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Rotating Boson Star with Large Self-interaction in (2+1) dimensions

Kenji Sakamoto·Kiyoshi Shiraishi
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Abstract

Solutions for rotating boson stars in (2+1) dimensional gravity with a negative cosmological constant are obtained numerically. The mass, particle number, and radius of the (2+1) dimensional rotating boson star are shown. Consequently we find the region where the stable boson star can exist.

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Kenji Sakamoto, Kiyoshi Shiraishi. 1999-12-10. Rotating Boson Star with Large Self-interaction in (2+1) dimensions. https://doi.org/10.1103/physrevd.62.124014

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