  The existence of even the simplest magnetized wormholes may lead to
observable consequences. In the case where both the wormhole and the magnetic
field around its mouths are static and spherically symmetric, and gas in the
region near the wormhole falls radially into it, the former's spectrum contains
bright cyclotron or synchrotron lines due to the interaction of charged plasma
particles with the magnetic field. At the same time, due to spherical symmetry,
the radiation is non-polarized. The emission of this just-described exotic type
(non-thermal, but non-polarized) may be a wormhole signature. Also, in this
scenario, the formation of an accretion disk is still quite possible at some
distance from the wormhole, but a monopole magnetic field could complicate this
process and lead to the emergence of asymmetrical and one-sided relativistic
jets.
