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Thursday, February 11, 2010

Gould, Stephen Jay


Biography of Gould, Stephen Jay

Gould was born and raised in the community of Bayside, a quiet suburb located in the Queens borough of New York City, NY. His father Leonard was a court stenographer, and his mother Eleanor was an artist. When Gould was five years old, his father took him to the Hall of Dinosaurs in the American Museum of Natural History, where he first encountered Tyrannosaurus rex. "I had no idea there were such things—I was awestruck," Gould once recalled.[3] It was in that moment that he decided to become a paleontologist.

Raised in a secular Jewish home, Gould did not formally practice religion and preferred to be called an agnostic.[2] Though he "had been brought up by a Marxist father," he has stated that his father's politics were "very different" from his own.[4] In describing his own political views he has said they "tend to the left of center".[5] According to Gould the most influential political books he read were C. Wright Mills' The Power Elite and the political writings of Noam Chomsky.[5] While attending Antioch College in the early 1960s, Gould was active in the civil rights movement and often campaigned for social justice. When he attended the University of Leeds as a visiting undergraduate, he organized weekly demonstrations outside a Bedford dance hall which refused to admit Blacks. Gould continued these demonstrations until the policy was revoked.[6] Throughout his career and writings he spoke out against cultural oppression in all its forms, especially what he saw as pseudoscience used in the service of racism and sexism.[7]

Gould was twice married. His first marriage was to artist Deborah Lee on October 3, 1965. Gould met Lee while they were students together at Antioch College.[3] They had two sons Jesse and Ethan. His second marriage was in 1995 to artist and sculptor Rhonda Roland Shearer. Gould had two stepchildren, Jade and London, by his second marriage.

In July 1982, Gould was diagnosed with peritoneal mesothelioma, a deadly form of cancer affecting the abdominal lining and frequently found in people who have been exposed to asbestos. After a difficult two-year recovery, Gould published a column for Discover magazine, titled "The Median Isn't the Message", which discusses his reaction to discovering that mesothelioma patients had a median lifespan of only eight months after diagnosis.[8] He then describes the true significance behind this number, and his relief upon realizing that statistical averages are just useful abstractions, and do not encompass the full range of variation. The median is the halfway point, which means that 50% of patients will die before 8 months, but the other half will live longer, potentially much longer. He then needed to determine where his personal characteristics placed him within this range. Considering that the cancer was detected early, the fact he was young, optimistic, and had the best treatments available, Gould figured that he should be in the favorable half of the upper statistical range. After an experimental treatment of radiation, chemotherapy, and surgery, Gould made a full recovery, and his column became a source of comfort for many cancer patients.

Gould was also an advocate for medical marijuana. During this bout with cancer, he smoked the illegal drug to alleviate the nausea associated with his medical treatments. According to Gould, his use of marijuana had a "most important effect" on his eventual recovery.[9] In 1998 he testified in the case of Jim Wakeford, a Canadian medical-marijuana user and activist.

His scientific essays for Natural History frequently refer to his nonscientific interests and pastimes. As a boy he collected baseball cards and remained a fiercely avid baseball fan throughout his life. As an adult he was fond of science fiction movies but often lamented about their mediocrity (not just in their presentation of science, but in their storytelling as well).[10] His other interests included singing in the Boston Cecilia (a madrigal choir), and he was a great aficionado of Gilbert and Sullivan operettas. He collected rare antiquarian books and textbooks. He often traveled to Europe, and spoke French, German, Russian, and Italian. He admired Renaissance architecture. When discussing the Judeo-Christian tradition, he usually referred to it simply as "Moses". He sometimes alluded ruefully to his tendency to put on weight.[11]

Gould died on May 20, 2002 from a metastatic adenocarcinoma of the lung, a form of cancer which had spread to his brain.[12] This cancer was unrelated to his abdominal cancer, from which he had fully recovered twenty years earlier. He died in his home "in a bed set up in the library of his SoHo loft, surrounded by his wife Rhonda, his mother Eleanor, and the many books he loved."[13]
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Scientific career

Gould began his higher education at Antioch College, graduating with double major in geology and philosophy in 1963.[14] During this time, he also studied abroad at the University of Leeds in the United Kingdom.[15] After completing his graduate work at Columbia University in 1967 under the guidance of Norman Newell, he was immediately hired by Harvard University where he worked until the end of his life (1967–2002). In 1973, Harvard promoted him to Professor of Geology and Curator of Invertebrate Paleontology at the institution's Museum of Comparative Zoology. In 1982, Harvard awarded him with the title of Alexander Agassiz Professor of Zoology. The following year, in 1983, he was awarded fellowship into the American Association for the Advancement of Science, where he later served as president (1999–2001). The AAAS news release cited his "numerous contributions to both scientific progress and the public understanding of science". He also served as president of the Paleontological Society (1985–1986) and the Society for the Study of Evolution (1990–1991). In 1989 Gould was elected into the body of the National Academy of Sciences. Through 1996–2002 Gould was Vincent Astor Visiting Research Professor of Biology at New York University. In 2001 the American Humanist Association named him the Humanist of the Year for his lifetime of work. In 2008, he was posthumously awarded the Darwin-Wallace Medal, along with 12 other recipients. Until 2008, this medal had been awarded every 50 years by the Linnean Society of London.[16]
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Punctuated equilibrium

Early in his career, Gould and Niles Eldredge developed the theory of punctuated equilibrium, in which evolutionary change occurs relatively rapidly, as compared to longer periods of relative evolutionary stability.[1] According to Gould, punctuated equilibrium revised a key pillar "in the central logic of Darwinian theory."[4] Some evolutionary biologists have argued that while punctuated equilibrium was "of great interest to biology,"[17] it merely modified neo-Darwinism in a manner that was fully compatible with what had been known before.[18] Others however emphasized its theoretical novelty, and argued that evolutionary stasis had been "unexpected by most evolutionary biologists" and "had a major impact on paleontology and evolutionary biology."[19]

Some critics jokingly referred to the theory as "evolution by jerks," which elicited Gould to respond in kind by describing gradualism as "evolution by creeps."[20]
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Evolutionary developmental biology

Gould made significant contributions to evolutionary developmental biology,[21] especially in his work Ontogeny and Phylogeny.[14] In this book he emphasized the process of heterochrony, which encompasses two distinct processes: pedomorphosis and terminal additions. Pedomorphosis is the process where ontogeny is slowed down and the organism does not reach the end of its development. Terminal addition is the process by which an organism adds to its development by speeding and shortening earlier stages in the developmental process. Gould's influence in the field of evolutionary developmental biology continues to be seen, such areas as the evolution of feathers.[22]
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Selectionism and sociobiology

Gould championed biological constraints such as the limitations of developmental pathways on evolutionary outcomes, as well as other non-selectionist forces in evolution. In particular, he considered many higher functions of the human brain to be the unintended side consequence or by-product of natural selection, rather than direct adaptations. To describe such co-opted features he coined the term exaptation with Elisabeth Vrba.[23] Gould believed this understanding undermines an essential premise of human sociobiology and evolutionary psychology.
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Against "Sociobiology"

In 1975, E. O. Wilson introduced his analysis of human behavior based on a sociobiological framework.[24] In response, Gould, Richard Lewontin and others from the Boston area wrote the subsequently well referenced letter to The New York Review of Books titled "Against 'Sociobiology'". This open letter criticised Wilson's notion of a "deterministic view of human society and human action."[25]

But Gould did not rule out sociobiological explanations for many aspects of animal behavior, writing: "Sociobiologists have broadened their range of selective stories by invoking concepts of inclusive fitness and kin selection to solve (successfully I think) the vexatious problem of altruism—previously the greatest stumbling block to a Darwinian theory of social behavior. . . . Here sociobiology has had and will continue to have success. And here I wish it well. For it represents an extension of basic Darwinism to a realm where it should apply."[26]
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Spandrels and the Panglossian Paradigm

A spandrel from the Holy Trinity Church in Fulnek, Czech Republic.

With Richard Lewontin, Gould wrote an influential 1979 paper entitled "The Spandrels of San Marco and the Panglossian Paradigm",[27] which introduced the architectural term "spandrel" into evolutionary biology. In architecture, a spandrel is a curved area of masonry which exists between arches supporting a dome. Spandrels, also called pendentives in this context, are found particularly in gothic churches.

When visiting Venice in 1978, Gould noted that the spandrels of the San Marco cathedral, while quite beautiful, were not spaces planned by the architect. Rather the spaces arise as "necessary architectural byproducts of mounting a dome on rounded arches." Gould and Lewontin thus defined spandrels in evolutionary biology to mean any biological feature of an organism that arises as a necessary side consequence of other features, which is not directly selected for by natural selection. Examples include the "masculinized genitalia in female hyenas, exaptive use of an umbilicus as a brooding chamber by snails, the shoulder hump of the giant Irish deer, and several key features of human mentality."[28]

In Voltaire's Candide, Dr. Pangloss is portrayed as a clueless scholar who, despite the evidence, says that "all is for the best in this best of all possible worlds." Gould and Lewontin asserted that it is Panglossian for evolutionary biologists to view all traits as atomized things that had been naturally selected for, and criticised biologists for not granting theoretical space to other causes, such as phyletic and developmental constraints. The relative frequency of spandrels, so defined, versus adaptive features in nature, remains a controversial topic in evolutionary biology.[29] An illustrative example of Gould's approach can be found in Elisabeth Lloyd's case study of the female orgasm as a by-product of shared developmental pathways.[30] Gould also wrote on this topic in his essay "Male Nipples and Clitoral Ripples",[31] prompted by Lloyd's earlier work.
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Evolutionary progress

Gould favored the argument that evolution has no inherent drive towards long-term progress. Uncritical commentaries often portray evolution as a ladder of progress, leading towards bigger, faster, and smarter organisms. The assumption being that evolution is somehow driving organisms to get more complex, and ultimately more like humankind. Gould argued that evolution's drive was not towards complexity, but towards diversification. Because life is constrained to begin with a simple starting point, any diversity resulting from this left wall will be perceived to move in the direction of higher complexity. But life, Gould argued, can easily adapt towards simplification, as is often the case with parasites.[32]

In a review of Full House, Richard Dawkins approved of Gould's general argument, but suggested that he saw evidence of a "tendency for lineages to improve cumulatively their adaptive fit to their particular way of life, by increasing the numbers of features which combine together in adaptive complexes. ... By this definition, adaptive evolution is not just incidentally progressive, it is deeply, dyed-in-the wool, indispensably progressive."[33]
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Cladistics

Gould never embraced cladistics as a method of investigating evolutionary lineages and process, possibly because he was concerned that such investigations would lead to neglect of the details in historical biology, which he considered all-important. In the early 1990s this led him into a debate with Derek Briggs, who had begun to apply quantitative cladistic techniques to the Burgess Shale fossils, about the methods to be used in interpreting these fossils.[34] Around this time cladistics rapidly became the dominant method of classification in evolutionary biology. Cheap but increasingly powerful personal computers made it possible to process large quantities of data about organisms and their characteristics. Around the same time the development of effective polymerase chain reaction techniques made it possible to apply cladistic methods of analysis to biochemical features as well.[35]
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Technical work on land snails

Most of Gould's empirical research pertained to land snails. He focused his early work on the Bermudian genus Poecilozonites, while his later work concentrated on the West Indian genus Cerion. According to Gould "Cerion is the land snail of maximal diversity in form throughout the entire world. There are 600 described species of this single genus. In fact, they're not really species, they all interbreed, but the names exist to express a real phenomenon which is this incredible morphological diversity. Some are shaped like golf balls, some are shaped like pencils.…Now my main subject is the evolution of form, and the problem of how it is that you can get this diversity amid so little genetic difference, so far as we can tell, is a very interesting one. And if we could solve this we'd learn something general about the evolution of form."[36]

Given Cerion's extensive geographic diversity, Gould later lamented that if Christopher Columbus had only cataloged a single Cerion it would have ended the scholarly debate over which island Columbus had first set foot on America.[37]
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Influence

Gould is also one of the most frequently cited scientists in the field of evolutionary theory. His 1979 "spandrels" paper has been cited more than 3,000 times.[38] In Palaeobiology—the flagship journal of his own speciality—only Charles Darwin and G.G. Simpson have been cited more often.[39] Gould was also a considerably respected historian of science. Historian Ronald Numbers has been quoted as saying: "I can't say much about Gould's strengths as a scientist, but for a long time I've regarded him as the second most influential historian of science (next to Thomas Kuhn)."[40]
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The Structure of Evolutionary Theory

Shortly before his death, Gould published a long treatise recapitulating his version of modern evolutionary theory: The Structure of Evolutionary Theory (2002).
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As a public figure

Gould became widely known through his popular science essays in Natural History magazine and his best-selling books on evolution. Many of his essays were reprinted in collected volumes, such as Ever Since Darwin and The Panda's Thumb, while his popular treatises included books such as The Mismeasure of Man, Wonderful Life and Full House.

A passionate advocate of evolutionary theory, Gould wrote prolifically on the subject, trying to communicate his understanding of contemporary evolutionary biology to a wide audience. A recurring theme in his writings is the history and development of evolutionary, and pre-evolutionary, thought. He was also an enthusiastic baseball fan and made frequent references to the sport in his essays. Many of his baseball essays were anthologized in his posthumously published book Triumph and Tragedy in Mudville (2003).[41]

Although a proud Darwinist, his emphasis was less gradualist and reductionist than most neo-Darwinists. He fiercely opposed many aspects of sociobiology and its intellectual descendant evolutionary psychology. He devoted considerable time to fighting against creationism (and the related constructs Creation science and Intelligent design). Most notably, Gould provided expert testimony against the equal-time creationism law in McLean v. Arkansas. Gould later developed the term "non-overlapping magisteria" (NOMA) to describe how, in his view, science and religion could not comment on each other's realm. Gould went on to develop this idea in some detail, particularly in the books Rocks of Ages (1999) and The Hedgehog, the Fox, and the Magister's Pox (2003). In a 1982 essay for Natural History Gould wrote:
Our failure to discern a universal good does not record any lack of insight or ingenuity, but merely demonstrates that nature contains no moral messages framed in human terms. Morality is a subject for philosophers, theologians, students of the humanities, indeed for all thinking people. The answers will not be read passively from nature; they do not, and cannot, arise from the data of science. The factual state of the world does not teach us how we, with our powers for good and evil, should alter or preserve it in the most ethical manner.[42]

The anti-evolution petition A Scientific Dissent From Darwinism spawned the National Center for Science Education's anti-petition Project Steve, which is named in Gould's honor.

Gould also became a noted public face of science, often appearing on television. In 1984 Gould received his own NOVA special on PBS.[43] Other appearances included interviews on CNN's Crossfire, NBC's The Today Show, and regular appearances on the Charlie Rose show. Gould was also a guest in all seven episodes of the Dutch talk-series A Glorious Accident, which he appeared with his good friend Oliver Sacks.[44]

Gould was featured prominently as a guest in Ken Burns' PBS documentary Baseball, as well as PBS's highly produced Evolution series. Gould was also on the Board of Advisers to the influential Children's Television Workshop television show, 3-2-1 Contact, where he made frequent guest appearances.

In 1997 he voiced a cartoon version of himself on the television series The Simpsons. In the episode "Lisa the Skeptic", Lisa finds a skeleton that many people believe is an apocalyptic angel. Lisa contacts Gould and asks him to test the skeleton's DNA. However the fossil is discovered to be a marketing gimmick for a new mall.[45] During production the only phrase Gould objected to was a line in the script that introduced him as the "world's most brilliant paleontologist".[46] In 2002 the show paid tribute to Gould after his death, dedicating the season 13 finale to his memory. Gould had died 2 days before the episode aired.
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Controversies

Gould received many accolades for his scholarly work and popular expositions of natural history,[12][47] but was not immune from criticism by those in the biological community who felt his public presentations were, for various reasons, out of step with mainstream evolutionary theory.[48] The public debates between Gould's proponents and detractors have been so quarrelsome that they have been dubbed "The Darwin Wars" by several commentators.[49][50][51][52]

John Maynard Smith, an eminent British evolutionary biologist, was among Gould's strongest critics. Maynard Smith thought that Gould misjudged the vital role of adaptation in biology, and was also critical of Gould's acceptance of species selection as a major component of biological evolution.[53] In a review of Daniel Dennett's book Darwin's Dangerous Idea, Maynard Smith wrote that Gould "is giving non-biologists a largely false picture of the state of evolutionary theory."[54] But Maynard Smith has not been consistently negative, writing in a review of The Panda's Thumb that "Stephen Gould is the best writer of popular science now active. . . . Often he infuriates me, but I hope he will go right on writing essays like these."[55] Maynard Smith was also among those who welcomed Gould's reinvigoration of evolutionary paleontology.[18]

One reason for such criticism was that Gould appeared to be presenting his ideas as a revolutionary way of understanding evolution, and argued for the importance of mechanisms other than natural selection, mechanisms which he believed had been ignored by many professional evolutionists. As a result, many non-specialists sometimes inferred from his early writings that Darwinian explanations had been proven to be unscientific (which Gould never tried to imply). Along with many other researchers in the field, Gould's works were sometimes deliberately taken out of context by creationists as a "proof" that scientists no longer understood how organisms evolved.[56] Gould himself corrected some of these misinterpretations and distortions of his writings in later works.[57]

Gould and Dawkins also disagreed over the importance of gene selection in evolution. Dawkins argued that evolution is best understood as competition among genes (or replicators), while Gould advocated the importance of multi-level competition, including selection amongst genes, cell lineages, organisms, demes, species, and clades.[52] Criticism of Gould and his theory of punctuated equilibrium can be found in chapter 9 of Dawkins' The Blind Watchmaker and chapter 10 of Dennett's Darwin's Dangerous Idea.
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Opposition to sociobiology and evolutionary psychology

Gould also had a long-running public feud with E. O. Wilson and other evolutionary biologists over human sociobiology and its later descendant evolutionary psychology (which Gould, Lewontin, and Maynard Smith opposed, but which Richard Dawkins, Daniel Dennett, and Steven Pinker advocated).[58] These debates reached their climax in the 1970s, and included strong opposition from groups like the Sociobiology Study Group and Science for the People.[59] Pinker accuses Gould, Lewontin and other opponents of evolutionary psychology of being "radical scientists," whose stance on human nature is influenced by politics rather than science.[60] Gould stated that he made "no attribution of motive in Wilson's or anyone else's case" but cautioned that all human beings are influenced, especially unconsciously, by our personal expectations and biases. He wrote:
I grew up in a family with a tradition of participation in campaigns for social justice, and I was active, as a student, in the civil rights movement at a time of great excitement and success in the early 1960s. Scholars are often wary of citing such commitments. … [but] it is dangerous for a scholar even to imagine that he might attain complete neutrality, for then one stops being vigilant about personal preferences and their influences—and then one truly falls victim to the dictates of prejudice. Objectivity must be operationally defined as fair treatment of data, not absence of preference.[61]

Gould's primary criticism held that human sociobiological explanations lacked evidential support, and argued that adaptive behaviors are frequently assumed to be genetic for no other reason than their supposed universality, or their adaptive nature. Gould emphasized that adaptive behaviors can be passed on through culture as well, and either hypothesis is equally plausible.[62] Gould did not deny the relevance of biology to human nature, but reframed the debate as "biological potentiality vs. biological determinism." Gould stated that the human brain allows for a wide range of behaviors. Its flexibility "permits us to be aggressive or peaceful, dominant or submissive, spiteful or generous… Violence, sexism, and general nastiness are biological since they represent one subset of a possible range of behaviors. But peacefulness, equality, and kindness are just as biological—and we may see their influence increase if we can create social structures that permit them to flourish."[62]
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Cambrian fauna

Gould's interpretation of the Cambrian Burgess Shale fossils in his book Wonderful Life emphasized the striking morphological disparity (or "weirdness") of the Burgess Shale fauna, and the role of chance in determining which members of this fauna survived and flourished. He used the Cambrian fauna as an example of the role of contingency in the broader pattern of evolution.

Gould's view was criticized by Simon Conway Morris in his 1998 book The Crucible Of Creation.[63] Conway Morris stressed those members of the Cambrian fauna that resemble modern taxa. He also promoted convergent evolution as a mechanism producing similar forms to similar environmental circumstances, and argued in a subsequent book that the appearance of human-like animals is likely. Paleontologists Derek Briggs and Richard Fortey have also argued that much of the Cambrian fauna may be regarded as stem groups of living taxa,[64] though this is still a subject of intense research and debate, and the relationship of many Cambrian taxa to modern phyla has not been established in the eyes of many palaeontologists.

Paleontologist Richard Fortey noted that prior to the release of Wonderful Life, Conway Morris shared many of Gould's sentiments and views. It was only after publication of Wonderful Life that Conway Morris revised his interpretation and adopted a more progressive stance towards the history of life.[65]
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Mismeasure of Man
Main article: The Mismeasure of Man

Stephen Jay Gould was also the author of The Mismeasure of Man (1981), a history and skeptical inquiry of psychometrics and intelligence testing. Gould investigated the methods of nineteenth century craniometry, as well as the current practice of psychological testing. Gould claimed that both theories developed from an unfounded belief in biological determinism, the view that "social and economic differences between human groups—primarily races, classes, and sexes—arise from inherited, inborn distinctions and that society, in this sense, is an accurate reflection of biology."[66] It was reprinted in 1996 with the addition of a new foreword and a critical review of The Bell Curve. The Mismeasure of Man has generated perhaps the greatest controversy of all of Gould's books. It has received both widespread praise (by skeptics)[67] and extensive criticism (by a number of psychologists),[68] which included claims of misrepresentation.[69]
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Non-overlapping magisteria
Main article: Non-overlapping magisteria

In his book Rocks of Ages (1999), Gould put forward what he described as "a blessedly simple and entirely conventional resolution to...the supposed conflict between science and religion."[70] He defines the term magisterium as "a domain where one form of teaching holds the appropriate tools for meaningful discourse and resolution."[70] The non-overlapping magisteria (NOMA) principle therefore divides the magisterium of science to cover "the empirical realm: what the Universe is made of (fact) and why does it work in this way (theory). The magisterium of religion extends over questions of ultimate meaning and moral value. These two magisteria do not overlap, nor do they encompass all inquiry."[70] He suggests that "NOMA enjoys strong and fully explicit support, even from the primary cultural stereotypes of hard-line traditionalism" and that NOMA is "a sound position of general consensus, established by long struggle among people of goodwill in both magisteria."[70]

This view has not been without criticism, however. In his book The God Delusion, Richard Dawkins argues that this division is not quite as simple as it seems, as few religions exist without miracles impinging on the scientific magisterium

Johann Wolfgang von Goethe


Bibliography of Johann Wolfgang von Goethe

Johann Wolfgang von Goethe , 1749-1832, German poet, dramatist, novelist, and scientist, b. Frankfurt. One of the great masters of world literature, his genius embraced most fields of human endeavor; his art and thought are epitomized in his great dramatic poem Faust.

Early Life and Works

Goethe describes his happy and sheltered childhood in his autobiography, Dichtung und Wahrheit (1811-33). In 1765 he went to Leipzig to study law. There he spent his time in the usual student dissipations, which perhaps contributed to a hemorrhage that required a long convalescence at Frankfurt. His earliest lyric poems, set to music, were published in 1769. In 1770-71 he completed his law studies at Strasbourg, where the acquaintance of Herder filled him with enthusiasm for Shakespeare, for Germany's medieval past, and for the German folk song.

Goethe's lyric poems for Friederike Brion, daughter of the pastor of nearby Sesenheim, were written at this time as new texts for folk-song melodies. Among the lasting influences of Goethe's youth were J. J. Rousseau and Spinoza, who appealed to Goethe's mystic and poetic feeling for nature in its ever-changing aspects. It was in this period that Goethe began his lifelong study of animals and plants and his research in biological morphology.

Goethe first attracted public notice with the drama Götz von Berlichingen (1773; see Berlichingen, Götz von ), a pure product of Sturm und Drang . Still more important was the epistolary novel Die Leiden des jungen Werthers (1774, tr. The Sorrows of Young Werther, 1957) which Goethe, on the verge of suicide, wrote after his unrequited love for Charlotte Buff. Werther gave him immediate fame and was widely translated. While the writing had helped Goethe regain stability, the novel's effect on the public was the opposite; it encouraged morbid sensibility.

The Weimar Years

In 1775, Goethe was invited to visit Charles Augustus, duke of Saxe-Weimar, at whose court he was to spend the rest of his life. For ten years Goethe was chief minister of state at Weimar. He later retained only the directorship of the state theater and the scientific institutions.

Italian and French Influences

A trip to Italy (1786-88) fired his enthusiasm for the classical ideal, as Goethe tells us in his travel account Die italienische Reise (1816) and in Winckelmann und sein Jahrhundert [ Winckelmann and his century] (1805). Also written under the classical impact were the historical drama Egmont (1788), well known for Beethoven's incidental music; Römische Elegien (1788); the psychological drama Torquato Tasso (1789); the domestic epic Hermann und Dorothea (1797); and the final, poetic version (1787) of the drama Iphigenie auf Tauris.

In 1792 Goethe accompanied Duke Charles Augustus as official historian in the allied campaign against revolutionary France. He appreciated the principles of the French Revolution but resented the methods employed. A reformer in his own small state, Goethe wished to see social change accomplished from above. Later he refused to share in the patriotic fervor that swept Germany during the Napoleonic Wars.

Novels and Poetry

His novel Die Wahlverwandtschaften (1809, tr. Elective Affinities, 1963) is one of his most significant novels, but perhaps his best-known work in that genre is the Wilhelm Meister series. The novel Wilhelm Meisters Lehrjahre [the apprenticeship of Wilhelm Meister] (1796), became the prototype of the German Bildungsroman, or novel of character development. In 1829 the last installment of Wilhelm Meisters Wanderjahre [Wilhelm Meister's journeyman years], a series of episodes, was published.

His most enduring work, indeed, one of the peaks of world literature, is the dramatic poem Faust. The first part was published in 1808, the second shortly after Goethe's death. Goethe recast the traditional Faust legend and made it one of the greatest poetic and philosophic creations the world possesses. His main departure from the original is no doubt the salvation of Faust, the erring seeker, in the mystic last scene of the second part.

Many women passed through Goethe's life, with Charlotte von Stein probably the most intellectual of them. He married (1806) Christiane Vulpius (1765-1816), who had borne him a son. Goethe's unsuccessful marriage offer (1822) to young Ulrike von Levetzow inspired his poems Trilogie der Leidenschaft [trilogy of passion]. Westöstlicher Diwan (1819), a collection of Goethe's finest lyric poetry, was inspired by his young friend Marianne von Willemer, who figures as Suleika in the cycle. The Diwan strikes a new note in German poetry, introducing Eastern elements derived from Goethe's reading of the Persian poet Hafiz .

Other Accomplishments

Increasingly aloof from national, political, or even literary partisanship, Goethe became more and more the Olympian divinity, to whose shrine at Weimar all Europe flocked. The variety and extent of his accomplishments and activities were monumental. Goethe knew French, English, Italian, Latin, Greek, and Hebrew and translated works by Diderot, Voltaire, Cellini, Byron, and others. His approach to science was one of sensuous experience and poetic intuition. Well known is his stubborn attack on Newton's theory of light in Zur Farbenlehre (1810). A corresponding treatise on acoustics remained unfinished.

An accomplished amateur musician, Goethe conducted instrumental and vocal ensembles and directed opera performances in Weimar. His search for an operatic composer with whom he could collaborate failed; although many of his operetta librettos were composed, none achieved lasting fame. Goethe's exquisite lyrical poems, often inspired by existing songs, challenged contemporary composers to give their best in music, and such songs as "Nur wer die Sehnsucht kennt" [only the lonely heart], "Kennst du das Land" [know'st thou the land], and Erlkönig were among the song texts most often set to music.

Goethe's aim was to make his life a concrete example of the full range of human potential, and he succeeded as few others did. The friendship of Friedrich von Schiller and his death (1805) made a deep impression on Goethe. He is buried, alongside Schiller, in the ducal crypt at Weimar. The opinions of Goethe are recorded not only in his own writings but also in conversations recorded by his secretary J. P. Eckermann and in extensive correspondence with the composer Zelter and with Schiller, Byron, Carlyle, Manzoni, and others. It would be difficult to overestimate Goethe's influence on the subsequent history of German literature.

Galileo Galilei


Bibliography of Galileo Galilei

Galileo Galilei was born in 1564 at Pisa. Galileo began his studies in medicine at the University of Pisa, but soon dropped out, preferring to study mathematics with Ostilio Ricci. In 1592 he obtained the chair of mathematics at Padua, and began working on the inclined plane and the pendulum. By 1598, Galileo believed in the truth of the Copernican theory, as he wrote to Kepler. Around 1604, he began working on astronomy in order to lecture on the new star that had appeared that year.

In 1609, Galileo heard of the telescope while in Venice, and on his return, constructed one for himself. In 1610, Galileo published his telescopic discoveries in The Starry Messenger, and dedicated the four satellites of Jupiter that he had discovered to Cosimo II, Grand Duke of Tuscany, naming them 'the Medicean stars'.

In The Starry Messenger, in addition to the satellites of Jupiter, Galileo reported that the milky-way was a collection of stars and how the moon in fact had a ragged surface like earth. The Starry Messenger was a sensational success, and Galileo became well known throughout Europe. In 1611, Galileo traveled to Rome, where the Collegio Romano, at the behest of Robert Bellarmino, confirmed Galileo's findings. Frederico Cesi hosted a banquet in honour of Galileo, and was elected to Cesi's 'Accademia dei Lincei' (Academy of the Lynxes). In Rome, Galileo also met Cardinal Maffeo Barberini, who later sided with him on the controversy over floating bodies at a court dinner in Florence.

Picture of Jupiter's satellites from the Sidereus Nuncius.
Image by kind permission of the Master and Fellows of Trinity College, Cambridge.

Large image (89K).
Very large image (1M).
One morning in 1613, at breakfast, Cosimo de' Medici and his mother, the Grand Duchess Christina began discussing the truth of Jupiter's satellites. Benedetto Castelli, Galileo's student, who was present, asked Galileo to comment on the central point of that conversation Ü the conflict between the Bible and the heliocentric doctrine. The reply was the famous 'Letter to Grand Duchess Christina' which circulated widely in manuscript form at the time. In it, Galileo famously declared that the Bible teaches how to go to heaven, not how the heavens go. Galileo's belief in the truth of the Copernican hypothesis alarmed Dominicans such as Tommaso Caccini and Niccolo Lorini, and the Inquisition examined Galileo's letter to Christina. Thus began Galileo's trouble with the Catholic Church.

Galileo's run-in with the Church is famous to this day, though often over-romanticized or misunderstood. For instance, his declaration in the wake of the condemnation: 'And yet the earth still moves!' is apocryphal. It is therefore important to appreciate the precise nature of the affair.

There were two occasions (1616 and 1632) when Galileo was called to Rome over the truth of Copernicus' theory. As a result of inspecting Galileo's letter, in February 1616, it was agreed by the Inquisition that 1) the immobility of the Sun at the centre of the universe was absurd in philosophy and formally heretical, and that 2) the mobility of Earth was absurd in philosophy and at least erroneous in theology.

At the order of the Pope, Galileo was then summoned (February 1616) by Robert Bellarmino to be cautioned against speaking out on behalf of the Copernican claim. Rumours, however, quickly began to circulate that Galileo had been condemned and prosecuted. In defence, Galileo secured from Bellarmino a letter stating that this was not the case but that he had had been notified of the Papal decision to censor Copernicus' De Revolutionibus because a heliostatic claim was contrary to the literal meaning of Scripture.

Galileo duly kept away from writing on cosmological matters, concentrating instead, on applying his discovery of Jupiter's satellites for determining longitude at sea. In 1623 he wrote the Assayer, published by the Academy of the Lynxes and dedicated to Barberini. There, Galileo famously wrote:
Philosophy is written in this grand book - the universe - which stands continuously open to our gaze. But the book cannot be understood unless one first learns to comprehend the language and interpret the characters in which it is written. It is written in the language of mathematics, and its characters are triangles, circles, and other geometrical figures, without which it is humanly impossible to understand a single word of it; without these one is wandering about in a dark labyrinth. (As quoted by Machamer in The Cambridge Companion to Galileo, pp.64f.)
His sympathizer and patron Barberini had just been elected Pope, as Urban VIII. In 1624 Galileo had an audience with the Pope, who favourably received the Assayer. In the meetings he had with the Pope, Galileo believed he was encouraged to discuss the Copernican theory so long as it was treated as an hypothesis and began to compose the Dialogue on the Two Chief World Systems, which was published in 1632 and dedicated to the Grand Duke. The work caused a furore because Galileo seemed to have gone against the injunction not to advocate the physical truth of Copernicus' claim. The sale of the book was suspended six months after its publication.

In September 1632, Galileo was summoned to Rome, where he arrived in January 1633. First the inquisitors tried to get Galileo to admit that he had earlier been officially banned from teaching Copernicus' theory as true, but Galileo produced Bellarmine's letter to contradict this. By then, both Bellarmine (1621) and Cesi (1630) were dead, and Galileo had few powerful patrons left to defend him. A plea bargain to plead guilty to a lesser charge was scuppered, however, when Urban VIII decided in June that Galileo should be imprisoned for life. Galileo was then interrogated under threat of torture, and made to abjure the 'vehement suspicion of heresy'. He was sentenced to life imprisonment. Galileo spent the rest of his life at his home at Arcetri, under house arrest with the archbishop of Siena. Pleas for pardons or for medical treatment were refused.

Galen


Biography of Galen

Galen (130-200), Greek physician, anatomist, physiologist, philosopher, and lexicographer, was probably the most influential physician of all time.

Throughout his life Galen was a prolific writer, producing his first books, Three Commentaries on the Syllogistic Works of Chrysippus, at the age of 13 and his last, Introduction to Dialectics, in the year of his death. His total output has been estimated at more than 2 1/2 million words. Those of his writings which survive make up over half the extant works of ancient medicine.

Various birth dates from 127 to 132 have been suggested, but 130 is generally accepted. Galen was born at Pergamon, Asia Minor, into a well-to-do family with strong scholarly traditions and influenced by the renaissance in Greek culture which had started at the end of the 1st century A.D. This renaissance had led to increasing Hellenization of the Roman world, the adoption of Greek models of learning, and the use of Greek as the cultural language.

Galen's father, Nicon, mathematician, architect, astronomer, philosopher, and devotee of Greek literature, was not only his sole instructor up to the age of 14, but the example of Stoic virtues on which Galen consciously modeled his own life. In his book On the Passions and Errors of the Soul he says he was "fortunate in having the least irascible, the most just, the most devoted of fathers," but of his mother he says "she was so very much prone to anger that sometimes she bit her handmaids; she constantly shrieked at my father and fought with him." Galen continues, "When I compared my father's noble deeds with the disgraceful passions of my mother I decided to embrace and love his deeds and flee and hate her passions." He defined passion as "that unbridled energy rebellious to reason" and had its control as one of his life's aims. Not surprisingly, perhaps, he himself remained unmarried.

In his fourteenth year Galen attended lectures given by Stoic, Platonic, Peripatetic, and Epicurean philosophers from Pergamon. Encouraged by Nicon, he refused to "proclaim [himself] a member of any of these sects" and said "there was no need for [the philosophy] teachers to disagree with one another, just as there was no disagreement among the teachers of geometry and arithmetic." Later in life he adopted the same attitude to the medical sects, and he urged physicians to take whatever is useful from wherever they find it and not to follow one sect or one man because that produces "an intellectual slave."

Galen relates that Nicon "advised by a dream made me take up medicine together with philosophy

if I had not devoted the whole of my life to the practice of medical and philosophical precepts, I would have learned nothing of importance ... the great majority of men practicing medicine and philosophy are proficient in neither, for they were not well born or not instructed in a fitting way or did not persevere in their studies but turned to politics."


Galen, being well born, fittingly instructed, and eschewing politics, persevered with his studies at Pergamon for the next 4 years, as he puts it, "urging [myself] above [my] companions to such a degree that I was studying both day and night." His first anatomy teacher was Satyrus, a pupil of Quintus, who through his students played a major role in the resurgence of anatomical activity that culminated in Galen's work.
Nicon died in 150 and the following year Galen went to Smyrna. While there he wrote his first treatise, On the Movements of the Heart and Lung. In 152 he went to Corinth and on to Alexandria, where he remained for 4 years studying with Numisianus, Quintus's most famous pupil. Although Galen admired Numisianus and "the physicians [who] employ ocular demonstrations [of human bones] in teaching osteology," he tells us that "in Alexandria the art of medicine was taught by ignoramuses in a sophistical fashion in long, illogical lectures to crowds of fourteen-year-old boys who never got near the sick." He "went away surprised and sorrowful--sorrowful at [Julian the sectarian methodist's] lack of sense, and surprised ... there could be sufficient stupid pupils to fill his classes."

To counteract the poor teaching and the misunderstandings of the students, Galen produced a number of dictionaries, both literary and medical. He also started a major work, On Demonstration. Unfortunately, no copy survives.

Physician to the Gladiators

In 157 Galen returned to Pergamon, where he "had the good fortune to think out and publicly demonstrate a cure for wounded tendons" which gained him, in 158, the position of physician to the gladiators.
He was reappointed annually until the outbreak of the Parthian War in 161.


The traumatic injuries of the arena provided Galen with excellent opportunities to extend his knowledge of anatomy, surgery, and therapeutics, and throughout his life he drew on this fund of experience to illustrate his arguments. While physician to the gladiators, whose daily lives can be reconstructed from his writings, Galen produced some of his most original work, including his demonstration of the part played by the recurrent laryngeal nerve in controlling the production of the voice. This for him and his contemporaries had wide implications, since it impinged on their ideas of the soul.

Practice in Rome

In 163 Galen went to Rome, where he was befriended by the philosopher Eudemus and the consul Flavius Boethius. Galen's public anatomical demonstrations and his success as a physician so aroused the jealousies of the Roman physicians that Eudemus "warned him he was putting himself in danger of assassination." Galen, who accepted the Stoic teachings "to scorn honors and worldly goods and to hold only truth in esteem," scorned the self-seeking of his adversaries and deplored their inability to understand honesty of motive and intellect when they encountered it

Enrico Fermi


Bibliography of Enrico Fermi

Enrico Fermi (29 September 1901 – 28 November 1954) was an Italian physicist, particularly remembered 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. Awarded the Nobel Prize in Physics in 1938 for his work on induced radioactivity, Fermi is widely regarded as one of the leading scientists of the 20th century, highly accomplished in both theory and experiment.[1] Fermium, a synthetic element created in 1952, the Fermi National Accelerator Lab, the Fermi Gamma-ray Space Telescope, and a type of particles called fermions are named after him
Enrico Fermi was born in Rome, Italy, to Alberto Fermi, a Chief Inspector of the Ministry of Communications, and Ida de Gattis, an elementary school teacher who built her own pressure cooker[2]. 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 that 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 assimilated quickly.
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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 physics 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 journal Nuovo Cimento: the first was entitled: "On the dynamics of a solid system of electrical charges in transient conditions"; the second: "On the electrostatics 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 journal "Physikalische Zeitschrift".

In 1922 he published his first important scientific work in the Italian journal 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 a 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 (E = mc2), 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.

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 Segrè. 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 Segrè 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, with the inclusion of the neutrino postulated in 1930 by Pauli, 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[3]. 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 received 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".

Fermi (bottom left), Leo Szilárd (second from right on bottom), and the rest of the pile team.

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;[4] simultaneously, they communicated these results to Lise Meitner. Meitner, and her nephew Otto Robert Frisch, correctly interpreted these results as being nuclear fission.[5] Frisch confirmed this experimentally on 13 January 1939.[6]

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.”[3] 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,[7] 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.[3]

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:

Fermi's ID badge photo from Los Alamos.
"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."[8]

An image from the Fermi–Szilárd "neutronic reactor" patent.

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 nuclear power 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[9]. 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 National Laboratory 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:“ As the shock wave hit Base Camp, Aeby saw Enrico Fermi with a handful of torn paper. "He was dribbling it in the air. When the shock wave came it moved the confetti. He thought for a moment."

Fermi had just estimated the yield of the first nuclear explosion. It was in the ball park.[10] ”


Fermi's strips-of-paper estimate was ten kilotons of TNT; the actual yield was about 19 kilotons

In 1947, Fermi invented the FERMIAC, an analog computer that used the Monte Carlo Method to study neutron transport through fissionable materials.

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[1]. 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. Later on, his method of getting approximate and quick answers through back-of-the-envelope calculations became informally known as the 'Fermi method'.

The sign at Enrico Fermi street in Rome

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.

He also 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.

Toward the end of his life, Fermi questioned his faith in society at large to make wise choices about nuclear technology[13]. He said[14]:
"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."

Fermi died at age 53 of stomach cancer in Chicago, Illinois, and was interred at Oak Woods Cemetery. 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.[15]

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 and thinkers 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:
Fermi 1 & Fermi 2 nuclear power plants in Newport, Michigan
Enrico Fermi Nuclear Power Plant (Italy).
RA-1 Enrico Fermi, a research reactor in Argentina.

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.
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Fermi Family and Legacy

Fermi and Laura Capon's two children, daughter Nella Fermi Weiner, PhD (1931–1995), and son Giulio ("Judd") Fermi PhD (1936–1997), became respectively an artist and feminist; and a biologist who worked with the Nobel laureate Max Perutz on the structure of hemoglobin.

His wife, Laura Fermi (1907–1977), an 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"[16] said, of our nuclear dilemma[17]:
"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 third grandchild, continued to question the sanity of nuclear weapons in her book, "Picturing the Bomb"[18]. 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 Olivia (nee Weiner) Caton, M.A. A.B.S.—Leadership in Human Systems, ConRes Cert, photoartist and writer, Laura's and Enrico's first grandchild, is currently researching the legacy of her grandparents for a series of books she plans to publish.[19] 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."[20]

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.

Euclid


The Greek mathematician Euclid (active 300 BC) wrote the Elements, a collection of geometrical theorems. The oldest extant major mathematical work in the Western world, it set a standard for logical exposition for over 2,000 years.


Virtually nothing is known of Euclid personally. It is not even known for certain whether he was a creative mathematician himself or was simply good at compiling the work of others. Most of the information about Euclid comes from Proclus, a 5th-century-AD. Greek scholar. Because Archimedes refers to Euclid and Archimedes lived immediately after the time of Ptolemy I, King of Egypt (ca. 306-283 BC), Proclus concludes they were contemporaries. Euclid's mathematical education may well have been obtained from Plato's pupils in Athens, since it was there that most of the earlier mathematicians upon whose work the Elements is based had studied and taught.

No earlier writings comparable to the Elements of Euclid have survived. One reason is that Euclid's Elements superseded all previous writings of this type, making it unnecessary to preserve them. This makes it difficult for the historian to investigate those earlier mathematicians whose works were probably more important in the development of Greek mathematics than Euclid's. About 600 B.C. the Greek mathematician Thales is said to have discovered a number of theorems that appear in the Elements. It might be noted too that Eudoxus is also given credit for the discovery of the method of exhaustion, whereby the area of a circle and volume of a sphere and other figures can be calculated. Book XII of the Elements makes use of this method. Although mathematics may have been initiated by concrete problems, such as determining areas and volumes, by the time of Euclid mathematics had developed into an abstract construction, an intellectual occupation for philosophers rather than scientists.

The Elements

The Elements consists of 13 books. Within each book is a sequence of propositions or theorems, varying from about 10 to 100, preceded by definitions. In Book I, 23 definitions are followed by five postulates. After the postulates, five common notions or axioms are listed. The first is, "Things which are equal to the same thing are also equal to each other." Next are 48 propositions which relate some of the objects that were defined and which lead up to Pythagoras's theorem: in right-angled triangles the square on the side subtending the right angle is equal to the sum of the squares on the sides containing the right angle. The usual elementary course in Euclidean geometry is based on Book I.

The remaining books, although not so well known, are more advanced mathematically. Book II is a continuation of Book I, proving geometrically what today would be called algebraic identities, such as (a + b)2 = a2 + b2 + 2ab, and generalizing some propositions of Book I. Book III is on circles, intersections of circles, and properties of tangents to circles. Book IV continues with circles, emphasizing inscribed and circumscribed rectilinear figures.

Book V of the Elements is one of the finest works in Greek mathematics. The theory of proportions discovered by Eudoxus is here expounded masterfully by Euclid. The theory of proportions is concerned with the ratios of magnitudes (rational or irrational numbers) and their integral multiples. Book VI applies the propositions of Book V to the figures of plane geometry. A basic proposition in this book is that a line parallel to one side of a triangle will divide the other two sides in the same ratio.

As in Book V, Books VII, VIII, and IX are concerned with properties of (positive integral) numbers. In Book VII a prime number is defined as that which is measured by a unit alone (a prime number is divisible only by itself and 1). In Book IX proposition 20 asserts that there are infinitely many prime numbers, and Euclid's proof is essentially the one usually given in modern algebra textbooks. Book X is an impressively well-finished treatment of irrational numbers or, more precisely, straight lines whose lengths cannot be measured exactly by a given line assumed as rational.

Books XI-XIII are principally concerned with three-dimensional figures. In Book XII the method of exhaustion is used extensively. The final book shows how to construct and circumscribe by a sphere the five Platonic, or regular, solids: the regular pyramid or tetrahedron, octahedron, cube, icosahedron, and dodecahedron.

Manuscript translations of the Elements were made in Latin and Arabic, but it was not until the first printed edition, published in Venice in 1482, that geometry, which meant in effect the Elements, became important in European education. The first complete English translation was printed in 1570. It was during the most active mathematical period in England, about 1700, that Greek mathematics was studied most intensively. Euclid was admired, mastered, and utilized by all major mathematicians, including Isaac Newton.

The growing predominance of the sciences and mathematics in the 18th and 19th centuries helped to keep Euclid in a prominent place in the curriculum of schools and universities throughout the Western world. But also the Elements was considered educational as a primer in logic.

Euclid's Other Works

Some of Euclid's other works are known only through references by other writers. The Data is on plane geometry. The word "data" means "things given." The treatise contains 94 propositions concerned with the kind of problem where certain data are given about a figure and from which other data can be deduced, for example: if a triangle has one angle given, the rectangle contained by the sides including the angle has to the area of the triangle a given ratio.

On Division (of figures), also on plane geometry, is known only in the Arabic, from which English translations were made. Proclus refers to it when speaking of dividing a figure into other figures different in kind, for example, dividing a triangle into a triangle and a quadrilateral. On Division is concerned with more general problems of division. As an example, one problem is to draw in a given circle two parallel chords cutting off between them a given fraction of the area of the circle.

The Conics appears to have been lost by the time of the Greek astronomer Pappus (late 3d century A.D.). It is frequently referred to by Archimedes. As the name suggests, it dealt with the conic sections: the ellipse, parabola, and hyperbola, to use the names given them later by Apollonius of Perga.

A work which has survived is Phaenomena. This is what today would be called applied mathematics; it is about the geometry of spheres applicable to astronomy. Another applied work which has survived is the Optics. It was maintained by some that the sun and other heavenly bodies are actually the size they appear to be to the eye. This work refuted such a view by analyzing the relationship between what the eye sees of an object and what the object actually is. For example, the eye always sees less than half of a sphere, and as the observer moves closer to the sphere the part of it seen is decreased although it appears larger.

Another lost work is the Porisms, known only through Pappus. A porism is intermediate between a theorem and a problem; that is, rather than something to be proved or something to be constructed, a porism is concerned with bringing out another aspect of something that is already there. To find the center of a circle or to find the greatest common divisor of two numbers are examples of porisms. This work appears to have been more advanced than the Elements and perhaps if known would give Euclid a higher place in the history of mathematics.

Dulong, Pierre Louis


Dulong was born in Rouen, France. He worked on the specific heat capacity and the expansion and refractive indices of gases.

He gained his secondary education in Auxerre and Rouen before entering the École Polytechnique, Paris in 1801. He began studying medicine, but gave this up to concentrate on science, working under the direction of Thénard. Dulong succeeded Alexis Thérèse Petit as professor of physics, from 1820 to 1829, then was directeur des études until his death.

In chemistry, he contributed to knowledge on:
the double decomposition of salts (1811)
nitrous acid (1815)
the oxides of phosphorus (1816)
the oxides of nitrogen
catalysis by metals (1823, with Thénard)

Dulong also discovered the dangerously sensitive nitrogen trichloride in 1812, losing two fingers and an eye in the process.[1]

In 1819 Dulong collaborated with Petit to show that the mass heat capacity of metallic elements are inversely proportional to their atomic masses, this being now known as the Dulong-Petit law.[2] Dulong also worked on the elasticity of steam, on the measurement of temperatures, and on the behavior of elastic fluids. He made the first precise comparison of the mercury- and air-temperature scales. At the time of his death, he was working on the development of precise methods in calorimetry.

In 1830, he was elected a foreign member of the Royal Swedish Academy of Sciences.