De Sitter and Schwarzschild-De Sitter According to Schwarzschild and De Sitter

Abstract

When de Sitter first introduced his celebrated spacetime, he claimed, following Schwarzschild, that its spatial sections have the topology of the real projective space RP^3 (that is, the topology of the group manifold SO(3)) rather than, as is almost universally assumed today, that of the sphere S^3. (In modern language, Schwarzschild was disturbed by the non-local correlations enforced by S^3 geometry.) Thus, what we today call "de Sitter space" would not have been accepted as such by de Sitter. There is no real basis within classical cosmology for preferring S^3 to RP^3, but the general feeling appears to be that the distinction is in any case of little importance. We wish to argue that, in the light of current concerns about the nature of de Sitter space, this is a mistake. In particular, we argue that the difference between "dS(S^3)" and "dS(RP^3)" may be very important in attacking the problem of understanding horizon entropies. In the approach to de Sitter entropy via Schwarzschild-de Sitter spacetime, we find that the apparently trivial difference between RP^3 and S^3 actually leads to very different perspectives on this major question of quantum cosmology.

26 pages, 8 figures, typos fixed, references added, equation numbers finally fixed, JHEP version

References in corpus (7)

• Asymmetries in the CMB anisotropy field
• The significance of the largest scale CMB fluctuations in WMAP
• The Statistical Significance of the Low CMB Mulitipoles
• Generic Cosmic Censorship Violation in anti de Sitter Space
• Inflationary Perturbations from Deformed CFT
• Transplanckian Entanglement Entropy
• Nearly Degenerate dS Horizons from a 2-D Perspective

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