Skip to content
DraconiticResearch
Search Sources API
203,234 studies31 sourcesUpdated 6 min ago
PreprintCC BY 4.0arXiv

Dymnikova Black Holes in Unimodular Gravity: Maxwell Sources and Vacuum Contributions

Abstract

In this work, we investigate the Dymnikova regular black hole within the framework of unimodular gravity, emphasizing the role of the effective vacuum sector in the regularization of the geometry. By allowing a controlled violation of the covariant conservation of the energy--momentum tensor, the cosmological contribution emerges dynamically as a radial-dependent function, Λ=Λ(r). We first reinterpret the Dymnikova spacetime as a charged configuration supported by nonlinear electrodynamics and derive the corresponding electric and magnetic sources. Subsequently, we demonstrate that the same geometry can be consistently generated by standard Maxwell electrodynamics in unimodular gravity. In this construction, the resulting electric field is everywhere regular and corresponds to a localized charge distribution with vanishing asymptotic charge, indicating that the spacetime does not behave as an asymptotically charged object.

Related

  1. Lifshitz Phase of Quantum Gravity: The Infrared Fixed Point of the (2+1)D Unimodular Hořava-Chern-Simons Model
    Maxim Zelenko, Dam Thanh Son
    arXivPreprintarXiv licenceFull textCondensed matterGravitation & general relativityarXiv
  2. Spherical thin shells with charge in unimodular gravity
    Gabriel R. Bengochea, Ernesto F. Eiroa, Griselda Figueroa-Aguirre
    arXivPreprintarXiv licenceFull textGravitation & general relativityarXiv
  3. Unimodular Gravity with Arbitrary Diffusion Function: A Dynamical System Reconstruction Approach
    Gabriel Gómez, Guillermo Palma, Norman Cruz
    arXivPreprintarXiv licenceFull textGravitation & general relativityarXiv
  4. Observational constraints on Diffusion Cosmologies in Unimodular Gravity from DESI DR2
    Gabriel Gomez, Guillermo Palma, Norman Cruz
    arXivPreprintCC BY 4.0Full textGeneral physicsarXiv
  5. Static Spherically Symmetric Solutions in Nonconservative Unimodular Gravity
    Anuar Idrissov, Hernando Quevedo
    arXivPreprintCC BY 4.0Full textGravitation & general relativityarXiv
BibTeX
@misc{alencar2026dymnikova,
  title = {{Dymnikova Black Holes in Unimodular Gravity: Maxwell Sources and Vacuum Contributions}},
  author = {G. Alencar and V. H. U. Borralho},
  howpublished = {arXiv},
  year = {2026},
  month = sep,
  doi = {10.48550/arxiv.2605.15255},
  eprint = {2605.15255},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2605.15255},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Dymnikova Black Holes in Unimodular Gravity: Maxwell Sources and Vacuum Contributions
AU  - G. Alencar
AU  - V. H. U. Borralho
PY  - 2026
DA  - 2026/09/07
PB  - arXiv
DO  - 10.48550/arxiv.2605.15255
UR  - https://arxiv.org/abs/2605.15255
AB  - In this work, we investigate the Dymnikova regular black hole within the framework of unimodular gravity, emphasizing the role of the effective vacuum sector in the regularization of the geometry. By allowing a controlled violation of the covariant conservation of the energy--momentum tensor, the cosmological contribution emerges dynamically as a radial-dependent function, Λ=Λ(r). We first reinterpret the Dymnikova spacetime as a charged configuration supported by nonlinear electrodynamics and derive the corresponding electric and magnetic sources. Subsequently, we demonstrate that the same geometry can be consistently generated by standard Maxwell electrodynamics in unimodular gravity. In this construction, the resulting electric field is everywhere regular and corresponds to a localized charge distribution with vanishing asymptotic charge, indicating that the spacetime does not behave as an asymptotically charged object.
ER  -