2005
DOI: 10.4310/atmp.2005.v9.n1.a3
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A gluing construction for non-vacuum solutions of the Einstein-constraint equations

Abstract: We extend the conformal gluing construction of [18] by establishing an analogous gluing result for field theories obtained by minimally coupling Einstein's gravitational theory with matter fields. We treat classical fields such as perfect fluids and the Yang-Mills equations as well as the Einstein-Vlasov system, which is an important example coming from kinetic theory. In carrying out these extensions, we extend the conformal gluing technique to higher dimensions and codify it in such a way as to make more tra… Show more

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Cited by 45 publications
(60 citation statements)
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“…This deformation is done so that we are in the setting in which a generalization of the gluing theorem of [2] to compact manifolds with boundary (and to include matter fields) may be applied. This constitutes the third step in the construction and is essentially done by repeating the arguments of [2,10] in this new setting. We thus obtain a one parameter family of initial data which satisfies the constraint equations, and which contains a neck connecting the spheres S(p a , r).…”
Section: The Constructionmentioning
confidence: 99%
“…This deformation is done so that we are in the setting in which a generalization of the gluing theorem of [2] to compact manifolds with boundary (and to include matter fields) may be applied. This constitutes the third step in the construction and is essentially done by repeating the arguments of [2,10] in this new setting. We thus obtain a one parameter family of initial data which satisfies the constraint equations, and which contains a neck connecting the spheres S(p a , r).…”
Section: The Constructionmentioning
confidence: 99%
“…[1] A justification for this way of specifying initial data for perfect fluids is presented in Section 4.1 of [32].…”
Section: Acknowledgmentsmentioning
confidence: 99%
“…Theorems 1.1 and 1.4 are established in Section 4. The proofs are a mixture of gluing techniques developed in [17][18][19] and those of [12][13][14]. In fact, the proof proceeds via a generalisation of the analysis in [18,19] to compact manifolds with boundary; this is carried through in Section 2 in vacuum with cosmological constant Λ = 0, and in Section 3 with matter and Λ ∈ R. These results may be of independent interest.…”
Section: Introductionmentioning
confidence: 99%
“…Although the paper [18] only treats the case n = 3, since the generalization to higher dimensions is not difficult (the necessary modifications are discussed in [17]), we work here in general dimension n ≥ 3. We begin with an initial data set (M ,γ,K) whereM has non-empty smooth boundary ∂M and we assume first thatK has constant traceτ = trγK (i.e., these are constant mean curvature, or CMC, initial data sets).…”
Section: Introductionmentioning
confidence: 99%