GlobalNuclearNews

Nuclear History archive — page 15

A glowing pearl-like sphere inside a clear glass ring carrying a luminous wave with exactly four crests, above soft ripples on a bright pale-blue background

de Broglie's Matter Waves (1924)

In November 1924 Louis de Broglie defended a thesis giving every particle a wavelength λ = h/p; Davisson, Germer and G. P. Thomson confirmed electron waves in 1927, and the idea underpins quantum mechanics and reactor neutron physics.

A cluster of glowing amber glass spheres forming an atomic nucleus with one empty dashed outline, examined by a brass magnifying glass on a bright blue background

Rutherford Predicts the Neutron (1920)

On 3 June 1920 Ernest Rutherford proposed a neutral particle of mass about 1, a 'neutral doublet' of proton and electron, which James Chadwick finally found as the neutron in 1932.

A small glowing sun held inside a clear glass sphere on a stone pedestal, with a tiny lump of coal beside it

Eddington's Stellar Energy Hypothesis (1920)

On 24 August 1920 Arthur Eddington argued in Cardiff that gravitational contraction could not power the Sun and that stars must run on sub-atomic energy released as hydrogen becomes helium.

A polished brass balance with four small glowing blue spheres on one pan slightly outweighing one glowing amber sphere on the other, against a bright sky-blue background

Aston's Mass Spectrograph and the Mass Defect (1919–1922)

In 1919 Francis Aston built the mass spectrograph, established the whole-number rule for isotopes, and measured that helium weighs less than four hydrogen atoms, earning the 1922 Nobel Prize in Chemistry.

A brass and glass gas chamber in which a glowing particle strikes a blue nucleus and a thin beam of light flies on to a small glowing screen, on a bright background

Rutherford's First Artificial Transmutation (1919)

In 1919 Rutherford showed that alpha particles knock hydrogen nuclei out of nitrogen, the first artificial transmutation; in 1925 Blackett's cloud chamber revealed that the nitrogen becomes oxygen-17.

A glass laboratory flask and a brass vacuum tube on a sunlit bench beside a worn leather notebook with a red remembrance poppy

Scientists in the First World War (Haber and Moseley)

The First World War mobilized science as never before: Fritz Haber directed the 1915 chlorine attack at Ypres, Henry Moseley was killed at Gallipoli aged 27, and James Chadwick spent four years interned at Ruhleben.

A clear glass cube holding three glowing golden spheres of different sizes beneath an antique brass balance scale on a bright blue background

Soddy and the Isotope (1913)

In 1913 the displacement law of Fajans and Soddy showed that atoms of different weight can share one place in the periodic table; Soddy named them isotopes in Nature on 4 December 1913, and lead from radioactive minerals confirmed it in 1914.

A row of glowing translucent glass tiles shading from blue to amber, with evenly stepped lines of light on the wall behind them

Moseley and the Atomic Number (1913)

In 1913–1914 Henry Moseley found that X-ray frequencies step up regularly from element to element, proving that the atomic number is the nuclear charge, fixing cobalt at 27 and nickel at 28, and exposing gaps at 43, 61 and 75.

A floating glass-and-brass staircase above a glowing core, with a small blue sphere stepping down and emitting a thin red beam of light

Bohr's Atomic Model (1913)

In 1913 Niels Bohr proposed that electrons occupy only fixed stationary states and emit light when they jump between them, reproducing the Balmer lines of hydrogen and saving Rutherford's nuclear atom.

A huge, almost empty clear glass sphere with one tiny glowing golden bead at its centre and light beams passing through, one bending away

Rutherford and the Atomic Nucleus (1911)

In 1911 Ernest Rutherford showed that an atom's mass and charge are concentrated in a tiny central charge, predicted the 1/sin⁴(φ/2) scattering law, and saw it confirmed by Geiger and Marsden in 1913.