Rotating boson stars with large self-interaction in 2+1 dimensions

Kenji Sakamoto and Kiyoshi Shiraishi
Phys. Rev. D 62, 124014 – Published 22 November 2000
PDFExport Citation
Abstract
Authors
References

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.

  • Received 18 July 2000

DOI:https://doi.org/10.1103/PhysRevD.62.124014

©2000 American Physical Society

Authors & Affiliations

Kenji Sakamoto*

  • Graduate School of Science and Engineering, Yamaguchi University, Yoshida, Yamaguchi-shi, Yamaguchi 753-8512, Japan
  • Institute of Particle and Nuclear Studies, High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan

Kiyoshi Shiraishi†

  • Graduate School of Science and Engineering, Yamaguchi University, Yoshida, Yamaguchi-shi, Yamaguchi 753-8512, Japan
  • Faculty of Science, Yamaguchi University, Yoshida, Yamaguchi-shi, Yamaguchi 753-8512, Japan

  • *Email address: b1795@sty.cc.yamaguchi-u.ac.jp, saka@ccthmail.kek.jp
  • †Email address: shiraish@sci.yamaguchi-u.ac.jp

References (Subscription Required)

Click to Expand
Issue

Vol. 62, Iss. 12 — 15 December 2000

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required

Log In
Other Options
×

Download & Share

PDFExportReuse & PermissionsCiting Articles (3)
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Log In

Cancel
×

Search

Article Lookup

Paste a citation or DOI
Enter a citation
×