Hideki Yukawa 2026-10-18
A physicist.[ref]
https://www.ndl.go.jp/portrait/datas/6080. Independent professional profile
[ref]https://www.kyoto-u.ac.jp/sites/default/files/embed/jaaboutpublicissueresearch_activitiesdocuments2012nobelvol2nobelallpages.pdf. Independent professional profile
Portrait of Hideki Yukawa
. Source. Nobel Prize in Physics in 1949 2026-10-18
Yukawa meson theory of nuclear forces 2026-10-18
In 1935, Hideki Yukawa proposed a new massive exchange quantum to explain nucleon binding. His paper began with the inadequacy of an Electron–neutrino exchange description of the binding strength. It then required a potential energy falling faster with distance than a Coulomb potential, introduced an exponentially decaying field, and related its inverse range to the exchange particle's rest mass. This was a theoretical proposal, not a detection with an apparatus of his own.[ref]
On the Interaction of Elementary Particles. I by Hideki Yukawa. On the Interaction of Elementary Particles. I, opening motivation, equations (1)–(3) and (12); text inspected in a retypeset mirror
The crucial idea is that a finite rest mass supplies a length scale even in empty space. In a scalar model, the static limit of a Klein-Gordon equation produces the modified Helmholtz equation. Its decaying Green's function gives the Yukawa potential. The derivation below isolates this range mechanism; one-pion exchange also carries spin and isospin structure.
The nuclear emulsion track experiment used developed photographic emulsions exposed to cosmic rays and inspected microscopically. Stopping pions gave daughter muon tracks with closely grouped ranges. Comparing penetrating muons with pion-induced nuclear breakup distinguished their interactions; this was not a direct static force measurement. The muon is a lepton, not Yukawa's strongly interacting meson.[ref]
The Cosmic Radiation by Cecil Frank Powell. The Cosmic Radiation, printed pp. 144–145 and 151–152, especially Fig. 5; inspected in the Columbia-hosted Nobel volume
