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J. Robert Oppenheimer and Albert Einstein at the Institute for Advanced Study in Princeton |
A hundred years ago in November, 1915, Albert Einstein sent a paper to the Prussian Academy of Sciences which was to become one of the great scientific papers of all time. In this paper Einstein published the full treatment of his so-called field equations which present the curvature of spacetime by gravity; the paper heralded the the culmination of his general theory of relativity.
Forty years later when Einstein died, the implications of that paper had completely changed our view of the cosmos. They had explained the anomalous precession of Mercury, predicted the bending of starlight and most importantly, the expansion of the universe. Einstein enthusiastically accepted all these conclusions. One conclusion that he did not however accept and which in fact he did not seem interested in was the implications of the equations in areas of the cosmos where the force of gravity is so strong that it does not allow even light to escape – a black hole. Today we know that black holes showcase Einstein’s general theory of relativity in all its incandescent glory. In addition black holes have become profound playgrounds for some of the deepest mysteries of the universe, including quantum mechanics, information theory and quantum gravity.
And yet Einstein seemed almost pathologically uninterested in them. He had heard about them from many of his colleagues; in particular his Princeton colleague John Wheeler had taken it upon himself to fully understand these strange objects. But Einstein stayed aloof. There was another of the same persuasion whose office was only one floor away from him – J. Robert Oppenheimer, the architect of the atomic bomb and the Delphic director of the Institute for Advanced Study where Einstein worked. Oppenheimer in fact had been the first to mathematically describe these black holes in a seminal paper in 1939. Unfortunately Oppenheimer’s paper was published on the same day that Hitler attacked Poland. In addition its importance was eclipsed by another article in the same issue of the journal Physical Review: an article by Niels Bohr and John Wheeler describing the mechanism of nuclear fission, a topic that would soon herald urgent and ominous portents for the fate of the world.
The more general phenomena of gravitational contraction and collapse that black holes exhibit were strangely phenomena that seemed doomed to obscurity; in a strange twist of fate, those who truly appreciated them stayed obscure, while those who were influential ignored them. Among the former were Subrahmanyan Chandrasekhar and Fritz Zwicky; among the latter were Oppenheimer, Einstein and Arthur Eddington. In 1935, Chandrasekhar had discovered a limiting formula for white dwarfs beyond which a white dwarf could no longer thwart its inward gravitational pull. He was roundly scolded by Eddington, one of the leading astronomers of his time, who stubbornly refused to believe that nature would behave in such a pathological manner. Knowing Eddington’s influence in the international community of astronomers, Chandrasekhar wisely abandoned his pursuit until others validated it much later.
The Swiss-born Fritz Zwicky was a more pugnacious character, and in the 1930s he and his Caltech colleague Walter Baade published an account of what we now call a neutron star as a plausible explanation for the tremendous energy powering the luminous explosion of a supernova. Zwicky’s prickly and slightly paranoid personality led to his distancing from other mainstream scientists and his neutron stars were taken seriously by only a few scientists, among them the famous Soviet physicist Lev Landau. It was building on Landau’s work in 1938 and 1939 that Oppenheimer and his students published three landmark papers which pushed the envelope on neutron stars and asked what would be the logical, extreme conclusion of a star completely unable to support itself against its own gravity. In the 1939 paper in particular, Oppenheimer and his student Hartland Snyder presented several innovations, among them the difference between time as measured by an external observer outside a black hole’s so-called event horizon and a free falling observer inside it.
Then World War 2 intervened. Einstein got busy signing letters to President Franklin Roosevelt warning him of Germany’s efforts to acquire nuclear weapons while Oppenheimer got busy leading the Manhattan Project. When 1945 dawned both of them had forgotten about the key theoretical insights regarding black holes which they had produced before the war. It was a trio of exceptional scientists – Dennis Sciama in the UK, John Wheeler at Princeton and Yakov Zeldovich in the USSR – who got interested in black holes after the war and pioneered research into them.
What is strangest about the history of black holes is Einstein and Oppenheimer’s utter indifference to their existence. What exactly happened? Oppenheimer’s lack of interest wasn’t just because he despised the free-thinking and eccentric Zwicky who had laid the foundations for the field through the discovery of black holes’ parents – neutron stars. It wasn’t even because he achieved celebrity status after the war, became the most powerful scientist in the country and spent an inordinate amount of time consulting in Washington until his carefully orchestrated downfall in 1954. All these factors contributed, but the real reason was something else entirely – Oppenheimer simply wasn’t interested in black holes. Even after his downfall, when he had plenty of time to devote to physics, he never talked or wrote about them. He spent countless hours thinking about quantum field theory and particle physics, but not a minute thinking about black holes. The creator of black holes basically did not think they mattered.
Oppenheimer’s rejection of one of the most fascinating implications of modern physics and one of the most enigmatic objects in the universe – and one he sired – is documented well by Freeman Dyson who tried to initiate conversations about the topic with him. Every time Dyson brought it up Oppenheimer would change the subject, almost as if he had disowned his own scientific children.
“Oppenheimer in his later years believed that the only problem worthy of the attention of a serious theoretical physicist was the discovery of the fundamental equations of physics. Einstein certainly felt the same way. To discover the right equations was all that mattered. Once you had discovered the right equations, then the study of particular solutions of the equations would be a routine exercise for second-rate physicists or graduate students.”