For the solution of the inelastic scattering
problem we employed the R-matrix technique (Burke et al.
1971; Berrington et al. 1987; Burke & Berrington
1993; Hummer et al. 1993). This method has
been implemented in the Queen's University Belfast R-matrix suite of
programs, the latest and most updated version of which is thoroughly
described in Berrington et al. (1995).
The scattering calculation is carried out in LS coupling, but the mass and Darwin relativistic energy corrections are included (Saraph & Storey 1996). The transformation to pair coupling including the effects of intermediate coupling in the target are included as discussed in the first IRON Project paper (Hummer et al. 1993).
Two sets of R-matrix calculations have been performed in order to analyse critically previous computations and to provide new electron scattering data for FeXII. These will be described in the two following subsections.
Our initial set of R-matrix calculations was aimed at studying
the effect of varying target representations on collisional data and,
in particular, on the resonance structure of the collision strengths
below the highest excitation threshold in the target. As in Tayal et al. (1987) the lowest seven LS coupling terms,
,
,
,
,
,
,
, were included
in the expansion of the total wavefunction for the target. The
energies for these excitation thresholds were calculated as averages
of observed values, weighted over the fine-structure levels, and are
tabulated as the first seven entries in Table 5 (click here).
Experimental energies were preferred to theoretical values in order to
determine as accurately as possible the positions of the convergence
limits for Rydberg series of resonances. The seven target terms were
represented by CI expansions constructed with a common set of radial
functions, describing the radial charge distribution of the
target. Three different combinations of seven orthogonal one-electron
orbitals 1s, 2s, 2p, 3s, 3p, 3d and 4f were selected, in order to
match as closely as possible the details of Tayal et al. (1987)
calculation. In the first computation radial waves were obtained in
the way described in Sect. 2 (click here) by including nine configurations in the
basis set,
,
,
,
,
,
,
,
,
, where the
correlation
orbital was chosen of Thomas-Fermi type (
).
The bar over the principal quantum number n indicates the correlation
nature of the orbital. In the second calculation we added the two extra
configurations
and
to the basis set, hence investigating the
effect of a
correlation orbital of hydrogenic type
(
). In these two calculations the size of the
R-matrix "box'', within which exchange and
correlation
interactions are treated explicitly by performing a CI expansion of the
collision complex wavefunction, was set at a = 3.22 a.u.
and 16 continuum orbitals were included to ensure
convergence for electron energies spanning the range 0.4 to 100 Ry. In
our third calculation the same set of eleven configurations was kept
in the basis expansion, but this time with 3d and 4f orbitals of
spectroscopic type. Due to the presence of a diffuse 4f spectroscopic
orbital, compared to the more contracted correlation type equivalent
(see Table 6 (click here)),
it was necessary to increase a
to 5.34 a.u. and to include a total of 24 continuum orbitals
in the problem. The wavefunction for the
collision
complex was, in all three cases, expanded on a basis set of 72
intermediate states, including partial waves of singlet, triplet and
quintet spin multiplicities, both odd and even parities and with total
orbital angular momenta L from 0 to 12, which corresponds to an
expansion in intermediate coupling with values of J=L+S from 0 to
10. The variation of the collision strength, as a
function of electron energy, with target structure is
presented in the three plots of Fig. 1 (click here), Fig. 2 (click here) and
Fig. 3 (click here), corresponding to the three calculations described above.
Here collision strengths for the fine-structure forbidden transition
are plotted in the energy
region between the
and
target thresholds, revealing the complicated pattern of different
series of resonances. A very fine energy mesh of
was chosen to delineate this complex resonance structure. Clearly it
is the correlation nature of the
orbital which
introduces the broad resonant features visible in Fig. 2 (click here).
This important point will be further discussed in Sect. 4 (click here).
Figure 1: Collision strength for FeXII forbidden transition
.
R-matrix calculation
including 7 LS coupling target terms with
correlation orbital
Figure 2: Collision strength for FeXII forbidden transition
.
R-matrix calculation
including 7 LS coupling target terms with
,
correlation orbitals
Figure 3: Collision strength for FeXII forbidden transition
.
R-matrix calculation
including 7 LS coupling target terms with 3d, 4f spectroscopic orbitals
Configuration | Term | E(Ry) | ||
3s23p3 | 4S![]() | 0.0 | ||
2D![]() | 0.40346 | |||
2P![]() | 0.71424 | |||
3s3p4 | 4P | 2.55069 | ||
2D | 3.10674 | |||
2P | 3.56514 | |||
2S | 3.73984 | |||
3s23p23d | (3P)4F | 3.91364 | ||
(3P)4D | 4.03242 | |||
(1D)2F | 4.08134 | |||
(1D)2G | 4.49761 | |||
(3P)2P | 4.60933 | |||
(3P)4P | 4.69420 | |||
(1S)2D | 4.85952 | |||
(1D)2D | 5.05186 | |||
(1D)2S | 5.22953 | |||
(1D)2P | 5.23802 | |||
(3P)2F | 5.27875 | |||
(3P)2D | 5.50906 | |||
|
Orbital | 3d, 4f spectroscopic | ![]() ![]() ![]() ![]() | ![]() ![]() ![]() ![]() | ![]() ![]() ![]() ![]() | ![]() ![]() ![]() ![]() | |||||
3d | 0.68862 | 0.69790 | 0.69789 | 0.67926 | 0.67929 | |||||
4f | 1.42519 | 0.83966 | 0.84152 | 0.83838 | 0.83985 | |||||
|
A higher quality set of collisional data for FeXII was
obtained by increasing the size of the expansion for both the target
and the system total wavefunctions. In a new, ab
initio R-matrix calculation we extended the target representation
by including in the target the 12 LS coupling terms of the
configuration,
(
, (
, (
, (
,
(
, (
, (
(
,
(
, (
, (
, (
.
The list of energies for the total set of 19 LS coupling target terms
employed in this calculation is given in Table 5 (click here). The lowest four
energy values for the
configuration (italic type)
have been calculated from the corrected level energies presented in
Table 3 (click here), due to lack of observed energies for the corresponding
fine-structure levels, as discussed in
Sect. 2 (click here). It should be noted that the energy value for the
(
term in Table 5 (click here) does not
correspond to the experimental energy given in Table 3 (click here). This
observed value was modified in order to preserve the theoretical ordering of
the term energies, as determined by the R-matrix computer code, where the
(
term falls in between the (
and
(
terms. Failing to preserve the theoretical ordering can
lead to indexing problems in the R-matrix program. The correction was
taken as the difference between the
calculated and experimental energy values for the (
term. The radial waves describing the distribution of the bound
electrons in the target were obtained with the twelve configuration
basis of set 2 in Table 1 (click here). This represented a good compromise
between target quality and computational speed. The scaling parameters for
the potential employed in the set 2 structure calculation are
,
,
,
,
,
. A total of 16
continuum orbitals was included and the inner region boundary was set at
3.09 a.u. An initial expansion of the
system total
wavefunction on a basis set including partial waves with total angular
momenta
turned out to be insufficient to ensure convergence
of the collision strengths for some of the forbidden transitions at
high electron energies. The final 19 state calculation was
therefore carried out for all partial waves with
, again for
both odd and even parities and singlet, triplet and quintet spin
states, including a total of 102 intermediate states. In Fig. 4 (click here) we
present results for the same transition illustrated in Fig. 1 (click here), this
time spanning the whole closed channel energy range, going from the
lowest (
) to the
highest (
) excitation threshold.
Figure 4: Collision strength for FeXII forbidden transition
.
R-matrix calculation
including 19 LS coupling target terms
The rapidly varying behaviour of
the collision strength as a function of electron energy is again
noticeable, this time enriched by the additional series of resonances
converging to the extra thresholds belonging to the
configuration.
A top-up procedure to estimate the contributions to the collision
strengths from partial waves with
was adopted in the open
channel energy region, above the highest excitation threshold. By
assuming that the partial collision strengths form a geometric series
with a geometric scaling factor equal to the ratio of the last two
adjacent terms explicitly included, we obtain for the contribution, S,
from
This top-up procedure was found to be
appropriate for the ten optically forbidden transitions within the
ground configuration, with a maximum correction for
of
at the highest electron
energy considered (100 Ry). At the lowest energy in the open channel
region (6 Ry) the maximum correction due to
is found to be
.
Below 6 Ry, no top-up is considered necessary.
However for the optically allowed transitions
the contribution from predicted by Eq. (1)
is much larger (
).
Alternative top-up techniques are needed and results for these
transitions will be presented elsewhere. Final collision strength
values
for the forbidden
transitions between the five levels of the
ground
configuration are presented in Table 7 (click here), on a grid of energy points
above the highest excitation threshold.
Transition | E(Ry) | |||||||||||||
| 6.5 | 10 | 15 | 20 | 30 | 50 | 100 | |||||||
4S![]() ![]() | 0.055 | 0.047 | 0.038 | 0.032 | 0.024 | 0.016 | 0.011 | |||||||
4S![]() ![]() | 0.086 | 0.073 | 0.061 | 0.052 | 0.041 | 0.030 | 0.021 | |||||||
4S![]() ![]() | 0.009 | 0.007 | 0.005 | 0.004 | 0.003 | 0.001 | 0.001 | |||||||
4S![]() ![]() | 0.017 | 0.013 | 0.009 | 0.007 | 0.004 | 0.002 | 0.001 | |||||||
2D![]() ![]() | 0.170 | 0.153 | 0.136 | 0.125 | 0.111 | 0.098 | 0.088 | |||||||
2D![]() ![]() | 0.295 | 0.291 | 0.286 | 0.288 | 0.286 | 0.290 | 0.290 | |||||||
2D![]() ![]() | 0.203 | 0.197 | 0.191 | 0.190 | 0.187 | 0.186 | 0.186 | |||||||
2D![]() ![]() | 0.223 | 0.219 | 0.214 | 0.215 | 0.213 | 0.215 | 0.216 | |||||||
2D![]() ![]() | 0.675 | 0.665 | 0.652 | 0.655 | 0.650 | 0.656 | 0.658 | |||||||
2P![]() ![]() | 0.068 | 0.062 | 0.055 | 0.050 | 0.045 | 0.040 | 0.036 | |||||||
|
Electron excitation rates, obtained by averaging collision cross
sections over a Maxwellian distribution of electron energies, are
better represented in terms of effective (or thermally
averaged) collision strengths, given by
where Ej is the colliding electron kinetic energy relative to
the upper level j of the transition.
Transition | ![]() | ||||||||||
4 | 6 | 8 | 10 | 12 | 14 | 16 | 18 | 20 | 25 | 30 | |
4S![]() ![]() | 0.268 | 0.227 | 0.196 | 0.174 | 0.157 | 0.143 | 0.132 | 0.123 | 0.115 | 0.100 | 0.088 |
4S![]() ![]() | 0.268 | 0.233 | 0.207 | 0.187 | 0.171 | 0.158 | 0.148 | 0.139 | 0.131 | 0.117 | 0.106 |
4S![]() ![]() | 0.074 | 0.063 | 0.055 | 0.048 | 0.043 | 0.039 | 0.035 | 0.032 | 0.030 | 0.025 | 0.022 |
4S![]() ![]() | 0.304 | 0.257 | 0.219 | 0.190 | 0.168 | 0.150 | 0.136 | 0.124 | 0.114 | 0.096 | 0.082 |
2D![]() ![]() | 2.375 | 1.989 | 1.699 | 1.482 | 1.315 | 1.184 | 1.078 | 0.991 | 0.918 | 0.778 | 0.680 |
2D![]() ![]() | 0.763 | 0.679 | 0.617 | 0.570 | 0.535 | 0.507 | 0.485 | 0.466 | 0.451 | 0.423 | 0.403 |
2D![]() ![]() | 1.418 | 1.236 | 1.084 | 0.966 | 0.874 | 0.800 | 0.740 | 0.691 | 0.650 | 0.570 | 0.514 |
2D![]() ![]() | 0.556 | 0.490 | 0.444 | 0.411 | 0.385 | 0.366 | 0.350 | 0.337 | 0.327 | 0.307 | 0.293 |
2D![]() ![]() | 1.779 | 1.572 | 1.421 | 1.311 | 1.227 | 1.162 | 1.110 | 1.068 | 1.032 | 0.966 | 0.919 |
2P![]() ![]() | 1.241 | 1.082 | 0.940 | 0.826 | 0.736 | 0.663 | 0.604 | 0.555 | 0.514 | 0.434 | 0.378 |
|
Transition | ![]() | |||||||||||||
4 | 5 | 6 | 7 | 8 | 9 | 10 | ||||||||
4S![]() ![]() | 0.0732 | 0.0631 | 0.0559 | 0.0505 | 0.0463 | 0.0429 | 0.0401 | |||||||
4S![]() ![]() | 0.0901 | 0.0796 | 0.0720 | 0.0663 | 0.0617 | 0.0580 | 0.0549 | |||||||
4S![]() ![]() | 0.0175 | 0.0147 | 0.0126 | 0.0111 | 0.0100 | 0.0090 | 0.0083 | |||||||
4S![]() ![]() | 0.0642 | 0.0529 | 0.0450 | 0.0392 | 0.0347 | 0.0312 | 0.0283 | |||||||
2D![]() ![]() | 0.5487 | 0.4655 | 0.4080 | 0.3658 | 0.3335 | 0.3079 | 0.2872 | |||||||
2D![]() ![]() | 0.3764 | 0.3600 | 0.3488 | 0.3407 | 0.3345 | 0.3297 | 0.3258 | |||||||
2D![]() ![]() | 0.4399 | 0.3929 | 0.3606 | 0.3370 | 0.3190 | 0.3048 | 0.2934 | |||||||
2D![]() ![]() | 0.2751 | 0.2638 | 0.2561 | 0.2505 | 0.2463 | 0.2430 | 0.2403 | |||||||
2D![]() ![]() | 0.8580 | 0.8199 | 0.7940 | 0.7752 | 0.7609 | 0.7497 | 0.7407 | |||||||
2P![]() ![]() | 0.3020 | 0.2538 | 0.2205 | 0.1960 | 0.1773 | 0.1625 | 0.1505 | |||||||
|
We have integrated our collision strengths using the linear
interpolation technique described in Burgess & Tully (1992)
and results are tabulated in Table 8 (click here) and Table 9 (click here) for two
different temperature ranges. In integrating the collision strengths we
made the assumption , i.e. constant
at energies
above the last calculated point. The contribution coming from this
energy region to the total
increases with
and is generally
. When it is
we used italic
type in Table 9 (click here). For the transitions
, in particular, this contribution can be as high as
at the
highest temperatures. However, from Table 7 (click here) we see that the
assumption of constant
at high energies,
particularly for the transitions
, is
excellent.