From the Janis-Newman-Winicour naked singularities to Einstein-Maxwell phantom wormholes
Changjun Gao, Jianhui Qiu

TL;DR
This paper explores the relationships between Janis-Newman-Winicour naked singularities, wormholes, and dilaton black holes, revealing that certain parameter choices lead to physically forbidden solutions, thus questioning their physical viability.
Contribution
It establishes connections between naked singularities, wormholes, and dilaton black holes through complex transformations and parameter analysis, clarifying the physical meaning of key parameters.
Findings
Janis-Newman-Winicour solution relates to dilaton black holes with negative mass.
Wormhole solutions are derived from naked singularities via complex transformations.
Certain parameter values imply physically forbidden negative mass black holes.
Abstract
The Janis-Newman-Winicour spacetime corresponds to a static spherically symmetric solution of Einstein equations with the energy momentum tensor of a massless quintessence field. It is understood that the spacetime describes a naked singularity. The solution has two parameters, and . To our knowledge, the exact physical meaning of the two parameters is still unclear. In this paper, starting from the Janis-Newman-Winicour naked singularity solution, we first obtain a wormhole solution by a complex transformation. Then let the parameter approaching infinity, we obtain the well-known exponential wormhole solution. After that, we embed both the Janis-Newman-Winicour naked singularity and its wormhole counterpart in the background of de Sitter or anti-de Sitter Universe with the energy momentum tensor of massive quintessence and massive phantom fields, respectively. To our…
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Taxonomy
TopicsRelativity and Gravitational Theory
