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Search for wormhole candidates in active galactic nuclei: radiation from colliding accreting flows

M. Yu. PiotrovichCentral Astronomical Observatory at Pulkovo, 196140 Saint-Petersburg, RussiaS. KrasnikovCentral Astronomical Observatory at Pulkovo, 196140 Saint-Petersburg, RussiaS. D. BuligaCentral Astronomical Observatory at Pulkovo, 196140 Saint-Petersburg, RussiaT. M. NatsvlishviliCentral Astronomical Observatory at Pulkovo, 196140 Saint-Petersburg, Russia
2020en
ABI

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ABSTRACT The underlying hypothesis of this work is that the active galactic nuclei (AGNs) are wormhole mouths rather than supermassive black holes. Under some – quite general – assumptions such wormholes may emit gamma radiation as a result of a collision of accreting flows inside the wormholes. This radiation has a distinctive spectrum much different from those of jets or accretion discs of AGNs. An observation of such radiation would serve as evidence of the existence of wormholes.

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