4e : the quantum universe5 the hydrogen atom in its full quantum mechanical glory r 222 2 222 2 2 2...

10
4E : The Quantum Universe Lecture 23, May 11 Vivek Sharma [email protected]

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Page 1: 4E : The Quantum Universe5 The Hydrogen Atom In Its Full Quantum Mechanical Glory r 222 2 222 2 2 2 2 2 2 2 2 2 for spherical polar coordinates: 1 = Instead of writing Laplacian ,

4E : The Quantum Universe

Lecture 23, May 11Vivek Sharma

[email protected]

Page 2: 4E : The Quantum Universe5 The Hydrogen Atom In Its Full Quantum Mechanical Glory r 222 2 222 2 2 2 2 2 2 2 2 2 for spherical polar coordinates: 1 = Instead of writing Laplacian ,

2

The Coulomb Attractive Potential That Binds the electron and Nucleus (charge +Ze) into a

Hydrogenic atom

F V

me

+e

r

-e

2

( ) kZeU rr

=

Page 3: 4E : The Quantum Universe5 The Hydrogen Atom In Its Full Quantum Mechanical Glory r 222 2 222 2 2 2 2 2 2 2 2 2 for spherical polar coordinates: 1 = Instead of writing Laplacian ,

3

The Hydrogen Atom In Its Full Quantum Mechanical Glory

2 2 2

As in case of particle in 3D box, we should use seperation of variables (x,y,z ??) to derive 3 independent differential. eq

1 1( ) x,y,z all mixe

This approach

d up

willns.

get very

!

ugly

U rr x y z

∝ = ⇒+ +

To simplify the situation, choose more appropriate variablesCartesian coordinates (x,y,z)

since we have a "co

Spherical Polar (r

njoined triplet"

, , ) coordinatesθ φ→

r

2

( ) kZeU rr

=

Page 4: 4E : The Quantum Universe5 The Hydrogen Atom In Its Full Quantum Mechanical Glory r 222 2 222 2 2 2 2 2 2 2 2 2 for spherical polar coordinates: 1 = Instead of writing Laplacian ,

4

Spherical Polar Coordinate System

dV

2

( sin )Vol

( )( ) = r si

ume Element dV

ndV r d rd dr

drd dθ φ θ

θ θ φ

=

Page 5: 4E : The Quantum Universe5 The Hydrogen Atom In Its Full Quantum Mechanical Glory r 222 2 222 2 2 2 2 2 2 2 2 2 for spherical polar coordinates: 1 = Instead of writing Laplacian ,

5

The Hydrogen Atom In Its Full Quantum Mechanical Glory

r 2 2 22

2 2 2

2

2 22 2

2

222

for spherical polar coordinates:

1=

Instead of writing Laplacian ,

write

1sin

Thus the T.I.S.Eq. for (x,y,z) = (r, , ) be

sin

come

i1r s n

rr r r

x y z

r θ φ

ψ ψ

θ θ

φ

θθ

θ

∂ ∂⎛ ⎞⎜ ⎟∂ ∂⎝ ⎠

∂ ∂ ∂∇ = + +

∂ ∂ ∂

∂ ∂⎛ ⎞∇ + +⎜ ⎟∂ ∂⎝ ∂⎠

2

2 2

2

2 2 2

2

22

2

1 (r, , ) (r, , )r

(r, , ) (r, , ) =

s

1

1

0

2m+ (E-U(r))si

sinsin

1 1with )

n

(

r

r

U r

r r

r x y z

r

θ

θ

φ

ψ θ φ ψ θ φ

ψ θ φ ψ

θ

θ

θ

φ

θ∂ ∂⎛ ⎞⎜ ⎟∂ ∂⎝ ⎠

∂ ∂⎛ ⎞+ +⎜ ⎟∂ ∂⎝ ⎠

∝ =+

+

Page 6: 4E : The Quantum Universe5 The Hydrogen Atom In Its Full Quantum Mechanical Glory r 222 2 222 2 2 2 2 2 2 2 2 2 for spherical polar coordinates: 1 = Instead of writing Laplacian ,

6

The Schrodinger Equation in Spherical Polar Coordinates (is bit of a mess!)

22

2 2 2

2

22

2 2

2

2

The TISE is :1 2m+ (E-U(r))

sin

Try to free up second last

1 (r, , ) =0 r

all except

T

term fro

1 sinsin

his requires multiplying thr

m

uout by sin

sin

rr r

r

rr

r rψ ψ ψ ψ θ φ

θ φθ

θ θ

θ

θ

θ

φ

∂ ∂⎛ ⎞+ +⎜ ⎟∂ ∂⎛ ⎞⎜ ⎟∂ ∂⎝ ∂ ∂⎠

⎠∂

⎝ ∂

2

2

2 2

2

22m ke+ (E+ )r

(r, , ) = R(r)

sin sin

. ( ) . ( ) Plug it into the TISE above & divide thruout by (r, , )=R(r). ( ). ( )

sin =0

For Seperation of Variables, Write

rr

θ θφ

ψ θ φ θ φψ θ φ θ

θ θψ θ

φ

ψ ψ ψ∂ ∂⎛ ⎞+ +⎜∂⎛ ⎞

⎜ ⎟∂⎝ ⎠∂∂⎟∂

Θ

∂ ⎠

ΦΦ

Θ

R(r) r

( ) when substituted in TISE

( )

( , ,

) ( ). ( )r

( , , )Note that : ( ) ( )

( , , ) ( ) ( )

r

r R r

r R r

θθ

θ φ θ φ

θ φ φθθ φ φθ φ

θ

∂Ψ= Θ Φ

∂∂Ψ

= Φ∂

∂Ψ= Θ

∂∂

∂Θ⇒

∂∂Φ∂

Page 7: 4E : The Quantum Universe5 The Hydrogen Atom In Its Full Quantum Mechanical Glory r 222 2 222 2 2 2 2 2 2 2 2 2 for spherical polar coordinates: 1 = Instead of writing Laplacian ,

7

Solving For the Hydrogen Atom: Separation of VariablesD

on’t

Pani

c: It

s sim

pler

than

you

thin

k !

2 2 22

2 2

2 2

2 2

2 2

2 2 22

1 2m ke+ (sin sin =0

Rearrange b

E+ )r

2m ke 1+ (E+ )r

LHS

y taking

i

the term

s f

sin sin

sin

on RHS

sin sin =-s

n.

in

R rrR r r

R rrR r r

θ θ

φ

θ θ

θ θ

θ θ

θφθ θ

φ

θ

∂ ∂Θ⎛ ⎞+ +⎜ ⎟Θ ∂ ∂∂ ∂⎛ ⎞⎜ ⎟∂ ∂⎝ ⎠

∂ ∂⎛ ⎞⎜ ⎟∂ ∂

∂ ΦΦ ∂

∂ ΦΦ ∂

⎝ ⎠

∂ ∂Θ⎛ ⎞+ ⎜ ⎟Θ ∂ ∂⎠ ⎝ ⎠⎝

2

of r, & RHS is fn of only , for equality to be true for all r, ,

LHS= constant = RHS = m l

θ φ θ φ

Page 8: 4E : The Quantum Universe5 The Hydrogen Atom In Its Full Quantum Mechanical Glory r 222 2 222 2 2 2 2 2 2 2 2 2 for spherical polar coordinates: 1 = Instead of writing Laplacian ,

8

Deconstructing The Schrodinger Equation for Hydrogen

2 2 22 2

2

2

2

2

sin sin =m

Divide Thruout by sin and arrange all terms with r aw

Now go break up LHS to seperate the terms...r .. 2m keLHS: + (E+ )

a

& sin si

y from

r

1

n lR r

r

rr

r

R r

R

θ θ

θ

θ θθ θ

θ

θ

∂ ∂Θ⎛ ⎞+ ⎜ ⎟Θ ∂ ∂⎝ ⎠∂ ∂⎛

∂∂

⎜ ⎟∂ ∂⎝ ⎠

⇒2

2

2 2

2

m 1 sinsin sin

Same argument : LHS is fn of r, RHS is fn of ;

For them to be equal for a LHS = const = RHS

What is the mysterious ( 1) ?

2m ke(E+ )=

ll r, =

r

( 1)

l

l l

l

r

l

Rr

θθ θ θ θ

θ

θ

∂ ∂Θ⎛ ⎞− ⎜ ⎟Θ ∂ ∂⎝ ⎠⎛ ⎞ +

+

⎟⎠

+

⎜ ∂

Just a number like 2(2+1)

Page 9: 4E : The Quantum Universe5 The Hydrogen Atom In Its Full Quantum Mechanical Glory r 222 2 222 2 2 2 2 2 2 2 2 2 for spherical polar coordinates: 1 = Instead of writing Laplacian ,

9

2

22

2

22

2

do we have after all the shuffling!

m1 sin ( 1) ( ) 0.....(2)si

So What

d ..... ............(1)

1

n sin

m 0..

l

l

d d l l

d Rrr d

d

d

r r

dθ θ

θ θ θ

φ

θ⎡ ⎤Θ⎛ ⎞ + + − Θ =⎜ ⎟ ⎢ ⎥

Φ

∂⎛ ⎞ +⎜ ⎟∂⎝

Φ

⎣ ⎦

+ =

2 2

2 2

2m ke ( 1)(E+ )- ( ) 0....(3)r

These 3 "simple" diff. eqn describe the physics of the Hydrogen atom.

All we need to do now is guess the solutions of the diff. equations

Each of them, clearly,

r l l R rr

⎡ ⎤+=⎢ ⎥

⎣ ⎦

has a different functional form

Page 10: 4E : The Quantum Universe5 The Hydrogen Atom In Its Full Quantum Mechanical Glory r 222 2 222 2 2 2 2 2 2 2 2 2 for spherical polar coordinates: 1 = Instead of writing Laplacian ,

10

And Now the Solutions of The S. Eqns for Hydrogen Atom

22

2

dThe Azimuthal Diff. Equation : m 0

Solution : ( ) = A e but need to check "Good Wavefunction Condition"Wave Function must be Single Valued for all ( )= ( 2 )

( ) = A e

l

l

l

im

im

φ

φ

φφ φ φ π

φ

Φ+ Φ =

Φ⇒ Φ Φ +

⇒Φ ( 2 )

2

2

A e 0, 1, 2, 3....( )

m1The Polar Diff. Eq: sin ( 1) ( ) 0 sin sin

Solutions : go by the name of "Associated Legendr

Q

e Functions"

uantum

#

liml

l

m

d d l

Magneti

d d

c

l

φ π

θ θθ θ θ θ

+= ⇒ = ± ± ±

⎡ ⎤Θ⎛ ⎞ + + − Θ =⎜ ⎟ ⎢ ⎥⎝ ⎠ ⎣ ⎦

only exist when the integers and are related as follows 0, 1, 2, 3.... ; positive number

: Orbital Quantum Number

l

l

l mm l l

l

= ± ± ± ± =

Φ