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Ta b l e 2 . 22 Radiative parameters and the absorption coefficient for the spectral line center for
resonant radiative transitions in atoms of the first and second groups of the periodic table [8,
146].
v σ t ,10 7 cm 3 /s
k 0 ,10 5 cm 1
Element
Transition
λ ,nm
τ ,ns
g / g 0
1 2 S
2 2 P
H
!
121.57
1.60
3
0.516
8.6
1 1 S
2 1 P
He
!
58.433
0.56
3
0.164
18
2 2 S
3 2 P
Li
!
670.8
27
3
5.1
1.6
2 1 S
2 1 P
Be
!
234.86
1.9
3
9.6
1.4
3 2 S 1/2 !
3 2 P 1/2
Na
589.59
16
1
3.1
1.1
3 2 S 1/2 !
3 2 P 3/2
Na
589.0
16
2
4.8
1.4
3 1 S
3 1 P
Mg
!
285.21
2.1
3
5.5
3.4
4 2 S 1/2 !
4 2 P 1/2
K
769.0
27
1
4.1
0.85
4 2 S 1/2 !
4 2 P 3/2
K
766.49
27
2
6.3
1.1
4 1 S
4 1 P
Ca
!
422.67
4.6
3
7.3
2.5
4 2 S 1/2 !
4 2 P 1/2
Cu
327.40
7.0
1
1.1
2.1
4 2 S 1/2 !
4 2 P 3/2
Cu
324.75
7.2
2
1.7
2.8
4 1 S
4 1 P
Zn
!
213.86
1.4
3
3.3
4.8
5 2 S 1/2 !
5 2 P 1/2
Rb
794.76
28
1
3.9
0.91
5 2 S 1/2 !
5 2 P 3/2
Rb
780.03
26
2
6.2
1.2
5 1 S
5 1 P
Sr
!
460.73
6.2
3
9.4
1.7
5 2 S 1/2 !
5 2 P 1/2
Ag
338.29
7.9
1
1.1
2.0
5 2 S 1/2 !
5 2 P 3/2
Ag
328.07
6.7
2
1.7
2.9
5 1 S
5 1 P
Cd
!
228.80
1.7
3
3.3
4.5
6 2 S 1/2 !
6 2 P 1/2
Cs
894.35
31
1
5.3
0.77
6 2 S 1/2 !
6 2 P 3/2
Cs
852.11
27
2
8.1
1.0
6 1 S
6 1 P
Ba
!
553.55
8.5
3
9.0
1.9
6 2 S 1/2 !
6 2 P 1/2
Au
267.60
6.0
1
0.49
1.9
6 2 S 1/2 !
6 2 P 3/2
Au
242.80
4.6
2
0.75
4.2
6 1 S
6 1 P
Hg
!
184.95
1.3
3
2.2
5.7
Note that in the case under consideration, broadening of a spectral line is deter-
mined by atomic collisions and corresponds to the criterion
N 0 d 2
ω c
,
(2.150)
where
T ,which
allows us to ignore stimulated radiation processes. Using (2.145) for the absorption
cross section, we have for the absorption coefficient (2.149) in the spectral line
center
is a typical velocity of atoms. In addition, we assume
ω
v
c 2
ω
a 0
τ
k 0
D
N 0
σ ω
N 0
.
2
r
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