Analysis of stability in wormholes under scalar-tensor theories, revealing conditions for stability.
In our previous papers we have analyzed the stability of vacuum and electrovacuum static, spherically symmetric space-times in the framework of the Bergmann-Wagoner-Nordtvedt class of scalar-tensor theories (STT) of gravity. In the present paper, we continue this study by examining the stability of exceptional solutions of the Brans-Dicke theory with the coupling constant $ω=0$ that were not covered in the previous studies. Such solutions describe neutral or charged wormholes and involve a conformal continuation: the standard conformal transformation maps the whole Einstein-frame manifold ME to only a part of the Jordan-frame manifold MJ, which has to be continued beyond the emerging regular boundary S, and the new region maps to another manifold ME-. The metric in MJ is symmetric with respect to S only if the charge q is zero. Our stability study concerns radial (monopole) perturbations, and it is shown that the wormhole is stable if q ≠ 0 and unstable only in the symmetric case $q=0$
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Бронников et al. (2025) studied this question.
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