Stephen Hawking

6 Books

Stephen William Hawking was born on 8 January 1942 in Oxford, England. His parents' house was in north London, but during the second world war Oxford was considered a safer place to have babies. When he was eight, his family moved to St Albans, a town about 20 miles north of London. At eleven Stephen went to St Albans School, and then on to University College, Oxford, his father's old college. Stephen wanted to do Mathematics, although his father would have preferred medicine. Mathematics was not available at University College, so he did Physics instead. After three years and not very much work he was awarded a first class honours degree in Natural Science.

Stephen then went on to Cambridge to do research in Cosmology, there being no-one working in that area in Oxford at the time. His supervisor was Denis Sciama, although he had hoped to get Fred Hoyle who was working in Cambridge. After gaining his Ph.D. he became first a Research Fellow, and later on a Professorial Fellow at Gonville and Caius College. After leaving the Institute of Astronomy in 1973 Stephen came to the Department of Applied Mathematics and Theoretical Physics, and since 1979 has held the post of Lucasian Professor of Mathematics. The chair was founded in 1663 with money left in the will of the Reverend Henry Lucas, who had been the Member of Parliament for the University. It was first held by Isaac Barrow, and then in 1669 by Isaac Newton.

Stephen Hawking worked on the basic laws which govern the universe. With Roger Penrose he showed that Einstein's General Theory of Relativity implied space and time would have a beginning in the Big Bang and an end in black holes. These results indicated it was necessary to unify General Relativity with Quantum Theory, the other great Scientific development of the first half of the 20th Century. One consequence of such a unification that he discovered was that black holes should not be completely black, but should emit radiation and eventually evaporate and disappear. Another conjecture is that the universe has no edge or boundary in imaginary time. This would imply that the way the universe began was completely determined by the laws of science.

His many publications include The Large Scale Structure of Spacetime with G.F.R. Ellis, General Relativity: An Einstein Centenary Survey, with W. Israel, and 300 Years of Gravity, with W. Israel. Stephen Hawking has three popular books published; his best seller A Brief History of Time, Black Holes and Baby Universes and Other Essays and most recently in 2001, The Universe in a Nutshell.

Professor Hawking received twelve honorary degrees, was awarded the CBE in 1982, and was made a Companion of Honour in 1989. He was the recipient of many awards, medals and prizes and is a Fellow of The Royal Society and a Member of the US National Academy of Sciences.


Stephen Hawking's final interview: A beautiful Universe

By Pallab Ghosh

Science correspondent, BBC News

26 March 2018

Last October I invited Prof Stephen Hawking to comment on the detection of gravitational waves from the collision of two neutron stars. It turned out to be his final broadcast interview.

The collision was a really big story for many reasons, not least because within minutes of the detection the world's telescopes were trained on what was an incredible cosmic event.

This meant that as well as detecting the ripples in space-time from the merger, astronomers could see also for the first time what happens when two incredibly massive objects come together in a process that may be the only way of creating gold and platinum in the Universe.

It was definitely one for Prof Hawking to explain.

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In recent years, he made comments about climate change, space travel and artificial intelligence. His interviews always captivated audiences. I was lucky enough to have interviewed him many times and for me he was at his most enthralling when he was on 'home turf' - talking about the physics he so loved and bending our minds with the implications of new discoveries. And I was so touched and honoured to hear from his staff that he had always enjoyed our encounters.

I was only able to use one answer in my news report and so the rest of his interview was not broadcast or published. Here it is now in full. He leaves us with his trademark, awe-inspiring take on a cosmos that, as we look through his eyes, we should view as both beautiful and mysterious.

Tell us how important is the detection of two colliding neutron stars?

It is a genuine milestone. It is the first ever detection of a gravitational wave source with an electromagnetic counterpart. It confirms that short gamma-ray bursts occur with neutron star mergers. It gives a new way of determining distances in cosmology. And it teaches us about the behaviour of matter with incredibly high density.

What will we learn from the electromagnetic waves emanating from the collision?

The electromagnetic radiation gives us a precise location on the sky. It also tells us the 'redshift' of the event. The gravitational waves tell us the luminosity distance. Combining these measures give us a new way of measuring distances in cosmology. This is the first rung of what will become a new cosmological distance ladder. The matter inside a neutron star is much denser than anything we can produce in a laboratory. The electromagnetic signal from merging neutron stars will tell us about the behaviour of matter at such high density.

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Will it give us insights into how black holes form?

The fact that a black hole can form from the merger of two neutron stars was known from theory. But this event is the first test, or observation. The merger probably produces a rotating, hyper-massive neutron star which then collapses to form a black hole.

This is very different from other ways of forming black holes, such as in a supernova or when a neutron star accretes matter from a normal star. With careful analysis of the data and theoretical modelling on supercomputers, there is vast scope for new insights to be obtained about the dynamics of black hole formation and gamma-ray bursts.

Will gravitational wave measurements bring us a greater insight of how space-time and gravity operates and so transform our understanding of the Universe?

Yes, without a shadow of a doubt. An independent cosmological distance ladder may provide independent confirmation of cosmological observations or it may reveal huge surprises. Gravitational wave observations let us test general relativity in situations where a gravitational field is strong and highly dynamical. Some people think that general relativity needs modifying in order to avoid introducing dark energy and dark matter. Gravitational waves are a new way to search for a signature of possible modifications of general relativity. A new observational window on the Universe typically leads to surprises that cannot yet be foreseen. We are still rubbing our eyes, or rather ears, as we have just woken up to the sound of gravitational waves.

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Is the collision of neutron stars one of the very few ways, or possibly the only way, that gold is produced in Universe. Could this explain why it's so rare on Earth?

Yes, the collision of neutron stars is one way of producing gold. It can also be formed from fast neutron capture in supernovas. Gold is rare everywhere, not just on Earth. The reason it's rare is that by nuclear-binding energy peaks at iron, making it hard to produce heavier elements in general. Also strong electromagnetic repulsion must be overcome by the nuclear force in order to form stable heavy nuclei like gold.

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