Conveners
Parallel Session B: Black Hole Perturbation
- Katerina Chatziioannou (California Institute of Technology)
Parallel Session B: Alternative Black Holes
- Georgios Antoniou (INFN Rome & Sapienza University of Rome)
Parallel Session B: Alternative Black Holes
- Eleni-Alexandra Kontou (King's College London)
Parallel Session B: Charged Bodies
- Perseas Christodoulidis (Ewha Womans University)
Parallel Session B: Mathematical Relativity
- Damianos Iosifidis (Scuola Superiore Meridionale, Napoli)
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Ms Cynthia Belen Arias Pruna (Charles University, Prague)02/09/2025, 15:00talk
We study a class of symmetry operators acting on vector perturbations in the Kerr spacetime and employ them to generate new solutions of Maxwell equations. The operators are second-order in derivatives and are directly constructed from the principal Killing-Yano tensor. One of them reproduces a known result from the Debye potential theory, while the other yields a novel symmetry. When applied...
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Bertha Cuadros-Melgar (University of Sao Paulo)02/09/2025, 15:20talk
In this work we present a new solution of a black hole surrounded by massive vector fields in the context of Kaluza-Klein theory. This vector field corresponds to a spin-1 graviton that modifies the law of gravity and allows the effects attributed to dark matter in the universe. In order to analyze the influence of the parameters associated to this solution, we perturb the geometry with a...
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Dr Petr Kotlařík (Astronomical Institute, Czech Academy of Sciences)02/09/2025, 15:40talk
When a black hole (BH) rings due to some external perturbation, it emits gravitational waves described by quasi-normal modes (QNMs) – a series of exponentially damped harmonic oscillations. If the Kerr(-Newman) metric fully describes the BH, QNMs carry a unique signature of the BH parameters encoded in the modes' complex frequencies. Consequently, any deviation in the QNMs spectrum from the...
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George Cristache (Institute of Space Science- INFLPR subsidiary)02/09/2025, 16:00talk
Gravitational Waves (GW) emission is usually studied within the framework of the Regge-Wheeler-Zerilli equations, which are not exact and often times require numerical integration or extrapolation (a process which involves tuning additional parameters). Our aim is to prescribe a theoretical framework which alleviates some of these technical challenges by employing a Lehmann-Symanzik-Zimmerman...
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Zakaria Belkhadria (Université de Genève / Università di Cagliari)02/09/2025, 16:20talk
We present a model of black hole scalarization where a scalar field couples simultaneously to the Gauss–Bonnet invariant and a U(1) gauge field (can be identified as a dark photon or an electromagnetic field). This combined interaction broadens the conditions for spontaneous scalarization and unify the previous models in one. framework. We track how the electric charge and the two coupling...
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Mrs Natalia Astudillo (Charles University)02/09/2025, 17:00talk
We derive the explicit form of the Einstein-Gauss-Bonnet field equations for D-dimensional geometries that admit non-twisting, shear-free, and expanding null geodesic congruences, forming thus the famous Robinson-Trautman class of spacetimes, and discuss their structure and particular solutions. In D=4 GR, this class contains Weyl type II spacetimes or algebraically more special solutions such...
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Dr Jose Manuel Barrientos Ortiz (Universidad de Tarapacá)02/09/2025, 17:20talk
We construct explicit rotating solutions in Einstein's theory of relativity with a minimally coupled free scalar field rederiving and finding solutions in four or five spacetime dimensions. These spacetimes describe, in particular, the back-reaction of a free scalar field evolving in a Kerr spacetime. Adapting the general integrability result obtained many years ago from Eriş-Gürses to simpler...
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Dr Theodoros Nakas (Institute for Basic Science, CTPU-CGA)02/09/2025, 17:40talk
We present an algorithm to obtain exact black holes endowed with primary scalar hair within the shift-symmetric and $Z_2$-symmetric subclass of beyond Horndeski theories. These solutions depend, in addition to the conventional mass parameter, on a second free parameter encoding primary scalar hair. In the limit of vanishing scalar hair, the solutions smoothly reduce to the Schwarzschild,...
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Kostas Tzanavaris (Higgs Centre for Theoretical Physics)02/09/2025, 18:00talk
Einstein's equations imply that a gravitationally collapsed object forms an event horizon. But what lies on the other side of this horizon? In this talk, I am going to discuss the results of our new paper (https://arxiv.org/abs/2412.09558 ), presenting an alternative, topologically distinct solution: the Black Mirror. In the black hole solution, the horizon connects the exterior metric to an...
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Prof. Diego Rubiera-Garcia (Complutense University of Madrid)03/09/2025, 15:00talk
The recent detections from the EHT Collaboration of the shadows generated by the supermassive objects at the heart of M87 and Milky Way galaxies has prompted a new era in theoretical strong-field astrophysics. In this talk I will discuss the theoretical and basis of this new observational window and its latent power for distinguishing between canonical black holes, regular black holes, and...
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Agustín Silva (Radboud University)03/09/2025, 15:20talk
Extended gravitational models have gained large attention in the last couple of decades. In this talk, I'll examine the solution space of vacuum, static, and spherically symmetric spacetimes within F(R) theories, introducing novel methods that reduce the vacuum equations to a single second-order equation. I'll derive analytic expressions for the metric functions in terms of the arbitrary...
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Alex Giacomini03/09/2025, 15:40talk
New exact pulsed and spinning self-gravitating solutions for the four dimensional SU(2) Einstein-non-linear-sigma model and the Einstein-Skyrme model both minimally coupled to the Maxwell field will be presented. These solutions describe mesonic tubes with finite energy and angular momentum and which are asymptotically gyratons. We show that the found solutions are free of curvature invariants...
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Aravindhan Srinivasan (Charles University, Prague and IM CAS, Prague)03/09/2025, 16:00talk
Almost four decades have passed since the generalization of vacuum Kerr solutions to higher dimensions in the form of Myers–Perry black holes, yet an exact solution generalizing their charged extension (Kerr-Newman) to higher dimensions remains unknown in Einstein-Maxwell theory. In this talk, I will discuss this issue from the viewpoint of the (generalized) Kerr–Schild class. Time permitting,...
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Dr Eugeny Babichev (IJCLab)03/09/2025, 16:20talk
I will discuss properties of general stationary and axisymmetric spacetimes, with a particular focus on circularity - an accidental symmetry enjoyed by the Kerr metric, and therefore widely assumed when searching for rotating black hole solutions in alternative theories of gravity as well as when constructing models of Kerr mimickers. It can be shown the local existence of a Kerr-like gauge,...
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Dr Filip Hejda (CENTRA, IST, Lisbon & CEICO, FZU, Prague)03/09/2025, 17:00talk
There has been a surge of interest into collisional Penrose process after Bañados, Silk and West described an idealised edge case, in which particles coming from rest at infinity can collide with arbitrarily high centre-of-mass collision energy close to the horizon of a black hole. However, it turned out that in the vacuum case, there is an unconditional upper bound on the efficiency of...
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Georgios Kraniotis (University of Ioannina)03/09/2025, 17:20talk
In this work we compute novel analytical expressions for differential curvature invariants for accelerating Kerr-Newman black holes in (anti-)de Sitter spacetime. We explore and prove that some of the calculated frame agnostic scalar polynomial invariants (SPIs), can be used on the detection of horizon and ergosurfaces of this important class of black holes. Using the Bianchi identities we...
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Christos Ragiadakos03/09/2025, 17:40talk
Imposing the metric as the fundamental structure of the 4-dimensional spacetime, Einstein derived the gravitational interaction. If instead of the metric we assume as fundamental structure the Frobenius integrable system of geodetic and shear-free Newman-Penrose null tetrad, all the elementary particles and gauge interactions are derived. This fundamental geometric structure is called...
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Prof. Yakov Shnir03/09/2025, 18:00talk
We construct black holes in U(1) gauged scalar theories, minimally coupled to Einstein gravity in asymptotically flat space. Particular examples include non-linear O(3) sigma model, Einstein-Maxwell-Friedberg-Lee-Sirlin type model and in the Einstein-Maxwell-Skyrme theory. We analyze the properties of the hairy black holes and determine their domain of existence. Our discussion focuses mostly...
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Prof. Mauricio Valenzuela Uribe (CECs - Universidad San Sebastián)04/09/2025, 15:00talk
This talk explores the overlooked spin-1/2 sector of basic supergravity, challenging the long-standing view—present since the origins of supergravity in the late 1970s—that it is non-physical. We show that this belief arose from assuming the validity of the Dirac conjecture of the theory of constrained Hamiltonian systems. We demonstrate that the conjecture does not hold in this particular...
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Dionysios Kokkinos (Hellenic Mediterranean University)04/09/2025, 15:20talk
Algebraically general solutions in General Relativity are notably rare and less mathematically tractable compared to their algebraically special counterparts. Nevertheless, this kind of solutions is quite interesting in mathematical and physical point of view.
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In a previous study conducted in vacuum with cosmological constant under the framework of Newman-Penrose formalism, we explored an... -
Dr Marcelo Rubio (Gran Sasso Science Institute (GSSI))04/09/2025, 15:40talk
I will discuss the Cauchy problem of self-interacting massive vector fields, and explain why they often face instabilities and apparent pathologies. After showing that these issues are due to the breakdown of the well-posedness of the corresponding initial-value problem, I will characterize the well-posedness breakdowns and explicity show that they can be avoided by fixing the equations in a...
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