Static axionlike dark matter clouds around magnetized rotating wormholes -- probe limit case

Abstract

The problem of the distribution of axionlike particle, being the model of dark matter, in the nearby of rotating wormholes has been investigated numerically. In the model in question the axion scalar is non-trivially coupled to the Maxwell gauge field. We consider two toy models of rotating wormholes embedded in magnetic field, Kerr-like and Teo rotating wormholes. Moreover one assumes that the matter fields will not backreact on the wormhole spacetimes, i.e., we shall study the problem in the probe limit case. We point out the differences in the distribution of dark matter comparing to the location of it in the vicinity of rotating magnetized black holes.

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Cited by in corpus (6)

• Thermodynamics and evaporation of perfect fluid dark matter black hole in phantom background
• Influence of dark photon on magnetized and charged particle orbits around static spherically symmetric black hole
• Damour-Solodukhin Wormhole as a Black Hole Mimicker: The Role of Observers' Location
• Can synchrotron radiation reveal the presence of {\it dark sector} around black hole?
• Uniqueness of electrically and magnetically charged phantom wormholes
• Black hole dark monopole system