Self-similar cosmological solutions with dark energy. II: black holes, naked singularities and wormholes
| dc.creator | Maeda, Hideki | |
| dc.creator | Harada, Tomohiro | |
| dc.creator | Carr, B. J. | |
| dc.date | 2007-07-04 | |
| dc.date | 2008-01-02 | |
| dc.date.accessioned | 2026-07-07T11:17:29Z | |
| dc.date.available | 2026-07-07T11:17:29Z | |
| dc.description | We use a combination of numerical and analytical methods, exploiting the equations derived in a preceding paper, to classify all spherically symmetric self-similar solutions which are asymptotically Friedmann at large distances and contain a perfect fluid with equation of state $p=(γ-1)μ$ with $0<γ<2/3$. The expansion of the Friedmann universe is accelerated in this case. We find a one-parameter family of self-similar solutions representing a black hole embedded in a Friedmann background. This suggests that, in contrast to the positive pressure case, black holes in a universe with dark energy can grow as fast as the Hubble horizon if they are not too large. There are also self-similar solutions which contain a central naked singularity with negative mass and solutions which represent a Friedmann universe connected to either another Friedmann universe or some other cosmological model. The latter are interpreted as self-similar cosmological white hole or wormhole solutions. The throats of these wormholes are defined as two-dimensional spheres with minimal area on a spacelike hypersurface and they are all non-traversable because of the absence of a past null infinity. | |
| dc.description | 12 pages, 19 figures, 1 table, final version to appear in Physical Review D | |
| dc.identifier | https://arxiv.org/abs/0707.0530 | |
| dc.identifier | http://arxiv.org/abs/0707.0530 | |
| dc.identifier | Phys.Rev.D77:024023,2008 | |
| dc.identifier | doi:10.1103/PhysRevD.77.024023 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/193025 | |
| dc.subject | General Relativity and Quantum Cosmology | |
| dc.subject | Astrophysics | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | Self-similar cosmological solutions with dark energy. II: black holes, naked singularities and wormholes | |
| dc.type | text |