Counterrotational effects on stability of 2+1-dimensional thin-shell wormholes

In this paper we choose our throat geometry in the 2 + 1- dimensional TSW such that the pressure vanishes, the energy density becomes positive, and as a result all energy condi-

3 Stability of the thin-shell wormhole against a linear perturbation Recently, we have generalized the stability of TSWs in cylindrical symmetric bulks in [37].. Here we apply the

(24) that negative energy density violates the WEC, and consequently we are in need of the exotic matter for constructing thin-shell WH.... By changing the values of l

We construct a charged, regular extension of the BTZ black hole solution by employing nonlinear Born-Infeld elec- trodynamics, supplemented with the Hoffmann term and gluing

In this paper, we have studied a thin-shell traversable wormhole with rotation in five dimensions constructed using a Myers-Perry black hole with cosmological constants using

From this token, we wish to consider a general class of cylindrically symmetric spacetimes in which the metric functions depend only on the radial function r to construct TSWs..

To conclude this chapter we would like to add that using the thin-shell formalism and the Israel junction conditions we established a dynamic spherical symmetric timelike

Chapter two: We have investigated the possibility of thin-shell wormholes in EYMGB theory in higher (d ≥ 5) dimensions with particular emphasis on stability against spherical,