Akademik Veri Yönetim Sistemi
EUROPEAN PHYSICAL JOURNAL C, cilt.86, sa.3, 2026 (SCI-Expanded, Scopus)
We propose a covariant extension of general relativity in which the local effective dimension of spacetime is promoted to a dynamical, curvature-induced field on an underlying four-dimensional manifold. Deviations from four dimensions are encoded in a scalar degree of freedom epsilon(x)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\varepsilon (x)$$\end{document}, defining Deff(x)=4-epsilon(x)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$D_{\textrm{eff}}(x)=4-\varepsilon (x)$$\end{document}, which enters the gravitational action through a dimension weight v(epsilon)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$v(\varepsilon )$$\end{document} multiplying the Einstein-Hilbert term and a scalar potential U(epsilon)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$U(\varepsilon )$$\end{document}. At the level of the field equations, these ingredients combine into a curvature-sensitive effective potential V(epsilon,R)\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$V(\varepsilon ,R)$$\end{document} for the dynamical dimension field, where R is the Ricci scalar. In the limit epsilon -> 0\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\varepsilon \rightarrow 0$$\end{document} and v(epsilon)-> 1\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$v(\varepsilon )\rightarrow 1$$\end{document}, the weak-field regime of general relativity is continuously recovered. We derive the modified Einstein equations and the equation of motion for epsilon\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\varepsilon $$\end{document}, showing that the resulting framework is scalar-tensor-like in structure, with the additional field controlling the local effective dimensionality of spacetime rather than describing an independent matter component. As benchmark applications, we study static, spherically symmetric configurations and a spatially flat Friedmann-Lema & icirc;tre-Robertson-Walker background, where curvature-induced dimensional effects lead to controlled deformations of the mass-radius relation in compact objects and small corrections to the background expansion history.