Complex Variables in Quantum Gravity

A special issue of Axioms (ISSN 2075-1680). This special issue belongs to the section "Mathematical Physics".

Deadline for manuscript submissions: 30 June 2025 | Viewed by 1343

Special Issue Editor


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Guest Editor
Grupo de Matemática Aplicada & Grupo de Física de Altas Energías & Centro de Ciencias Exactas & Departamento de Ciencias Básicas, Universidad del Bío-Bío, Campus Fernando May, Av. Andres Bello 720, Casilla 447, Chillán 3780227, Chile
Interests: integral transforms; quantum field theory; applied mathematics

Special Issue Information

Dear Colleagues,

This Special Issue is dedicated to the application of integral transformations to calculations of Green functions and scattering amplitudes in quantum gravity via the utilization of complex analysis, the Cauchy integral formula, the residue calculus technique and complex mapping. The Slavnov–Taylor identity relates different Green functions of quantum fields in gravity as well as in the Yang–Mills theory.  In turn, the Slavnov–Taylor identity follows from the BRST symmetry of the classical action extended by certain additional terms. For the classical action, the BRST symmetry coincides with gauge symmetry. In gravitational theory, the gauge symmetry is represented by diffeomorphisms. The Green functions are defined in terms of the path integral whose measure is invariant with respect to BRST transformations. As a result of this BRST invariance, the Slavnov–Taylor identity appears in gravity.

Although the aim of this Special Issue is to publish original research articles on higher loop calculations in quantum gravity, focused on integral transformations involving complex variables, review articles on this subject are also welcome.

Dr. Igor Kondrashuk
Guest Editor

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Keywords

  • integral transforms
  • quantum field theory
  • quantum gravity
  • complex mappings

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Published Papers (2 papers)

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Research

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18 pages, 251 KiB  
Article
Complex Riemannian Spacetime: Removal of Black Hole Singularities and Black Hole Paradoxes
by John W. Moffat
Axioms 2025, 14(6), 440; https://doi.org/10.3390/axioms14060440 - 4 Jun 2025
Viewed by 47
Abstract
An approach is presented to resolve key paradoxes in black hole physics through the application of complex Riemannian spacetime. We extend the Schwarzschild metric into the complex domain, employing contour integration techniques to remove singularities while preserving the essential features of the original [...] Read more.
An approach is presented to resolve key paradoxes in black hole physics through the application of complex Riemannian spacetime. We extend the Schwarzschild metric into the complex domain, employing contour integration techniques to remove singularities while preserving the essential features of the original solution. A new regularized radial coordinate is introduced, leading to a singularity-free description of black hole interiors. Crucially, we demonstrate how this complex extension resolves the long-standing paradox of event horizon formation occurring only in the infinite future of distant observers. By analyzing trajectories in complex spacetime, we show that the horizon can form in finite complex time, reconciling the apparent contradiction between proper and coordinate time descriptions. This approach also provides a framework for the analytic continuation of information across event horizons, resolving the Hawking information paradox. We explore the physical interpretation of the complex extension versus its projection onto real spacetime. The gravitational collapse of a dust sphere with negligible dust is explored in the complex spacetime extension. The approach offers a mathematically rigorous framework for exploring quantum gravity effects within the context of classical general relativity. Full article
(This article belongs to the Special Issue Complex Variables in Quantum Gravity)

Review

Jump to: Research

38 pages, 678 KiB  
Review
Very Special Relativity Models: Infrared Regularization and Loop Corrections
by Jorge Alfaro
Axioms 2025, 14(6), 441; https://doi.org/10.3390/axioms14060441 - 4 Jun 2025
Viewed by 60
Abstract
We review the Sim(2) invariant infrared regularization of Very Special Relativity models that we have proposed recently and apply it to compute loop corrections in quantum electrodynamics with VSR masses for neutrino and photon. Then, we compute the [...] Read more.
We review the Sim(2) invariant infrared regularization of Very Special Relativity models that we have proposed recently and apply it to compute loop corrections in quantum electrodynamics with VSR masses for neutrino and photon. Then, we compute the axial anomaly. Finally, we study the Gross–Neveu model with a VSR mass in the large N limit uncovering a new phase of the model. Full article
(This article belongs to the Special Issue Complex Variables in Quantum Gravity)
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