Comparison of Electromagnetically Induced Transparency (EIT) Spectra for Six-level Lambda \(\Lambda\) and Five-level V-type Systems

Dipankar Bhattacharyya, A. Ghosh, A. Bandyopadhyay, S. Saha, S. De
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引用次数: 1

Abstract

Electromagnetically induced transparency (EIT) is experimentally studied in a rubidium vapour cell (without buffer gas, both \(^{87}\)Rb and \(^{85}\)Rb present according to their natural abundance) kept within two-layers of \(\mu(\mu)\)-metal shields to avoid the effect of Earth's magnetic field on the energy levels of atomic rubidium. An external cavity diode laser (ECDL), used as a low power probe laser, is locked to the hyperfine cross-over peak of \(F = 2 \rightarrow  F' = 2, 3\) transitions of \(^{87}\)Rb. The frequency of another ECDL, the pump laser, is set to scan the \(F=1 \rightarrow  F' = 0, 1, 2\) transitions of \(^{87}\)Rb. These form the  \(\Lambda\)-type six level system. In the V-type system, both the pump and the probe lasers share the same \(F = 2\) ground level. The probe beam coming out of the cell is detected by a low noise fast photodetector. The resulting spectra show signature of EIT in the "peak" for the  \(\Lambda\)-type system and in the "dip" for the V-type system. Numerical calculation based simulated spectra are also compared with the experimental spectra. In both the cases very narrow EIT linewidth \((\Gamma_{t} < \Gamma)\) is observed even at high value of pump Rabi-frequency \((\Omega_{c}\gg \Gamma)\). Narrower value of EIT linewidth is due to Doppler averaging phenomena.
六能级Lambda \(\Lambda\)与五能级v型系统的电致透明光谱比较
实验研究了电磁感应透明(EIT)在铷蒸汽电池(没有缓冲气体,\(^{87}\) Rb和\(^{85}\) Rb根据其天然丰度存在)保持在两层\(\mu(\mu)\) -金属屏蔽内,以避免地球磁场对原子铷能级的影响。外腔二极管激光器(ECDL)作为一种低功率探测激光器,被锁定在\(^{87}\) Rb的\(F = 2 \rightarrow  F' = 2, 3\)跃迁的超精细交叉峰上。另一个ECDL的频率,泵浦激光器,被设置为扫描\(^{87}\) Rb的\(F=1 \rightarrow  F' = 0, 1, 2\)跃迁。这些构成了\(\Lambda\)型六级系统。在v型系统中,泵浦激光器和探测激光器共享相同的\(F = 2\)地平面。探头光束由一个低噪声快速光电探测器检测。所得光谱显示了\(\Lambda\)型体系的“峰”和v型体系的“倾角”的EIT特征。基于数值计算的模拟光谱也与实验光谱进行了比较。在这两种情况下,即使在泵浦rabi频率\((\Omega_{c}\gg \Gamma)\)的高值时,也观察到非常窄的EIT线宽\((\Gamma_{t} < \Gamma)\)。较窄的EIT线宽值是由于多普勒平均现象。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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