On the stability of exceptional Brans–Dicke wormholes

Abstract 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 $$\omega =0$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>ω</mml:mi> <mml:mo>=</mml:mo> <mml:mn>0</mml:mn> </mml:mrow> </mml:math> 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 $${\mathbb {M}}_\textrm{E}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>M</mml:mi> <mml:mtext>E</mml:mtext> </mml:msub> </mml:math> to only a part of the Jordan-frame manifold $${\mathbb {M}}_\textrm{J}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>M</mml:mi> <mml:mtext>J</mml:mtext> </mml:msub> </mml:math> , which has to be continued beyond the emerging regular boundary S, and the new region maps to another manifold $${\mathbb {M}}_\textrm{E}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>M</mml:mi> <mml:mtext>E</mml:mtext> </mml:msub> </mml:math> $${}_{-}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mo>-</mml:mo> <mml:mrow/> </mml:mmultiscripts> </mml:math> . The metric in $${\mathbb {M}}_\textrm{J}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>M</mml:mi> <mml:mtext>J</mml:mtext> </mml:msub> </mml:math> 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 $$q \ne 0$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>q</mml:mi> <mml:mo>≠</mml:mo> <mml:mn>0</mml:mn> </mml:mrow> </mml:math> and unstable only in the symmetric case $$q=0$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>q</mml:mi> <mml:mo>=</mml:mo> <mml:mn>0</mml:mn> </mml:mrow> </mml:math> .

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Publication Details

Journal
The European Physical Journal C
Published
2025-09-25
DOI
https://doi.org/10.1140/epjc/s10052-025-14794-7
Citations
1
Primary Topic
Geometric Analysis and Curvature Flows
Type
article
Field-Weighted Citation Impact
3.73

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article

On the stability of exceptional Brans–Dicke wormholes

S. V. Bolokhov, К. А. Бронников, M. V. Skvortsova, Rustam Ibadov et al.
1 citations
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article

On the stability of exceptional Brans–Dicke wormholes

S. V. Bolokhov, К. А. Бронников, M. V. Skvortsova, Rustam Ibadov, Feruza Y. Shaymanova
article en
1 citations

Abstract

Abstract 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 $$\omega =0$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>ω</mml:mi> <mml:mo>=</mml:mo> <mml:mn>0</mml:mn> </mml:mrow> </mml:math> 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 $${\mathbb {M}}_\textrm{E}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>M</mml:mi> <mml:mtext>E</mml:mtext> </mml:msub> </mml:math> to only a part of the Jordan-frame manifold $${\mathbb {M}}_\textrm{J}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>M</mml:mi> <mml:mtext>J</mml:mtext> </mml:msub> </mml:math> , which has to be continued beyond the emerging regular boundary S, and the new region maps to another manifold $${\mathbb {M}}_\textrm{E}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>M</mml:mi> <mml:mtext>E</mml:mtext> </mml:msub> </mml:math> $${}_{-}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mmultiscripts> <mml:mrow/> <mml:mo>-</mml:mo> <mml:mrow/> </mml:mmultiscripts> </mml:math> . The metric in $${\mathbb {M}}_\textrm{J}$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:msub> <mml:mi>M</mml:mi> <mml:mtext>J</mml:mtext> </mml:msub> </mml:math> 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 $$q \ne 0$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>q</mml:mi> <mml:mo>≠</mml:mo> <mml:mn>0</mml:mn> </mml:mrow> </mml:math> and unstable only in the symmetric case $$q=0$$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mrow> <mml:mi>q</mml:mi> <mml:mo>=</mml:mo> <mml:mn>0</mml:mn> </mml:mrow> </mml:math> .

The European Physical Journal CVol. 85(9)
Peoples' Friendship University of Russia (RU), Samarkand State University named after Sharof Rashidov (UZ), National metrology institute VTT MIKES (FI), Karshi State University (UZ), Institute of Anthropology and Ethnography (RU), Federal Research Centre «Fundamentals of Biotechnology» of the Russian Academy of Sciences (RU), National Research Nuclear University MEPhI (RU)
RUDN University
Openalex Percentile: Top 7%
Geometric Analysis and Curvature Flows
3.73
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