Three Dimensional Gravity in the Presence of Scalar Fields

Tolga Birkandan; M. Hortaçsu

doi:10.1023/A:1022378101870

Three Dimensional Gravity in the Presence of Scalar Fields

Tolga Birkandan, M. Hortaçsu^*

^*Corresponding author for this work

Department of Physics Engineering

Istanbul Technical University

Research output: Contribution to journal › Article › peer-review

7 Citations (Scopus)

Abstract

We study a scalar field in curved space in three dimensions. We obtain a static perturbative solution and show that this solution satisfies the exact equations in the asymptotic region at infinity. The new solution gives rise to a singularity in the curvature scalar at the origin. Our solution, however, necessitates the excising the region near the origin, thus avoiding the naked singularity.

Original language	English
Pages (from-to)	457-466
Number of pages	10
Journal	General Relativity and Gravitation
Volume	35
Issue number	3
DOIs	https://doi.org/10.1023/A:1022378101870
Publication status	Published - Mar 2003

Funding

We thank very illuminating discussions with Professors Alikram Aliev and Nes¸e Özdemir. This work is partially supported by TUBITAK, the Scientific and Technical Research Council of Turkey. M.H. is also supported by TUBA, The Academy of Sciences of Turkey.

Funders	Funder number
Academy of Sciences of Turkey
TUBA
TUBITAK
Türkiye Bilimsel ve Teknolojik Araştirma Kurumu

Keywords

Blackholes
Choptuik formation
Singularity

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abstract = "We study a scalar field in curved space in three dimensions. We obtain a static perturbative solution and show that this solution satisfies the exact equations in the asymptotic region at infinity. The new solution gives rise to a singularity in the curvature scalar at the origin. Our solution, however, necessitates the excising the region near the origin, thus avoiding the naked singularity.",

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AB - We study a scalar field in curved space in three dimensions. We obtain a static perturbative solution and show that this solution satisfies the exact equations in the asymptotic region at infinity. The new solution gives rise to a singularity in the curvature scalar at the origin. Our solution, however, necessitates the excising the region near the origin, thus avoiding the naked singularity.

KW - Blackholes

KW - Choptuik formation

KW - Singularity

UR - https://www.scopus.com/pages/publications/0347128380

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EP - 466

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Three Dimensional Gravity in the Presence of Scalar Fields

Abstract

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Keywords

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