In 1s22s2nl (C II), 1s22snl (C III) and 1s2nl (C IV) configurations, the outer nl electron moves in the resultant field of the nucleus and the inner electrons. In such cases, the deviations between the observed term energies and the exact hydrogen-like values, caused by small core-penetration and polarization effects, are accurately described by the Ritz formalism. In this semi-empirical technique, discussed in detail by Edlén (1964) and more recently by Drake (1994), the term energies are written as
where is the ionization energy, Ry is the reduced mass Rydberg
constant (Ry = 109732.3 cm-1 for carbon),
is the net charge of the core
(
= 2, 3, 4 for C II, C III and C IV respectively) and n* is the
effective principal quantum number given by
(n,l) is the so-called quantum defect which is strongly
dependent on the l-quantum number but only weakly on n and which can
be expressed, in the Ritz formalism, by
The energies of high l (non-penetrating) states can also be given to a good approximation by the polarization formula (Edlén 1964):
The hydrogenic, , and relativistic,
, terms are given by
where is the fine structure constant. The polarization
term,
, can be written as
with
and
In Eq. (7), the factors A and k can be expressed respectively by
and
where is the dipole polarizability of the atomic core in
units
of a03 and
represents the quadrupole polarizability of the core
in units of a05.
Using the values 196664.7 and 386241.0 cm-1 (Moore 1970) for the ionization
energies of C II and C III respectively and the observed term energies deduced
from the compilation of Bashkin & Stoner (1975), new Ritz
formulae were derived
for the 1s22s2nf, 1s22s2ng (C II) and 1s22sng (C III) series.
The Ritz parameters (a, b, c) obtained in the present work as well as the standard
deviations between the experimental term energies and those calculated from the
Ritz formulae are given in Table 1 (click here). For the 1s22s2nh-ni (C II),
1s22snh-nk (C III) and 1s2nf-nk (C IV) series, the polarization
Eq. (4) was used. In the cases of C II and C III, only the dipole contribution
was retained (k was set equal to zero) with the dipole polarizabilities
= 3.77 and 3.46 a03 respectively. These values were derived
from the oscillator strengths published for C III and C IV using the following formula:
where (Ei-E0/Ry) are the transition energies (in Rydbergs) for lines connecting
the ground level in C III and C IV and f0i the corresponding oscillator
strengths taken from the Opacity Project (the Opacity Project Team 1995)
and corrected with experimental wavelengths by Verner et al. (1994).
In the case of C IV, we used the
polarization Eq. (4) including both dipole and quadrupole polarizabilities
published recently by Tunklev et al. (1997), i.e. a03
and
= 0.00111 a05, and the ionization energy
= 520175.9 cm-1
obtained by the same authors.
Ion | Series | a | b | c | standard deviation |
C II | nf 2F![]() | 0.028958 | -0.221105 | 0.828474 | 0.50 cm-1 |
C II | ng 2G | 0.006837 | -0.040060 | -0.242426 | 0.32 cm-1 |
C III | ng 1,3G | 0.026138 | -0.672472 | 6.720485 | 0.41 cm-1 |
The term energies calculated in our work are compared with available
experimental values in Table 2 (click here). Examining this table, it is seen that the
discrepancies between both sets of values are very small (the mean difference
being 0.8 cm-1) if we except the 6h 2H term belonging to C II. For
this term, the difference between our value, calculated using the polarization
formula, and the measured energy (Bashkin & Stoner 1975) reaches 64.6 cm-1
which probably means that this particular term energy should be redetermined
experimentally.
Tables 3 (click here), 4 (click here) and 5 (click here) contain the term energies adopted in the present study for the nf, ng, nh, ni series in C II, for the ng, nh, ni, nk series in C III and for the nf, ng, nh, ni, nk series in C IV respectively for n up to 30. Following the hereabove discussion, the mean uncertainty affecting our predicted values in these series should not exceed 1 cm-1.
Ion | Term | Experiment | This work | ![]() |
C II | 4f 2F![]() | 168978.8a | 168979.3c | -0.5 |
C II | 5f 2F![]() | 178956.4a | 178956.5c | -0.1 |
C II | 6f 2F![]() | 184376.5a | 184376.5c | 0.0 |
C II | 7f 2F![]() | 187642.0a | 187643.3c | -1.3 |
C II | 5g 2G | 179073.5a | 179073.5c | 0.0 |
C II | 6g 2G | 184449.7a | 184449.7c | 0.0 |
C II | 7g 2G | 187691.8a | 187691.8c | 0.0 |
C II | 8g 2G | 189794.6a | 189795.9c | -1.3 |
C II | 6h 2H![]() | 184529.9a | 184465.3d | 64.6 |
C II | 7h 2H![]() | 187701.0a | 187702.2d | -1.2 |
C III | 5g 1G | 346579.3a | 346579.9c | -0.6 |
C III | 5g 3G | 346579.3a | 346579.9c | -0.6 |
C III | 6g 1G | 358692.2a | 358692.6c | -0.4 |
C III | 6g 3G | 358692.3a | 358692.6c | -0.3 |
C III | 7g 3G | 365998.4a | 365998.6c | -0.2 |
C III | 6h 3H![]() | 358776.3a | 358775.8d | 0.5 |
C IV | 4f 2F![]() | 410431.5b | 410431.3d | 0.2 |
C IV | 5f 2F![]() | 449941.3b | 449939.8d | 1.5 |
C IV | 6f 2F![]() | 471402.4b | 471401.3d | 1.1 |
C IV | 7f 2F![]() | 484341.9b | 484341.8d | 0.1 |
C IV | 8f 2F![]() | 492740.8b | 492740.7d | 0.1 |
C IV | 5g 2G | 449945.2b | 449945.0d | 0.2 |
C IV | 6g 2G | 471405.8b | 471404.5d | 1.3 |
C IV | 7g 2G | 484345.6b | 484343.9d | 1.7 |
C IV | 8g 2G | 492743.8b | 492742.1d | 1.7 |
C IV | 6h 2H![]() | 471406.8a | 471405.3d | 1.5 |
C IV | 7h 2H![]() | 484345.8a | 484344.4d | 1.4 |
C IV | 8h 2H![]() | 492743.8a | 492742.4d | 1.4 |
C IV | 9h 2H![]() | 498501.4a | 498500.1d | 1.3 |
C IV | 7i 2I | 484346.0a | 484344.7d | 1.3 |
C IV | 8i 2I | 492743.9a | 492742.6d | 1.3 |
C IV | 9i 2I | 498501.4a | 498500.2d | 1.2 |
a Bashkin & Stoner (1975). | ||||
b Tunklev et al. (1997). | ||||
c Calculated using the Ritz formula. | ||||
d Calculated using the polarization formula. | ||||
n | nf 2F![]() | ng 2G | nh 2H![]() | ni 2I |
4 | 168978.8a | |||
5 | 178956.4a | 179073.5a | ||
6 | 184376.5a | 184449.7a | 184529.9a | |
7 | 187642.0a | 187691.8a | 187701.0a | 187705.1c |
8 | 189762.2b | 189794.6a | 189803.0c | 189805.1c |
9 | 191214.0b | 191238.2b | 191243.3c | 191244.8c |
10 | 192251.8b | 192269.8b | 192273.6c | 192274.6c |
11 | 193019.2b | 193032.9b | 193035.8c | 193036.6c |
12 | 193602.6b | 193613.3b | 193615.5c | 193616.1c |
13 | 194056.4b | 194064.9b | 194066.6c | 194067.1c |
14 | 194416.3b | 194423.1b | 194424.6c | 194425.0c |
15 | 194706.6b | 194712.2b | 194713.3c | 194713.7c |
16 | 194944.1b | 194948.7b | 194949.7c | 194949.9c |
17 | 195140.9b | 195144.7b | 195145.5c | 195145.7c |
18 | 195305.7b | 195309.0b | 195309.6c | 195309.8c |
19 | 195445.2b | 195448.0b | 195448.5c | 195448.7c |
20 | 195564.3b | 195566.6b | 195567.1c | 195567.3c |
21 | 195666.7b | 195668.8b | 195669.2c | 195669.3c |
22 | 195755.5b | 195757.3b | 195757.6c | 195757.7c |
23 | 195832.9b | 195834.5b | 195834.8c | 195834.9c |
24 | 195900.9b | 195902.2b | 195902.5c | 195902.6c |
25 | 195960.8b | 195962.0b | 195962.3c | 195962.4c |
26 | 196014.0b | 196015.1b | 196015.3c | 196015.4c |
27 | 196061.3b | 196062.3b | 196062.5c | 196062.6c |
28 | 196103.7b | 196104.6b | 196104.8c | 196104.8c |
29 | 196141.8b | 196142.5b | 196142.7c | 196142.8c |
30 | 196176.1b | 196176.8b | 196176.9c | 196177.0c |
a Deduced from the experimental energy levels | ||||
(Bashkin & Stoner 1975). | ||||
b Calculated from the Ritz formula (see text). | ||||
c Calculated from the polarization formula (see text). | ||||
n | ng 1,3G | nh 1,3H![]() | ni 1,3I | nk 1,3K![]() |
5 | 346579.3a | |||
6 | 358692.2a | 358776.3a | ||
7 | 365998.4a | 366063.8c | 366077.5c | |
8 | 370743.2b | 370794.1c | 370803.6c | 370807.1c |
9 | 373997.4b | 374037.0c | 374043.8c | 374046.4c |
10 | 376325.4b | 376356.4c | 376361.5c | 376363.5c |
11 | 378047.8b | 378072.5c | 378076.3c | 378077.8c |
12 | 379357.8b | 379377.6c | 379380.6c | 379381.7c |
13 | 380377.1b | 380393.2c | 380395.5c | 380396.5c |
14 | 381185.8b | 381198.9c | 381200.9c | 381201.6c |
15 | 381838.1b | 381849.0c | 381850.6c | 381851.2c |
16 | 382371.8b | 382381.0c | 382382.3c | 382382.8c |
17 | 382814.1b | 382821.8c | 382822.9c | 382823.3c |
18 | 383184.7b | 383191.3c | 383192.2c | 383192.6c |
19 | 383498.3b | 383503.9c | 383504.7c | 383505.0c |
20 | 383766.0b | 383770.9c | 383771.5c | 383771.8c |
21 | 383996.3b | 384000.6c | 384001.1c | 384001.4c |
22 | 384195.9b | 384199.6c | 384200.1c | 384200.3c |
23 | 384370.1b | 384373.3c | 384373.8c | 384373.9c |
24 | 384522.9b | 384525.8c | 384526.1c | 384526.3c |
25 | 384657.7b | 384660.3c | 384660.6c | 384660.7c |
26 | 384777.2b | 384779.5c | 384779.8c | 384779.9c |
27 | 384883.8b | 384885.8c | 384886.1c | 384866.2c |
28 | 384979.0b | 384980.9c | 384981.1c | 384981.2c |
29 | 385064.6b | 385066.3c | 385066.5c | 385066.6c |
30 | 385141.8b | 385143.3c | 385143.5c | 385143.6c |
a Deduced from the experimental energy levels | ||||
(Bashkin & Stoner 1975). | ||||
b Calculated from the Ritz formula (see text). | ||||
c Calculated from the polarization formula (see text). | ||||
n | nf 2F![]() | ng 2G | nh 2H![]() | ni 2I | nk 2K![]() |
4 | 410431.5a | ||||
5 | 449941.3a | 449945.2a | |||
6 | 471402.4a | 471405.8a | 471406.8b | ||
7 | 484341.9a | 484345.6a | 484345.8b | 484346.0b | |
8 | 492740.8a | 492743.8a | 492743.8b | 492743.9b | 492742.7c |
9 | 498498.8c | 498499.8c | 498501.4b | 498501.4b | 498500.3c |
10 | 502617.6c | 502618.3c | 502618.5c | 502618.6c | 502618.6c |
11 | 505665.0c | 505665.5c | 505665.7c | 505665.7c | 505665.8c |
12 | 507982.7c | 507983.2c | 507983.3c | 507983.3c | 507983.4c |
13 | 509786.5c | 509786.8c | 509786.9c | 509787.0c | 509787.0c |
14 | 511217.7c | 511218.0c | 511218.1c | 511218.1c | 511218.1c |
15 | 512372.4c | 512372.6c | 512372.6c | 512372.7c | 512372.7c |
16 | 513317.3c | 513317.5c | 513317.6c | 513317.6c | 513317.6c |
17 | 514100.5c | 514100.7c | 514100.7c | 514100.7c | 514100.7c |
18 | 514756.8c | 514756.9c | 514757.0c | 514757.0c | 514757.0c |
19 | 515312.2c | 515312.4c | 515312.4c | 515312.4c | 515312.4c |
20 | 515786.5c | 515786.6c | 515786.6c | 515786.6c | 515786.6c |
21 | 516194.6c | 516194.6c | 516194.7c | 516194.7c | 516194.7c |
22 | 516548.3c | 516548.3c | 516548.4c | 516548.4c | 516548.4c |
23 | 516856.9c | 516856.9c | 516856.9c | 516857.0c | 516857.0c |
24 | 517127.7c | 517127.7c | 517127.8c | 517127.8c | 517127.8c |
25 | 517366.7c | 517366.7c | 517366.7c | 517366.7c | 517366.7c |
26 | 517578.6c | 517578.7c | 517578.7c | 517578.7c | 517578.7c |
27 | 517767.5c | 517767.5c | 517767.5c | 517767.5c | 517767.5c |
28 | 517936.4c | 517936.4c | 517936.5c | 517936.5c | 517936.5c |
29 | 518088.2c | 518088.2c | 518088.2c | 518088.2c | 518088.2c |
30 | 518225.1c | 518225.1c | 518225.1c | 518225.1c | 518225.1c |
a Deduced from the experimental energy levels | |||||
(Tunklev et al. 1997). | |||||
b Deduced from the experimental energy levels | |||||
(Bashkin & Stoner 1975). | |||||
c Calculated from the polarization formula (see text). | |||||