Chemiluminescence from electronitiy excited HS2 radi&s has be&n detected between 950 and 2100 nm in gas-pha;9 flow systems. The emission essentially consits of u:sequences of the I$ (Al 'A' -t x 'A") tra&iion wi& the 000 -000 lxmd origin at 1378 nm. DS2 was also studied For HSp the following spectro
The sodium superoxide radical: X̃2A2 and à 2B2 potential energy surfaces
✍ Scribed by David A. Horner; Wesley D. Allen; Attila G. Császár; Henry F. Schaefer III
- Publisher
- Elsevier Science
- Year
- 1991
- Tongue
- English
- Weight
- 814 KB
- Volume
- 186
- Category
- Article
- ISSN
- 0009-2614
No coin nor oath required. For personal study only.
✦ Synopsis
The two lowest electronic states of NaO, have been studied using ab initio methods, including RHF SCF, CISD, Davidsoncorrected CISD, UHF SCF, UMPZ-UMP4, CASSCF, and CISD based on CASSCF natural orbitals, with basis sets ranging in qualityfmmNa( lls7p/7s5p), 0(9sSpld/5s3pld) toNa(l3slDp2dlf/7s6p2dlf),O( lls7p2dlf/6s4pZdlf), i.e.fromTZtdto TZZP+f+R. Total and relative energies, geometries, vibrational frequencies, and dipole moments of stationary points on the it 2A2 and ii 2B2 surfaces have been determined. A Czv minimum is proposed for 2 *A2 NaOL with r,(O-0) = 1.335 and r,(Na-0) ~2.10 A. The analogous structure for the A *B2 state is predicted to have r,(O-0) = 1.34 and r,(Na-0) = 2.13 A with an adiabatic excitation energy of r,= 8.5 kcal mol-'. Linear, *II NaOO, which correlates to the 2A2 and 2B2 minima via C, transition states, is predicted to be a shallow minimum lying 17 kcal mol-' above the 2 *A2 structure but with a barrier to rearrangement of less than 1 kcal mol-I. The dissociation energy of the ground state of NaOz is deduced to be Do=38 kcal mol-'. a value substantially lower than recent experimental estimates.
📜 SIMILAR VOLUMES
spectra and the fluorescence hfetlme of HSO (x 2A'-%2A") rddlcals XC measured m the g.~s phase III the wawlcngth range 570-700 nm The progresslon of the SO strctchmg mode (u3) IS observed m cmlsslon and cxc~tat~on spectra The zero-pressure hfetune cxtrapolatcd from the Stern-Volmer plots IS 11 3:: "