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Particle Acceleration on the Background of the Kerr-Taub-NUT Spacetime · Around

2010

Particle Acceleration on the Background of the Kerr-Taub-NUT Spacetime

Liu, Changqing, Chen, Songbai, Ding, Chikun et al.

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We study the collision of two particles with the different rest masses moving in the equatorial plane of a Kerr-Taub-NUT spacetime and get the center-of-mass (CM) energy for the particles.

We find that the CM energy depends not only on the rotation parameter, $a$, but also on the NUT charge of the Kerr-Taub-NUT spacetime, $n$.
Especially, for the extremal Kerr-Taub-NUT spacetime, an unlimited CM energy can be approached if the parameter $a$ is in the range $[1,\sqrt{2}]$, which is different from that of the Kerr and Kerr-Newman black holes.

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