原子通过施罗丁格方程和真空波动吸收光子的例子
1Science College, Liaoning Technical University, Fuxin, 123000, China. yong.j.zhang@gmail.com.
Scientific reports
|January 10, 2024
概括
真空波动为原子的光子吸收引入随机性,解决量子不可预测性. 这种机制允许光子吸收完成,否则由于原子纠而保持不完整.
科学领域:
- 量子力学就是量子力学.
- 原子物理 原子物理
- 量子光学就是量子光学.
背景情况:
- 原子对光子的吸收是一种基本的量子过程.
- 吸收结果中固有的不可预测性表明了潜在的随机性.
- 仅靠施罗丁格方程无法完全描述这个过程,在某些场景中导致不完全吸收.
研究的目的:
- 为了证明真空波动可以是光子吸收中随机性的来源.
- 解释真空波动如何解决双原子系统中的纠问题.
- 探索真空波动,波恩定律和通过卡西米尔效应进行实验验证之间的潜在联系.
主要方法:
- 一个单一光子与两个对称排列的原子相互作用的理论建模.
- 分析由施罗丁格方程支配的系统的时间演变.
- 包括真空波动来研究它们对纠原子状态的影响.
主要成果:
- 在没有真空波动的情况下,原子会纠在一起,停止吸收过程.
- 真空波动诱导随机波动,打破原子纠.
- 吸收过程结束时,一个原子被激发,另一个原子保持基本状态,表明哪个原子吸收了光子.
- 真空波动也可能导致波恩规则的出现.
结论:
- 真空波动被认为是原子对光子吸收随机性的起源.
- 这种机制解决了由原子纠引起的不完全吸收问题.
- 卡西米尔效应为验证这些发现提供了一个潜在的实验途径,并有可能扩展到多原子系统.
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