Up: Atomic data from the
Subsections
In the present work we have calculated all the E1, E2 and M1 transitions
within the n=2 complex for Z=6-28; this amounts to 2254 transitions.
The E2 and M1 transitions are of less importance than the considerably
larger E1s,
with the notable exception perhaps of the astrophysically relevant
forbidden transitions within the
P
ground term. They are nevertheless listed for database
purposes. The computed transition probabilities are listed in
Tables 3-25.
Comparing the present A-values with previous datasets
(see histograms in Fig. 4),
it is found that DT list 272 E1 transitions for Z=6-26 of which 77% agree
to the desired accuracy (10%), and 6 transitions show discrepancies larger
than 50%; namely, the
2s2p
S1/2-2s
2p
P
spin-allowed
transitions for Z=22 and Z=26 which are affected by the avoided crossing
and are discussed
![\begin{figure}
\centering
\includegraphics[]{1506f4.eps}\end{figure}](/articles/aas/full/1998/15/ds1506/Timg52.gif) |
Figure 4:
Histograms showing the percentage difference of the previously
computed transition probability datasets with respect to the present results.
a) DT, 272 A-values for Z=6-26 (excluding 6 A-values showing differences
greater than 50%).
b) MVGK, 686 A-values for Z=8-26 (excluding 32 A-values).
c) CKD, 1100 A-values for Z=7-28 (excluding
134 A-values for the same reason).
It can be concluded that the CKD dataset is of lower statistical reliability |
in Sect. 4.1; the
2p
D
2s2p
P
for Z=6 which
are
perturbed by intermixing n=3 states; and the
2s2p
P1/2-2s
2p
P
intercombination
transition for Z=6 (see Sect. 4.2).
MVGK list 686 E1 transitions for
Z=8-26, of which 70% agree with present A-values to 10% and 32 are
discrepant by more than 50%; namely, transitions affected by the
avoided crossing (Z>17);
2p
S
2s2p
D
intercombination
transitions for Z<18; and transitions for Z=8.
The dataset by CKD contains
1100 transitions for Z=7-28, mostly E1s but the E2 and
M1 transitions within the
P
ground term are also listed;
only 46% agree with the present dataset to within 10% and for 134 transitions
the discrepancies are larger than 50%. In general, large discrepancies are
found for: the low members of the sequence (Z<10); the transitions affected
by the avoided
crossing (e.g. 2s2p
S1/2-2s
2p
P
,2p
P
2s2p
S1/2 for Z>18); and the
intersystem transitions involving the
P
and
S
levels for low and intermediate Z.
From this comparison it is found that in the range Z=7-28, specially for
low Z, the CKD dataset differs considerably from the DT, MVGK and present
sets.
The present rates allow us to compute radiative lifetimes which can
also be compared with recent experiments for C II
(Reistad et
al. 1986 and Nandi et al. 1996) and N III
(Bengtsson et al. 1995). It is found that
our theoretical lifetimes lie within the experimental error bars.
We now discuss the problems leading to the larger discrepancies in an
attempt to estimate accuracy ratings.
Most of the present transition probabilities for spin-allowed transitions
should be accurate to 10%, with the exception of (i) a few transitions for
Z=6-7 where strong admixture with the low n=3 levels can lead to
sensitive A-values and (ii) transitions in highly ionised members of the
sequence that are
affected by strong relativistic couplings such as those that lead to
the avoided crossing of the 2s2p
S1/2 at
.For low Z, this assertion is supported by the excellent agreement
(
10%) obtained with the detailed computations by
Nussbaumer & Storey (1981),
Lennon et
al. (1985) and Froese Fischer (1994) on C II;
Nussbaumer & Storey (1979), Bell et
al. (1995) and Brage et al. (1995) on N III; and
Brage et al. (1996) on O IV.
We are therefore not worried, for instance, with the 35% and 40%
discrepancies found with DT for the spin-allowed transitions
2p
S
2s2p
P
in N III and
2s2p
P3/2-2s
2p
P
in O IV, respectively.
As mentioned before, for high Z a notably problematic transition is
2s2p
S1/2- 2s
2p
P
which, as seen
in Fig. 5a, is strongly perturbed by the avoided crossing.
Due to the good overall agreement between DT, MVGK and present data,
our A-values for Z<17 can be expected to be well within 10%, but for
an accuracy rating would be uncertain. It would have been useful to have
A-values for this transition for Z=23,25,27 from DT and
MVGK, as these would have provided a
better picture of the troublesome region.
A similar situation is found for the
2p
P
2s2p
S1/2 (Fig. 5b) and
2p
P
2s2p
P1/2
(Fig. 5c) transitions, where the destructive perturbation caused by the
avoided crossing leads to poor accuracy ratings for the range
17<Z<22. The accuracy of the A-value at Z=6 for the former transition
(see Fig. 5b) is also questionable as it seems to be perturbed by a state
belonging to the n=3 configurations. A similar situation is encountered
in C II for the transitions 2p
D
2s2p
P
.As shown in Fig. 5d,
destructive interference is also found for
in the 2s2p
D3/2-2s
2p
P
transition,
causing the accuracy of the rates for Z>26 to be of lower quality.
For most of these difficult transitions (see Figs. 5a-c) the data by CKD are
consistently discrepant (differences are greater than 20%) with DT, MVGK and
the
present dataset throughout the sequence. Also the data by MVGK begin to show
significant differences from the present ones for Z<12 where correlation
effects are more conspicuous and the present CI method is expected to
perform with higher reliability.
![\begin{figure}
\centering
\includegraphics[]{1506f5.eps}\end{figure}](/articles/aas/full/1998/15/ds1506/Timg65.gif) |
Figure 5:
A-values (s ) for troublesome spin-allowed transitions
as a function of Z. a) .b) .c) .d) .Filled squares: present results. Open circles: DT. Open triangles: CKD.
Open squares: MVGK |
In contrast to the good rating assigned to most spin-allowed
transitions, the accuracy for the intercombination transitions is noticeably
poorer. The typical situation is illustrated in Fig. 6 with the important
2s2p
P
2s
2p
P
transitions. With regard to the DT, CKD, MVGK and present datasets,
differences larger than 10% begin to show up for these transitions
for Z<20, and for Z<10 the situation becomes critical.
In order to assign ratings to this transition array,
we compare in Table 26 present rates for Z=6-8 with DT, CKD, MVGK, detailed
single-system calculations and recent experiments. It may be appreciated
that differences between the present data and DT are as large as a factor of 2
for C II and diminish
to
% for N III and O IV. The situation with respect to
CKD is even considerably
worse as the differences reach an order of magnitude. Discrepancies with
MVGK for O IV are generally small except for
where
they reach a factor of 2. A comparison of the present results
with the detailed calculations and experiment allows us to
assign a realistic 20% rating to the present A-values
for Z=6-8. Furthermore, a recent measurement of the lifetime of the
level in Fe XXII by Hutton et al. (1997)
of 14.8
1.0 ns is in excellent agreement with those given by DT (14.2 ns),
CKD (14.3 ns), MVGK (13.4 ns) and the present work (13.7 ns). Therefore the
20% rating for these transitions can be safely extended to the whole sequence.
The situation with the
transitions
is even more
serious since, as shown in Fig. 7, the rates can be strongly perturbed by
the avoided crossing. Taking into account the good agreement between the
present data and those by Bell et al. (1995) for Z=7
we are encouraged to also maintain the 20% rating for such transitions except
for Z=6 and around the perturbation (
).
For the intersystem transitions involving the
, in spite of very large differences found
with CKD for Z<20, we find good agreement with MVGK (
%) for
Z>12. However, as shown in Fig. 8, the situation is complicated for
Z<9 where very significant differences are encountered with the detailed
calculations. For this range we do not attempt a rating assignment.
![\begin{figure}
\centering
\includegraphics[]{1506f7.eps}\vspace{-4mm}\end{figure}](/articles/aas/full/1998/15/ds1506/Timg81.gif) |
Figure 7:
A-values (s ) for the intercombination transition
plotted
as a function of Z.
a) showing
the perturbation caused by the avoided crossing
at . b) showing large
differences with MVGK for the whole sequence.
Filled squares: present results. Open triangles: CKD.
Open squares: MVGK. Open circles: Bell et al (1995) |
![\begin{figure}
\centering
\includegraphics[]{1506f8.eps}\end{figure}](/articles/aas/full/1998/15/ds1506/Timg85.gif) |
Figure 8:
A-values (s ) for the
intercombination transitions plotted
as a function of Z.
a) .b) .Filled squares: present results. Open triangles: CKD.
Open squares: MVGK. Open circles: Bell et al. (1995). Asterix:
Nussbaumer & Storey (1981).
It may be seen that the
agreement for Z<9 is poor and that large discrepancies exist with
CKD for even fairly high Z |
The only forbidden transitions that have been previously
considered for the B-like ions are the E2 and M1 transitions
within the 2s
2p
P
term. In this context present results
are in excellent agreement (better than 10%) with those by
Froese Fischer (1983). Taking this outcome as a reference, the
A-values listed by CKD are found to be highly unreliable for Z<12.
Table 3:
Transition probabilities (s-1) for C II
|
Table 4:
Transition probabilities (s-1) for N III
|
Table 5:
Transition probabilities (s-1) for O IV
|
Table 6:
Transition probabilities (s-1) for F V
|
Table 7:
Transition probabilities in s-1 for Ne VI
|
Table 8:
Transition probabilities (s-1) for Na VII
|
Table 9:
Transition probabilities (s-1) for Mg VIII
|
Table 10:
Transition probabilities (s-1) for Al IX
|
Table 11:
Transition probabilities (s-1) for Si X
|
Table 12:
Transition probabilities (s-1) for P XI
|
Table 13:
Transition probabilities (s-1) for S XII
|
Table 14:
Transition probabilities (s-1) for Cl XIII
|
Table 15:
Transition probabilities (s-1) for Ar XIV
|
Table 16:
Transition probabilities (s-1) for K XV
|
Table 17:
Transition probabilities (s-1) for Ca XVI
|
Table 18:
Transition probabilities (s-1) for Sc XVII
|
Table 19:
Transition probabilities (s-1) for Ti XVIII
|
Table 20:
Transition probabilities (s-1) for V XIX
|
Table 21:
Transition probabilities (s-1) for Cr XX
|
Table 22:
Transition probabilities (s-1) for Mn XXI
|
Table 23:
Transition probabilities (s-1) for Fe XXII
|
Table 24:
Transition probabilities (s-1) for Co XXIII
|
Table 25:
Transition probabilities (s-1) for Ni XXIV
|
Table 26:
Comparison of present A-values (s
) for the
intercombination transitions in Z=6-8 with other theoretical results
and experiment.
a) DT.
b) Nussbaumer & Storey (1981).
c) Lennon et al. (1985).
d) Froese Fischer (1994).
e) Nussbaumer & Storey (1979).
f) Bell et al. (1995).
g) Brage et al. (1995).
h) CKD.
i) Brage et al. (1996).
j) MVGK.
Experiment by Fang et al. (1993a,b); the experimental uncertainties are
given by the quantities in brackets.
From the present comparison, a 20% accuracy rating is assigned to the
present data
|
Up: Atomic data from the
Copyright The European Southern Observatory (ESO)