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Jordan-frame reconstruction of Einstein-Rosen-type geometries in generalized Brans-Dicke theory

László Árpád Gergely1,2,*, Bence Racskó1, and Kata Karácsonyi1,2

  • *Contact author: gergely.laszlo@wigner.hu

Phys. Rev. D 114, 104023 – Published 6 November, 2026

DOI: https://doi.org/10.1103/v1f8-cwtp

Abstract

We investigate vacuum generalized Brans-Dicke theory with scalar-dependent coupling ω(ϕ) in an Einstein-Rosen-type metric. Let W be the area density of the two-dimensional Killing orbits, ϕ the Brans-Dicke scalar, and Ω=Wϕ their composite area density. On regions where the gradient of Ω is non-null, we impose W=W(ϕ) and local invertibility of Ω(ϕ). The scalar equation admits the exact first integral (3+2ω)[(Ω/ϕ)(dϕ/dΩ)]2=κ, where κ is a signed integration constant, giving direct and inverse reconstruction of the coupling. For ϕ=b(Ω/Ω*)aeqΩ one obtains 3+2ω=κ/(a+qΩ)2. The choices Ω=ρ and Ω=t define the spacelike- and timelike-gradient branches, each yielding a closed exact solution family. Their mode functions obey the cylindrical Einstein-Rosen and Euler-Poisson-Darboux equations, respectively. In the Einstein frame the normalized scalar is σ=σ0+|κ|ln(Ω/Ω0), while q cancels from the metric. In the spacelike branch the scalar contributes to the radial C-energy profile separately from the tensor flux, and the reconstructed smooth-mode class has no curvature-regular axis. In the static subclass, q=0 reproduces the circular-speed law of a singular isothermal dark-matter halo, while q<0 gives a local correspondence with the rising inner NFW rotation curve. The homogeneous timelike subclass is locally Bianchi I, reduces in the Einstein frame to an exact scalar-Kasner geometry, and has a Jordan-frame effective Planck mass that evolves monotonically with Jordan-frame comoving proper time on each connected time interval on which the reconstructed scalar profile is locally invertible.

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