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Hermann Bondi

 
Scientist: Sir Hermann Bondi

British–Austrian mathematician and cosmologist (1919–2005)

See Hoyle, Sir Fred.
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Biography: Hermann Bondi
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English astrophysicist Hermann Bondi (born 1919) made his career out of studying the universe and its origins. Although his "steady state" theory was eventually discarded in favor of the "big bang" theory of creation, Bondi opposed what he called the "arrogance of certainty" that discouraged scientists and others from questioning current theories of the universe's origins.

Born in Vienna, Austria, on November 1, 1919, Bondi grew up with Jewish parents who disagreed about the importance of religious observances. "My father didn't believe, but liked the religious observances and rituals as social cement. My mother was a nonbeliever who didn't like the forms," he said in an interview in Free Inquiry. He credited his attraction to humanism to this division between his parents.

By 1933, social strife in Austria was peaking; Nazi leader Adolf Hitler had come to power, and Bondi's country struggled to remain independent. The increasing prominence of the Nazi party in Austria led to two civil wars within six months. In his autobiography, Bondi recalled, "It was against this background that I threw myself into my mathematical physics and dreamt of going to live elsewhere." By 1936, Bondi realized that his academic potential could never be realized while still living in Austria, and he began to work toward acceptance at Cambridge University, in England. He moved to England to attend Trinity College, Cambridge, in 1937 and considered it his home ever since.

Despite his allegiance to England, anti-German and anti-Nazi fervor during World War II put all immigrants and foreigners under suspicion, and Bondi, despite his Jewish heritage, was not an exception. In May of 1940, he was interned along with most other foreigners in Britain, remaining confined on the Isle of Man. He was later transferred to Canada and while there he attempted to immigrate to the United States, where his family had moved to escape Nazi persecution. Because he had arrived in Canada as an internee, very nearly a prisoner of the British government, the United States refused to permit his immigration. He returned to the Isle of Man, still under internment, and was not released until August 1941.

Advanced the Steady-State Theory

Upon returning to Cambridge, Bondi worked with other astro-physicists who would be influential in his career: Thomas Gold and Fred Hoyle. In the Bulletin of the Institute of Mathematics and its Applications, Hoyle claimed that he persuaded both Bondi and Gold to become interested in astronomy. "Hermann was the most confident manipulator of equations I had ever seen," Hoyle recalled. Hoyle reported that Bondi had a very theoretical mind, which "led him at times of course to lose contact with physical reality."

In 1948, Gold and Bondi worked together to develop the steady-state theory of the creation of the universe, which held that the universe is ever-expanding, without a beginning and without an end. They supported the theory by appealing to the perfect cosmological principle, according to which the universe is the same at all points; their colleague Hoyle advanced the same theory according to physical laws. The theory addressed a crucial problem of astrophysics: How do the stars continually recede without disappearing altogether? Dr. Edwin Hubble had already demonstrated that the stars actually do recede, but no one had yet explained why their recession did not leave a void in the universe.

As Bondi explained in his book Cosmology, "Since the universe must be expanding, new matter must be continually created in order to keep the density constant." Cosmologists had previously believed that the expansion of the universe marked the beginning of time, and that as it expanded outward it was approaching the end of its existence. These views were based on the belief that there was a moment when everything was suddenly created together in a dense mass. According to Bondi and Gold's steady-state theory, creation was continuous: it did not occur suddenly, and it was still occurring. The spontaneous creation of matter, they maintained, was brought about by the interchangeability of matter and energy, as demonstrated by Albert Einstein.

While Bondi accepted that the steady-state theory was as yet only an unproven hypothesis, he argued that the theory would create more possibilities for scientific discovery than the belief that creation was an event in the past: "The hypothetical character of continual creation has been pointed out, but why is it more of a hypothesis to say that creation is taking place now than that it took place in the past? On the contrary, the hypothesis of continual creation is more fertile in that it answers more questions and yields more results, and results that are, at least in principle, observable. To push the entire question of creation into the past is to restrict science to a discussion of what happened after creation while forbidding it to examine creation itself. This is a counsel of despair to be taken only if everything else fails."

Failed Theory Led to Applied Science

Bondi later worked with R.A. Lyttleton of Imperial College, London. In 1959, the two proposed that the outward movement of planets and stars was the result of electrical "leaks" in space. The theory was founded on the assumption that galaxies have electrical charges on the surface, producing a force of repulsion that surpassed the force of gravitational attraction. As the New York Times reported, one of the strengths of the theories was its potential to explain the origin of cosmic rays. The equipment to test their theory, however, was not available, although physicists were not able to find a flaw in their logic.

A strong believer in scientists' responsibility to explain their work to society, Bondi began writing books for students and laypeople and appearing on BBC educational programs in Britain. Chief among his efforts was his attempt to explain the theory of relativity and the works of Isaac Newton and Albert Einstein. As John Durston explained in the preface to Bondi's book Relativity and Common Sense: A New Approach to Einstein, "Where previous writers have tried to develop relativity in opposition to the ideas of Isaac Newton, Professor Bondi derives relativity from Newtonian ideas. He pictures relativity as being neither revolutionary nor destructive of classical dynamics but rather as being an organic growth." Bondi felt strongly that all scientific advancement came from, as Newton had said, "standing on the shoulders of giants."

As Bondi was reflecting on the inevitable evolution of scientific theories, he saw his own steady-state theory threatened with obsolescence. In 1965, Arno Penzias and Robert Wilson discovered a radiation background in microwaves. This radiation, it was hypothesized, was background noise from the "big bang." Although the "big bang" theory has roots as early as 1922, the discovery of this radiation brought it back into prominence. Cambridge radio astronomer Martin Ryle told Newsweek, "I think after this few students will go into the steady-state theory in detail."

While Bondi's colleague, Hoyle, began revising the steady-state theory to take into account the new data, Bondi moved on to problems in applied science. In 1967, Bondi was appointed director of the European Space Research Organization. One of his main achievements while in office was the development of plans for phone and air-traffic satellites for Western Europe. These satellites would enable international phone connections that had previously required several hours to complete. Perhaps more important, they would increase air-traffic controllers knowledge of a plane's location, particularly as it began to "disappear" over the horizon of the Atlantic Ocean. In 1971, he became chief scientific advisor to Britain's Ministry of Defence, a post he maintained through 1977, when he became chief scientist for the Department of Energy. Bondi also served as chairman and chief executive of the Natural Environment Research Council (NERC), for which he traveled widely, attempting to generate interest and income for scientific research.

Returned to Cambridge

Throughout this time, Bondi continued his scholarly pursuits, publishing several papers and serving twice as president of the Institute of Mathematics and its Application. Staying active in his academic discipline enabled him to return to Cambridge when he retired from government service in 1980. He took the position of Master of Churchill College, Cambridge, from 1983-1990, and continued as a fellow there from 1990 onward.

Bondi was also an active advocate for humanism, signing in 1973 the "Humanist Manifesto II," in which 120 religious leaders, philosophers, scientists, and other thinkers declared, "Reason and intelligence are the most effective instruments that humankind possesses. There is no substitute: neither faith nor passion suffices in itself. The controlled use of scientific methods, which have transformed the nature and social sciences since the Renaissance, must be extended further in the solution of human problems. But reason must be tempered by humility, since no group has a monopoly on wisdom or virtue."

In 1992 Bondi became president of the British Humanist Association, through which he lobbied for tolerance of differing viewpoints and appreciation for the life-enhancing benefits of science. In particular, he stressed the importance of continuing to question the origins of life and of the universe. "I don't think answers to these question are the business of us humans," he said in Free Inquiry, "Trying to get there-asking questions, investigating, discussing, sharing views, sharing arguments-that is the important thing. The continuing quest is what we humans must work for, not achieving the final answer."

Further Reading

Bondi, Hermann, Cosmology, Cambridge University Press, 1952.

Bondi, Hermann, Relativity and Common Sense: A New Approach to Einstein, Heinemann, 1965.

Bondi, Hermann, Science, Churchill and Me: The Autobiography of Hermann Bondi, Pergamon, 1990.

Bulletin of the Institute of Mathematics and its Applications, December, 1989.

Free Inquiry, Spring 1992.

Newsweek, October 25, 1965.

New York Times, May 24, 1952; May 24, 1959; October 13, 1970; August 26, 1973.

Wikipedia: Hermann Bondi
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Sir Hermann Bondi

Born November 1, 1919(1919-11-01)
Austria
Died September 10, 2005 (aged 85)
Cambridge, Cambridgeshire, England
Nationality England
Fields mathematician
physical cosmology
Known for steady-state theory of the universe
Religious stance Humanism

Sir Hermann Bondi, KCB, FRS (1 November 191910 September 2005) was an Anglo-Austrian mathematician and cosmologist. He is best known for developing the steady-state theory of the universe with Fred Hoyle and Thomas Gold as an alternative to the Big Bang theory, but his most lasting legacy will probably be his important contributions to the theory of general relativity.

Contents

Early life

Bondi was born in Austria, the son of a medical doctor. He was brought up in Vienna, where he studied at the Realgymnasium. He showed early prodigious ability at mathematics, and was recommended to Sir Arthur Eddington by Abraham Frankel. Frankel was a distant relation, the only mathematician in the extended family, and Hermann's mother had the foresight to engineer a meeting between her young son and the famous man, knowing that this might be the key to enabling him to follow his wishes and become a mathematician himself. Eddington encouraged him to travel to England to study at Trinity College, Cambridge. He arrived in Cambridge in 1937, escaping from anti-semitism in Austria. Realising the perilous position of his parents in 1938, shortly before the Anschluss, he sent them a telegram telling them to leave Austria at once. They managed to reach Switzerland, and later settled in New York.

In the early years of World War II, he was interned on the Isle of Man and in Canada as an enemy alien. Other internees included Thomas Gold and Max Perutz. Bondi and Gold had been released by the end of 1941, and worked with Fred Hoyle on radar at the Admiralty Signals Establishment. He became a British subject in 1946.

Bondi lectured in mathematics at the University of Cambridge from 1945 to 1954.

Theoretical work

In 1948, Bondi, Hoyle and Gold formulated the steady-state theory, which holds that the universe is constantly expanding but matter is constantly created to form new stars and galaxies to maintain a constant average density. It is probably fair to say that this theory dominated over the rival Big Bang theory until the discovery of the cosmic background radiation caused a sudden change in fortune.

Bondi was a major contributor to the golden age of general relativity (roughly 1960-1975). He was one of the first to correctly appreciate the nature of gravitational radiation, introducing Bondi radiation coordinates, the Bondi k-calculus, and the notion of Bondi mass, and writing influential review articles. He popularized the sticky bead argument which was said to be originally due, anonymously, to Richard Feynman, for the claim that physically meaningful gravitational radiation is indeed predicted by general relativity, an assertion which was controversial up until about 1955. An influential 1947 paper revived interest in the Lemaitre-Tolman metric, an inhomogeneous, spherically symmetric dust solution (often called the LTB or Lemaître-Tolman-Bondi metric). Bondi also contributed to the theory of accretion of matter from a cloud of gas onto a star or a black hole, working with Raymond Lyttleton and giving his name to "Bondi accretion" and the "Bondi radius".

He became a professor at King's College London in 1954, and was given the title of Emeritus Professor there in 1985. He was secretary of the Royal Astronomical Society from 1956 to 1964.

Other work

Bondi was also active outside the confines of academic lecturing and research. He held many positions:

He became a fellow of the Royal Society in 1959 and was appointed a Knight Commander of the Bath in 1973. He was awarded the Einstein Society Gold Medal in 1983, the Gold Medal of the Institute of Mathematics and its Applications in 1988, the G.D. Birla International Award for Humanism, and the Gold Medal of the Royal Astronomical Society in 2001.

His report into the flooding of London in 1953 led eventually to the building of the Thames Barrier. He also supported the proposal for a Severn Barrage to generate electricity, but this project was not carried forward.

His papers from 1940 to 2000 are archived in 109 archive boxes by the Janus Project in Cambridge.

Personal life

His parents were Jewish, but he never "felt the need for religion" and was a lifelong humanist. He was president of the British Humanist Association from 1982 to 1999, and president of the Rationalist Press Association from 1982.

He married his wife, Christine, in 1947; she had been one of Hoyle's research students and like him she went on to be active in the humanist movement. Together, they had two sons and three daughters. He died in Cambridge [1]

See also

References

  1. ^ GRO Register of deaths: SEP 2005 D67C 21 CAMBRIDGE - Hermann Bondi, DoB = 1 Nov 1919, aged 85

External links



Academic offices
Preceded by
William Hawthorne
Master of Churchill College
1983–1990
Succeeded by
Alec Broers

 
 
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Sir Fred Hoyle (British astrophysicist)
Olbers' paradox (astrophysics)
Max Ferdinand Perutz (Austrian–British biochemist)

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