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Rotating Bowen-York initial data with a positive cosmological constant

Abstract

A generalization of the Bowen-York initial data to the case with a positive cosmological constant is investigated. We follow the construction presented recently by Bizo\'n, Pletka and Simon, and solve numerically the Lichnerowicz equation on a compactified domain S1Ă—S2\mathbb S^1 \times \mathbb S^2. In addition to two branches of solutions depending on the polar variable on S2\mathbb S^2 that were already known, we find branches of solutions depending on two variables: the polar variable on S2\mathbb S^2 and the coordinate on S1\mathbb S^1. Using Vanderbauwhede's results concerning bifurcations from symmetric solutions, we show the existence of the corresponding bifurcation points. By linearizing the Lichnerowicz equation and solving the resulting eigenvalue problem, we collect numerical evidence suggesting the absence of additional branches of solutions.Comment: 24 pages, 9 figure

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