Skip to content
DraconiticResearch
Search Sources API
203,234 studies31 sourcesUpdated 3 min ago
Peer-reviewedCC BY 4.0Journal of High Energy Physics

Eikonal, nonlocality and regular black holes

  1. 1Università di Cagliari
  2. 2I.N.F.N, Sezione di Cagliari

Abstract

A bstract : We investigate the leading gravitational eikonal in nonlocal D dimensional theories of gravity. We analyze the simplest cases of 2 → 2 massless and massive scalar scattering at tree level, studying the effects of nonlocal form factors in the gravitational sector. We give an interpretation of our results in terms of geodesic motion in effective generalized Aichelburg-Sexl geometries for the massless case, and in smeared linearized Schwarzschild metrics for the massive case in the probe limit. Combining our results for the geometries at linearized level with general requirements about the behavior of the solutions in the core, we propose a nonlinear completion of the geometries. The resulting spacetimes describe singularity-free, asymptotically flat deformations of the Schwarzschild solution with a de Sitter core. We also analyze the main geometric and thermodynamic features of these solutions.

Related

  1. Rotating black holes surrounded by PFDM in STVG: Shadows and eikonal quasinormal modes
    Muhammad Zahid, Zhiling Liu, Saeed Ullah Khan +1
    arXivPreprintarXiv licenceFull textGravitation & general relativityarXiv
  2. Constraining the geometry of rotating black holes with eikonal QNMs
    Ciro De Simone, Sebastian H. Völkel, Kostas D. Kokkotas
    arXivPreprintarXiv licenceFull textGravitation & general relativityarXiv
  3. Regular hairy black holes by gravitational decoupling: de Sitter and Minkowski cores
    Daulet Berkimbayev
    Nuclear Physics BPeer-reviewedCC BY 4.0Full textHigh-energy & particle physicsCrossref
  4. Parameter constraints on rotating ABG regular black holes from quasi-periodic oscillations
    Meng-He Wu, Xiao-Mei Kuang
    Physics Letters BPeer-reviewedCC BY 4.0Full textHigh-energy & particle physicsCrossref
  5. Electric Penrose process in spherically symmetric regular black holes with and without a cosmological constant
    Haowei Chen, Hengyu Xu, Yizhi Zhan +1
    Classical and Quantum GravityPeer-reviewedLicence not statedFull text7 citedHigh-energy & particle physicsOpenAlex
BibTeX
@article{cadoni2026eikonal,
  title = {{Eikonal, nonlocality and regular black holes}},
  author = {Mariano Cadoni and Lorenzo Herres and Leonardo Modesto and Lorenzo Orlando and Mirko Pitzalis},
  journal = {Journal of High Energy Physics},
  year = {2026},
  month = nov,
  doi = {10.1007/jhep11(2026)035},
  url = {https://link.springer.com/article/10.1007/JHEP11(2026)035},
  note = {CC BY 4.0},
}
RIS
TY  - JOUR
TI  - Eikonal, nonlocality and regular black holes
AU  - Mariano Cadoni
AU  - Lorenzo Herres
AU  - Leonardo Modesto
AU  - Lorenzo Orlando
AU  - Mirko Pitzalis
PY  - 2026
DA  - 2026/11/04
JO  - Journal of High Energy Physics
DO  - 10.1007/jhep11(2026)035
UR  - https://link.springer.com/article/10.1007/JHEP11(2026)035
AB  - A bstract : We investigate the leading gravitational eikonal in nonlocal D dimensional theories of gravity. We analyze the simplest cases of 2 → 2 massless and massive scalar scattering at tree level, studying the effects of nonlocal form factors in the gravitational sector. We give an interpretation of our results in terms of geodesic motion in effective generalized Aichelburg-Sexl geometries for the massless case, and in smeared linearized Schwarzschild metrics for the massive case in the probe limit. Combining our results for the geometries at linearized level with general requirements about the behavior of the solutions in the core, we propose a nonlinear completion of the geometries. The resulting spacetimes describe singularity-free, asymptotically flat deformations of the Schwarzschild solution with a de Sitter core. We also analyze the main geometric and thermodynamic features of these solutions.
SN  - 1029-8479
ER  -