The pure rotational spectrum of the ground state of NH3/ND3
and the Stark effect
NH3
The data files given here were
constructed by
fitting to the line positions and
intensities in the HITRAN 2008 (http://www.hitran.com)
database.
The
fit
was
restricted
to
J
< 16, and is sufficient to reproduce the line positions to better
than 0.001 cm-1 and the intensities to better than 10-20
cm2 cm-1 Molecule-1. There
are two points that are slightly non-standard:
- The point group used is D3h, rather than C3v.
This
is
necessary
to
account
for
the
inversion
doubling
in
the
ground
state,
which appears in the data file as two vibrational states:
- s/0+ with A1'
symmetry
- a/0- with A2"
symmetry
- To fit the K = 3n
levels
requires three perturbation
operators:
- <0+|J+-^6|0+>
= J+6 + J-6
- <0+|J^2J+-|0+>
= J2(J+6
+ J-6)
- <0+|J+-^12|0+>
= J+12 + J-12
Two separate data files are provided,
with the required constants. The first is
nh3x0.pgo which has the two
inversion doublets in separate manifolds (s and a), with a transition
moment acting between the two manifolds. This is a good starting point
for simulating electronic spectra, where the transitions will typically
be from one inversion doublet or other.
The Stark Effect
The second file,
nh3x0one.pgo, has
the same constants in, but with the
two inversion doublets in the same manifold. The resulting energy
levels will be the same, but as the dipole moment now acts within the
manifold, the Stark effect in the ground state can be simulated with
this file. To give quick calculation times Jmax has been set to 5 for
this file. The
energy level plot window
can then be used to produce a plot of energy against field, as for
example:

This shows the K = 1, M = 1 levels show a strong Stark
effect, but the other levels show a
rather weaker effect. In development version 7.1.194 or above the
"Summary" button gives the
following information:
M Sym # g Population Name J K (kl) Sym M Energy Linear Dipole Err Quadratic Err Two Level Delta C Dipole2 Err
0 - 1 4 .660533316 a 0 0 A2" 0 0.7933 -5.20523347e-9 -.0309983 15.8% -1.0409798e-15 .02 %
0 - 2 2 .036129526 s 1 1 E" 0 16.1730 -1.47243024e-9 -.0087686 15.8% -2.9448374e-16 .002%
0 - 3 2 .032246486 a 1 1 E' 0 16.9632 -1.53137719e-9 -.0091197 15.8% -3.0627282e-16 .002%
0 - 4 4 .042329414 s 1 0 A2' 0 19.8899 3.241105275e-9 .01930147 15.8% 6.48153456e-16 .033%
1 - 1 2 .036129526 s 1 1 E" 1 16.1730 -7.02797997e-8 -.4185312 13.9% -1.3786935e-14 5.18% 16.583449 .82098935 -1.25126674e-7 -.7451561 .013%
1 - 2 2 .032246486 a 1 1 E' 1 16.9632 6.802667704e-8 .40511341 13.9% 1.33363101e-14 5.36% 16.583784 .75886528 1.190970869e-7 .70924861 .015%
1 - 3 4 .042329414 s 1 0 A2' 1 19.8899 -1.47290548e-9 -.0087715 15.8% -2.9457878e-16 .002%
This indicates that the K = 1
levels are intermediate between a first and second order Stark effect,
and the others are essentially showing a second order (quadratic) Stark
effect. See External Fields - The Zeeman and
Stark Effects for more information.
ND3
A similar set of data files for ND3 is given below. The data
sources are L Fusina and S N Murzin, J. Molec. Spectrosc. 167 464 (1994), L H Coudert and E
Roueff, Astron. Astrophys. 449
855 (2006) and the ND3
linelist from the Cologne
Database
for
Molecular
Spectroscopy (CDMS).
- nd3x0.pgo, similar to the
nh3x0.pgo
file
above.
This was derived by from an unweighted fit to all lines in
the CDMS linelist with J <
16, which gave an average error of 7×10-5 cm-1
and a maximum error of 0.003 cm-1. This has the two ground
state inversion doublets in different manifolds, giving a simpler
description than in the next file.
- nd3x0one.pgo, equivalent to
the nh3x0one.pgo file above, with both ground state inversion
doublets in the same manifold to allow the Stark effect to be
simulated.
This uses exactly the Hamiltonian and constants used in the Fusina and
Murzin paper. This includes perturbations acting between the two
inversion doublets, though note that the sign of the αJ and αK constants must be changed
in PGOPHER to give
consistent matrix elements. The line
positions agree with the CDMS linelist to < 0.006 cm-1 (<
0.0005
cm-1 for J
< 15).
- nd3x0hyp.pgo which has the
hyperfine structure due to the nitrogen nucleus added to the
simulation, giving a linelist consistent with the Coudert and Roueff
paper.