Ab initio study of the X2
and A2
+ states of OH. I. Potential curves and properties
J. Chem. Phys. 61, 5389 (1974); doi:10.1063/1.1681891
Issue Date: 15 December 1974
You are not logged in to this journal. Log in
Accurate ab initio CI potential curves and molecular properties are presented for the X2
and A2
+ states of OH. Results with known experimental values in parentheses are Re(X2
) = 1.841(1.834) bohr, Re(A2
+) = 1.906(1.913) bohr, De(X2
) = 4.43(4.63) eV, De(A2
+) = 2.29(2.53) eV, µ(OH,X2
,
=0) = 1.634(1.668) D, and µ(OD,A2
+,
=0) = 1.861(1.72±0.10) D. Spectroscopic constants calculated from the theoretical potential curves are in satisfactory agreement with experimental results. Other molecular properties studied include quadrupole moments and the electric field gradient at the nuclei.
©1975 American Institute of Physics
and A2
+ states of OH. Results with known experimental values in parentheses are Re(X2
) = 1.841(1.834) bohr, Re(A2
+) = 1.906(1.913) bohr, De(X2
) = 4.43(4.63) eV, De(A2
+) = 2.29(2.53) eV, µ(OH,X2
,
=0) = 1.634(1.668) D, and µ(OD,A2
+,
=0) = 1.861(1.72±0.10) D. Spectroscopic constants calculated from the theoretical potential curves are in satisfactory agreement with experimental results. Other molecular properties studied include quadrupole moments and the electric field gradient at the nuclei.
©1975 American Institute of Physics
| History: | Received 21 August 1974 |
| Permalink: |
http://link.aip.org/link/?JCPSA6/61/5389/1 |
REFERENCES (19)
For access to fully linked references, you need to log in.
For access to fully linked references, you need to Log in.
- G. H. Dieke and H. M. Crosswhite, Bumblebee Report No. 87, Johns Hopkins University, 1948.
- G. H. Dieke and H. M. Crosswhite,
J. Quant. Spectrosc. Radiat. Transfer 2, 97 (1962) . - (a) C. Carlone and F. W. Dalby,
Can. J. Phys. 47, 1945 (1969) ; - (b) E. A. Moore and W. G. Richards,
Phys. Scr. 3, 223 (1971) . - (a) S. Green, P. S. Bagus, B. Liu, A. D. McLean, and M. Yoshimine,
Phys. Rev. A 5, 1614 (1972) ; - (b) M. Yoshimine, S. Green, and P. Thaddeus,
Astrophys. J. 183, 899 (1973) . - M. Yoshimine, A. D. McLean, and B. Liu, J. Chem. Phys. 58, 4412 (1973).
- (a) G. C. Lie, J. Hinze, and B. Liu, J. Chem. Phys. 59, 1872 (1973);
- E. Clementi,
IBM J. Res. Dev. 9, 2 (1965) . - B. Liu, J. Chem. Phys. 58, 1925 (1973).
- J. Hinze and B. Liu (unpublished).
- P. E. Cade and W. M. Huo, J. Chem. Phys. 47, 614 (1967).
- A. D. McLean and B. Liu, J. Chem. Phys. 58, 1066 (1973).
- B. Liu (unpublished).
- V. Bondybey, P. K. Pearson, and H. F. Schaefer, III, J. Chem. Phys. 57, 1123 (1972).
- W. J. Stevens, G. Das, A. C. Wahl, M. Krauss, and D. Neumann (unpublished).
- W. L. Meerts and A. Dyamnus,
Chem. Phys. Lett. 23, 45 (1973) . - R. E. Murphy, J. Chem. Phys. 54, 4852 (1971).
- S. Green, J. Chem. Phys. 58, 4327 (1973).
- E. M. Weinstock and R. N. Zare, J. Chem. Phys. 54, 4319 (1973).
- E. A. Scarl and F. W. Dalby,
Can. J. Phys. 49, 2825 (1971) .
(c) J. Hinze, G. C. Lie, and B. Liu, Astrophys. J. (to be published).








