On a Class of Harko-Kovacs-Lobo Wormholes

The Harko, Kovács, and Lobo wormhole (HKLWH) metric contains two free parameters: one is the throat r0, other a dimensionless deviation parameter γ with values 0<γ<1, latter ensuring needed violation of null energy condition at throat. In this paper, we study energetics HKLWH influence on tidal forces in Lorentz-boosted frame. Finally, apply new concept, namely, probabilistic identity object observed by different external observers terms Fresnel coefficients derived Tangherlini. intriguing result that observations can differ depending location observer, i.e., there nonzero probability will be identified as black hole even when γ≠0.