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

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.

14 pages, 6 figures, RevTeX

References in corpus (5)

• Localizing Gravity on a String-Like Defect in Six Dimensions
• Solving the Hierarchy Problem with Noncompact Extra Dimensions
• Nonsingular global string compactifications
• Warp Factors and Extended Sources in Two Transverse Dimensions
• Polytropic stars in three-dimensional spacetime

Cited by in corpus (4)

• TOPICAL REVIEW: General relativistic boson stars
• Rotating Boson Stars in 2+1 Dimensions
• Q-stars in 2+1 dimensions
• Non-topological soliton in three-dimensional supergravity