Gravitational Cheshire effect: Nonminimally coupled scalar fields may not curve spacetime
| dc.creator | Ayón-Beato, Eloy | |
| dc.creator | Martínez, Cristián | |
| dc.creator | Troncoso, Ricardo | |
| dc.creator | Zanelli, Jorge | |
| dc.date | 2005-05-10 | |
| dc.date | 2005-06-07 | |
| dc.date.accessioned | 2026-07-07T04:18:19Z | |
| dc.date.available | 2026-07-07T04:18:19Z | |
| dc.description | It is shown that flat spacetime can be dressed with a real scalar field that satisfies the nonlinear Klein-Gordon equation without curving spacetime. Surprisingly, this possibility arises from the nonminimal coupling of the scalar field with the curvature, since a footprint of the coupling remains in the energy-momentum tensor even when gravity is switched off. Requiring the existence of solutions with vanishing energy-momentum tensor fixes the self-interaction potential as a local function of the scalar field depending on two coupling constants. The solutions describe shock waves and, in the Euclidean continuation, instanton configurations in any dimension. As a consequence of this effect, the tachyonic solutions of the free massive Klein-Gordon equation become part of the vacuum. | |
| dc.description | 8 pages, 1 figure, CECS style; small changes to match published version, title changed by journal | |
| dc.identifier | https://arxiv.org/abs/hep-th/0505086 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0505086 | |
| dc.identifier | Phys.Rev. D71 (2005) 104037 | |
| dc.identifier | doi:10.1103/PhysRevD.71.104037 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/53130 | |
| dc.subject | High Energy Physics - Theory | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.title | Gravitational Cheshire effect: Nonminimally coupled scalar fields may not curve spacetime | |
| dc.type | text |