The Campanelli-Lousto and veiled spacetimes
Luciano Vanzo, Sergio Zerbini (University of Trento, INFN, Trento), Valerio Faraoni (Bishop's University)

TL;DR
This paper reexamines the Campanelli-Lousto solutions in Brans-Dicke theory, revealing they can represent wormholes or naked singularities depending on parameters, and discusses implications for conformal transformations in spacetime interpretations.
Contribution
It clarifies the physical nature of Campanelli-Lousto solutions and explores their conformal counterparts, highlighting caution in interpreting conformally related spacetimes.
Findings
Campanelli-Lousto solutions can describe wormholes or naked singularities.
The veiled Schwarzschild metric is a special case of the CL metric.
Conformal transformations can alter the physical interpretation of solutions.
Abstract
The Campanelli-Lousto solutions of Brans-Dicke theory, usually reported as black holes are reconsidered and shown to describe, according to the values of a parameter, wormholes or naked singularities. The veiled Schwarzschild metric recently used as an example to discuss conformal frames and their equivalence corresponds to a special case of the CL metric. The conformal cousins of these solutions, and of the Riegert black hole solution of conformally invariant Weyl theory, are analysed, leading to a word of caution when interpreting physically spacetimes generated via conformal transformations from known seed solutions.
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