a multiply-connected space–time structure, where two distant regions were linked by a tunnel, namely, the geon. Furthermore, Misner and Wheeler conducted a series of research projects on differential geometry and abstract topology in physics. In their 1957 paper [@46], they introduced the term “wormhole” for the first time. During the following 30 years, the wormhole field lay dormant once again, except for Bronnikov’s tunnel-like solutions [@47] and Ellis’s drainhole [@48; @49]. In 1988, a new era of wormhole physics was opened by Morris and Thorne in light of their milestone paper [@50], where they analyzed in detail the construction of the wormhole, energy conditions, time machines, the stability problem, and traversabilities of wormholes. In succession, Visser and Possion introduced the interesting “thin-shell wormhole” by conjecturing that all the “exotic matter” is confined to a thin shell between universes [@51; @52; @53; @54]. Because of the discovery of the late-time acceleration of the universe in 1998, a great deal of related research about wormholes has been motivated by developments of various kinds of phantom-like dynamical dark energy scenarios or MOG scenarios [@55; @56]. Subsequently, for the first time, we investigated traversable wormholes constrained by modern astrophysical observations [@57; @58; @59]. This 