Einstein's static universe
Einstein's static universe is the cosmological model Albert Einstein proposed in 1917, only months after finishing his general theory of relativity. It described a universe that neither grew nor shrank. To make the equations work, Einstein had to insert an extra term of his own invention. That fix would not last through the next decade. What forced Einstein toward a universe standing still, and what finally convinced him to let it go?
Spherical spatial curvature is what general relativity produced once Einstein applied it to the whole universe, assuming even matter and no change over time. That combination gave Einstein a universe that was finite in size, closed back on itself rather than stretching out forever.
The cosmological constant is the term Einstein introduced to keep this static, matter-filled universe from collapsing under its own gravity. Einstein tied this constant, written as Λ, to two other quantities: the universe's radius R and its matter density ρ. The relation was Λ equals 1 over R squared, and also equals κ times ρ divided by 2, where κ is the Einstein gravitational constant. That relationship would soon meet a challenge from observations Einstein had not built into his equations.
In 1929, Edwin Hubble discovered a linear relationship between the redshifts of galaxies and how far away they sat. Faced with this evidence, Einstein abandoned his static model for universes that could expand, including the Friedmann-Einstein universe and the Einstein-de Sitter universe. In both new models he set the cosmological constant to zero, calling it "no longer necessary... and theoretically unsatisfactory."
Many Einstein biographies claim that he later called the cosmological constant his "biggest blunder." The astrophysicist Mario Livio has cast doubt on this claim, suggesting it may be exaggerated. Whether Einstein ever spoke those exact words remains unresolved, leaving one of physics' most quoted lines still unverified.
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Common questions
What is Einstein's static universe?
Einstein's static universe, also called the Einstein universe or Einstein static eternal universe, is a relativistic model of the cosmos that Albert Einstein proposed in 1917. It described a finite universe with spherical spatial curvature, assuming a uniform distribution of matter and no change over time.
Why did Einstein introduce the cosmological constant?
Einstein introduced the cosmological constant to find a consistent solution to his field equations for a static universe containing a non-zero density of matter. Without it, the equations could not describe a universe that stayed the same size while still containing matter.
What is the equation linking Einstein's cosmological constant to the universe's radius and density?
In Einstein's static universe, the cosmological constant Λ relates to the radius R and matter density ρ through Λ equals 1 over R squared, which also equals κ times ρ divided by 2. Here κ stands for the Einstein gravitational constant.
Why did Einstein abandon his static universe model?
Einstein abandoned his static universe after Edwin Hubble discovered a linear relationship between the redshifts of galaxies and their distance in 1929. Einstein then proposed expanding models, including the Friedmann-Einstein universe and the Einstein-de Sitter universe, setting the cosmological constant to zero in both.
Did Einstein really call the cosmological constant his biggest blunder?
Many Einstein biographies claim he referred to the cosmological constant in later years as his "biggest blunder," but this is disputed. Astrophysicist Mario Livio has cast doubt on the claim, suggesting it may be exaggerated.
What models did Einstein propose after giving up on a static universe?
After abandoning his static model, Einstein proposed the Friedmann-Einstein universe and the Einstein-de Sitter universe, both allowing for expansion. In each, he set the cosmological constant to zero, calling it "no longer necessary... and theoretically unsatisfactory."
All sources
10 references cited across the entry
- 1JournalKosmologische Betrachtungen zur allgemeinen RelativitätstheorieAlbert Einstein — 1917
- 2BookThe Principle of RelativityLorentz H.A. et al. — Metheun & Co. — 1923
- 3JournalEinstein's 1917 static model of the universe: a centennial reviewO'Raifeartaigh — 2017
- 4JournalA relation between distance and radial velocity among extra-galactic nebulaeEdwin Hubble — 1929
- 5JournalZum kosmologischen Problem der allgemeinen RelativitätstheorieAlbert Einstein — 1931
- 6BookRelativity: The Special and General TheoriesAlbert Einstein — Metheun — 1946
- 7JournalEinstein's cosmic model of 1931 revisited: an analysis and translation of a forgotten model of the universeO'Raifeartaigh and McCann — 2014
- 8BookDiscovering the Expanding UniverseNussbaumer and Bieri — Cambridge University Press — 2009
- 9JournalOn the Instability of Einstein's Spherical WorldA. S. Eddington — 9 May 1930
- 10NewsThe Genius of Getting It Wrong: Brilliant Blunders by Mario LivioZimmer — 9 June 2013