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    Matter maps to geometry in gravitational collapse

    H. Khodabakhshi1,*, Zhi-Chao Li1,†, H. Lü1,2,‡, and F. Shojai3,§

    • 1Center for Joint Quantum Studies and Department of Physics, School of Science, Tianjin University, Tianjin 300350, China
    • 2The International Joint Institute of Tianjin University, Fuzhou, Tianjin University, Tianjin 300350, China
    • 3Department of Physics, University of Tehran, P.O. Box 14395-547, Tehran, Iran

    • *Contact author: h_khodabakhshi@tju.edu.cn
    • †Contact author: lizc@tju.edu.cn
    • ‡Contact author: mrhonglu@gmail.com
    • §Contact author: fshojai@ut.ac.ir

    Phys. Rev. D 114, 024075 – Published 27 July, 2026

    DOI: https://doi.org/10.1103/m6v7-9cyg

    Abstract

    We establish an exact bidirectional map between the effective homogeneous interior density of a collapsing star and the exterior metric function in generalized Oppenheimer-Snyder collapse. The Darmois-Israel junction conditions reduce this relation to a purely algebraic form, providing a direct way to reconstruct candidate static geometries and their surface dynamics without solving the corresponding differential field equations separately. Correction powers diagnose models; integer exponents signal ultraviolet completions, while fractional powers identify phenomenological ones. Our framework not only simplifies the construction of regular black holes but also provides a universal benchmark for testing singularity resolution and cosmic censorship in quantum gravity phenomenology.

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