• Open Access

Compact, charged boson stars and shells in the CPN gravitating nonlinear sigma model

Nobuyuki Sawado and Shota Yanai
Phys. Rev. D 102, 045007 – Published 6 August 2020

Abstract

We study U(1) gauged gravitating compact Q-ball, Q-shell solutions in a nonlinear sigma model with the target space CPN. The models with odd integer N and a special potential can be parameterized by Nth complex scalar fields and they support compact solutions. By implementing the U(1) gauge field in the model, the behavior of the solutions becomes complicated than the global model. Especially, they have branches, i.e., two independent solutions with the same shooting parameter. The energy of the solutions in the first branch behaves as EQ5/6 for small Q, where Q stands for the U(1) Noether charge. For the large Q, it gradually deviates from the scaling EQ5/6 and, for the Q-shells it is EQ7/6, which forms the second branch. A coupling with gravity allows for harboring of the Schwarzschild black holes for the Q-shell solutions, forming the charged boson shells. The space-time then consists of a charged black hole in the interior of the shell, surrounded by a Q-shell, and the outside becomes a Reissner-Nordström space-time. These solutions inherit the scaling behavior of the flat space-time.

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  • Received 10 June 2020
  • Accepted 27 July 2020

DOI:https://doi.org/10.1103/PhysRevD.102.045007

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Nobuyuki Sawado* and Shota Yanai

  • Department of Physics, Tokyo University of Science, Noda, Chiba 278-8510, Japan

  • *sawadoph@rs.tus.ac.jp
  • phyana0513@gmail.com

Article Text

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Issue

Vol. 102, Iss. 4 — 15 August 2020

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