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Living Life: April 25, 2019

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that had eluded scientists for 47 years – he<br />

discovered the solution to Einstein’s equations<br />

that define the space outside a rotating star or<br />

black hole. This was something many in the field<br />

doubted could be done.<br />

Professor Kerr’s discovery triggered a revolution<br />

in the field of astrophysics and is now known as<br />

the ‘Kerr Vacuum’.<br />

Dr Kerr returned to New Zealand and the<br />

University of Canterbury in 1971, where he<br />

became a Professor of Mathematics for 22 years<br />

until his retirement in 1993. Professor Kerr<br />

developed strong links with the department of<br />

physics and astronomy, where his seminal work<br />

on the Kerr Vacuum provided the basis of much<br />

research and teaching.<br />

Professor Kerr was awarded the British Royal<br />

Society’s Hughes Medal in 1984 and the<br />

Rutherford Medal from the New Zealand Royal<br />

Society in 1993. He was made a Companion of<br />

the New Zealand Order of Merit in 2011, and was<br />

awarded the 2013 Albert Einstein medal by the<br />

Albert Einstein Society in Switzerland.<br />

The University of Canterbury awarded the rare<br />

honour of the title Canterbury Distinguished<br />

Professor to Emeritus Professor Roy Kerr who<br />

also received the prestigious Crafoord Prize<br />

in Sweden in 2016. Canterbury Distinguished<br />

Professor is the highest academic title that can be<br />

awarded by the University and has been conferred<br />

only twice before in the University’s history. Title<br />

recipients are Nobel Prize winners or equivalent,<br />

such as the Crafoord Prize, which is worth over<br />

$NZ1 million.<br />

STEPHEN HAWKING ON<br />

ROY KERR:<br />

One of the world’s foremost theoretical physicists<br />

famous for his work on black holes, Stephen<br />

Hawking, described Kerr’s discovery in his<br />

celebrated book, A Brief History of Time.<br />

Hawking wrote: “In 1963, Roy Kerr, a New<br />

Zealander, found a set of solutions of the<br />

equations of general relativity that described<br />

rotating black holes. These ‘Kerr’ black holes<br />

rotate at a constant rate, their size and shape<br />

depending only on their mass and rate of<br />

rotation. If the rotation is zero, the black hole<br />

is perfectly round, and the solution is identical<br />

to the Schwarzschild solution. If the rotation is<br />

non-zero, the black hole bulges outward near<br />

its equator (just as the Earth or the Sun bulge<br />

due to their rotation), and the faster it rotates,<br />

the more it bulges. So ... it was conjectured that<br />

any rotating body that collapsed to form a black<br />

hole would eventually settle down to a stationary<br />

state described by the Kerr solution. In 1970 a<br />

colleague and fellow research student of mine at<br />

Cambridge, Brandon Carter, took the first step<br />

toward proving this conjecture. He showed that,<br />

provided a stationary rotating black hole had<br />

an axis of symmetry, like a spinning top, its size<br />

and shape would depend only on its mass and<br />

rate of rotation. Then, in 1971, I proved that any<br />

stationary rotating black hole would indeed have<br />

such an axis of symmetry. Finally, in 1973, David<br />

Robinson at Kings College, London, used Carter’s<br />

and my results to show that the conjecture had<br />

been correct: such a black hole had indeed to be<br />

the Kerr solution.”<br />

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