Mechanism of classical wormhole formation
Determine the physical mechanism responsible for the formation of classical wormholes.
References
At the same time, the mouth of a wormhole can simulate the behavior of the event horizon of a black hole. Features of the observational characteristics of wormholes include characteristics of accretion disks , models of wormholes with a thin shell, the outer region of which is described by solutions for black holes , characteristics of gravitational lensing in both weak and strong field limits and wormhole shadows . Apart from these, there could be other distinctive properties of wormholes. For instance, wormholes resulting from the merger of two Schwarzschild black holes can emit gravitational waves . Such ring-down emissions can occur also from the perturbations of massive Ellis-Bronnikov wormholes .