Dynamical and thermodynamical stability of a charged thin-shell wormhole
| dc.contributor.author | Ernesto F. Eiroa | |
| dc.contributor.author | Griselda Figueroa-Aguirre | |
| dc.contributor.author | Miguel L. Peñafiel | |
| dc.contributor.author | Santiago Esteban Perez Bergliaffa | |
| dc.coverage.spatial | Bolivia | |
| dc.date.accessioned | 2026-03-22T14:58:29Z | |
| dc.date.available | 2026-03-22T14:58:29Z | |
| dc.date.issued | 2024 | |
| dc.description | Citaciones: 3 | |
| dc.description.abstract | Abstract A study of the dynamical and thermodynamical stability of a charged thin-shell wormhole built by gluing two Reissner–Nordström geometries is presented. The charge on the shell is linearly related to the matter content. For the dynamical stability, a concise inequality is obtained, valid for any barotropic equation of state that relates the pressure with the energy density at the throat. A thermodynamical description of the system is introduced, which leads to the temperature and the electric potentials. Adopting a linear equation of state for the pressure and a definite form for the entropy function, the set of equilibrium configurations that are both dynamically and thermodynamically stable is found. | |
| dc.identifier.doi | 10.1140/epjc/s10052-024-13465-3 | |
| dc.identifier.uri | https://doi.org/10.1140/epjc/s10052-024-13465-3 | |
| dc.identifier.uri | https://andeanlibrary.org/handle/123456789/49646 | |
| dc.language.iso | en | |
| dc.publisher | Springer Science+Business Media | |
| dc.relation.ispartof | The European Physical Journal C | |
| dc.source | Institute of Astronomy and Space Physics | |
| dc.subject | Wormhole | |
| dc.subject | Stability (learning theory) | |
| dc.subject | Shell (structure) | |
| dc.subject | Physics | |
| dc.subject | Statistical physics | |
| dc.subject | Materials science | |
| dc.subject | Classical mechanics | |
| dc.title | Dynamical and thermodynamical stability of a charged thin-shell wormhole | |
| dc.type | article |