George David Birkhoff
American mathematician known for the ergodic theorem.
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George David Birkhoff (March 21, 1884 – November 12, 1944) was an American mathematician and a leading figure in his field during his era. His work spanned differential equations, dynamical systems, the four-color problem, the three-body problem, and general relativity. He is most famous today for the ergodic theorem. His home in Cambridge, Massachusetts, is a National Historic Landmark.
Birkhoff was born in Overisel Township, Michigan, to Dutch immigrant parents. His father, David Birkhoff, arrived in the U.S. in 1870 and worked as a physician in Chicago. As a teenager, Birkhoff attended the Lewis Institute from 1896 to 1902.
He belonged to the first generation of American mathematicians to be trained entirely in the United States. After the Lewis Institute, he spent a year at the University of Chicago, then earned his A.B. and A.M. from Harvard. He returned to Chicago for his Ph.D., graduating summa cum laude in 1907 at age twenty-three. Though E. H. Moore was his advisor, Henri Poincaré’s writings influenced him most. He taught at the University of Wisconsin–Madison (1907–1909) and Princeton (1909–1912) before joining Harvard in 1912, where he remained until his death. As the only American familiar with all three major U.S. mathematical institutions—Chicago, Harvard, and Princeton—he was highly respected by his peers.
Within the American Mathematical Society, Birkhoff served as vice president in 1919 and edited its *Transactions* from 1920 to 1924. He was president from 1925 to 1926, during which he pushed for a lectureship program to travel the U.S. promoting mathematics. In 1926, he traveled to Europe as an unofficial representative of the Rockefeller Foundation’s International Education Board, working to build ties between American and French institutions, partly due to his fondness for Paris. In 1937, he became president of the American Association for the Advancement of Science, an unusual honor for a mathematician that reflected his standing in the scientific community.
In 1912, while working on the four-color problem, Birkhoff introduced the chromatic polynomial. Though it didn’t solve the problem, it became important in algebraic graph theory. In 1913, he proved Poincaré’s “Last Geometric Theorem,” a special case of the three-body problem, which brought him worldwide fame and boosted the international reputation of American mathematics. He also contributed to general relativity, writing on its foundations and quantum mechanics, and co-authoring *Relativity and Modern Physics* (1923) with R. E. Langer. That same year, he proved that the Schwarzschild geometry is the only spherically symmetric solution to Einstein’s field equations, showing that black holes could arise from any sufficiently massive spherical star—a result later used in the Oppenheimer–Snyder model. He published *Dynamical Systems* in 1927.
His most lasting work came in 1931 with the ergodic theorem, which combined insights from physics on the ergodic hypothesis with measure theory to address a core problem in statistical mechanics. This theorem also influenced dynamics, probability, group theory, and functional analysis. He worked on number theory, the Riemann–Hilbert problem, and the four-color problem, and proposed an axiomatization of Euclidean geometry different from Hilbert’s (Birkhoff’s axioms), culminating in *Basic Geometry* (1941). In 1933, he published *Aesthetic Measure*, a mathematical theory of aesthetics, for which he studied art, music, and poetry from various cultures. His 1938 book *Electricity as a Fluid* blended philosophy and science. His 1943 theory of gravitation is puzzling because, despite knowing it, Birkhoff accepted that it allowed only matter that is a perfect fluid where the speed of sound equals the speed of light.
Birkhoff believed foreign fellowships could raise U.S. mathematical standards, but he wanted stricter qualifications, arguing that standards in less-developed countries differed and that access should be limited. He insisted foreign fellows meet language requirements. Albert Einstein and Norbert Wiener accused Birkhoff of promoting antisemitic selection processes. During the 1930s, as many Jewish mathematicians fled Europe for the U.S., Birkhoff allegedly influenced hiring to exclude Jews. Saunders Mac Lane, then at Harvard, dismissed Einstein’s claims as “worthless,” saying Einstein was unfamiliar with American processes and had competing ideas about general relativity. Mac Lane also rebutted reports of antisemitism toward Wiener, noting that Birkhoff clearly listened to Wiener’s ideas.
- born
- March 21, 1884
- died
- November 12, 1944
- field
- Mathematics
- nationality
- American
- known_for
- Ergodic theorem, Birkhoff's theorem, chromatic polynomial, Birkhoff's axioms
Verified Timeline
Lore & Background
Birkhoff was born in Overisel Township, Michigan, the son of two Dutch immigrants, David Birkhoff and Jane Gertrude Droppers. His father worked as a physician in Chicago while he was a child. From 1896 to 1902, he attended the Lewis Institute as a teenager. He then spent a year at the University of Chicago, obtained his A.B. and A.M. from Harvard University, returned to the University of Chicago in 1905, and at age twenty-three graduated summa cum laude with his Ph.D. in 1907 in differential equations. While E. H. Moore was his supervisor, he was most influenced by the writings of Henri Poincaré. After teaching at the University of Wisconsin–Madison from 1907 to 1909 and at Princeton University from 1909 to 1912, he taught at Harvard from 1912 until his death. He was the only American familiar with the three main mathematical institutions within the United States—Chicago, Harvard and Princeton. In 1912, attempting to solve the four color problem, Birkhoff introduced the chromatic polynomial. In 1913, he proved Poincaré's 'Last Geometric Theorem,' a special case of the three-body problem, a result that made him world-famous and improved the international recognition of American mathematics. In 1923, Birkhoff proved that the Schwarzschild geometry is the unique spherically symmetric solution of the Einstein field equations, a consequence being that black holes could result from any spherical star having sufficient mass. His most durable result has been his 1931 discovery of what is now called the ergodic theorem, combining insights from physics on the ergodic hypothesis with measure theory. He also proposed an axiomatization of Euclidean geometry different from Hilbert's (see Birkhoff's axioms), culminating in his text Basic Geometry (1941). His 1933 Aesthetic Measure proposed a mathematical theory of aesthetics.
Reader's Guide
Birkhoff's significance lies in his foundational contributions across multiple areas of mathematics and physics. His ergodic theorem solved, at least in principle, a fundamental problem of statistical mechanics and has had repercussions for dynamics, probability theory, group theory, and functional analysis. His proof of Poincaré's last geometric theorem advanced the three-body problem and raised the international recognition of American mathematics. In general relativity, his uniqueness theorem for the Schwarzschild solution was later used to develop the Oppenheimer–Snyder model. He served as president of the American Mathematical Society from 1925 to 1926 and as president of the American Association for the Advancement of Science in 1937, a rare occurrence for mathematicians. His legacy includes the George David Birkhoff Prize in applied mathematics, awarded jointly by the American Mathematical Society and the Society for Industrial and Applied Mathematics. However, his career is also marked by controversy: Albert Einstein and Norbert Wiener accused Birkhoff of advocating antisemitic selection processes during the 1930s. Saunders Mac Lane called Einstein's allegations 'worthless' and stated Birkhoff's efforts were motivated by a desire to find jobs for home-grown American mathematicians, but correspondence later revealed that his views of Jews were antisemitic. Yet he was close to Jewish mathematician Stanislaw Ulam, and Gian-Carlo Rota wrote that Birkhoff 'would occasionally feel the urge to shower his protective instincts on some good-looking young Jew.'
Did You Know?
- Birkhoff graduated summa cum laude with his Ph.D. at age twenty-three in 1907.
- He proved Poincaré's 'Last Geometric Theorem' in 1913, a special case of the three-body problem, which made him world-famous.
- In 1923, Birkhoff proved that the Schwarzschild geometry is the unique spherically symmetric solution of the Einstein field equations.
- He served as president of the American Association for the Advancement of Science in 1937, a rare occurrence for mathematicians.
- Birkhoff's 1933 book Aesthetic Measure proposed a mathematical theory of aesthetics, for which he spent a year studying art, music, and poetry.
Frequently Asked Questions
Who is George David Birkhoff?
He was an American mathematician born in 1884 who is widely regarded as one of the leading figures in American mathematics of his era. His work spanned differential equations, dynamical systems, and several other areas of pure and applied math.
What is Birkhoff best known for?
His most celebrated result is the ergodic theorem, a foundational statement about the long-term average behavior of dynamical systems. He is also recognized for Birkhoff's theorem in relativity, his work on chromatic polynomials, and his axiomatic approach to convex geometry.
What fields did Birkhoff contribute to?
He made significant advances in differential equations, dynamical systems, the four-color problem, the three-body problem, and general relativity. His contributions to convex geometry and combinatorics also remain influential in those fields.
When was Birkhoff born and when did he die?
He was born on March 21, 1884, and passed away on November 12, 1944. His sixty-year life produced a body of work that placed him at the center of American mathematical research in the early twentieth century.
Why is Birkhoff considered important in the history of mathematics?
His ergodic theorem laid the groundwork for modern ergodic theory, which now underpins areas ranging from statistical mechanics to information theory. Beyond that single result, his breadth across geometry, combinatorics, and physics-related mathematics made him a defining voice of his generation.
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