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Einstein’s Static Universe

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Einstein’s Static Universe. (1917). De Sitter’s Accelerating Universe. Always expanding exponential curve R = exp[t /3] No matter – only  It has no beginning and no end (1917). Willem De Sitter 1872-1934. Friedmann’s universes. 1888-1925. 1922,1924. Edwin Hubble. (1889-1953). - PowerPoint PPT Presentation

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Page 1: Einstein’s Static Universe
Page 2: Einstein’s Static Universe

Einstein’s Static UniverseEinstein’s Static Universe

(1917)(1917)

Page 3: Einstein’s Static Universe

De Sitter’s Accelerating UniverseDe Sitter’s Accelerating Universe

Always expandingAlways expandingexponential curve R = exp[texponential curve R = exp[t/3]/3]

No matter – only No matter – only It has no beginning and no endIt has no beginning and no end

(1917)(1917)Willem De SitterWillem De Sitter

1872-19341872-1934

Page 4: Einstein’s Static Universe

Friedmann’s universesFriedmann’s universes

1922,19241888-1925

Page 5: Einstein’s Static Universe

Edwin HubbleEdwin Hubble(1889-1953)

Hubble-Humason Law todayHubble-Humason Law today

Milton HumasonMilton Humason(1891-1972)

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The Einstein-de Sitter UniverseThe Einstein-de Sitter Universe

‘‘I do not think the paper very important I do not think the paper very important myself, but de Sitter was keen on it’myself, but de Sitter was keen on it’ EinsteinEinstein

‘‘the paper by Einstein and myself I do the paper by Einstein and myself I do not myself consider the result of muchnot myself consider the result of muchimportance, but Einstein seemed to thinkimportance, but Einstein seemed to thinkIt was’It was’ De SitterDe Sitter

1932

= 0= 0

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Lemaître's UniverseLemaître's Universe

The best description of The best description of the visible universethe visible universe todaytoday

1927

> 0> 0

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Tolman’s Oscillating Tolman’s Oscillating UniverseUniverse

Richard Tolman and Einstein at Cal Tech

1932

Page 9: Einstein’s Static Universe

Tolman includes theTolman includes the22ndnd Law of thermodynamics: Law of thermodynamics:

Oscillations growOscillations grow(1932)(1932)

JDB + Dabrowski include theJDB + Dabrowski include thecosmological constant:cosmological constant:Oscillations always end Oscillations always end

(1995)(1995)

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Kasner’s Anisotropic UniverseKasner’s Anisotropic Universe

Edward KasnerEdward Kasner(1878-1955)(1878-1955)

19211921

Volume abc time

Page 11: Einstein’s Static Universe

expansionexpansion shearshear rotationrotation

Page 12: Einstein’s Static Universe

Gödel's Rotating UniverseGödel's Rotating Universe

Allows time travelAllows time travelto occur !to occur !

1949

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Real Universes Tend to Get LumpyReal Universes Tend to Get Lumpy

Is this the origin of Is this the origin of galaxies ?galaxies ?

Newton 1693Newton 1693Jeans 1902Jeans 1902

Lifshitz 1946Lifshitz 1946

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The Big Bang UniversesThe Big Bang Universes

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The Evidence of a Hot Early HistoryThe Evidence of a Hot Early History

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A temporary lambdaA temporary lambda

The Inflationary UniverseThe Inflationary Universe

1981

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Even Smaller BeginningsEven Smaller Beginnings

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Chaotic InflationChaotic Inflation

Geography is more complicated than we thoughtGeography is more complicated than we thought

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Eternal InflationEternal Inflation

More than 10More than 1010107777

by-universes from our patch aloneby-universes from our patch alone

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Lemaître's universe describes our visible universe to high precisionLemaître's universe describes our visible universe to high precision

The Universe is Accelerating AgainThe Universe is Accelerating Again

> 0

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The Return of Lambda ?The Return of Lambda ?

?

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