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Efficiency of magnetic Penrose process in higher dimensional Myers-Perry black hole spacetimes

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arxiv 2402.02471 v2 pith:MVKZRV26 submitted 2024-02-04 gr-qc

classification gr-qc
keywords efficiencyenergyblackholesdimensionalextractionhigherrotations
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abstract

In this paper, we consider a well-established magnetic Penrose process (MPP) and bring out its impact on the efficiency of energy extraction from higher dimensional (i.e., $D>4$) black holes. We derive the field equations of motion and determine the expressions for the energy efficiency of energy extraction for the case of higher dimensional black holes. We also examine the efficiency of energy extraction from black holes with $(n-1)$ and $n$ rotations. We demonstrate that black holes with $(n-1)$ rotations has only one horizon, resulting in infinitely large energy efficiency even without MPP. On the other hand, for black holes with $n$ rotations in $D>4$, the energy efficiency is not infinitely large, but the efficiency can be significantly enhanced by MPP. This enhancement allows for arbitrarily large energy efficiency. We find that the efficiency of energy extraction can exceed over $>100\%$ for $D=5,6$ and $D=7,8$ dimensions. Interestingly, for rotation parameters near the extremal value, the energy efficiency remains above $100 \%$ in $D=7,8$ compared to $D=5,6$. MPP can eventually make higher dimensional black holes more efficient even with $n$ rotations.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Extending the Comisso-Asenjo Energy Extraction Mechanism to Pure Lovelock Gravity

    gr-qc 2026-07 conditional novelty 4.0 of 10

    For rotating pure Lovelock black holes in 6–9 dimensions, magnetic reconnection extracts more rotational energy as dimension grows, with the 9-dimensional case most efficient and sometimes outpacing the Blandford-Znaj...

  2. Gravitational wave signatures of magnetized Ernst black hole

    gr-qc 2026-07 conditional novelty 4.0 of 10

    Magnetic fields in the Ernst black-hole spacetime alter zoom-whirl EMRI waveforms, spectra, and characteristic strain in ways the authors claim LISA-class detectors could probe.

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