Stephen Hawking

Theoretical physicist and cosmologist

8 January 1942, Oxford – 14 March 2018, Cambridge

  • Hawking radiation from black holes
  • Singularity theorems with Roger Penrose
  • A Brief History of Time (1988)

Stephen Hawking spent his life on the largest questions in physics: how the universe began, what happens inside black holes, and how gravity and quantum theory fit together. He also showed that these questions could be explained to anyone willing to follow the argument.

Life and Career

Hawking studied physics at University College, Oxford, and completed his PhD at Cambridge in 1966. At 21 he was diagnosed with motor neurone disease (ALS) and given only a few years to live. He lived and worked for more than five decades, communicating through a speech synthesiser in his later years.

With Roger Penrose he proved theorems showing that general relativity implies singularities, both at the beginning of the universe and inside black holes. In 1974 he showed that, once quantum effects are taken into account, black holes are not completely black: they emit radiation and slowly lose energy. This Hawking radiation linked gravity, thermodynamics and quantum theory in one result. From 1979 to 2009 he held the Lucasian Professorship of Mathematics at Cambridge, the chair once held by Isaac Newton. His book A Brief History of Time (1988) sold millions of copies worldwide.

Why His Work Matters Here

Hawking radiation is a lesson in energy accounting: even a black hole gives energy back to its surroundings, and the books always balance. The same discipline applies to every energy conversion on Earth. Output can only come from energy that is actually coupled in, and the Schubart Master Formula makes that balance explicit for materials exposed to ambient radiation.