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

TL;DR

This paper explores the possibility that active galactic nuclei are wormholes emitting distinctive gamma radiation from colliding accreting flows, proposing a method to identify wormholes through their unique radiation signatures.

Contribution

It introduces a hypothesis that AGNs could be wormholes and suggests gamma radiation from colliding flows as a distinctive observational signature.

Findings

Wormholes may emit unique gamma radiation spectra.

Such radiation differs from typical AGN jets or disks.

Observation of this radiation could confirm wormhole existence.

Abstract

The underlying hypothesis of this work is that the active galactic nuclei (AGNs) are wormhole mouths rather than supermassive black holes (SMBHs). 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 disks of AGNs. An observation of such radiation would serve as evidence of the existence of wormholes.