, , 7-9. n 0 1 2

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7-9. (a) For n = 3, l = 0 1 2

(b) For l =

0 , m

=

0 . For l =

1 , m

= !

1 0 1 . For l =

2 , m

=

2 1 0 1 2 .

(c) There are nine different m -states, each with two spin states, for a total of 18 states for n = 3.

7-10. (a) For l = 4

L = ( + 1 ) h = h = 20 h m l

= 4 h

!

min

= cos " 1

4

20

# !

min

(b) For l =

2

L = 6 h

!

min

= cos " 1

2

6 m l

= 2 h

# !

min

=

7-12. (a) l = 1

L = 2 h

+1

0

(b)

− 1

+2

+1

=

°

°

0

l = 2

L = 6 h

(c)

+4

+3

+2 l = 4

L = 20 h

+1

0

− 1

− 2

− 3

− 4

(d) L = ( + )

7-13. L 2

= L 2 x

+ L 2 y

+ L 2 z

!

L 2 x

+ L 2 y

= L 2

" L 2 z

= ( + 1 ) h 2

" ( )

2

=

( 6 " m 2 ) h 2

(a) ( L 2 x

+ L 2 y

) min

=

(

!

2 ) h 2

= 2 h 2

(b) ( L 2 x

+ L 2 y

) max

=

(

!

2 ) h 2

= 6 h 2

(c) L 2 x

+ L 2 y

= ( 6 1 ) h 2

= h L L

(d) n = 3

7-15. L = r ? p d L dt

= d dt r

!

p + r !

d p dt d r dt

!

= !

m m

! =

0 and r

!

d p dt r F .

Since for V =V ( r ), i.e., central forces,

F is parallel to r , then 0 and d L dt

=

0

7-16. (a) For l = 3 , n = 4, 5, 6, … and m = − 3, − 2, − 1, 0, 1, 2, 3

(b) For l = 4 , n = 5, 6, 7, … and m = − 4, − 3, − 2, − 1, 0, 1, 2, ,3 ,4

(c) For l =

0 , n = 1 and m = 0

(d) The energy depends only on n . The minimum in each case is:

E

4

= !

2

= !

.

eV / 4 2

= !

eV

E

5

= !

.

eV / 5 2

= !

eV

E

1

= !

eV

7-17. (a) f n

=

6 , l =

3

(b) E

6

= !

13 6 eV n 2

= !

13 6 eV / 6 2

= !

eV

(c) L

= ( +

1 ) h = ( ) h =

12 h = "

!

34 J s

(d) L z

= m h L z

= !

3 h , !

2 h , !

h h h h

7-20. (a) For the ground state, ( ) $ r

= !

2 ( 4

" r 2 )

$ r

=

4 r 2 a

0

3 e # 2 /

0 $ r

" r =

For " r = 0 03 a

0

, at r = a

0

we have ( ) " r =

4 a 2

0 a

0

3 e !

2 ( a

0

) =

(b) For

.

a

0

, at r = a

0

( ) " r =

( a

0

)

2 a

0

3 e !

4 ( a

0

) =

7-21. ( ) = Cr e !

2 /

0

For P ( r ) to be a maximum, dP dt

= (

.

2

$

*

,

!

2 Z a

0

%

+

e !

2 /

0 + 2 re !

2 /

0

#

) = 0 & C '

2 a

Zr

0

$

* a

Z

0

!

!

2 /

0 = 0

This condition is satisfied with r = 0 or r = a

0

/Z.

For r = 0, P ( r ) = 0 so the maximum

P ( r ) occurs for r = a

0

/Z.

7-22. ' "

2 d # =

&

' ' '

0 0 0

" sin $ $ % = 1

=

#

4 ! "

0

+ = 4 !

C 2

210

+

0

# % Zr &

'

) a

0

(

*

2

$ /

0 dr = 1

=

4 !

C 2

210

"

*

0

$

&

(

Letting a

0

2

%

'

) e # /

0 dr

=

1

=

0

we have that r

=

/ substituting these above,

&

"

2 d # =

4 !

a C 2

210

Z 3

&

0

$ x

Integrating on the right side

and dr

=

/

#

0

!

x

=

6

and

Solving for C 2

210

yields: C 2

210

=

Z 3

24 !

a 3

0

$ C

210

=

"

%

'

Z 3

24 !

a

0

3

#

&

(

7-26. For the most likely value of r , P ( r ) is a maximum, which requires that (see

Problem 7-24) dP dr

= A cos 2

!

#

' r 4

%

)

+

"

Z a

0

&

*

, e " /

0 + 4 " /

0

$

( = 0

For hydrogen Z = 1 and A cos 2

!

( /

0

) ( 4 a

0

" ) "

0 = 0 . This is satisfied for r = 0 and r = 4 a

0

. For r = 0, P ( r ) = 0 so the maximum P ( r ) occurs for r = 4 a

0

.

7-33. (a) There should be four lines corresponding to the four m

J values − 3/2, − 1/2,

+1/2, +3/2.

(b) There should be three lines corresponding to the three m l

values − 1, 0, +1.

7-68.

=

4 Z 3 a 3

0

!

2 /

0

(See Problem 7-63)

For hydrogen, Z = 1 and at the edge of the proton r = R

0

= 10 !

15 m .

At that point, the exponential factor in P (r) has decreased to: nucleus, e !

2 /

0 = e !

( !

15 ) (

"

!

10 m )

= e !

(

"

!

5 )

# !

"

!

5

#

1

Thus, the probability of the electron in the hydrogen ground state being inside the to better than four figures, is:

=

4 r 2 a 3

0 r

0

P = ( )

0

!

= !

0

R

0 4 r 2 4 a 3

0

= a

0

3

!

0

R

0

=

4 a

0

3 r 3

3

R

0

0

=

4 a

0

3

" R

0

3

#

%

'

3

&

(

=

(

( !

15 m )

3

$

!

10 m )

3

= $

!

15

7-70. (a) Substituting !

( ) into Equation 7-9 and carrying out the indicated operations

yields (eventually):

% h 2

2 µ

!

( ) 2 / r 2

% a

0

2

% h 2

2 µ

!

( ) (

%

2 / r 2 )

+

V

!

( ) =

E

!

( )

Canceling !

( ) and recalling that r 2

= 4 a

0

2 (because !

given is for n = 2) we

have

!

h 2

2 µ

(

!

1 4 a 2

0

)

+ =

E

The circumference of the n = 2 orbit is:

C = 2 !

( 4 a

0

) = 2 " # a

0

= "

/ 4 !

= 1 2 k .

Thus, # h 2

2 µ

!

'

#

1

4 4 k 2

"

(

+ V = E $ h

2 µ

+ V = E p 2

(b) or

2 m v E and Equation 7-9 is satisfied.

$

,

0

!

2 dx

= , A 2

& r '

2

(

* a

0

)

+ e % /

0 cos 2

" r 2 sin " drd d

A 2

,

0

$ & r '

2

(

* a

0

)

+ e % /

0 r dr

!

,

0

2 !

cos 2

" sin d d #

0

, = 1

Integrating (see Problem 7-22),

=

1

A 2 ( ) ( / )( ) =

1

A 2

= a

0

3

!

" A = a

0

3

!

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