Researchers construct the Schwarzschild–de Sitter solution, highlighting its implications in theoretical physics.
We construct the Schwarzschild–de Sitter metric as the unique spherically symmetric static exact solution of the vacuum Einstein equation derived in Paper [1] of this series. The cosmological constant Lambda = 3/R^2 is intrinsically determined by the central projection framework, requiring no additional assumptions. We examine the R -> 0 limit and connect it to the nested structure of Paper [4].
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Noriaki Kihara (2026) studied this question.
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