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Author Andrade, I.; Bazeia, D.; Marques, M.A.; Menezes, R.; Olmo, G.J.
Title Analytical solutions for Maxwell-scalar system on radially symmetric spacetimes Type Journal Article
Year (down) 2025 Publication European Physical Journal C Abbreviated Journal Eur. Phys. J. C
Volume 85 Issue 1 Pages 27 - 15pp
Keywords
Abstract We investigate Maxwell-scalar models on radially symmetric spacetimes in which the gauge and scalar fields are coupled via the electric permittivity. We find the conditions that allow for the presence of minimum energy configurations. In this formalism, the charge density must be written exclusively in terms of the components of the metric tensor and the scalar field is governed by first-order equations. We also find a manner to map the aforementioned equation into the corresponding one associated to kinks in (1, 1) spacetime dimensions, so we get analytical solutions for three specific spacetimes. We then calculate the energy density and show that the energy is finite. The stability of the solutions against contractions and dilations, following Derrick's argument, and around small fluctuations in the fields is also investigated. In this direction, we show that the solutions obeying the first-order framework are stable.
Address [Andrade, I.; Bazeia, D.] Univ Fed Paraiba, Dept Fis, BR-58051970 Joao Pessoa, Paraiba, Brazil, Email: andradesigor0@gmail.com;
Corporate Author Thesis
Publisher Springer Place of Publication Editor
Language English Summary Language Original Title
Series Editor Series Title Abbreviated Series Title
Series Volume Series Issue Edition
ISSN 1434-6044 ISBN Medium
Area Expedition Conference
Notes WOS:001399512300003 Approved no
Is ISI yes International Collaboration yes
Call Number IFIC @ pastor @ Serial 6445
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Author Lessa, L.A.; Olmo, G.J.
Title On the structure of black bounces sourced by anisotropic fluids Type Journal Article
Year (down) 2025 Publication Journal of Cosmology and Astroparticle Physics Abbreviated Journal J. Cosmol. Astropart. Phys.
Volume 03 Issue 3 Pages 019 - 18pp
Keywords Exact solutions; black holes and black hole thermodynamics in GR and beyond; GR black holes; modified gravity; Wormholes
Abstract The field equations of static, spherically symmetric geometries generated by anisotropic fluids is investigated with the aim of better understanding the relation between the matter and the emergence of minimal area throats, like in wormhole and black bounce scenarios. Imposing some simplifying restrictions on the matter, which amounts to considering nonlinear electromagnetic sources, we find analytical expressions that allow one to design the type of sought geometries. We illustrate our analysis with several examples, including an asymmetric, bounded black bounce spacetime which reproduces the standard ReissnerNordstr & ouml;m geometry on the outside all the way down to the throat.
Address [Lessa, L. A.] Univ Fed Maranhao, Programa Posgrad Fis, Campus Univ Bacanga, BR-65080805 Sao Luis, MA, Brazil, Email: leandrophys@gmail.com;
Corporate Author Thesis
Publisher IOP Publishing Ltd Place of Publication Editor
Language English Summary Language Original Title
Series Editor Series Title Abbreviated Series Title
Series Volume Series Issue Edition
ISSN 1475-7516 ISBN Medium
Area Expedition Conference
Notes WOS:001443043800001 Approved no
Is ISI yes International Collaboration yes
Call Number IFIC @ pastor @ Serial 6553
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Author Alves Batista, R. et al; Mitsou, V.A.; Olmo, G.J.; Zornoza, J.D.
Title White paper and roadmap for quantum gravity phenomenology in the multi-messenger era Type Journal Article
Year (down) 2025 Publication Classical and Quantum Gravity Abbreviated Journal Class. Quantum Gravity
Volume 42 Issue 3 Pages 032001 - 47pp
Keywords quantum gravity phenomenology; Lorentz invariance violation and deformation; gamma-ray astronomy; cosmic neutrinos; ultra-high-energy cosmic rays; gravitational waves; spacetime foam
Abstract The unification of quantum mechanics and general relativity has long been elusive. Only recently have empirical predictions of various possible theories of quantum gravity been put to test, where a clear signal of quantum properties of gravity is still missing. The dawn of multi-messenger high-energy astrophysics has been tremendously beneficial, as it allows us to study particles with much higher energies and travelling much longer distances than possible in terrestrial experiments, but more progress is needed on several fronts. A thorough appraisal of current strategies and experimental frameworks, regarding quantum gravity phenomenology, is provided here. Our aim is twofold: a description of tentative multimessenger explorations, plus a focus on future detection experiments. As the outlook of the network of researchers that formed through the COST Action CA18108 'Quantum gravity phenomenology in the multi-messenger approach (QG-MM)', in this work we give an overview of the desiderata that future theoretical frameworks, observational facilities, and data-sharing policies should satisfy in order to advance the cause of quantum gravity phenomenology.
Address [Batista, R. Alves] Univ Autonoma Madrid, CSIC, Inst Fis Teor, C Nicolas Cabrera 13-15, Madrid 28049, Spain, Email: qgmm.cost@gmail.com;
Corporate Author Thesis
Publisher IOP Publishing Ltd Place of Publication Editor
Language English Summary Language Original Title
Series Editor Series Title Abbreviated Series Title
Series Volume Series Issue Edition
ISSN 0264-9381 ISBN Medium
Area Expedition Conference
Notes WOS:001412292900001 Approved no
Is ISI yes International Collaboration yes
Call Number IFIC @ pastor @ Serial 6555
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Author Maluf, R.V.; Silva, J.E.G.; Almeida, C.A.S.; Olmo, G.J.
Title Perturbative solutions for compact objects in (2+1)-dimensional Bopp-Podolsky electrodynamics Type Journal Article
Year (down) 2025 Publication European Physical Journal C Abbreviated Journal Eur. Phys. J. C
Volume 85 Issue 5 Pages 594 - 8pp
Keywords
Abstract We investigate the space-time geometry generated by compact objects in (2+1)-dimensional Bopp-Podolsky electrodynamics. Inspired by previous studies where the Bopp-Podolsky field acts as a source for spherically symmetric solutions, we revisit this question within the lower-dimensional (2+1) framework. Using a perturbative approach, we derive a charged BTZ-like black hole solution and compute corrections up to second order in a perturbative expansion valid far from the horizon. Our analysis suggests that the near-horizon and inner structure of the solution remain unaltered, indicating that no new non-black hole objects emerge in this regime. In particular, we do not find evidence of wormhole solutions in the (2+1)-dimensional version of this theory.
Address [Maluf, R. V.; Silva, J. E. G.; Almeida, C. A. S.; Olmo, Gonzalo J.] Univ Fed Ceara UFC, Dept Fis, Campus Pici,CP 6030, BR-60455760 Fortaleza, CE, Brazil, Email: r.v.maluf@fisica.ufc.br;
Corporate Author Thesis
Publisher Springer Place of Publication Editor
Language English Summary Language Original Title
Series Editor Series Title Abbreviated Series Title
Series Volume Series Issue Edition
ISSN 1434-6044 ISBN Medium
Area Expedition Conference
Notes WOS:001498735700001 Approved no
Is ISI yes International Collaboration yes
Call Number IFIC @ pastor @ Serial 6687
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Author Muniz, C.R.; Alencar, G.; Cunha, M.S.; Olmo, G.J.
Title Static and stationary black bounces inspired by loop quantum gravity Type Journal Article
Year (down) 2025 Publication Physical Review D Abbreviated Journal Phys. Rev. D
Volume 112 Issue 2 Pages 024018 - 14pp
Keywords
Abstract We construct static and stationary versions of a black bounce geometry using as inspiration a line element that arises in loop quantum gravity (LQG) scenarios. Analyzing the line element from the framework of general relativity, we trace its origin to nonlinear electrodynamics with electric and magnetic charges and check the energy conditions (null energy condition, weak energy condition, and strong energy condition). By extending the geometry using the Simpson-Visser procedure, we construct a black hole- wormhole bounce structure, influenced by LQG parameters. We analyze the horizon structure to constrain parameters for black holes and wormholes, and examine curvature and new sources, including a phantomtype scalar field, to ensure spacetime regularity and adherence to energy conditions. Thermodynamic properties are also studied, revealing the existence of remnants and phase transitions. Additionally, we derive a rotating black bounce solution, verifying its regularity, and putting forward that the spherical bouncing surface turns into an ellipsoid with no ring singularity. Finally, we find that increasing the LQG parameter leads to smaller ergospheres and reduced shadows, with potential implications for observational astrophysics and quantum gravitational signatures.
Address [Muniz, C. R.] Fac Educ Ciencias & Letras Iguatu, BR-63502253 Iguatu, CE, Brazil, Email: celio.muniz@uece.br;
Corporate Author Thesis
Publisher Amer Physical Soc Place of Publication Editor
Language English Summary Language Original Title
Series Editor Series Title Abbreviated Series Title
Series Volume Series Issue Edition
ISSN 2470-0010 ISBN Medium
Area Expedition Conference
Notes WOS:001532293100002 Approved no
Is ISI yes International Collaboration yes
Call Number IFIC @ pastor @ Serial 6768
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Author Pinto, M.A.S.; Maluf, R.V.; Olmo, G.J.
Title Regular black hole solutions in (2+1)-dimensional f(R, T) gravity coupled to nonlinear electrodynamics Type Journal Article
Year (down) 2025 Publication European Physical Journal C Abbreviated Journal
Volume 85 Issue 8 Pages 835
Keywords
Abstract In this paper, we investigate regular black hole solutions in the (2+1)-dimensional versions of general relativity and f(R, T) gravity, both coupled to nonlinear electrodynamics. By admitting that the matter content that generates such geometries satisfies the Maxwell limit condition, we obtain a class of regular black holes that give rise to new solutions and successfully reproduce particular cases found in earlier studies of (2+1)-dimensional general relativity. Moreover, we discover the first regular black hole solutions in (2+1)-dimensional f(R, T) gravity and explore both qualitatively and quantitatively the non-conservation of the energy-momentum tensor present in those solutions.
Address
Corporate Author Thesis
Publisher Place of Publication Editor
Language Summary Language Original Title
Series Editor Series Title Abbreviated Series Title
Series Volume Series Issue Edition
ISSN 1434-6044 ISBN Medium
Area Expedition Conference
Notes WOS:001543421400006 Approved no
Is ISI yes International Collaboration yes
Call Number IFIC @ pastor @ Serial 6790
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Author Bragado, A.; Olmo, G.J.
Title Periodic equatorial orbits in a black bounce scenario Type Journal Article
Year (down) 2025 Publication Classical and Quantum Gravity Abbreviated Journal Class. Quantum Gravity
Volume 42 Issue 18 Pages 185004 - 30pp
Keywords general relativity; black bounce; Simpson-Visser model; periodic orbits
Abstract We study equatorial closed orbits in a popular black bounce model to see if the internal structure of these objects could lead to peculiar observable features. Paralleling the analysis of the Schwarzschild and Kerr metrics, we show that in the black bounce case each orbit can also be associated with a triplet of integers which can then be used to construct a rational number characterizing each periodic orbit. When the black bounce solution represents a traversable wormhole, we show that the previous classification scheme is still applicable with minor adaptations. We confirm in this way that this established framework enables a complete description of the equatorial dynamics across a spectrum of cases, from regular black holes to wormholes. Varying the black bounce parameter rmin, we compare the trajectories in the Simpson-Visser model with those in the Schwarzschild metric (and the rotating case with Kerr). We find that in some cases even small increments in rmin can lead to significant changes in the orbits.
Address [Bragado, Anderson; Olmo, Gonzalo J.] Univ Fed Ceara UFC, Dept Fis, Campus Pici,CP 6030, BR-60455760 Fortaleza, CE, Brazil, Email: andersonbragado@fisica.ufc.br;
Corporate Author Thesis
Publisher IOP Publishing Ltd Place of Publication Editor
Language English Summary Language Original Title
Series Editor Series Title Abbreviated Series Title
Series Volume Series Issue Edition
ISSN 0264-9381 ISBN Medium
Area Expedition Conference
Notes WOS:001569025300001 Approved no
Is ISI yes International Collaboration yes
Call Number IFIC @ pastor @ Serial 6833
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Author Di Valentino, E. et al; Barenboim, G.; Bombacigno, F.; Hajjar, R.; Mena, O.; Mitsou, V.A.; Olmo, G.J.; Wang, D.
Title The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics Type Journal Article
Year (down) 2025 Publication Physics of the Dark Universe Abbreviated Journal Phys. Dark Universe
Volume 49 Issue Pages 101965 - 263pp
Keywords
Abstract The standard model of cosmology has provided a good phenomenological description of a wide range of observations both at astrophysical and cosmological scales for several decades. This concordance model is constructed by a universal cosmological constant and supported by a matter sector described by the standard model of particle physics and a cold dark matter contribution, as well as very early-time inflationary physics, and underpinned by gravitation through general relativity. There have always been open questions about the soundness of the foundations of the standard model. However, recent years have shown that there may also be questions from the observational sector with the emergence of differences between certain cosmological probes. In this White Paper, we identify the key objectives that need to be addressed over the coming decade together with the core science projects that aim to meet these challenges. These discordances primarily rest on the divergence in the measurement of core cosmological parameters with varying levels of statistical confidence. These possible statistical tensions may be partially accounted for by systematics in various measurements or cosmological probes but there is also a growing indication of potential new physics beyond the standard model. After reviewing the principal probes used in the measurement of cosmological parameters, as well as potential systematics, we discuss the most promising array of potential new physics that may be observable in upcoming surveys. We also discuss the growing set of novel data analysis approaches that go beyond traditional methods to test physical models. These new methods will become increasingly important in the coming years as the volume of survey data continues to increase, and as the degeneracy between predictions of different physical models grows. There are several perspectives on the divergences between the values of cosmological parameters, such as the model-independent probes in the late Universe and model-dependent measurements in the early Universe, which we cover at length. The White Paper closes with a number of recommendations for the community to focus on for the upcoming decade of observational cosmology, statistical data analysis, and fundamental physics developments.
Address [Di Valentino, Eleonora; van de Bruck, Carsten; Escamilla, Luis A.; Giare, William; Ozulker, Emre; Specogna, Enrico; Poulot, Gaspard; Cheng, Hanyu; De Angelis, Mariaveronica; Neves, Rita B.; Zhai, Yuejia; Lee, Dong Ha] Univ Sheffield, Sch Math & Phys Sci, Hounsfield Rd, Sheffield S3 7RH, S Yorkshire, England, Email: e.divalentino@sheffield.ac.uk;
Corporate Author Thesis
Publisher Elsevier Place of Publication Editor
Language English Summary Language Original Title
Series Editor Series Title Abbreviated Series Title
Series Volume Series Issue Edition
ISSN ISBN Medium
Area Expedition Conference
Notes WOS:001545480700001 Approved no
Is ISI yes International Collaboration yes
Call Number IFIC @ pastor @ Serial 6911
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Author Lima Junior, H.C.D.; Magalhaes, R.B.; Olmo, G.J.; Rubiera-Garcia, D.
Title On the resolution of space-time singularities in spherically symmetric black holes: geodesic completeness, curvature scalars, and tidal forces Type Journal Article
Year (down) 2025 Publication Classical and Quantum Gravity Abbreviated Journal Class. Quantum Gravity
Volume 42 Issue 22 Pages 225004 - 34pp
Keywords geodesic completeness; space-time singularities; tidal forces; regular black holes
Abstract The existence of black holes in the Universe is nowadays established on the grounds of a blench of astrophysical observations, most notably those of gravitational waves from binary mergers and the imaging of supermassive objects at the heart of M87 and Milky Way galaxies. However, this success of Einstein's general relativity (GR) to connect theory of black holes with observations is also the source of its doom, since Penrose's theorem proves that, under physically sensible conditions, the development of a space-time singularity (as defined by the existence of a focal point for some geodesic paths in finite affine time) within black holes as described by GR is unavoidable. In this work, we thoroughly study how to resolve space-time singularities in spherically symmetric black holes. To do it so we find the conditions on the metric functions required for the restoration of geodesic completeness without any regards to the specific theory of the gravitational and matter fields supporting the amended metric. Our discussion considers both the usual trivial radial coordinate case and the bouncing radial function case and arrives to two mechanisms for this restoration: either the focal point is displaced to infinite affine distance or a bounce prevents the focusing of geodesics. Several explicit examples of well known (in)complete space-times are given. Furthermore, we consider the connection of geodesic (in)completeness with another criterion frequently used in the literature to monitor singular space-times: the blow up of (some sets of) curvature scalars and the infinite tidal forces they could bring with them, and discuss the conditions required for the harmlessness upon physical observers according to each criterion.
Address [Lima Junior, Haroldo C. D.] Univ Fed Maranhao, Dept Fis, Campus Univ Bacanga, BR-65080805 Sao Luis, Maranhao, Brazil, Email: haroldo.lima@ufma.br;
Corporate Author Thesis
Publisher IOP Publishing Ltd Place of Publication Editor
Language English Summary Language Original Title
Series Editor Series Title Abbreviated Series Title
Series Volume Series Issue Edition
ISSN 0264-9381 ISBN Medium
Area Expedition Conference
Notes WOS:001613672000001 Approved no
Is ISI yes International Collaboration yes
Call Number IFIC @ pastor @ Serial 6930
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Author Olmo, G.J.; Rosa, J.L.; Rubiera-Garcia, D.; Rueda, A.; Saez-Chillon Gomez, D.
Title Shadows from thin accretion disks of parametrized black hole solutions Type Journal Article
Year (down) 2025 Publication Physical Review D Abbreviated Journal Phys. Rev. D
Volume 112 Issue 8 Pages 084059 - 19pp
Keywords Relativistic MagnetoHydroDynamic (GRMHD) simula-
Abstract We discuss the optical appearance from thin accretion disks in parametrized black holes, namely, solutions characterized by an arbitrarily large number of parameters without any regards to the theory of the gravitational and matter fields they come from. More precisely, we consider the leading-order terms of the spherically symmetric Johanssen-Psaltis (JP) and Konoplya-Rezzolla-Zhidenko (KRZ) parametrizations after imposing constraints from asymptotic flatness and solar system observations. Furthermore, we use the inferred correlation, by the Event Horizon Telescope Collaboration, between the size of the bright ring (which is directly observable) and the size of the central brightness depression (which is not) of M87 and Sgr A* central supermassive objects, to constrain the parameters of the leading-order JP and KRZ solutions. Using ten samples of the Standard Unbound distribution previously employed in the literature to reproduce certain scenarios of General Relativistic HydroDynamical simulations, we produce images of four samples of JP and KRZ geometries enhancing and diminishing the shadow's size, respectively. Via a qualitative and quantitative analysis of the features of the corresponding photon rings and, in particular, of their relative brightness, we argue that it should be possible to distinguish between such parametrized solutions and the Schwarzschild geometry via future upgrades of very long baseline interferometry. We furthermore consider images of some naked objects within these parametrizations, and also discuss the role of inclination in comparing images of different black holes.
Address [Olmo, Gonzalo J.] Univ Valencia, Ctr Mixto Univ Valencia, Dept Fis Teor, CSIC, Valencia 46100, Spain, Email: gonzalo.olmo@uv.es;
Corporate Author Thesis
Publisher Amer Physical Soc Place of Publication Editor
Language English Summary Language Original Title
Series Editor Series Title Abbreviated Series Title
Series Volume Series Issue Edition
ISSN 2470-0010 ISBN Medium
Area Expedition Conference
Notes WOS:001616050700014 Approved no
Is ISI yes International Collaboration yes
Call Number IFIC @ pastor @ Serial 6937
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