首页> 外文期刊>The Journal of Chemical Physics >EFFECTS OF MAGNETIC-FIELD ON THE 15V 31 344.9 BAND OF CS2 STUDIED BY SUB-DOPPLER HIGH-RESOLUTION SPECTROSCOPY
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EFFECTS OF MAGNETIC-FIELD ON THE 15V 31 344.9 BAND OF CS2 STUDIED BY SUB-DOPPLER HIGH-RESOLUTION SPECTROSCOPY

机译:磁场对亚多普勒高分辨率光谱法研究CS2的15V 31 344.9能带的影响

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Effects of an external magnetic field on the excitation spectrum of the 15 V 31 344.9 band of the CS2 molecule are measured with sub-Doppler resolution. New lines ale observed to appear near the R(2) and P(4) lines when a magnetic field is applied. These lines are observed to be composed of five components both for the pi pump and for the sigma pump. From a theoretical analysis, we identify the new lines as transitions to the (3)A(2)(A(1)-B-1)(nu(-);12M) levels, which become allowed by Zeeman interaction with the V B-1(2)(nu';03M) level that is mixed with the (3)A(2)(B-2)(nu;03M) level by spin-orbit interaction. Variations of energy shifts and intensities with the magnetic field strength are explained quantitatively by this analysis. M-dependent perturbation and the quenching of fluorescence are observed. The reason why large Zeeman splittings are observed at many lines in the V system of CS2 can be attributed to the spin-orbit interaction between the V B-1(2)(nu';KJM) level and the (3)A(2)(B-2)(nu;KJM) level Combined with the rotational and/or the Zeeman interactions:: between (3)A(2)(B-2)(nu;KJM) level and either (3)A(2)(A(1)+B-1)(nu(0);K+/-1JM) or (3)A(2)(A(1)-B-1)(V-+/-;K+/-1J+/-1M) levels which are accidentally close in energy. (C) 1995 American Institute of Physics. [References: 24]
机译:用亚多普勒分辨率测量外部磁场对CS2分子15 V 31 344.9谱带激发光谱的影响。当施加磁场时,观察到新的线出现在R(2)和P(4)线附近。观察到这些管线由pi泵和sigma泵的五个组件组成。通过理论分析,我们确定新的行是到(3)A(2)(A(1)-B-1)(nu(-); 12M)的过渡,这是由于Zeeman与V相互作用而允许的B-1(2)(nu'; 03M)水平通过自旋轨道相互作用与(3)A(2)(B-2)(nu; 03M)水平混合。通过该分析定量地解释了能量转移和强度随磁场强度的变化。观察到M依赖性扰动和荧光猝灭。在CS2的V系统中的许多行观察到大的塞曼分裂的原因可以归因于V B-1(2)(nu'; KJM)能级与(3)A(2)之间的自旋轨道相互作用(B-2)(nu; KJM)水平与旋转和/或Zeeman相互作用结合::(3)A(2)(B-2)(nu; KJM)水平与(3)A( 2)(A(1)+ B-1)(nu(0); K +/- 1JM)或(3)A(2)(A(1)-B-1)(V-+ /-; K + / -1J +/- 1M)的能量水平偶然接近。 (C)1995年美国物理研究所。 [参考:24]

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