Physics, Pixelated

Two glowing nucleons in a nucleus exchanging a bright meson across the tiny gap between them

Hideki Yukawa and the Meson: How a Force’s Rang...

In 1934 Hideki Yukawa asked why the force that holds the nucleus together reaches only about the width of a proton. His answer: a force carried by a particle with...

Hideki Yukawa and the Meson: How a Force’s Rang...

In 1934 Hideki Yukawa asked why the force that holds the nucleus together reaches only about the width of a proton. His answer: a force carried by a particle with...

A vast field of glowing up and down spin arrows, aligned on one side and breaking into domains of every size

The Ising Model Explained: How Tiny Arrows Expl...

The Ising model is the simplest picture of a magnet: a grid of arrows that can only point up or down, each wanting to match its neighbours. Heat scrambles them;...

The Ising Model Explained: How Tiny Arrows Expl...

The Ising model is the simplest picture of a magnet: a grid of arrows that can only point up or down, each wanting to match its neighbours. Heat scrambles them;...

An observatory beside a glowing Airy disk with its rings, and an X-ray beam reflecting off a crystal lattice

The Airy Disk and the Diffraction Limit: Why Ev...

A perfect lens still cannot focus light to a point. Waves spread out after passing through any opening, so every star becomes a tiny bright disk with faint rings, the...

The Airy Disk and the Diffraction Limit: Why Ev...

A perfect lens still cannot focus light to a point. Waves spread out after passing through any opening, so every star becomes a tiny bright disk with faint rings, the...

A spinning pulsar sweeping twin radio beams over a field of wire radio antennas at night

Jocelyn Bell Burnell and the Discovery of Pulsars

In late 1967 Jocelyn Bell, a PhD student at Cambridge, noticed a strange signal among miles of chart paper. It turned out to be a pulsar, a spinning neutron star....

Jocelyn Bell Burnell and the Discovery of Pulsars

In late 1967 Jocelyn Bell, a PhD student at Cambridge, noticed a strange signal among miles of chart paper. It turned out to be a pulsar, a spinning neutron star....

An ancient dim halo star glowing above a distant spiral galaxy

The Cosmological Lithium Problem: Big Bang’s Mi...

The Big Bang’s first minutes forged hydrogen, helium and a trace of lithium, and the theory matches deuterium and helium beautifully. Lithium-7 is the odd one out: the oldest stars...

The Cosmological Lithium Problem: Big Bang’s Mi...

The Big Bang’s first minutes forged hydrogen, helium and a trace of lithium, and the theory matches deuterium and helium beautifully. Lithium-7 is the odd one out: the oldest stars...

A proton cut open to show three coloured quarks inside a turbulent glowing sea of gluon energy

Where Does the Proton’s Mass Come From? (Hint: ...

A proton weighs 938 MeV/c², but its two up quarks and one down quark add up to only about 9 MeV/c², roughly 1%. The rest is energy: the motion of...

Where Does the Proton’s Mass Come From? (Hint: ...

A proton weighs 938 MeV/c², but its two up quarks and one down quark add up to only about 9 MeV/c², roughly 1%. The rest is energy: the motion of...