134 3 Quantum Mechanics – II
Table 3.2Some selected eigen functions of hydrogen atom
State NLm u
1S 1 0 0 Ane−x
2S 2 0 0 Ane−x(1−x)
2P 2 1 0 Ane−xxcosθ
2P 2 1 ± 1 An
e−xxsinθe±iφ
√
2
3S 3 0 0 Ane−x(
1 − 2 x+^2 x
2
3)3P 3 1 0 Ane−x√
2
3
x(2−x)cosθ3P 3 1 ± 1 Ane−x
1
√
3x(2−x)sinθe±iΦ3d 3 2 0 Ane−x
1
2√
3x^2 (3 cos^2 θ−1)3d 3 2 ± 1 Ane−x
x^2
√
3sinθcosθe±iφ3d 3 2 ± 2 Ane−x
1
2√
3x^2 sin^2 θe±iφwherex=r/na 0 ;An=(1/√
π)(1/na 0 )^3 /^2 ;a 0 =^2 /me^2 is the Bohr radiusMolecular spectra
Three types:
i. Electronic (Visible and ultraviolet)
ii. Vibrational (Near infrared)
iii. Rotational (Far infrared)
Because electron mass is much smaller than the nuclear mass, the three types of
motion can be treated separately. This is the Born–Oppenheimer approximation, in
which the completeψ– function appears as the product of the wave functions of the
three types of motion, and the total energy as the sum of the energies of electronic
motion, of vibration, and of rotation.
ψ=ψel·ψv·ψrot
E=Eel+Evibr+Erot (3.17)
Eel:Evibr:Erot=1:√
m/M:m/M (3.18)wheremandMare the mass of electron and nucleus.
ThusEelEvibrErot.
The rotational energy
ER=
^2
2 I 0
·J(J+1) (3.19)
Permanent dipole moment is necessary, molecules with center of symmetry such
as C 2 H 2 or O 2 have no dipole moment and do not exhibit rotational spectrum.