Shadows of generalized Hayward spacetimes are computed in vacuum and plasma, and EHT Sgr A* constraints favor wormholes with multi-peak effective potentials over single-peak ones.
Bardeen presented at GR5, Tiflis, U.S.S.R., and published in the conference proceedings in the U.S.S.R
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Shadows of generalised Hayward spacetimes : in vacuum and with plasma
Shadows of generalized Hayward spacetimes are computed in vacuum and plasma, and EHT Sgr A* constraints favor wormholes with multi-peak effective potentials over single-peak ones.