1000 Solved Problems in Modern Physics

(Romina) #1

2.3 Solutions 121


deciding the model of the nucleus, that is discarding the electron–proton
hypothesis. Consider the nitrogen nucleus. The electron–proton hypothesis
implies 14 prorons+7 electrons. This means that it must have odd spin because
the total number of particles is odd (21) and Fermi statistics must be obeyed.
In the neutron–proton model the nitrogen nucleus has 7n+ 7 p=14 parti-
cles (even). Therefore Bose statistics must be obeyed. If the electronic wave
function for the molecules is symmetric it was shown that the interchange of
nuclei produces a factor (−1)J(J=rotational quantum number) in the total
wave function of the molecule. Thus, if the nuclei obey Bose statistics sym-
metric nuclear spin function must be combined with evenJrotational states
and antisymmetric with oddJ. Because of the statistical weight attached to
spin states, the intensity of even rotational lines will be (I+1)/Ias great
as that of neighboring odd rotational lines whereIis the nuclear spin. For
Fermi statistics of the nuclei the spin and rotational states combine in a manner
opposite to that stated previously, the odd rotational lines being more intense
in the ratio (I+1)/I. The experimental ratio (I+1)/I=2 for even to odd
lines, givingI=1, is consistent with the neutron–proton model.

2.60 The vibrational energy level is


En=

(

n+

1

2

)

ω,n= 0 , 1 , 2 ...

withω=


(k/μ),kbeing the force constant andμthe reduced mass of the
oscillating atoms.

μ=

mcm 0
mc+m 0

=

12 × 16

12 + 16

= 6 .857 amu

ω=

(

1908

6. 857 × 1. 67 × 10 −^27

) 1 / 2

= 4. 082 × 1014 S−^1

Number of molecules in stateEnis proportional to exp(−nω/kT),kbeing
the Boltzmann constant andTthe Kelvin temperature. The probability that
the molecule is in the first excited state is

P 1 =

exp(−ω/kT)
∑∞
0 exp(−nω/kT)

=exp(−ω/kT)[1−exp(−ω/kT)]


kT

=

1. 054 × 10 −^34 × 4. 082 × 1014

1. 38 × 10 −^23 × 1 , 000

= 3. 1177

Therefore,P 1 =exp(− 3 .117)[1−exp(− 3 .1177)]
= 0. 042

2.61 The rotational energy state is given by


EJ=J

(J+1)^2

2 I

, J= 0 , 1 , 2 ...

The state with quantum number J is proportional to (2J+1) exp(−EJ/kT)
The factor (2J+1) arises from the J state.
N 0 /N 1 =(1/3) exp

(
^2 /IokT

)
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