Construct · 1 fields · 3 citations
One name. One construct. A landmark on the map.
● anchor · a standalone constant Nearest construct by meaningRydberg constantcompare the meaningsEvery construct on the map is compared with every other by the meaning of its definitions, and the closest one is surfaced here. The nearest construct to fine-structure constant is Rydberg constant.
Hold this as a prompt, not a verdict. Two constructs sitting close in meaning is a reason to read them side by side and decide for yourself whether they are one idea under two names. It is not proof that they are. Compare the meanings in the Collider.
A single standalone construct; nearby constructs are located against it in the Collider. Tap a field for its definition, unit, and measures.
Arnold Sommerfeld introduced the fine-structure constant in 1916, in his relativistic extension of the Bohr model of the atom, where it first appeared as the ratio of the speed of an electron in the innermost hydrogen orbit to the speed of light and governed the small splitting, the fine structure, of atomic spectral lines. Written as the Greek letter alpha and equal to about 1/137, it is a pure number with no physical units: it combines the elementary charge, the speed of light, Planck's constant, and the electric constant into a single ratio that fixes how strongly electrically charged particles couple to light and to one another. Because it is dimensionless, its value is the same in every system of units and for every observer, which is why it serves as the standard measure of the strength of the electromagnetic interaction across atomic physics, quantum electrodynamics, and cosmology. Modern determinations, such as the atom-recoil measurement reported by Morel and colleagues in 2020 and the periodically adjusted CODATA recommended values, pin it down to better than one part in a billion, placing it among the most precisely known quantities in physics.[1][2][3]
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