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- W2047792022 abstract "I discuss a solution to the dark energy problem, which arises when the visible universe is approximated by a black hole, in a quasi-static asymptotically-flat approximation. Using data, provided by WMAP7, I calculate the Schwarzschild radius rs and compare to the measured physical radius of the visible universe, bounded by the surface of last scatter. The ratio, ε(t0) = r/rs is found to be comparable to ε = 1, as allowed by the holographic principle. The measurement of a shift parameter, σ, introduced by Bond, Efstathiou and Tegmark in 1997, plays an important role in the accuracy of the calculation. The approximation leads to a surprisingly small discrepancy, presumably explicable by the de Sitter, and expanding, nature of the actual universe." @default.
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- W2047792022 date "2010-11-01" @default.
- W2047792022 modified "2023-09-23" @default.
- W2047792022 title "Holographic Principle and the Surface of Last Scatter" @default.
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- W2047792022 doi "https://doi.org/10.1088/1742-6596/259/1/012015" @default.
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