Recently, a line list including positions and transition strengths was published for the NH X3Σ− rovibrational and rotational transitions. The calculation of the transition strengths requires a conversion of transition matrix elements from Hund’s case (b) to (a). The method of this conversion has recently been improved during other work on the OH X2Π rovibrational transitions, by removing an approximation that was present previously. The adjusted method has been applied to the NH line list, resulting in more accurate transition strengths. An updated line list is presented that contains all possible transitions with v′ and v″ up to 6, and J up to between 25 and 44, depending on the band.
REFERENCES
1.
J. S. A.
Brooke
et al., J. Chem. Phys.
141
, 054310
(2014
).2.
J. S. A.
Brooke
et al., “Line strengths of rovibrational and rotational transitions within the X2Π ground state of OH
,” J. Quant. Spectrosc. Radiat. Transfer
(submitted).3.
4.
M.
Asplund
et al., Annu. Rev. Astron. Astrophys.
47
, 481
(2009
).5.
D. L.
Lambert
et al., Astrophys. J.
284
, 223
(1984
).6.
D. L.
Lambert
et al., Astrophys. J., Suppl. Ser.
62
, 373
(1986
).7.
V. V.
Smith
and D. L.
Lambert
, Astrophys. J.
311
, 843
(1986
).8.
9.
M. M.
Litvak
and E. N. R.
Kuiper
, Astrophys. J.
253
, 622
(1982
).10.
D. M.
Meyer
and K. C.
Roth
, Astrophys. J. Lett.
376
, L49
(1991
).11.
I. A.
Crawford
and D. A.
Williams
, Mon. Not. R. Astron. Soc.
291
, L53
(1997
).12.
J. R.
Goicoechea
et al., Astrophys. J.
600
, 214
(2004
).13.
T.
Weselak
et al., Mon. Not. R. Astron. Soc.
400
, 392
(2009
).14.
J. A.
Miller
and C. T.
Bowman
, Prog. Energy Combust. Sci.
15
, 287
(1989
).15.
L. D.
Smoot
et al., Prog. Energy Combust. Sci.
24
, 385
(1998
).16.
W. C.
Campbell
et al., Phys. Rev. Lett.
98
, 213001
(2007
).17.
S.
Hoekstra
et al., Phys. Rev. A
76
, 063408
(2007
).18.
W. C.
Campbell
et al., Phys. Rev. Lett.
100
(2008
).19.
M. T.
Hummon
et al., Phys. Rev. A
78
, 050702
(2008
).20.
M.
Kajita
, Phys. Rev. A
74
, 032710
(2006
).21.
L. M. C.
Janssen
et al., Phys. Rev. A
83
, 022713
(2011
).22.
L. M. C.
Janssen
et al., J. Chem. Phys.
134
, 124309
(2011
).23.
L. M. C.
Janssen
et al., Eur. Phys. J. D
65
, 177
(2011
).24.
D.
Demille
, Phys. Rev. Lett.
88
, 067901
(2002
).25.
M.
Kajita
, Phys. Rev. A
74
, 035403
(2006
).26.
H. L.
Bethlem
and W.
Ubachs
, Faraday Discuss.
142
, 25
(2009
).27.
J. S. A.
Brooke
et al., Astrophys. J., Suppl. Ser.
210
, 23
(2014
).28.
R. J.
Le Roy
, University of Waterloo Chemical Physics Research Report
(University of Waterloo
, 2004
), http://scienide2.uwaterloo.ca/~rleroy/rkr/.29.
R. J.
Le Roy
, University of Waterloo Chemical Physics Research Report
(University of Waterloo
, 2007
), http://scienide2.uwaterloo.ca/~rleroy/level/.30.
J.
Espinosa-García
et al., Chem. Phys. Lett.
233
, 220
(1995
).31.
W. R. M.
Graham
and H.
Lew
, Can. J. Phys.
56
, 85
(1978
).32.
K. P.
Huber
and G.
Herzberg
, “Molecular spectra and molecular structure. Volume IV: Constants of diatomic molecules
,” in Molecular Spectra and Molecular Structure
(Van Nostrand Reinhold
, 1979
).33.
A.
Hofzumahaus
and F.
Stuhl
, J. Chem. Phys.
82
, 5519
(1985
).34.
C. W.
Bauschlicher
, Jr. and S. R.
Langhoff
, Chem. Phys. Lett.
135
, 67
(1987
).35.
C. M.
Western
, PGOPHER, a program for simulating rotational structure (v. 7.1.293), 2014.36.
P. F.
Bernath
, Spectra of Atoms and Molecules
, 3rd ed. (Oxford University Press
, 2015
).37.
See supplementary material at http://dx.doi.org/10.1063/1.4923422 for RKR potential energy curve and its interpolation/extrapolation bylevel, ab initio potential and DMF, line list including positions and intensities, Av′v and fv′v values, and pgopher input file.
© 2015 AIP Publishing LLC.
2015
AIP Publishing LLC
You do not currently have access to this content.