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The He2 band systems 4pπ i3Πg → 2s a3Σu+ and 5pπ l3Πg → 2s a3Σu+ are described in detail, and the i and l states characterized. A number of significant perturbations in the i and l states are identified, and the possible perturber states discussed. The following molecular constants (cm?1) are reported:
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The mutual perturbations of the A1Σu+ and b0u+ states of As2 are due to a strong spin-orbit interaction. The numerical treatment of these perturbations leads to the following parameters:
StateωeeBeαere (A?)
i3Πg1707.9535.007.242g0.2221.0782
l2Πg1703.8634.977.22640.21881.0794
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The emission spectrum of SeO in the far ultraviolet first observed by Haranath (1) at low dispersion has been photographed in the region 2480-1930 Å under medium resolution and a reanalysis of the vibrational structure of the bands has been presented. Beginning at the longer wavelength end, the spectrum has been analyzed into five band systems which are designated as c(1Σ+)-b(1Σ+), x2-x1, y2-y1, C(3Π)-X3Σ?, and D(3Σ?)-X3Σ?. The lower state of the c-b system is found to be the upper state of the b(1Σ+)-X3Σ? system observed recently by us (2). The derived constants in cm?1 for SeO are as follows (the constants of the b state are those derived from Ref. 2).
Te (cm?1)ωe (cm?1)ωexe (cm?1)Be (cm?1)
A1Σu+40 806 (3)297 (2)5.1 (2)0.0798 (12)
b0u+38 884 (3)422 (1)8.8 (1)0.0783 (12)
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13.
The 0-0, 1-1, 2-2, and 3-3 bands of the A2Π-X2Σ+ transition of the tritiated beryllium monohydride molecule have been observed at 5000 Å in emission using a beryllium hollow-cathode discharge in a He + T2 mixture. The rotational analysis of these bands yields the following principal molecular constants.
A2Π:Be = 4.192 cm?1; re = 1.333 A?
X2Σ:Be = 4.142 cm?1; re = 1.341 A?
ωe′ ? ωe″ = 16.36 cm?1; ωe′Xe′ ? ωe″Xe″ = 0.84 cm?1
From the pure electronic energy difference (EΠ - EΣ)BeT = 20 037.91 ± 1.5 cm?1 and the corresponding previously known values for BeH and BeD, the following electronic isotope shifts are derived
ΔEei(BeH?BeT) = ?4.7 ≠ 1.5cm1, ΔEei(BeH?BeT) = ?1.8 ≠ 1.5cm1
and related to the theoretical approach given by Bunker to the problem of the breakdown of the Born-Oppenheimer approximation.  相似文献   

14.
Laser-induced fluorescence of Cs2 molecules in the infrared (1.15–2.5 μm) and the visible (505–545 nm) regions has been observed using several excitation wavelengths from an argonion laser. Accurate molecular constants and potential energy curves for the pumped E1Σu+ state and the first excited gerade 1Π state are derived from more than 1300 fluorescence lines precisely measured with a high-resolution Fourier transform interferometer. The main molecular constants for the states are
StateTeωeωexeλ
y2y1 + 478309746.0
y1y190621.0
x2x1 + 460099932.0
x1x18778.0
c(1Σ+)5308095413.0
D(3Σ?)F2514229559.3
F1513569558.5~36
C(3Π)5087310349.3
b(1Σ+)9570.7834.95.5
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The emission spectrum of the A2Π-X2Π system of the SbO molecule has been photographed under high resolution, and the rotational structure in eight bands of the 2Π32-2Π32 component, involving v′ = 0–2 and v″ = 1–4, has been analyzed for both isotopic molecules 121SbO and 123SbO. The observed rotational lines of the corresponding 2Π12-2Π12 component are broad, with a width of about 0.2 cm?1 varying little with J. It is suggested that these broad lines represent unresolved components arising from magnetic hyperfine interaction with 121Sb or 123Sb nuclei. Isotopic shift observations contradict earlier vibrational assignments in the 2Π12-2Π12 subsystem and indicate that the A state is inverted in agreement with expectations from related systems. The principal molecular constants (in cm?1) obtained for 121SbO are
Te (cm?1)ωe (cm?1)Be (cm?1)Re (A?)
E1Σu+20195.2329.100.008915.340733
(1) 1Πg13913.4218.440.007815.697722
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17.
The investigation of the emission infrared spectrum of P2 was performed with a high resolution Fourier spectrometer. Two new electronic systems were attributed to b3Πgw3Δu and A1ΠgW1Δu transitions. The molecular parameters are obtained by a complete fitting procedure. The main equilibrium constants of the new states are (in cm?1):
ω3Δu Te = 243228.07 ωe = 591.3 ωeXe = 2.5
Be = 0.256040 δe = 0.001409 De = 19.0 X 10?8
W1ΔuTe = 31096.64 We = 627.206 WeXe = 2.331
Be = 0.2628 δe = 0.0014 De = 23 X 10?8
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18.
Single-mode cw dye laser excitation spectra of the (0, 0), (1, 1), and (2, 2) bands of the B2Σ+-X2Σ+ system of CaCl have been observed and assigned. Some 300 independent photo-luminescence spectra have been used in making the rotational assignment and demonstrate the power of the technique of line-by-line analysis in unraveling complex spectra. Spectroscopic constants (cm?1) obtained from a weighted least squares fit of the data are given below. Numbers in parentheses refer to 95% confidence limits in the last digit.
StateTeωeωeχeBe103αe107De
X2Π120818.74.2
X2Π32x ≈ 2272814.14.30.359202.382.8
A2Π1221 467.4565.82.9
A2Π32x + 18 521.7570.42.60.288561.822.9
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19.
Doppler-limited laser excitation spectroscopy employing narrow-band fluorescence detection was used to obtain a rotational and vibrational analysis in the (0, 0) and (1, 1) bands of the A2Π-X2Σ+ system and the (4, 2) (3, 1), (0, 0), (0, 1), (1, 2), (2, 3), and (3, 4) bands of the B2Σ+-X2Σ+ system of CaI. The A and B states are deperturbed to obtain spectroscopic constants and Franck-Condon factors. Deperturbation was necessary because of the small separation of the A and B states relative to the AB interaction strength and the A2Π spin-orbit splitting. The main deperturbed constants (in cm?1) are
X2Σ+B2Σ+
Te016856.69(2)
ωe369.8(10)366.8(10)
ωexe1.13(20)1.28(20)
Be0.15200(54)0.15448(54)
αe0.00063(34)0.00073(35)
De1.027(16) × 10?71.097(17) × 10?7
γe (spin-rotation)+0.003?0.0630(16)
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20.
A new weak emission band system of the SeO molecule consisting of 34 band heads degraded to shorter wavelengths has been observed for the first time in the spectral region 6730–8570 Å. The vibrational analysis of the system suggests that it arises from the transition A3Πreg-X0+, 1. All the five subsystems allowed by the selection rule ΔΩ = 0, ±1 have been identified. The constants in cm?1 derived for the A3Π state are
X2Σ+A2ΠB2Σ+
Te015 624.67(5)15 700.52(12)
ωe238.7496(33)241.19(7)242.63(17)
ωeχe0.62789(64)0.53(5) (Pekeris)1.17(12) (Pekeris)
Be0.0693254(84)0.070460(14)0.071572(22)
αe × 1042.640(35)2.15(10)3.95(2)
Ae45.8968(52)
Re(A?)2.8286(2)2.8057(3)2.7839(4)
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Teωeωexe
A33Π216 758ΔG(12) = 980
A23Π116 4429967.0
A13Π016 1319946.5
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