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Bertotti-Robinson and Melvin Spacetimes

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arxiv 1109.1535 v1 pith:P5N2FXJL submitted 2011-09-07 gr-qc

classification gr-qc
keywords bertotti-robinsonmelvinspacetimesconjecturediscussedformulatedsimilaritiesuniqueness
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Similarities between the Melvin and Bertotti-Robinson spacetimes are discussed and a uniqueness conjecture is formulated.

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Cited by 1 Pith paper

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  1. Optical Characteristics of the Kerr-Bertotti-Robinson Black Hole

    gr-qc 2025-08 conditional novelty 6.0 of 10

    For the Kerr-Bertotti-Robinson black hole, the magnetic field mainly enlarges the shadow and Einstein ring while rotation mainly distorts the shadow shape, and current M87* and Sgr A* data give only weak bounds on the field.

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