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arXiv · 1805.05382

Ultrarelativistic boost of a black hole in the magnetic universe of Levi-Civita--Bertotti--Robinson

Marcello Ortaggio·Marco Astorino
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Abstract

We consider an exact Einstein-Maxwell solution constructed by Alekseev and Garcia which describes a Schwarzschild black hole immersed in the magnetic universe of Levi-Civita, Bertotti and Robinson (LCBR). After reviewing the basic properties of this spacetime, we study the ultrarelativistic limit in which the black hole is boosted to the speed of light, while sending its mass to zero. This results in a non-expanding impulsive wave traveling in the LCBR universe. The wave front is a 2-sphere carrying two null point particles at its poles -- a remnant of the structure of the original static spacetime. It is also shown that the obtained line-element belongs to the Kundt class of spacetimes, and the relation with a known family of exact gravitational waves of finite duration propagating in the LCBR background is clarified. In the limit of a vanishing electromagnetic field, one point particle is pushed away to infinity and the single-particle Aichelburg-Sexl pp-wave propagating in Minkowski space is recovered.

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Marcello Ortaggio, Marco Astorino. 2018-05-14. Ultrarelativistic boost of a black hole in the magnetic universe of Levi-Civita--Bertotti--Robinson. https://doi.org/10.1103/physrevd.97.104052

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