Particle lifetimes from the uncertainty principle粒子寿命与不确定性原理
If the width of this distribution at half-maximum is labeled Γ , then the uncertainty in energy ΔE could be reasonably expressed as 如果这个分布在半高处的宽度标记为Γ,那么能量的不确定性ΔE可以合理地表示为
![]() where the particle lifetime τ is taken as the uncertainty in time τ = Δt. 其中,粒子寿命τ被取为时间的不确定性τ = Δt。
In high energy scattering experiments, the energy uncertainty ΔE can be determined and the lifetime implied from it. In other cases, the lifetime is most conveniently measured and the "particle width" in energy implied from that lifetime measurement. 在高能散射实验中,可以确定能量不确定性ΔE,并由此推断出寿命。在其他情况下,寿命最方便地通过测量来确定,而通过该寿命测量可以推断出‘粒子宽度’。
Γ is often referred to as the "natural line width". It is of great importance in high energy accelerator physics where it provides the means for determining the ultrashort lifetimes of particles produced. For optical spectroscopy it is a minor factor because the natural linewidth is typically 10-7 eV, about a tenth as much as the Doppler broadening. Another source of linewidth is the recoil of the source, but that is negligible in the optical range. Γ通常被称为“自然线宽”。它在高能加速器物理中具有重要意义,因为它为确定粒子的极短寿命提供了手段。对于光学光谱学来说,它是一个次要因素,因为自然线宽通常为10⁻⁷ eV,大约是多普勒展宽的十分之一。另一个导致线宽的因素是源的反冲,但在光学范围内可以忽略不计。
For nuclear transitions involving gamma emission in the 0.1-1 MeV range, the recoil width is typically much greater than the natural line width. The recoil of the emitting nucleus implies that the emitted gamma photon cannot be absorbed by an identical nucleus because its energy is reduced by an amount greater than the natural line width of potential absorbing levels. Mossbauer discovered that the absorption could be accomplished by putting the source on a rotating arm to give it enough speed to compensate for the recoil effect. The Mossbauer effect became a useful experimental tool when it was discovered that the recoil could be suppressed by putting the emitting nucleus in a crystal lattice. The emitted gammas then exhibited something close to the natural linewidth and could be absorbed by other identical nuclei. 对于涉及0.1-1 MeV范围内的伽马发射的核跃迁,反冲宽度通常远大于自然线宽。发射核的反冲意味着,发出的伽马光子不能被相同的核吸收,因为其能量减少了超过潜在吸收能级的自然线宽。莫塞莱发现,通过将源放在旋转臂上,使其获得足够的速度以补偿反冲效应,可以实现吸收。当发现通过将发射核置于晶体晶格中可以抑制反冲效应时,莫塞莱效应成为一种有用的实验工具。此时发出的伽马射线接近自然线宽,可以被其他相同的核吸收。
能量的不确定性可以取为该值的一半。 |
Index Uncertainty principle concepts Reference Rohlf Ch 5 索引 不确定性原理 概念 参考 Rohlf 第5章 | ||||
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