Abstract:We establish new existence results for the Einstein constraint equations for mean extrinsic curvature arbitrarily far from constant. The results hold for rescaled background metric in the positive Yamabe class, with freely specifiable parts of the data sufficiently small, and with matter energy density not identically zero. Two technical advances make these results possible: A new topological fixed-point argument without smallness conditions on spatial derivatives of the mean extrinsic curvature, and a new glo… Show more
“…In this paper, we prove a far-from-CMC result similar to [15,20,21,29] for the conformal Einstein-scalar field constraint equations on compact Riemannian manifolds with positive (modified) Yamabe invariant.
…”
supporting
confidence: 53%
“…This assumption however will turn out to be very important in our analysis and plays a role analog to the assumption that the metric g has positive Yamabe invariant in [20,21,29]. Another important assumption we will need is that (M, g) has no non-zero conformal Killing vector field.…”
Section: Acknowledgementsmentioning
confidence: 98%
“…In this section, we adapt the method of [20,21,29] to our context. The first step is to prove an existence result for solutions to the Lichnerowicz equation.…”
Section: An Implicit Function Argumentmentioning
confidence: 99%
“…It was only in 2008 that Holst, Nagy and Tsogtgerel found a method to construct solutions to the equations of the conformal method with arbitrarily prescribed mean curvature. See [20,21]. The method was then extended by Maxwell [29] to the vacuum case.…”
ABSTRACT. In this paper, we prove a far-from-CMC result similar to [15,20,21,29] for the conformal Einstein-scalar field constraint equations on compact Riemannian manifolds with positive (modified) Yamabe invariant.
“…In this paper, we prove a far-from-CMC result similar to [15,20,21,29] for the conformal Einstein-scalar field constraint equations on compact Riemannian manifolds with positive (modified) Yamabe invariant.
…”
supporting
confidence: 53%
“…This assumption however will turn out to be very important in our analysis and plays a role analog to the assumption that the metric g has positive Yamabe invariant in [20,21,29]. Another important assumption we will need is that (M, g) has no non-zero conformal Killing vector field.…”
Section: Acknowledgementsmentioning
confidence: 98%
“…In this section, we adapt the method of [20,21,29] to our context. The first step is to prove an existence result for solutions to the Lichnerowicz equation.…”
Section: An Implicit Function Argumentmentioning
confidence: 99%
“…It was only in 2008 that Holst, Nagy and Tsogtgerel found a method to construct solutions to the equations of the conformal method with arbitrarily prescribed mean curvature. See [20,21]. The method was then extended by Maxwell [29] to the vacuum case.…”
ABSTRACT. In this paper, we prove a far-from-CMC result similar to [15,20,21,29] for the conformal Einstein-scalar field constraint equations on compact Riemannian manifolds with positive (modified) Yamabe invariant.
“…One motivation for that study was to examine the uniqueness of solutions in the far-fromconstant mean curvature regime now that existence results for this case exist (see [8], [14]). He found interesting non-existence and non-uniqueness results showing that the constraints are ill-posed beyond the non-uniqueness that is introduced when one couples the lapse fixing equation to the four constraint equations, as in the extended conformal thin sandwich (XCTS) formulation (see [15], [2], [19]) and some constrained evolution schemes (see [16], [6] for a resolution of this scaling problem).…”
We study the stability of solution branches for the Lichnerowicz-York equation at moment of time symmetry with constant unscaled energy density. We prove that the weakfield lower branch of solutions is stable whilst the upper branch of strong-field solutions is unstable. The existence of unstable solutions is interesting since a theorem by Sattinger proves that the sub-super solution monotone iteration method only gives stable solutions.
We construct large classes of vacuum general relativistic initial data sets, possibly with a cosmological constant Λ ∈ R, containing ends of cylindrical type.
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