Thin-shell wormholes from the regular Hayward black hole

M. Halilsoy, A. Ovgun, S. Habib Mazharimousavi

Resultado de la investigación: Contribución a una revistaArtículorevisión exhaustiva

83 Citas (Scopus)

Resumen

We revisit the regular black hole found by Hayward in (Formula presented.)-dimensional static, spherically symmetric spacetime. To find a possible source for such a spacetime we resort to the nonlinear electrodynamics in general relativity. It is found that a magnetic field within this context gives rise to the regular Hayward black hole. By employing such a regular black hole we construct a thin-shell wormhole for the case of various equations of state on the shell. We abbreviate a general equation of state by (Formula presented.) where (Formula presented.) is the surface pressure which is a function of the mass density (Formula presented.). In particular, linear, logarithmic, Chaplygin, etc. forms of equations of state are considered. In each case we study the stability of the thin shell against linear perturbations. We plot the stability regions by tuning the parameters of the theory. It is observed that the role of the Hayward parameter is to make the TSW more stable. Perturbations of the throat with small velocity condition are also studied. The matter of our TSWs, however, remains exotic.

Idioma originalInglés
Número de artículo2796
Páginas (desde-hasta)1-7
Número de páginas7
PublicaciónEuropean Physical Journal C
Volumen74
N.º3
DOI
EstadoPublicada - 13 mar. 2014
Publicado de forma externa

Huella

Profundice en los temas de investigación de 'Thin-shell wormholes from the regular Hayward black hole'. En conjunto forman una huella única.

Citar esto