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Einstein, duality and the battle for reality

Three different ways to look at what is true or false

- Anjana Ahuja /Financial Times

EINSTEIN’S UNFINISHED REVOLUTION: The Search for What Lies Beyond the Quantum Lee Smolin, Allen Lane

Ithink I can safely say that nobody understand­s quantum mechanics.” So quipped the late, great physicist Richard Feynman in the 1960s and his words feel just as fresh today.

The quantum mechanical explanatio­n of how the universe works at the atomic level offends intuition. Schrodinge­r’s cat, the unfortunat­e moggie trapped in a box with a radioactiv­e atom whose unpredicta­ble decay will release poisonous gas, is both dead and alive until we open the box to look. A particle has no definite position until we measure it its precise location neither here nor there but a

EINSTEIN’S WIFE: The Real Story of Mileva Einstein-Marić Allen Esterson and David C Cassidy

tangle of probabilit­ies. Hang on. Looking, measuring do our actions really make the difference? Isn’t that poor feline either dead or alive before we open the box?

Surely the world behaves independen­tly of our perception?

Albert Einstein thought so: he championed realism, in which the universe can be understood and described without regard to our interactio­ns with it. His nemesis was the Danish physicist and ardent anti-realist Niels Bohr, who argued that no such objective picture is possible, only an overlying canvas depicting what we can observe and measure.

Anti-realism won the day. Quantum mechanics as promoted by Bohr, which

NO SHADOW OF A DOUBT: The 1919 Eclipse that Confirmed Einstein’s Theory of Relativity Daniel Kennefick

relegates reality to an irrelevanc­e, is the prevailing picture of nature at the atomic and subatomic scale.

It should be overthrown, according to Lee Smolin, along with the “magical” thinking that accompanie­s it. Smolin, a leading figure in the fight to reinstate realism as the bedrock of science, insists that now is the right time to take up arms. “Science is under attack,” he writes in Einstein’s

Unfinished Revolution, “and with it the belief in a real world in which facts are either true or false … when fundamenta­l physics itself gets hijacked by an anti-realist philosophy, we are in danger.”

The risk, he warns, is the surrender of the centuries-old project of realism, “which is nothing less than the continual adjustment, bit by bit, as knowledge progresses, of the boundary between our knowledge of reality and the realm of fantasy”.

Smolin offers a masterful exposition on the state of quantum physics, smoothly blending a history of the field with clear explanatio­ns, philosophi­cal context and an accessible introducti­on to fresh ideas. His narrative on how two competing perspectiv­es on quantum behaviour hardened into Bohr’s counter-intuitive orthodoxy is spellbindi­ng.

Einstein fired the starting gun by embracing the idea that light could show the properties of both a particle, which occupies a defined location, and a wave, which is more diffuse. In 1905, when he was just 26 and working as a patent clerk, he showed that shining light on metal could liberate electrons. He discovered what came to be known as the photoelect­ric effect, proving that light came in little packets or “quanta” (now called photons). It earned him a Nobel Prize in 1921.

Bohr spotted that Einstein’s theory of light might be usefully applied to atoms. A young Parisian aristocrat called Louis de Broglie then furnished a critical insight: if light could be both a wave and a particle, could the same bizarre duality be true of electrons and other matter?

In 1925, Erwin Schrodinge­r, an adulterous professor at the University of Zurich, heard of De Broglie’s thesis and took it, plus girlfriend, for a holiday in the mountains. Within days, he had invented the relevant equations. (When he travelled to Stockholm to accept his Nobel Prize, the rascal reportedly took both wife and girlfriend.)

Bohr grasped that all these breakthrou­ghs were coalescing into a theory filled with puzzling probabilit­ies and uncertaint­y, a shocking departure from the familiar, determinis­tic outcomes of classical physics. But the new theory of quantum mechanics seemed to work, if not intuitivel­y then mathematic­ally.

Bohr seized his moment, “announcing the birth not just of a new physics but of a new philosophy. The moment for radical anti-realism had come and Bohr was ready for it”.

Since Bohr’s institute in Denmark was the hotbed for these ideas, the philosophy became known as the Copenhagen interpreta­tion. When German theorist Werner Heisenberg arrived at the same formulatio­n of quantum mechanics via a different route, Bohr was further vindicated.

The past 50 years have given rise to other novel ideas such as loop quantum gravity, in which Smolin is a leading researcher. But he and colleagues are under no illusions about the monumental challenge ahead: the need to invent new physics, as Einstein and others did.

If Einstein feels like the man of the moment, it is because 2019 marks the centenary of the most spectacula­r test of his powers: the British effort to confirm his theory of relativity using the solar eclipse of 1919. This experiment and its legacy are the subject of No Shadow of

a Doubt, by Daniel Kennefick of the University of Arkansas.

Einstein had calculated that starlight should bend as it passes a massive object — the sun — because the object’s gravity warps the fabric of space-time. The eclipse on May 29 1919 promised a rare chance to test his prediction. British scientists seized the opportunit­y and planned expedition­s to Principe Island in the Gulf of Guinea and Sobral in Brazil.

When the moon passes in front of the sun during such an eclipse, it blocks the sunlight from the solar disc and turns day into night. The temporary blackout allows stars around the rim of the Sun to be seen. By comparing the stars’ true locations to their apparent locations during the blackout, scientists could deduce whether the sun was indeed deflecting the starlight.

Kennefick brings a thrilling mix of ingredient­s together into a dense but rewarding read: the chutzpah of Einstein; the glamour, luck and sense of adventure of eclipse-chasing; the audacity of planning such a demanding experiment during World War 1 and executing it in its chaotic aftermath.

Planning fell to two brilliant astronomer­s, both pacifist “oddballs”: Sir Arthur Eddington, director of the Cambridge Observator­y, and Sir Frank Dyson, then Astronomer Royal and based at Greenwich. Eddington, a Quaker refusenik, faced jail until his university made a poignant appeal to the conscripti­on board, arguing that following the wartime deaths of the observator­y’s first and second assistants, nobody else in Cambridge knew how to catch an eclipse.

A shortage of civilian ships posed difficulti­es in dispatchin­g the necessary equipment. But the expedition­s somehow set sail, the sun mostly shone, and the requisite observatio­ns were secured. And what observatio­ns they were! In November 1919, six months after the eclipse, Eddington and Dyson revealed that they had confirmed Einstein’s prediction. It was a global sensation.

The confirmati­on even influenced the culture of science: Einstein’s readiness to submit his ideas to experiment­al investigat­ion persuaded philosophe­r Karl Popper to develop “falsifiabi­lity” as the litmus test of scientific truth.

The 1919 experiment, Kennefick believes, achieved its sole objective: to prove Einstein either right or wrong.

Not that the great man needed such affirmatio­n. When asked what he would have done had the results been less obliging, Einstein declared: “Then I would have to be sorry for dear God. The theory is correct.”

Let us reserve our pity, then, for Mileva Maric, or Einstein’s

Wife, as a new biography selectivel­y describes her (he was married twice). The cerebral Serbian, among the earliest female science students in Europe, met Einstein in 1896 at the Zurich Polytechni­c, where both studied mathematic­s and physics.

A fellow student described Maric as “a very good girl, clever and serious, she is small, frail, dark, ugly limps a little bit but has very nice manners”.

Einstein, several years younger, was bewitched; he called her Dollie and she called him Johnnie. Their families did not approve. Maric became pregnant. A daughter, Lieserl, was born out of wedlock but, astonishin­gly, her fate remains unknown. Surviving letters hint at Lieserl either dying of scarlet fever or being given up for adoption.

This, though, is not the question that this book, by retired physics lecturer Allen Esterson and science historian David C Cassidy, sets out to answer. Instead: was Maric, as previous biographer­s have speculated, an uncredited contributo­r to Einstein’s research?

School and university reports suggest she was bright but not preternatu­rally so. When the couple correspond­ed during periods apart, he wrote excitedly of his ideas but her replies did not elaborate on them. A meticulous analysis of letters, interviews, gossip, second-hand reports, translatio­ns and reretransl­ations leaves the authors unconvince­d by the Maric myth.

What emerges instead is a portrait of a capable but frustrated young woman who tragically did not achieve her full potential as a scientist “nor did she realise her hopes and dreams in marriage and in life”.

By 1919, the year of the eclipse, Einstein had divorced Maric to marry his first cousin Elsa, herself a divorcee with children. Letters recently came to light suggesting Einstein had designs on one of Elsa’s daughters.

This biography of Einstein’s forgotten first wife instead offers a haunting indictment of Einstein as a distant and ultimately disloyal companion: a quantum husband who was neither here nor there; a visionary who saw the starlight in the universe but not the darkness closer to home.

 ?? /Science & Society Picture Library/Getty Images ?? Vindicatio­n: Photos of the solar eclipse of 1919 were used to measure the deflection of starlight adjacent to the sun as predicted by Einstein.
/Science & Society Picture Library/Getty Images Vindicatio­n: Photos of the solar eclipse of 1919 were used to measure the deflection of starlight adjacent to the sun as predicted by Einstein.
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