Braking--Radiation: An Energy Source for a Relativistic Fireball
C. Barrabes, P. A. Hogan

TL;DR
The paper shows that a moving black hole suddenly stopping emits a spherical shell of radiation with energy equal to its initial kinetic energy, observable as a relativistic fireball.
Contribution
It introduces a novel mechanism where a moving black hole's sudden halt produces a spherical relativistic fireball with energy matching its initial kinetic energy.
Findings
A moving black hole's sudden stop results in a spherical radiative shell.
The emitted energy equals the black hole's initial kinetic energy.
This process creates a relativistic fireball observable from afar.
Abstract
If the Schwarzschild black-hole is moving rectilinearly with uniform 3-velocity and suddenly stops, according to a distant observer, then we demonstrate that this observer will see a spherical light--like shell or "relativistic fireball" radiate outwards with energy equal to the original kinetic energy of the black-hole.
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