Schwarzschild-de Sitter spacetime in regular coordinates with cosmological time
Leonardo de Lima, Davi C. Rodrigues

TL;DR
This paper introduces two smooth, time-dependent coordinate systems for Schwarzschild-de Sitter spacetime that are valid across horizons, clarifying their equivalence and potential for better understanding black holes in cosmological backgrounds.
Contribution
It derives and proves the equivalence of two previously proposed coordinate systems for SdS spacetime, extending the set of tools for analyzing black holes in cosmological settings.
Findings
Both coordinate systems are equivalent descriptions of SdS spacetime.
Explicit transformations link these coordinates to Kottler and Lake-Israel coordinates.
The coordinates are smooth across black hole and cosmological horizons, requiring a positive cosmological constant.
Abstract
Starting from the Einstein equations in Schwarzschild-de Sitter (SdS) spacetime and imposing Friedmann-Robertson-Walker coordinates at large distances, we find two coordinate systems with time-dependent metrics that are smooth across both the black hole and cosmological horizons. These coordinates require a positive cosmological constant for regularity, and thus they are not de Sitter extensions of the Kruskal-Szekeres or Israel coordinates. One of the coordinate systems was only found in 1999 (Abbassi coordinates), and it has led to conflicting interpretations in the literature, while the other was briefly commented on and promptly dismissed as unphysical or incompatible with SdS. We derive that the second solution is equivalent to the first one, and that both are indeed equivalent descriptions of SdS spacetime. We also derive explicit coordinate transformations linking these…
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Taxonomy
TopicsAstrophysical Phenomena and Observations · Black Holes and Theoretical Physics · Relativity and Gravitational Theory
