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1.
Five new bands of the f1Δ-a1Δ TiO system have been observed in emission between 17774.0 cm?1 and 19801.0 cm?1. Rotational and vibrational analyses of the 0-1, 1-0, 1-2, 2-1, and 1-1 bands, as well as a reanalysis of the 0-0 band, yielded the following molecular constants (cm?1):
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2.
Laser excitation spectra have been recorded for Ca79Br and Ca81Br in the spectral region 600–630 nm. The use of a 1-m monochromator as a narrow band pass filter (1–2 cm?1) has allowed rotational analysis of the 0-0, 1-1, and 2-2 bands of the B2Σ+ - X2Σ+ transition and the 0-0 and 1-1 bands of the A2Π - X2Σ+ transition. A few additional lines of the 0-1, 1-2, 1-0, and 2-1 bands of the B-X system were used to obtain band origins for vibrational analysis. The main constants for Ca79Br are (in cm?1):
f1Δa1Δ
vBvDv (×106)BvDv (×106)
00.502277 (17)0.6411 (57)0.536168 (20)0.5938 (76)
10.499198 (32)0.630 (15)0.533227 (13)0.5971 (46)
20.530335 (26)0.636 (13)
ωe = 874.104 (4)ωe = 1018.273 (4)
ωeχe = 2.501 (4)ωeχe = 4.521 (4)
T′e?T″e = 19140.567 (8)
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3.
Optical-optical double-resonance (OODR) induced photoluminescence into the lowest excited electronic states of BaO—a3Σ+, A1Σ+, b3Π, and A′ 1Π—from C1Σ+ is described. These low-lying states are deperturbed to obtain spectroscopic constants and potential energy curves:
X2Σ+A2ΠB2Σ+
Te015 958.41 (10)16 383.137 (6)
ωe285.732 (9)288.56 (20)285.747 (9)
ωeχe0.840 (4)0.954 (4)
Be0.094466141 (30)0.0957343 (20)0.0965151 (20)
αe0.000403551 (40)0.0004327 (20)0.0004483 (15)
γe (spin-rot.)0.00301484 (50)0.068767 (79)
Pe?0.066834 (64)
Ae59.175 (1)
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4.
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.
a3Σ+A1Σ+b3ΠA′ 1Π
Te (cm?1)16 596(3)16 807.345(10)17 502.6(10)17 619.7(2)
ωe (cm?1)469.0(7)499.620(19)447.62(8)447.95(22)
ωexe (cm?1)1.48(4)1.716(8)2.287(12)2.139(8)
ωeye × 102 (cm?1)2.14(9)1.02(3)
Be (cm?1)0.2594(5)0.2583908(26)0.22426(16)0.22385(16)
αe × 103 (cm?1)1.44(5)1.111(3)1.18(4)1.15(4)
γe × 106 (cm?1)7.0(7)?4.0(21)
Re (A?)2.1294(20)2.133512(11)2.2901(8)2.2922(8)
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5.
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:
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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6.
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
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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7.
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
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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8.
Six bands of the A1Π-X1Σ system of CD+ in the region 3800–4800 Å have been recorded in emission using an aluminum hollow-cathode discharge in the HeC2H2 mixture. From the vibrational and rotational analysis of the observed bands, the following constants (cm?1) are obtained:
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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9.
The absolute vibrational numbering of the Na2b3Πu state has been established by direct observation of the v = 0–13 levels. These b3Πu levels appear as the lower levels in rotationally resolved fluorescence spectra resulting from OODR excitation of 3Πg, 3Δg, and 3Σg+ states via b3ΠuA1Σu+ mixed intermediate levels. The molecular constants for the Na2b3Πu state are (in cm?1, one standard error in parentheses)
T00ωeωexeωeyeBeDe·104αe
A1Π23 747.51367.360.60.756.4285.70.388
X1Σ020357.6504.10.190
(2101.6)(33.3)
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10.
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
Te13 517.2 (1.3)Be0.1434 (0.0027)
ωe153.6 (1.1)αe9×10?5 (4×10?4)
ωeξe0.47 (0.09)re3.20 (0.03) Å
Ae7.85 (0.60)αA0.19 (0.16)
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11.
The ν3 band of CD3F has been studied using coincidences with the 10.4 μm band of the CO2 laser. The majority of the 150 resonances measured have been studied using the Lamb dip technique. These resonances have been analyzed, together with recent microwave results, to give the following vibration-rotation parameters and dipole moments in the ν3 state.
Teωeωexe
A33Π216 758ΔG(12) = 980
A23Π116 4429967.0
A13Π016 1319946.5
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12.
The rotation-inversion spectrum of 15NH3 has been recorded between 38 and 280 cm?1 with a resolution of about 0.03 cm?1. By combining the present results with the inversion frequencies obtained by microwave spectroscopy, the following main rotational and centrifugal distortion constants were derived (in cm?1):
12CD3F
ν0992.29882 (19)cm?1
B20395.776 ± 0.08MHz
A-A0?35.73 ± 0.61MHz
DJ33.8 ± 0.5kHz
DJK203.9 ± 7kHz
μν31.8964 ± 0.0015D
μν3 ? μ00.02617 ± 0.0005D
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13.
Sub-Doppler optical-optical double-resonance excitation spectra of BaF were recorded using two single-mode cw dye lasers. In the 30 000-cm?1 region, the electronic states observed were E2Σ+ and F2Π. The latter had been previously assigned as the “F2Σ+” state by Fowler [Phys. Rev.59, 645–652 (1941)]. The (3, 0) and (4, 0) bands of the E2Σ+-B2Σ+ transition and the (1, 0) and (2, 0) bands of the F2Π-B2Σ+ transition were rotationally analyzed. The molecular constants suggest inferences about the dominant atomic orbital character of the Rydberg molecular orbitals responsible for the E2Σ+ and F2Π electronic states. A new electronic state, the E′ 2Π, is predicted. The molecular parameters obtained (in cm?1, 1σ uncertainty in parentheses) are
StateBDJDJK
vinv = 09.922350.0008493?0.001575
vinv = 19.917420.0008336?0.001532
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14.
Excitation spectra for the CaF A2Π-X2Σ(0, 0), (1, 1), and (1, 0) bands have been observed and assigned. The rotational analysis of the CaF A-X and B-X bands by B. S. Mohanty and K. N. Upadhya [Ind. J. Pure Appl. Phys.5, 523 (1967)] is shown to be incorrect. Because it is possible to make independent rotational assignments of each line in an excitation spectrum by observing frequency differences and relative intensities in photoluminescence spectra, tunable laser excitation spectroscopy promises less ambiguity than traditional techniques for assignment of dense, badly overlapped spectra.The following spectroscopic constants (in cm?1) are obtained for the CaF A2Π and X2Σ states. Numbers in parentheses correspond to three standard deviations uncertainty in the last digit.
v′EE2Σ+v′FF2Π
Tv′0329 767.32(1)129 997.29(1)
ΔGv′ + 123522.841(27)1522.553(2)
Be0.22990(22)0.22931(8)
αe0.00113(14)0.00108(2)
Av′156.9840(12)
pv′1?0.02426(6)
γv′3?0.17367(46)
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15.
The ν3 fundamental band (CO stretch) of HDCO at 1724 cm?1 has been studied using both conventional infrared absorption and CO laser Stark spectroscopy. In addition to the excited-state (v3 = 1) rotational constants, improved constants for the ground state of HDCO have been obtained by combining previous microwave data with some infrared combination differences. The following constants were determined:
X2ΣA2Π
ν0002Π1216493.1(6)
2Π1216565.6(6)
ΔG(12)581.1(9)2Π12586.8(9)
Be0.3385(11)0.3436(12)
Be(Ω = 32) ? B3(Ω = 12)0.00312(21)
α0.00255(48)0.00283(45)
D(estimated)4.44 × 10?74.55 × 10?7
γ(spin-spin)|γ| < 3 × 10?3
A0(spin-orbit)73.4(9)
p(lambda doubling)?0.045(4)
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16.
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).
ConstantGround statev3 = 1 stateUnits
ν01724.267cm?1
A198 119.75198 210.4MHz
B34 910.64634 676.6MHz
C29 561.48829 331.3MHz
μa2.33022.3486D
μb0.1950.190D
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17.
Laser Stark spectroscopy of the ν3 band of CH3F has been carried out using coincidences with the 9.4 μm band CO2 laser lines. About 350 Stark resonances were measured for the ν3 fundamental bands of 12CH3F and 13CH3F. About 30 of them were measured by using a Stark-Lamb dip technique to increase the resolution and the accuracy of the data. These Stark resonances, together with the recent results of infrared-microwave two-photon Lamb dip measurements, were analyzed to give the following vibration-rotation parameters and the dipole moments in the ν3 state,
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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18.
Laser excitation spectra of the A2Σ-X2Πi system have been recorded for 63CuS and 65CuS isotopic molecules with a single-mode dye laser operating in the region 17000–18000 cm?1. For highly overlapped sequences, use of a monochromator as a narrow band filter was necessary to allow rotational analysis. A simultaneous fit of all eight analyzed bands has led to the following spectroscopic constants for 63CuS (in cm?1):
12CH3F13CH3F
ν01048.610767 (62)1027.493191 (69)cm?1
B25197.57 ± 0.0324542.07 ± 0.43MHz
A - A0?294.09 ± 0.60?288.81 ± 0.37MHz
DJ55.5 ± 1.256 ± 12kHz
DJK575 ± 63464 ± 24kHz
μ1.9054 ± 0.00061.9039 ± 0.0006D
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19.
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
StatevTvBvDv × 106γvpvav × 106
A2Σ?017924.335 (7)0.17989 (4)0.177 (7)0.03853 (7)
X2Π121842.574 (7)0.18701 (4)0.163 (7)0.01496 (9)
0432.566 (6)0.18818 (4)0.162 (7)0.01508 (9)
X2Π321411.289 (7)0.18724 (4)0.184 (7)?0.96 (6)
00.18839 (4)0.160 (7)?0.11 (6)
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20.
The infrared absorption of HNCO has been measured in the region of the NH stretching fundamental and in that of the second overtone. The results for the excited states are (in cm?1):
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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Bandν0A- BBC
ν13533.127.0
110145.7922.67130.3684260.361722
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