Relic Gravitational Waves in the Noncommutative Foliated Riemannian Quantum Gravity

We present a study of relic gravitational waves based on a foliated gauge field theory defined over a spacetime endowed with a noncommutative algebraic–geometric structure. As an ontological extension of general relativity—concerning manifolds, metrics, and fiber bundles—the conventional space and t...

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Main Authors: César A. Zen Vasconcellos, Peter O. Hess, José A. de Freitas Pacheco, Fridolin Weber, Remo Ruffini, Dimiter Hadjimichef, Moisés Razeira, Benno August Ludwig Bodmann, Marcelo Netz-Marzola, Geovane Naysinger, Rodrigo Fraga da Silva, João G. G. Gimenez
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Language:English
Published: MDPI AG 2025-05-01
Series:Universe
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Online Access:https://www.mdpi.com/2218-1997/11/6/179
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author César A. Zen Vasconcellos
Peter O. Hess
José A. de Freitas Pacheco
Fridolin Weber
Remo Ruffini
Dimiter Hadjimichef
Moisés Razeira
Benno August Ludwig Bodmann
Marcelo Netz-Marzola
Geovane Naysinger
Rodrigo Fraga da Silva
João G. G. Gimenez
author_facet César A. Zen Vasconcellos
Peter O. Hess
José A. de Freitas Pacheco
Fridolin Weber
Remo Ruffini
Dimiter Hadjimichef
Moisés Razeira
Benno August Ludwig Bodmann
Marcelo Netz-Marzola
Geovane Naysinger
Rodrigo Fraga da Silva
João G. G. Gimenez
author_sort César A. Zen Vasconcellos
collection DOAJ
description We present a study of relic gravitational waves based on a foliated gauge field theory defined over a spacetime endowed with a noncommutative algebraic–geometric structure. As an ontological extension of general relativity—concerning manifolds, metrics, and fiber bundles—the conventional space and time coordinates, typically treated as classical numbers, are replaced by complementary quantum dual fields. Within this framework, consistent with the Bekenstein criterion and the Hawking–Hertog multiverse conception, singularities merge into a helix-like cosmic scale factor that encodes the topological transition between the contraction and expansion phases of the universe analytically continued into the complex plane. This scale factor captures the essence of an intricate topological quantum-leap transition between two phases of the branching universe: a contraction phase preceding the now-surpassed conventional concept of a primordial singularity and a subsequent expansion phase, whose transition region is characterized by a Riemannian topological foliated structure. The present linearized formulation, based on a slight gravitational field perturbation, also reveals a high sensitivity of relic gravitational wave amplitudes to the primordial matter and energy content during the universe’s phase transition. It further predicts stochastic homogeneous distributions of gravitational wave intensities arising from the interplay of short- and long-spacetime effects within the non-commutative algebraic framework. These results align with the anticipated future observations of relic gravitational waves, expected to pervade the universe as a stochastic, homogeneous background.
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spelling doaj-art-26d0fd9e4f0b411fbd514472f3a0361a2025-08-20T03:32:33ZengMDPI AGUniverse2218-19972025-05-0111617910.3390/universe11060179Relic Gravitational Waves in the Noncommutative Foliated Riemannian Quantum GravityCésar A. Zen Vasconcellos0Peter O. Hess1José A. de Freitas Pacheco2Fridolin Weber3Remo Ruffini4Dimiter Hadjimichef5Moisés Razeira6Benno August Ludwig Bodmann7Marcelo Netz-Marzola8Geovane Naysinger9Rodrigo Fraga da Silva10João G. G. Gimenez11Instituto de Fisica, Universidade Federal do Rio Grande do Sul (UFRGS), Porto Alegre 91501-970, BrazilInstituto de Ciencias Nucleares, Universidad Nacional Autonoma de Mexico (UNAM), A.P. 70-543, Mexico City 04510, MexicoObservatoire de la Cote d’Azur (OCA), 06300 Nice, FranceDepartment of Physics, San Diego State University (SDSU), San Diego, CA 92182, USAInternational Center for Relativistic Astrophysics Network (ICRANet), 65122 Pescara, ItalyInstituto de Fisica, Universidade Federal do Rio Grande do Sul (UFRGS), Porto Alegre 91501-970, BrazilUniversidade Federal do Pampa (UNIPAMPA), Campus Caçapava do Sul, Caçapava do Sul 96570-000, BrazilInstituto de Fisica, Universidade Federal do Rio Grande do Sul (UFRGS), Porto Alegre 91501-970, BrazilFrankfurt Institute for Advanced Studies (FIAS), J.W. von Goethe Universität, 60438 Frankfurt am Main, GermanyInstituto de Fisica, Universidade Federal do Rio Grande do Sul (UFRGS), Porto Alegre 91501-970, BrazilInstituto de Fisica, Universidade Federal do Rio Grande do Sul (UFRGS), Porto Alegre 91501-970, BrazilInstituto de Fisica, Universidade Federal do Rio Grande do Sul (UFRGS), Porto Alegre 91501-970, BrazilWe present a study of relic gravitational waves based on a foliated gauge field theory defined over a spacetime endowed with a noncommutative algebraic–geometric structure. As an ontological extension of general relativity—concerning manifolds, metrics, and fiber bundles—the conventional space and time coordinates, typically treated as classical numbers, are replaced by complementary quantum dual fields. Within this framework, consistent with the Bekenstein criterion and the Hawking–Hertog multiverse conception, singularities merge into a helix-like cosmic scale factor that encodes the topological transition between the contraction and expansion phases of the universe analytically continued into the complex plane. This scale factor captures the essence of an intricate topological quantum-leap transition between two phases of the branching universe: a contraction phase preceding the now-surpassed conventional concept of a primordial singularity and a subsequent expansion phase, whose transition region is characterized by a Riemannian topological foliated structure. The present linearized formulation, based on a slight gravitational field perturbation, also reveals a high sensitivity of relic gravitational wave amplitudes to the primordial matter and energy content during the universe’s phase transition. It further predicts stochastic homogeneous distributions of gravitational wave intensities arising from the interplay of short- and long-spacetime effects within the non-commutative algebraic framework. These results align with the anticipated future observations of relic gravitational waves, expected to pervade the universe as a stochastic, homogeneous background.https://www.mdpi.com/2218-1997/11/6/179relic gravitational wavesnoncommutative geometryfoliated quantum gravitybranch-cut quantum gravitytopological phase transitioninflationary cosmology
spellingShingle César A. Zen Vasconcellos
Peter O. Hess
José A. de Freitas Pacheco
Fridolin Weber
Remo Ruffini
Dimiter Hadjimichef
Moisés Razeira
Benno August Ludwig Bodmann
Marcelo Netz-Marzola
Geovane Naysinger
Rodrigo Fraga da Silva
João G. G. Gimenez
Relic Gravitational Waves in the Noncommutative Foliated Riemannian Quantum Gravity
Universe
relic gravitational waves
noncommutative geometry
foliated quantum gravity
branch-cut quantum gravity
topological phase transition
inflationary cosmology
title Relic Gravitational Waves in the Noncommutative Foliated Riemannian Quantum Gravity
title_full Relic Gravitational Waves in the Noncommutative Foliated Riemannian Quantum Gravity
title_fullStr Relic Gravitational Waves in the Noncommutative Foliated Riemannian Quantum Gravity
title_full_unstemmed Relic Gravitational Waves in the Noncommutative Foliated Riemannian Quantum Gravity
title_short Relic Gravitational Waves in the Noncommutative Foliated Riemannian Quantum Gravity
title_sort relic gravitational waves in the noncommutative foliated riemannian quantum gravity
topic relic gravitational waves
noncommutative geometry
foliated quantum gravity
branch-cut quantum gravity
topological phase transition
inflationary cosmology
url https://www.mdpi.com/2218-1997/11/6/179
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