2010
DOI: 10.1103/physrevd.81.104044
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McVittie’s legacy: Black holes in an expanding universe

Abstract: We prove that a class of solutions to Einstein's equations-originally discovered by G. C. McVittie in 1933-includes regular black holes embedded in Friedman-Robertson-Walker cosmologies. If the cosmology is dominated at late times by a positive cosmological constant, the metric is regular everywhere on and outside the black hole horizon and away from the big bang singularity, and the solutions asymptote in the future and near the horizon to the Schwarzschild-de Sitter geometry. For solutions without a positive… Show more

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Cited by 147 publications
(293 citation statements)
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References 40 publications
(88 reference statements)
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“…We note a possible weakness [36] of the McVittie spacetime we used here. Precisely, all McVittie descriptions take the background matter density to be homogeneous, ρ ≡ ρ(τ ), in addition to the usual, central overdensity.…”
Section: Discussionmentioning
confidence: 99%
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“…We note a possible weakness [36] of the McVittie spacetime we used here. Precisely, all McVittie descriptions take the background matter density to be homogeneous, ρ ≡ ρ(τ ), in addition to the usual, central overdensity.…”
Section: Discussionmentioning
confidence: 99%
“…[36] and references therein, also [38]), for which the metric g ab reads, when we are much outside the Schwarzschild radius of the body,…”
Section: The Maximum Turn Around Radiusmentioning
confidence: 99%
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“…However, Edwin Hubble [11] in 1929, proved that the universe was indeed expanding. A single black hole of mass M immersed in a homogeneous isotropic fluid has a metric given by McVittie's solution [12,13]:…”
Section: Exact Analytic Solutions Of Einstein's Field Equationsmentioning
confidence: 99%
“…See e.g., Refs. [20][21][22][23][24][25][26][27][28] for mathematical investigations of the geometrical properties of McVittie metric. In Ref.…”
Section: Introductionmentioning
confidence: 99%