The Einstein-scalar field constraints on asymptotically Euclidean manifolds

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dc.creatorChoquet-Bruhat, Yvonne
dc.creatorIsenberg, James
dc.creatorPollack, Daniel
dc.date2005-06-20
dc.date.accessioned2026-07-07T03:29:47Z
dc.date.available2026-07-07T03:29:47Z
dc.descriptionWe use the conformal method to obtain solutions of the Einstein-scalar field gravitational constraint equations. Handling scalar fields is a bit more challenging than handling matter fields such as fluids, Maxwell fields or Yang-Mills fields, because the scalar field introduces three extra terms into the Lichnerowicz equation, rather than just one. Our proofs are constructive and allow for arbitrary dimension (>2) as well as low regularity initial data.
dc.description31 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0506101
dc.identifierhttp://arxiv.org/abs/gr-qc/0506101
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35316
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectDifferential Geometry
dc.titleThe Einstein-scalar field constraints on asymptotically Euclidean manifolds
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