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Quantum physicist of black holes

Stephen Hawking

1942–2018

Stephen Hawking connected gravity, quantum physics and thermodynamics. He predicted that black holes can emit radiation, transforming the questions scientists ask about these extreme objects.

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Stephen Hawking
Documentary photograph.
Photographer: Doug Wheller, cropped and tweaked by W.carter · CC BY 2.0 · Portrait source
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A life of research

Born in Oxford, he studied there before moving to Cambridge. Living with a progressive neurological illness, he continued his research with human assistance and specially adapted communication technology.

His early work investigated singularities in general relativity, in close intellectual connection with Roger Penrose's research. These studies explored conditions under which classical descriptions of spacetime reach their limits.

Understanding the contribution

In 1974 he showed that quantum effects near an event horizon lead to a temperature and radiation associated with a black hole. An object usually described as completely dark can therefore lose energy.

This theoretical result, known as Hawking radiation, has not been directly observed from astrophysical black holes. It raises fundamental questions about information and about reconciling gravity with quantum mechanics.

What this work changed

His 1988 book A Brief History of Time brought these subjects to a large public audience. It presented major cosmological questions as matters for scientific investigation, even when their answers remain incomplete.

Sources and references