Stephen Hawking (1942–2018)

When Stephen Hawking was diagnosed with motor-neuron disease at the age of 21, it wasn’t clear that he would finish his PhD. Against all expectations, he lived on for 55 years, becoming one of the world’s most celebrated scientists.

Hawking, who died on 14 March 2018, was born in Oxford, UK, in 1942 to a medical-researcher father and a philosophy-graduate mother. After attending St Albans School near London, he earned a first-class degree in physics from the University of Oxford. He began his research career in 1962, enrolling as a graduate student in a group at the University of Cambridge led by one of the fathers of modern cosmology, Dennis Sciama.

The general theory of relativity was at that time undergoing a renaissance, initiated in part by Roger Penrose at Birkbeck College, London, who had introduced new mathematical techniques. These showed that generic gravitational collapse would lead to singularities — infinities that signal the need for new physics.

Stephen Hawking: A life in science

The implications for black holes and the Big Bang were developed by Hawking in a series of papers collated in the 1973 monograph The Large Scale Structure of Space-Time (Cambridge University Press), co-authored with George Ellis, a near-contemporary who had also been a student of Sciama. Especially important was the realization that the area of black holes’ horizons (‘one-way membranes’ that shroud the singularities, and from within which nothing can escape) could never decrease. The analogy with entropy — a measure of disorder that likewise can never decrease — was developed further by physicist Jacob Bekenstein.

These findings gained Hawking election to the Royal Society in London in 1974, at the age of 32. By then, he was so frail that both movement and speech were difficult, and most of us suspected that his days in front-line research were numbered. But in that same year, he came up with his most distinctive contribution to science: Hawking radiation.

By linking quantum theory and gravity, Hawking showed that a black hole would not be completely black, but would radiate with a well-defined temperature that depended inversely on its mass (S. W. Hawking Nature 248, 30–31; 1974). Black-hole entropy was more than just an analogy. The implication was that the radiation would cause black holes to ‘evaporate’. This process would be unobservably slow, except in ‘mini-holes’ the size of atoms — and these are thought not to exist. Yet Hawking radiation — and the related issue of whether information that falls into a black hole is lost or is somehow recoverable from the radiation — was a profound issue, and one that still engenders controversy among theoretical physicists. Indeed, theorist Andrew Strominger at Harvard University in Cambridge, Massachusetts, said in 2016 that one of Hawking’s papers on the subject (S. W. Hawking Phys. Rev. D 14, 2460–2473; 1976) had caused “more sleepless nights among theoretical physicists than any paper in history”.

By the end of the 1970s, Hawking had been appointed to the Lucasian Chair of Mathematics at Cambridge (former incumbents include Isaac Newton and Paul Dirac); he held the post until he retired in 2009. During these years, in which his focus shifted to the quantum aspects of the Big Bang, the issue of information loss in black holes continued to challenge him.

In 1985, Stephen underwent a tracheotomy, which removed his already limited powers of speech. He was able to control a cursor on a screen and type out sentences — albeit with increasingly painful slowness (first with his hand, and eventually only with a cheek muscle). A speech synthesizer processed his words and generated the androidal accent that became his trademark. In this way, he completed his best-selling book A Brief History of Time (Bantam, 1988), which propelled him to celebrity status.