Outgoing electromagnetic flux from rotating wormholes
Abstract We show for the first time that rotating wormholes are capable of emitting a Poynting flux in the process of accreting magnetized matter. To this end, we analyze the Damour–Solodukhin metric describing a Kerr-type wormhole and calculate the electromagnetic flux assuming a specific geometry...
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          | Main Authors: | , , | 
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| Format: | Article | 
| Language: | English | 
| Published: | SpringerOpen
    
        2024-11-01 | 
| Series: | European Physical Journal C: Particles and Fields | 
| Online Access: | https://doi.org/10.1140/epjc/s10052-024-13563-2 | 
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| Summary: | Abstract We show for the first time that rotating wormholes are capable of emitting a Poynting flux in the process of accreting magnetized matter. To this end, we analyze the Damour–Solodukhin metric describing a Kerr-type wormhole and calculate the electromagnetic flux assuming a specific geometry for the magnetic field contained by the wormhole ergosphere. We find that for highly rotating wormholes a mechanism similar to that of Blandford and Znajek is possible, and the emitted electromagnetic flux is of the same order as for a Kerr black hole. | 
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| ISSN: | 1434-6052 | 
 
       