ANALYSIS OF THIN SHELL WORMHOLES DERIVED FROM KISELEV BLACK HOLES

E. W. Likta, N. Ibraham and M. A. Ramat

ABSTRACT

It is known that Einsten-Rosen Bridge is a specific solution of Einsten field equations a wormhole. Also shell is known as a three dimensional solid structural element that the thickness is very small and a thin shell have minor deformations relative to thickness that is tiny in relationto its other dimensions. Black holes are an area of space time with intense gravity that nothing can escape from its event horizon. General relativity solution described a black holes can expand when taking it mass from its surrounds once it has created. The goal of this paper focuses on to determine the outcomes of unstable wormhole, to identify the stable zone and to determine the single horizon. The method used is the Kiselev black hole. The result obtained is the derivation of thin shell wormholes from Kiselev black holes. The outcomes of the unstable wormholes have been observed. The stable zone has been identified. The single horizon has been achieved. 

Keywords: Kiselev, Black Holes, Thin shell, Wormholes and Energy