1924
DOI: 10.1007/bf01328280
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�ber die M�glichkeit einer Welt mit konstanter negativer Kr�mmung des Raumes

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Cited by 621 publications
(437 citation statements)
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“…A lack of structure on the largest scales in maps of CMB temperature fluctuations would be a hint that the comoving spatial section of the Universe is multiply connected (de Sitter 1917;Friedmann 1923Friedmann , 1924Lemaître 1931;Robertson 1935) and that its size may have been detected (Starobinsky 1993;Stevens et al 1993). The WMAP observations have confirmed that the large-scale CMB signal analysed either as a quadrupole signal or as a two-point autocorrelation function signal is weak (Spergel et al 2003;Copi et al 2007Copi et al , 2009).…”
Section: Introductionmentioning
confidence: 98%
“…A lack of structure on the largest scales in maps of CMB temperature fluctuations would be a hint that the comoving spatial section of the Universe is multiply connected (de Sitter 1917;Friedmann 1923Friedmann , 1924Lemaître 1931;Robertson 1935) and that its size may have been detected (Starobinsky 1993;Stevens et al 1993). The WMAP observations have confirmed that the large-scale CMB signal analysed either as a quadrupole signal or as a two-point autocorrelation function signal is weak (Spergel et al 2003;Copi et al 2007Copi et al , 2009).…”
Section: Introductionmentioning
confidence: 98%
“…It represents one of the alternatives offered by Friedmann (1922Friedmann ( , 1924, whose analysis suggested that Einstein"s general relativity theory (GR) allows for expanding as well as for contracting universes, but not for a static one, unless a well-tuned repulsive cosmological constant (Λ) is introduced. Einstein"s own model (1917) relied on such a constant, which Einstein had introduced reluctantly, since it does not reflect anything known from physics.…”
Section: Introductionmentioning
confidence: 99%
“…Shortly before this, de Sitter (1917) had shown that in presence of Λ the solution for an empty space describes an exponential expansion. Friedmann (1922Friedmann ( , 1924 was the first to obtain exact solutions for the expanding universe that contained matter in presence of the cosmological constant Λ. Another exact solution for the metric in presence of Λ, around the gravitating point mass, was obtained by Carter (1973).…”
Section: Newtonian Approximation In Description Of Dementioning
confidence: 99%