Nanosecond-timescale development of Faraday rotation in an ultracold gas

J. Gilbert, Mark Watkins, J. Roberts
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Abstract

When a gas of ultracold atoms is suddenly illuminated by light that is nearly resonant with an atomic transition, the atoms cannot respond instantaneously. This non-instantaneous response means the gas is initially more transparent to the applied light than in steady-state. The timescale associated with the development of light absorption is set by the atomic excited state lifetime. Similarly, the index of refraction in the gas also requires time to reach a steady-state value, but the development of the associated phase response is expected to be slower than absorption effects. Faraday rotation is one manifestation of differing indices of refraction for orthogonal circular light polarization components. We have performed experiments measuring the time-dependent development of polarization rotation in an ultracold gas subjected to a magnetic field. Our measurements match theoretical predictions based on solving optical Bloch equations. We are able to identify how parameters such as steady-state optical thickness and applied magnetic field strength influence the development of Faraday rotation.
超冷气体中法拉第旋转的纳秒级发展
当一种由超冷原子组成的气体突然被几乎与原子跃迁共振的光照亮时,原子不能立即做出反应。这种非瞬时响应意味着气体最初对施加的光比在稳态时更透明。与光吸收发展有关的时间标度是由原子激发态寿命决定的。同样,气体中的折射率也需要时间才能达到稳态值,但相关相位响应的发展预计将比吸收效应慢。法拉第旋转是正交圆光偏振分量折射率不同的表现之一。我们进行了实验,测量了磁场作用下超冷气体中极化旋转的随时间发展。我们的测量结果与基于求解光学布洛赫方程的理论预测相符。我们能够确定诸如稳态光学厚度和外加磁场强度等参数如何影响法拉第旋转的发展。
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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