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首页> 外文期刊>The Journal of Chemical Physics >The 4051-A band of C_3 (A~1PI_u-X~1SIGMA_g~+ 000-0000):perturbed low-J lines and lifetime measurements
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The 4051-A band of C_3 (A~1PI_u-X~1SIGMA_g~+ 000-0000):perturbed low-J lines and lifetime measurements

机译:C_3的4051-A频段(A〜1PI_u-X〜1SIGMA_g〜+ 000-0000):扰动的低J线和寿命测量

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摘要

Rotational analyses have been carried out at high resolution for the 000-000 and 000-100 bands of the A ~1PI_u-X~1SIGMA_g~+ transition of supersonic jet-cooled C_3.Two different spectra have been recorded for each band,using time gatings of 20-150 and 800-2300 ns.At the shorter time delay the spectra show only the lines observed by many previous workers.At the longer time delay many extra lines appear,some of which have been observed previously by [McCall et al.Chem.Phys.Lett.374,583 (2003)] in cavity ring-down spectra of jet-cooled C_3.Detailed analysis of these extra lines shows that at least two long-lived states perturb the A ~1PI_u,000 state.One of these appears to be a ~3SIGMA_u~-vibronic state,which may possibly be a high vibrational level of the b ~3PI_g state,and the other appears to be a P=1 state with a low rotational constant B.Our spectra also confirm the reassignment by McCall et al.of the R(0) line of the 000-000 band,which is consistent with the spectra recorded towards a number of stars that indicate the presence of C_3 in the interstellar medium.Fluorescence lifetimes have been measured for a number of upper-state rotational levels.The rotational levels of the A ~1PI_u state have lifetimes in the range of 230-190 ns,decreasing slightly with J;the levels of the perturbing states have much longer lifetimes,with some of them showing biexponential decays.An improved value has been obtained for the nu_1 vibrational frequency of the ground state,nu_1,=1224.4933+-0.0029 cm~(-1).
机译:对超音速喷射冷却的C_3的A〜1PI_u-X〜1SIGMA_g〜+跃迁的000-000和000-100波段进行了高分辨率的旋转分析。每个波段记录了两个不同的光谱,使用时间门控时间为20-150 ns和800-2300 ns。在较短的时间延迟下,光谱仅显示许多以前的工作人员观察到的谱线。在较长的时间延迟下,出现了许多额外的谱线,其中一些以前已被[McCall等人观察到[Chem.Phys.Lett.374,583(2003)]在射流冷却的C_3的腔衰荡光谱中进行了详细分析,结果表明至少有两个长寿命状态扰动了A〜1PI_u,000状态。这些似乎是〜3SIGMA_u〜-振动状态,可能是b〜3PI_g状态的高振动水平,另一个似乎是具有低旋转常数B的P = 1状态。 McCall等人重新分配了000-000波段的R(0)线,这与记录到的光谱一致表示星际介质中存在C_3的许多恒星。已测量了许多上层自旋能级的荧光寿命.A〜1PI_u状态的自旋能级的寿命在230-190 ns范围内,随J的减小而减小;扰动态的寿命更长,其中一些表现出双指数衰减。基态的nu_1振动频率nu_1获得了一个改进值,nu_1 = 1224.4933 + -0.0029 cm〜( -1)。

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