首页> 外文期刊>The Astrophysical journal >OPTICAL ZEEMAN SPECTROSCOPY OF THE (0, 0) BANDS OF THE B ~3Π-X~3Δ AND A ~3Φ-X ~3Δ TRANSITIONS OF TITANIUM MONOXIDE, TiO
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OPTICAL ZEEMAN SPECTROSCOPY OF THE (0, 0) BANDS OF THE B ~3Π-X~3Δ AND A ~3Φ-X ~3Δ TRANSITIONS OF TITANIUM MONOXIDE, TiO

机译:一氧化钛,TiO的B〜3Π-X〜3Δ和A〜3Φ-X〜3Δ跃迁的(0,0)谱带的光学塞曼光谱

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The Zeeman effect on lines in the (0,0) band of the B ~3Π-X~3Δ (γ′) system and in the (0,0) band of the A ~3Φ-X~3Δ (γ) system of titanium monoxide, TiO, have been recorded and analyzed. Magnetic tuning of the low rotational spectral features recorded at high resolution (FWHM approx= 35 MHz) and at field strengths of up to 1.2 kG is accurately modeled using an effective Zeeman Hamiltonian. A comparison is made with previous predictions, which were based on field-free spectroscopic parameters. It is shown that the large Λ-doubling in the B ~3Π state necessitates the inclusion of ΔJ = ±1 matrix elements in the representation of the effective Hamiltonian operator. The observed spectra could only be modeled by allowing the electronic spin and orbital magnetic g-factors, g_S and g_L, of the B ~3Π and A ~3Φ states to deviate from 2.002 and 1.000. Nonadiabatic mixing with the nearby C ~3Δ state is proposed as the cause of these deviations.
机译:Zeeman效应对B〜3Π-X〜3Δ(γ')系统的(0,0)波段和A〜3Φ-X〜3Δ(γ)系统的(0,0)波段的线一氧化钛TiO已被记录和分析。使用有效的塞曼·哈密顿量可以精确地模拟以高分辨率(FWHM大约= 35 MHz)和最高1.2 kG的场强记录的低旋转光谱特征的磁调谐。与基于无场光谱参数的先前预测进行了比较。结果表明,在B〜3Π状态下较大的Λ加倍需要在有效哈密顿算子的表示中包括ΔJ=±1个矩阵元素。只能通过允许B〜3Π和A〜3Φ状态的电子自旋和轨道磁g因子g_S和g_L偏离2.002和1.000来对观察到的光谱进行建模。提出了具有附近C〜3Δ状态的非绝热混合作为这些偏差的原因。

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