On static solutions of the Einstein - Scalar Field equations
Martin Reiris

TL;DR
This paper investigates static solutions of the Einstein-ScalarField equations across various dimensions, establishing conditions for their existence or non-existence based on the scalar potential and cosmological constant, with geometric estimates and classifications.
Contribution
It provides a comprehensive analysis of geodesically complete static solutions for different scalar potentials, including Klein-Gordon and cosmological constant cases, with new existence and non-existence results.
Findings
Geodesically complete solutions with Klein-Gordon potential are Ricci-flat and vacuum.
In three dimensions, only Minkowski or quotients exist for Klein-Gordon potential.
No solutions exist with positive cosmological constant; specific conditions apply for negative cosmological constant.
Abstract
In this article we study self-gravitating static solutions of the Einstein-ScalarField system in arbitrary dimensions. We discuss the existence and the non-existence of geodesically complete solutions depending on the form of the scalar field potential , and provide full global geometric estimates when the solutions exist. Our main results are summarised as follows. For the Klein-Gordon field, namely when , it is proved that geodesically complete solutions have Ricci-flat spatial metric, have constant lapse and are vacuum, (that is is constant and equal to zero if ). In particular, when the spatial dimension is three, the only such solutions are either Minkowski or a quotient thereof (no nontrivial solutions exist). When , that is, when a vacuum energy or a cosmological constant is included, it is proved…
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