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Planck angle : ウィキペディア英語版
Planck angle

In physics, the Planck angle is a hypothesised limit on the smallest discernible angle. An observable example approaching this is the astronomical observation of one of the smaller astronomical bodies, a gamma ray burster, at the furthest possible observable distance. The angle subtended by such a small object, so far away, is considered to approach the Planck limit on angles.
The Planck angle is denoted ''φ''p, is related to the ratio of the Planck length
:\ell_\text =\sqrt\frac \approx 1.616\;199 (97) \times 10^ \text
to the classical electron radius or "electromagnetic length"
:r_\text = \frac\frac = 2.817 940 3267(27) \times 10^ \text,
so that
:\varphi_\text \sim \frac} \sim 5.73 \times 10^.
It is thought this angle is the smallest angle between the world lines of free photons, which may interact with electrons or pass through the QED vacuum.
== References ==


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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