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Research PaperResearchia:202608.31017

Finite-domain inverse reconstruction of a Morris--Thorne-type wormhole candidate with a derivative-consistent $f(R)$ curvature sector

Murat Metehan Türkoğlu

Abstract

We present a finite-domain inverse reconstruction of a Morris--Thorne-type wormhole candidate as a methodological benchmark for constrained numerical model building in modified gravity. The throat condition and local flare-out behaviour are embedded analytically in the shape-function parameterization, while the redshift profile is kept finite by construction. Rather than fitting $f(R)$, $f_R(R)$, and $f_{RR}(R)$ as independent numerical arrays, a positive analytic generator is assigned to $f_{RR...

Submitted: August 31, 2026Subjects: Physics; Physics

Description / Details

We present a finite-domain inverse reconstruction of a Morris--Thorne-type wormhole candidate as a methodological benchmark for constrained numerical model building in modified gravity. The throat condition and local flare-out behaviour are embedded analytically in the shape-function parameterization, while the redshift profile is kept finite by construction. Rather than fitting f(R)f(R), fR(R)f_R(R), and fRR(R)f_{RR}(R) as independent numerical arrays, a positive analytic generator is assigned to fRR(R)f_{RR}(R) and integrated to obtain a derivative-consistent reconstructed curvature sector. The frozen reconstruction is evaluated on 10,019 radial nodes over r[1,105]r\in[1,10^{5}]. The corresponding Ricci-scalar trajectory spans 1.1317×109R1.999999998-1.1317\times10^{-9}\leq R\leq1.999999998 and is weakly non-monotonic, so no inversion r=r(R)r=r(R) is required. On the same finite grid, the reconstructed source variables retain positive pointwise energy-condition margins, the coordinate-radial null-energy integrals are positive both globally and in the near-throat band, and the maximum normalized tidal-curvature ratio is 0.8666<10.8666<1. The reconstructed source-side closure diagnostic has a maximum absolute residual of 5.3246×1055.3246\times10^{-5}. The source closure is phenomenological rather than derived from a unique microphysical matter Lagrangian or a uniquely specified curvature--matter coupling function. Accordingly, the result is not presented as a full field-equation solution of a specified nonminimally coupled f(R)f(R) theory, a stability proof, an exterior-matched global spacetime, or an observer-dependent safe-traversal model. It instead provides a finite-domain computational benchmark for auditable inverse reconstruction of Morris--Thorne-type geometries in modified gravity.


Source: arXiv:2608.27485v1 - http://arxiv.org/abs/2608.27485v1 PDF: https://arxiv.org/pdf/2608.27485v1 Original Link: http://arxiv.org/abs/2608.27485v1

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Date:
Aug 31, 2026
Topic:
Physics
Area:
Physics
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Finite-domain inverse reconstruction of a Morris--Thorne-type wormhole candidate with a derivative-consistent $f(R)$ curvature sector | Researchia