.

61

(62)

Schrödinger equation for the particle in the 1D box model

Born probability interpretation Z1

1

2(x)dx= 1 ) (x) = r2

Lsin(n L x)

(x) =Dsin(n Lx) D2

Z 1

1sin2(n

Lx)dx=D2 ZL

0 sin2(n

L x)dx= 1 D=

r2 L (x) =

r2 Lsin(n

Lx)

z=n Lx dz=n

Ldx Zn

0 dz=n L

ZL 0 dx

sin2z=sin2z+ cos2z+ sin2z cos2z 2

=1 cos 2z 2

(63)

Schrödinger equation for the free particle,V(x) = 0,Ekin=Etot

~2 2m

d2 (x)

dx2 =Ekin (x)

@2 (x)

@x2 = 2mEkin

~2 (x) k2= 2mEkin

~2 (x) =A sin(kx)

(x) =A sin( 2x) k= 2

2mEkin= 2m 12mv2=p2 p2=k2~2=

2

2

h

2 2

=h p

63

(64)

Schrödinger equation for the particle in the 2D box model

~2 2m

@2

@x2 + @@y22

+V =E

V(x;y) =

(0; x 2 (0;L1) ^y2 (0;L2)

1; otherwise

(65)

Schrödinger equation for the particle in the 2D box model

~2 2m

@2

@x2 + @@y22

=E (x;y) =F(x) G(y)

separation of variables

=F(x) G(y)

@2

@x2 =G(y)d2F(x) dx2

@2

@y2 =F(x)d2G(y) dy2

~2 2m

(

G(y)d2F(x)

dx2 +F(x)d2G(y) dy2

)

=EF(x)G(y)

~2 2m

( 1 F(x)

d2F(x) dx2 + 1

G(y) d2G(y)

dy2 )

=E

~2 2m

1 F(x)

d2F(x) dx2 =Ex

~2 2m

1 G(y)

d2G(y) dy2 =Ey

~2 2m

d2F(x) dx2 =ExF(x)

~2 2m

d2G(y) dy2 =EyG(y)

65

(66)

Schrödinger equation for the particle in the 2D box model

~2 2m

d2F(x) dx2 =ExF(x)

Ex= n21h2 8mL21

F(x) = s2

L1sinn1 L1x

~2 2m

d2G(y) dy2 =EyG(y)

Ey= n22h2 8mL22

G(y) = s2

L2sinn2 L2y

(x;y) =F(x) G(y) =

r 4

L1L2 sinn1

L1 x sinn2 L2 y E =Ex+Ey =

(n1 L1

2 +

n2 L2

2) h2 8m

(67)

Schrödinger equation for the particle in the 2D box model

(x;y) = s 4

L1L2 sinn1 L1 x sinn2

L2 y

E(n1;n2) = n1

L1 2

+ n2

L2 2h2

8m

consequence of symmetry,L1=L2=L (x;y) =

r4

L2 sinn1

L x sinn2 L y E(n1;n2) = n21+n22 h2

8mL2 E(1; 2) =E(2; 1) but the wavefunctions are dierent degeneracy: same energies dierent wavefunctions

67

(68)

Schrödinger equation for the particle in the 2D box model

degeneracy is the consequence of symmetry

(69)

Schrödinger equation for the particle in the 3D box model

~2 2m

@2

@x2 + @@y22 + @@z22

=E (x;y;z) =F(x) G(y) H(z)

(x;y;z) =F(x) G(y) H(z) =

r 8

L1L2L3 sinn1

L1 x sinn2

L2 y sinn3 L3 z E =Ex+Ey+Ez =

(n1 L1

2 +

n2 L2

2 +

n3 L3

2) h2 8m

69

(70)

Schrödinger equation for the particle in the 3D box model

degenerate case: cubeL1=L2=L3=L (x;y;z) =

r8

L3 sinn1

L x sinn2

L y sinn3 L z E(n1;n2;n3) = n12+n22+n23 h2

8mL2 = n21+n22+n32 h2 8mV2=3

(71)

Postulates of Quantum Mechanics

postulate I

aP. Atkins, J. Paula, R. Friedman, Chapter 1

The state of a quantum-mechanical system is completely specied by the so-called wavefunction, (r; t ), that depends on the coordinates of the particles and on time.

(r; t) (r; t)dxdydz is the probability that the particle lies in the volume element d = dxdydz located at r at time t.

71

(72)

postulate I

properties of (r; t ) continuous

contiguously dierentiable (if the V (r) potential is realistic ...) nite (square integrable for bound states, i.e.,

R

1

1

j j

2

d < 1)

single valued

(73)

postulate II

To every observable in classical mechanics there exists a

corresponding linear, Hermitian operator in quantum mechanics.

73

(74)

correspondences

observables ^ operators

position x x^ multiplication byx

r ^r multiplication by r potential energy V(x) V^(^x) multiplication byV(x)

V(r) V^(^r) multiplication byV(r)

momentum px p^x i~@@x

p ^p i~(ex @

@x + ey @

@y + ez @

@z) kinetic energy Kx K^x ~2

2m @2

@x2

K K^ ~2m2(@@x22 +@@y22+@@z22)

total energy E H^ T + ^^ V

(75)

postulate III

In any measurement of the observable associated with the operator , the only values that will ever be observed are the eigenvalues ! ^

i

which satisfy the eigenvalue equation ^

i

= !

i i

75

(76)

linear Hermitian operators

~

2

2 m

@

2

@ x

2

+ V

( x ) = E ( x ) H ( ^ x ) = E ( x ) eigenvalue equation ^ = !

for an operator there can be more than one eigenfunction usually dierent eigenfunctions have dierent eigenvalues (non degenerate)

an operator is called linear if ^ ( + ) = ^ + ^ an operator is called Hermitian if R

i

^

j

d = nR

j

^

i

d o

eigenvalues for Hermitian operators are real

(77)

postulate IV

If the state of the system is described by a normalized wave function , then the average value of the observable corresponding to the operator ^ can be calculated as h!i = R

^ d

77

(78)

postulate V

The wave function of a system evolves in time according to the

time-dependent Schrödinger equation: ^ H (r; t ) = i ~

@ (r;@tt)

(79)

required properties: measurable physical quantities are real

postulate III: ^ i = !i i ) R

i ^ id = !i

(we assumed that i is normalized,R1

1

i id = 1) eigenvalue equation

= ! ^ Z 1

1

d^ = ! Z 1

1 d Z 1

1

d^ = !

its complex conjugate ^ = ! Z 1

1 ^ d = ! Z 1

1 d Z 1

1 ^ d = !

! is real if ! = !, i.e.,R1

1 d =^ R1

1 ^ d

79

(80)

required properties

hermitian operators R ^ d =R

^ d

let be a linear combination of functions and and ^ is hermitian =ca +cb ) =ca+cb

Z d^ = Z

(ca+cb) ^(ca +cb)d

= Z

(ca +cb) ^(ca+cb)d = Z

^ d

(81)

required properties

Z

(ca+cb) ^(ca +cb)d =Z

(ca +cb) ^(ca+cb)d Z

ca^cad +Z

ca^cbd +Z

cb^cad +Z

cb^cbd Z =

ca ^cad + Z

ca ^cbd + Z

cb ^cad + Z

cb ^cbd

81

(82)

required properties

Z

ca^cad +Z

ca^cbd +Z

cb^cad +Z

cb^cbd Z =

ca ^cad + Z

ca ^cbd + Z

cb ^cad + Z

cb ^cbd Z

ca^cbd +Z

cb^cad =Z

ca ^cbd +Z

cb ^cad cacb

Z

^ d Z

^d

=cacb Z

^d Z

^ d

complex number = its complex conjugate Z

^ d =Z

^d and Z

^d =Z

^ d

(83)

hermitian operators

general denition Z

^ d = Z

^

d special case ( = )

Z

^ d = Z

^

d

83

(84)

properties of hermitian operators

the sum of hermitian operators is also a hermitian operator = ^^ i+ ^j

Z ^i d =Z

^i d and Z

^j d =Z

^j d Z ^ d =Z

n

^i+ ^io d

=Z

^i d +Z

^j d

= Z

^i d + Z

^j d (hermitian property)

=Z n ^i

+ ^io

d

= Z

^ d

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