The Cosmological Constant
In 1917 Einstein added a term to his equations to keep the universe still — then abandoned it, reportedly called it his "biggest blunder," and watched it return decades later as dark energy. The documented story, with the legend labeled.
The problem: a universe that wouldn’t sit still
General relativity’s field equations (November 1915) describe how matter and energy curve spacetime. Applied to the entire universe, they had an unwelcome implication: the universe they described was dynamic — it had to be expanding or contracting. But in 1917, the universe was universally assumed to be static and eternal. Einstein, sharing the assumption, modified his equations.
In “Cosmological Considerations in the General Theory of Relativity” (Sitzungsberichte der Preussischen Akademie der Wissenschaften, 1917), he introduced Λ (lambda), the cosmological constant — a small repulsive term that exactly balanced gravity’s attraction, holding the cosmos in static equilibrium. It was, by his own later admission, an inelegant fix: the equations had been beautiful, and he had spoiled them to match a prejudice.
The evidence for expansion
The static universe did not survive the 1920s:
- Vesto Slipher had been measuring redshifts of spiral nebulae since 1912 — their light stretched toward the red, as if receding.
- Alexander Friedmann (1922) showed Einstein’s original equations, without the constant, naturally described an expanding or contracting universe.
- Georges Lemaître (1927) derived the expansion explicitly and connected it to the redshift data.
- Edwin Hubble (1929) published the redshift–distance relation: the farther a galaxy, the faster it recedes.
By the early 1930s Einstein had dropped the constant and accepted the expanding universe. The static cosmos — and the term invented to preserve it — were gone.
“My biggest blunder”?
Here the legend needs its label. The story that Einstein called the cosmological constant his “biggest blunder” comes from exactly one source: George Gamow’s memoir My World Line (1970), published fifteen years after Einstein’s death. Gamow, who knew Einstein, wrote that Einstein had said this to him. No letter, manuscript, or recorded remark of Einstein’s contains the phrase. This site follows its methodology: the claim is reported by Gamow, not documented as Einstein’s. (The verdict is also tested in Reception.)
What is documented is that Einstein regarded Λ as ugly and unnecessary, and abandoned it as soon as the evidence permitted.
The return: dark energy
Then came the twist. In 1998, two teams studying distant supernovae — the Supernova Cosmology Project and the High-Z Supernova Search Team — found that the universe’s expansion is accelerating: something is pushing outward against gravity’s pull. The simplest mathematical description of that push is… a cosmological constant. Modern cosmology’s standard model includes Λ as “dark energy,” the unknown driver of the acceleration (recognized with the 2011 Nobel Prize to Perlmutter, Schmidt, and Riess).
The irony is real, but it should not be oversold. Einstein did not “predict dark energy” — his constant was tuned to hold the universe still, the opposite of what dark energy does, and he introduced it for philosophical reasons, not from evidence. What the episode actually demonstrates is something about his equations: they were richer than his own assumptions. The mathematics permitted a dynamic universe before anyone believed in one, and permitted a repulsive term before anyone needed one.
Source notes
- The 1917 paper: Einstein, “Kosmologische Betrachtungen zur allgemeinen Relativitätstheorie,” Sitzungsberichte der Preussischen Akademie der Wissenschaften (1917) (CPAE Vol. 6).
- Friedmann (1922, Zeitschrift für Physik); Lemaître (1927, Annales de la Société scientifique de Bruxelles); Hubble (1929, Proceedings of the National Academy of Sciences); Slipher’s redshift measurements (1912–1917, Lowell Observatory).
- The “biggest blunder” attribution: George Gamow, My World Line (Viking, 1970) — secondhand report, labeled as such; see also reception.md.
- Accelerating expansion: Riess et al., Astronomical Journal 116 (1998); Perlmutter et al., Astrophysical Journal 517 (1999). 2011 Nobel Prize in Physics (Perlmutter, Schmidt, Riess) — NobelPrize.org.
- The claim that Einstein found Λ inelegant and abandoned it by the early 1930s follows Pais (1982) and the documentary record of his 1930s cosmology papers.