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Enrico Fermi (29 September 1901 – 28 November 1954) was an Italian physicist most noted for his work on the development of the first nuclear reactor, and for his contributions to the development of quantum theory, nuclear and particle physics, and statistical mechanics. Fermi was awarded the Nobel Prize in Physics in 1938 for his work on induced radioactivity and is today regarded as one of the top scientists of the 20th century. He is acknowledged as a unique physicist who was highly accomplished in both theory and experiment.
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Quotations
I cannot think of a single one, not even intelligence.
When asked what characteristics Nobel prize winning physicists had in common. As quoted in Physics Today (October 1994)
I hope it won't take long.
Comment to Eugene Wigner, ten days before his death from cancer, as quoted in The collected works of Eugene Paul Wigner (1992), p. 108
There are two possible outcomes: if the result confirms the hypothesis, then you've made a measurement. If the result is contrary to the hypothesis, then you've made a discovery.
As quoted in Nuclear Principles in Engineering (2005) by Tatjana Jevremovic, p. 397
Encyclopedia
Enrico Fermi (29 September 1901 – 28 November 1954) was an Italian physicist most noted for his work on the development of the first nuclear reactor, and for his contributions to the development of quantum theory, nuclear and particle physics, and statistical mechanics. Fermi was awarded the Nobel Prize in Physics in 1938 for his work on induced radioactivity and is today regarded as one of the top scientists of the 20th century. He is acknowledged as a unique physicist who was highly accomplished in both theory and experiment. Fermium, a synthetic element created in 1952 is named after him.
Biography
Early years
Enrico Fermi was born on September 29, 1901 in Rome, Italy to Alberto Fermi, a Chief Inspector of the Ministry of Communications, and Ida de Gattis, an elementary school teacher. As a young boy he enjoyed learning physics and mathematics and shared his interests with his older brother, Giulio. When Giulio died unexpectedly of a throat abscess in 1915, Enrico was distraught, and immersed himself in scientific study to distract himself. According to his own account, each day he would walk in front of the hospital where Giulio died until he became inured to the pain.
One of the first sources for the study of physics was a book found at the local market of Campo de' Fiori in Roma. The 900 page book, entitled Elementorum physicae mathematicae, was written in Latin by Father Andrea Caraffa, a professor at the Collegio Romano, covered subjects like mathematics, classical mechanics, astronomy, optics, and acoustics. Notes found in the book indicate Fermi studied it intensely.
Later, Enrico befriended another scientifically inclined student named Enrico Persico, and the two worked together on scientific projects such as building gyroscopes, and measuring the earth's magnetic field. Fermi's interest in physics was further encouraged by a friend of his father, Adolfo Amidei, who gave him several books on physics and mathematics, which he read and quickly assimilated.
Scuola Normale Superiore in Pisa
In 1918 Fermi enrolled at the Scuola Normale Superiore in Pisa, where he was later to receive his undergraduate and doctoral degree. In order to enter the Institute, candidates had to take an entrance exam which included an essay. For his essay on the given theme Characteristics of Sound, 17-year-old Fermi chose to derive and solve the Fourier analysis based partial differential equation for waves on a string. The examiner, Prof. Giulio Pittato, interviewed Fermi and concluded that his essay would have been commendable even for a doctoral degree. Enrico Fermi ended up at the first place in the classification of the entrance exam. During the years at the Scuola Normale Superiore, Fermi teamed up with a fellow student named Franco Rasetti with whom he used to indulge in light-hearted pranks. Later, Rasetti became Fermi's close friend and collaborator.
Beside attending the classes, Enrico Fermi found the time to work on his extracurricular activities, particularly with the help of his friend Enrico Persico, who remained in Rome to attend the university. Between 1919 and 1923 Fermi studied general relativity, quantum mechanics and atomic physics.
His knowledge of quantum mechanics reached such a high level that the head of the Physics Institute, Prof. Luigi Puccianti, asked him to organize seminars about that topic. During this time he learned tensor calculus, a mathematical instrument invented by Gregorio Ricci and Tullio Levi-Civita, and needed to demonstrate the principles of general relativity. In 1921, his third year at the university, he published his first scientific works in the Italian magazine Nuovo Cimento: the first was entitled: "On the dynamic of a solid system of electrical charges in transient conditions"; the second: "On the electrostatic of a uniform gravitational field of electromagnetic charges and on the weight of electromagnetic charges". At first glance, the first paper seemed to point out a contradiction between the electrodynamic theory and the relativistic one concerning the calculation of the electromagnetic masses. After one year with a work entitled "Correction of severe discrepancy between electrodynamic theory and the relativistic one of electromagnetic charges. Inertia and weight of electricity", Enrico Fermi showed the correctness of his paper. This last publication was so successful that was translated into German and published in the famous German scientific magazine "Physikalische Zeitschrift".
In 1922 he published his first important scientific work in the Italian magazine I Rendiconti dell'Accademia dei Lincei entitled "On the phenomena that happen close to the line of time", where he introduces for the first time the so-called "Fermi's coordinates", and proves that when close to the time line, space behaves as an euclidean one. In 1922 Fermi graduated from Scuola Normale Superiore.
In 1923, while writing the appendix for the Italian edition of the book "The Mathematical Theory of Relativity" written by A. Kopff, Enrico Fermi pointed out, for the first time, the fact that hidden inside the famous Einstein equation , there was a enormous amount of energy (nuclear energy) to be exploited.
Fermi's Ph.D advisor was Luigi Puccianti. In 1924 Fermi spent a semester in Göttingen, and then stayed for a few months in Leiden with Paul Ehrenfest.
From January 1925 to the autumn of 1926, he stayed at the University of Florence. In this period he wrote his work on the Fermi-Dirac statistics.
Professor in Rome
Aged 24, Fermi took a professorship at the University of Rome (first in atomic physics in Italy) which he won in a competition held by Professor Orso Mario Corbino, director of the Institute of Physics. Corbino helped Fermi in selecting his team, which soon was joined by notable minds like Edoardo Amaldi, Bruno Pontecorvo, Franco Rasetti and Emilio Segrč. For the theoretical studies only, Ettore Majorana also took part in what was soon nicknamed "the Via Panisperna boys" (after the name of the road in which the Institute had its labs).
The group went on with its now famous experiments, but in 1933 Rasetti left Italy for Canada and the United States, Pontecorvo went to France and Segrč left to teach in Palermo.
During their time in Rome, Fermi and his group made important contributions to many practical and theoretical aspects of physics. These include the theory of beta decay, and the discovery of slow neutrons, which was to prove pivotal for the working of nuclear reactors. His group systematically bombarded elements with slow neutrons, and during their experiments with uranium, narrowly missed observing nuclear fission. At that time, fission was thought to be improbable if not impossible, mostly on theoretical grounds. While people expected elements with higher atomic number to form from neutron bombardment of lighter elements, nobody expected neutrons to have enough energy to actually split a heavier atom into two light element fragments. However, the chemist Ida Noddack had criticised Fermi's work and had suggested that some of his experiments could have produced lighter elements. At the time, Fermi dismissed this possibility on the basis of calculations.
Fermi was well-known for his simplicity in solving problems. He began his inquiries with the simplest lines of mathematical reasoning, then later produced complete solutions to the problems he deemed worth pursuing. His abilities as a great scientist, combining theoretical and applied nuclear physics, were acknowledged by all. He influenced many physicists who worked with him, such as Hans Bethe, who spent two semesters working with Fermi in the early 1930s. From the time he was a boy, Fermi meticulously recorded his calculations in notebooks, and later used to solve many new problems that he encountered based on these earlier known problems.
When Fermi submitted his famous paper on beta decay to the prestigious journal Nature, the journal's editor turned it down because "it contained speculations which were too remote from reality". Thus Fermi saw the theory published in Italian and in German before it was published in English. Nature eventually did publish Fermi's report on beta decay on January 16, 1939.
Fermi remained in Rome until 1938.
The Manhattan Project
In 1938, Fermi won the Nobel Prize in Physics at the age of 37 for his "demonstrations of the existence of new radioactive elements produced by neutron irradiation, and for his related discovery of nuclear reactions brought about by slow neutrons".
After Fermi received the Nobel Prize in Stockholm, he, his wife Laura, and their children emigrated to New York. This was mainly because of the anti-Semitic laws promulgated by the fascist regime of Benito Mussolini which threatened Laura, who was Jewish. Also, the new laws put most of Fermi's research assistants out of work.
Soon after his arrival in New York, Fermi began working at Columbia University.
In December 1938, the German chemists Otto Hahn and Fritz Strassmann sent a manuscript to Naturwissenschaften reporting they had detected the element barium after bombarding uranium with neutrons; simultaneously, they communicated these results to Lise Meitner. Meitner, and her nephew Otto Robert Frisch, correctly interpreted these results as being nuclear fission. Frisch confirmed this experimentally on 13 January 1939. In 1944, Hahn received the Nobel Prize for Chemistry for the discovery of nuclear fission. Some historians have documented the history of the discovery of nuclear fission and believe Meitner should have been awarded the Nobel Prize with Hahn.
Meitner’s and Frisch’s interpretation of the work of Hahn and Strassmann crossed the Atlantic Ocean with Niels Bohr, who was to lecture at Princeton University. Isidor Isaac Rabi and Willis Lamb, two Columbia University physicists working at Princeton, heard the news and carried it back to Columbia. Rabi said he told Enrico Fermi; Fermi gave credit to Lamb. Bohr soon thereafter went from Princeton to Columbia to see Fermi. Not finding Fermi in his office, Bohr went down to the cyclotron area and found Herbert L. Anderson. Bohr grabbed him by the shoulder and said: “Young man, let me explain to you about something new and exciting in physics.” It was clear to a number of scientists at Columbia that they should try to detect the energy released in the nuclear fission of uranium from neutron bombardment. On 25 January 1939, a Columbia University team conducted the first nuclear fission experiment in the United States, which was done in the basement of Pupin Hall; the members of the team were Herbert L. Anderson, Eugene T. Booth, John R. Dunning, Enrico Fermi, G. Norris Glasoe, and Francis G. Slack. The next day, the Fifth Washington Conference on Theoretical Physics began in Washington, D.C. under the joint auspices of The George Washington University and the Carnegie Institution of Washington. There, the news on nuclear fission was spread even further, which fostered many more experimental demonstrations.
Fermi then went to the University of Chicago and began studies that led to the construction of the first nuclear pile Chicago Pile-1.
Fermi recalled the beginning of the project in a speech given in 1954 when he retired as President of the American Physical Society:
:"I remember very vividly the first month, January, 1939, that I started working at the Pupin Laboratories because things began happening very fast. In that period, Niels Bohr was on a lecture engagement at the Princeton University and I remember one afternoon Willis Lamb came back very excited and said that Bohr had leaked out great news. The great news that had leaked out was the discovery of fission and at least the outline of its interpretation. Then, somewhat later that same month, there was a meeting in Washington where the possible importance of the newly discovered phenomenon of fission was first discussed in semi-jocular earnest as a possible source of nuclear power."
In August 1939 Leó Szilárd prepared and Albert Einstein signed the famous letter warning President Franklin D. Roosevelt of the probability that the Nazis were planning to build an atomic bomb. Because of Hitler's September 1 invasion of Poland, it was October before they could arrange for the letter to be personally delivered. Roosevelt was concerned enough that the Uranium Committee was assembled, and awarded Columbia University the first atomic energy funding of US$6,000. However, due to bureaucratic fears of foreigners doing secret research, the money was not actually issued until Szilárd implored Einstein to send a second letter to the president in the spring of 1940. The money was used in studies which led to the first nuclear reactor — Chicago Pile-1, a massive "atomic pile" of graphite bricks and uranium fuel which went critical on December 2, 1942, built in a hard racquets court under Stagg Field, the football stadium at the University of Chicago. Due to a mistranslation, Soviet reports on Enrico Fermi claimed that his work was performed in a converted "pumpkin field" instead of a "squash court", squash being an offshoot of hard racquets. This experiment was a landmark in the quest for energy, and it was typical of Fermi's brilliance. Every step had been carefully planned, every calculation meticulously done by him. When the first self-sustained nuclear chain reaction was achieved, a coded phone call was made by one of the physicists, Arthur Compton, to James Conant, chairman of the National Defense Research Committee. The conversation was in impromptu code:
- Compton: The Italian navigator has landed in the New World.
- Conant: How were the natives?
- Compton: Very friendly.
This successful initiation of a chain-reacting pile was important not only for its help in assessing the properties of fission — needed for understanding the internal workings of an atomic bomb — but also because it would serve as a pilot plant for the massive reactors which would be created in Hanford, Washington, which would then be used to produce the plutonium needed for the bombs used at the Trinity site and Nagasaki. Eventually Fermi and Szilárd's reactor work was folded into the Manhattan Project.
Fermi moved to Los Alamos in the later stages of the Manhattan Project to serve as a general consultant. He was sitting in the control room of the Hanford B Reactor when it first went critical in 1944. His broad knowledge of many fields of physics was useful in solving problems that were of an interdisciplinary nature.
He became a naturalized citizen of the United States of America in 1944.
Fermi was present as an observer of the Trinity test on July 16, 1945. Engineer Jack Aeby saw Fermi at work:
Fermi's strips-of-paper estimate was ten kilotons of TNT; the actual yield was about 19 kilotons
Post-war work
In Fermi's 1954 address to the APS he also said, "Well, this brings us to Pearl Harbor. That is the time when I left Columbia University, and after a few months of commuting between Chicago and New York, eventually moved to Chicago to keep up the work there, and from then on, with a few notable exceptions, the work at Columbia was concentrated on the isotope separation phase of the atomic energy project, initiated by Booth, Dunning and Urey about 1940".
Fermi was widely regarded as the only physicist of the twentieth century who excelled both theoretically and experimentally. The well-known historian of physics, C. P. Snow, says about him, "If Fermi had been born a few years earlier, one could well imagine him discovering Rutherford's atomic nucleus, and then developing Bohr's theory of the hydrogen atom. If this sounds like hyperbole, anything about Fermi is likely to sound like hyperbole". Fermi's ability and success stemmed as much from his appraisal of the art of the possible, as from his innate skill and intelligence. He disliked complicated theories, and while he had great mathematical ability, he would never use it when the job could be done much more simply. He was famous for getting quick and accurate answers to problems which would stump other people. An instance of this was seen during the first atomic bomb test in New Mexico on July 16 1945. As the blast wave reached him, Fermi dropped bits of paper. By measuring the distance they were blown, he could compare to a previously computed table and thus estimate the bomb energy yield. He estimated that the blast was greater than 10 kilotons of TNT, the measured result was 18.6. (Rhodes, page 674). Later on, this method of getting approximate and quick answers through back-of-the-envelope calculations became informally known as the 'Fermi method'.
Fermi's most disarming trait was his great modesty, and his ability to do any kind of work, whether creative or routine. It was this quality that made him popular and liked among people of all strata, from other Nobel Laureates to technicians. Henry DeWolf Smyth, who was Chairman of the Princeton Physics department, had once invited Fermi over to do some experiments with the Princeton cyclotron. Walking into the lab one day, Smyth saw the distinguished scientist helping a graduate student move a table, under another student's directions. Another time, a Du Pont executive made a visit to see him at Columbia. Not finding him either in his lab or his office, the executive was surprised to find the Nobel Laureate in the machine shop, cutting sheets of tin with a big pair of shears.
After the war, Fermi served for a short time on the General Advisory Committee of the Atomic Energy Commission, a scientific committee chaired by J. Robert Oppenheimer which advised the commission on nuclear matters and policy. After the detonation of the first Soviet fission bomb in August 1949, he, along with Isidor Rabi, wrote a strongly-worded report for the committee which opposed the development of a hydrogen bomb on moral and technical grounds. But Fermi also participated in preliminary work on the hydrogen bomb at Los Alamos as a consultant, and along with Stanislaw Ulam, calculated that the amount of tritium needed for Edward Teller's model of a thermonuclear weapon would be prohibitive, and a fusion reaction could not be assured to propagate even with this large quantity of tritium.
In his later years, Fermi did important work in particle physics, especially related to pions and muons. He was also known to be an inspiring teacher at the University of Chicago, and was known for his attention to detail, simplicity, and careful preparation for a lecture. Later, his lecture notes, especially those for quantum mechanics, nuclear physics, and thermodynamics, were transcribed into books which are still in print.
Also in these later years he mused about a proposition which is now referred to as the "Fermi Paradox". This contradiction or proposition is this: that with the billions and billions of star systems in the universe, one would think that intelligent life would have contacted our civilization by now.
Fermi died at age 53 of stomach cancer and was interred at Oak Woods Cemetery in Chicago, Illinois. Two of his graduate students who assisted him in working on or near the nuclear pile also died of cancer. Fermi and his team knew that such work carried considerable risk but they considered the outcome so vital that they forged ahead with little regard for their own personal safety.
As Eugene Wigner wrote: "Ten days before Fermi had died he told me, 'I hope it won't take long.' He had reconciled himself perfectly to his fate".
A recent poll by Time magazine listed Fermi among the top twenty scientists of the century.
The Fermilab particle accelerator and physics lab in Batavia, Illinois, is named after him in loving memory from the physics community.
Three nuclear reactor installations have been named after Fermi:
Many schools are also named after him, such as Enrico Fermi High School in Enfield, Connecticut.
Fermi Court in Deep River, Ontario is named in his honour.
In 1952, element 100 on the periodic table of elements was isolated from the debris of a nuclear test. In honor of Fermi's contributions to the scientific community, it was named fermium after him.
Since the 1950s, the United States Atomic Energy Commission has named its highest honour, the Fermi Award, after him. Recipients of the award include well-known scientists like Otto Hahn, J. Robert Oppenheimer, Freeman Dyson, John Wheeler and Hans Bethe.
Legacy
Enrico Fermi's mother built her own pressure cooker and perhaps this inspired Enrico to build the first nuclear reactor in 1942. (A pressure cooker is a vessel which confines steam pressure, allowing a higher temperature to be reached.) Enrico's pile was graphite containing uranium from exploding (copyright Olivia Fermi 2001-2008, unpublished manuscript). In 1928, Fermi married Laura Capon. They had two children while living in Rome, Italy: a daughter Nella Fermi Weiner, PhD (1931–1995), artist and feminist; and a son Giulio ("Judd") Fermi, PhD (1936–1997). Laura and Enrico's son Giulio worked with the Nobel laureate Max Perutz on the structure of hemoglobin.
Toward the end of his life, Fermi questioned his faith in society at large to make wise choices about nuclear technology. He said:
- "Some of you may ask, what is the good of working so hard merely to collect a few facts which will bring no pleasure except to a few long-haired professors who love to collect such things and will be of no use to anybody because only few specialists at best will be able to understand them? In answer to such question[s] I may venture a fairly safe prediction.
- History of science and technology has consistently taught us that scientific advances in basic understanding have sooner or later led to technical and industrial applications that have revolutionized our way of life. It seems to me improbable that this effort to get at the structure of matter should be an exception to this rule. What is less certain, and what we all fervently hope, is that man will soon grow sufficiently adult to make good use of the powers that he acquires over nature."
His wife, Laura Fermi (1907–1977), early environmentalist, systems thinker, prolific writer and New York Times bestselling author of "Atoms in the Family: Life with Enrico Fermi, Architect of the Atomic Age" said, of our nuclear dilemma:
- "But above all, there were the moral questions. I knew scientists had hoped that the bomb would not be possible, but there it was and it had already killed and destroyed so much. Was war or was science to be blamed? Should the scientists have stopped the work once they realized that a bomb was feasible? Would there always be war in the future? To these kinds of questions there is no simple answer."
Rachel Fermi (1964–), photographer and teacher, Laura and Enrico Fermi's 3rd grandchild, continued to question the sanity of nuclear weapons in her book, "Picturing the Bomb". The authors juxtapose photos from the top secret world of the Manhattan Project with family photos from Los Alamos and Hanford.
Olivia Fermi (1957–), formerly Alice Caton, M.A. A.B.S. - Leadership in Human Systems, ConRes Cert, photoartist, writer and business consultant, Laura and Enrico's first grandchild, is currently researching the legacy of her grandparents for a series of books she plans to publish. On September 29, 2001, shortly after the destruction of the World Trade Center in New York City, Olivia flew to Rome, Italy to deliver a speech to the International Conference: Enrico Fermi and the Universe of Physics. She had been invited to speak to this gathering of physicists as a representative of the Laura and Enrico Fermi family. Olivia said:
- "All of us alive today, and all who will come after us, are heirs to Enrico Fermi’s scientific legacy. We all have a stake in it. Since the end of World War II, humanity has had knowledge of nuclear energy and its incredible potential for benefit as well as harm.
- "Enrico Fermi gave us a lot. And there is more to be done. Enrico Fermi’s work, and the work of other scientists, exists in a world full of people who, in a certain way, are like Enrico... [funny anecdotes about occasional Enrico errors]... He, like all of us, was both brilliant and fallible.
- "We have a collective, developmental task. We must learn to integrate our scientific knowledge and our human experience to find the answers to the nuclear dilemma, and to the many other dilemmas facing us today. ... Our world has yet to find the right nuclear recipe – how to harness nuclear power for the benefit of all living things.
- "We will need all of our human gifts to survive and flourish on this planet. From here, it looks to me like Enrico contributed all of his gifts. Now it’s up to us to contribute ours. We can look back to Enrico for inspiration, if we look to ourselves for the future."
The two male grandchildren of Laura and Enrico are Olivia's brother, Paul Weiner, PhD (1959–), mathematician and professor; and Rachel's brother, Daniel Fermi (1971–). Between Paul and Rachel, there are four great-grandchildren.
Patents
See also
Bibliography
- * , United States Department of Energy, (December 1982).
- Fermi, E. , United States Department of Energy (through predecessor agency the Atomic Energy Commission, (May 1946).
- Jones, E.M. , Los Alamos National Laboratory (LANL), United States Department of Energy, (March 1, 1985).
- Myers, W.D. & W.J. Swiatecki. , Lawrence Berkeley National Laboratory (LBNL), United States Department of Energy, (August 1, 1994).
- Beckerley, J.G. , United States Department of Energy (through predecessor agency the Atomic Energy Commission), (October 1951).
- Fermi, E. , Fermi National Accelerator Laboratory, United States Department of Energy (through predecessor agency the Atomic Energy Commission), (June 1943).
- Fermi, E., Pasta, J. & S. Ulam. , Los Alamos National Laboratory (through predecessor agency Los Alamos Scientific Laboratory, (May 1955).
- Fermi, E. , Los Alamos National Laboratory (through predecessor agency Los Alamos Scientific Laboratory, (September 1951).
- Compton, A. H. , United States Department of Energy (through predecessor agency the Atomic Energy Commission, (September 1942).
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