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Harvey Reall02/07/2025 10:15
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Eric Gourgoulhon02/07/2025 11:00
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Jose Navarro Salas02/07/2025 14:00
We analyze the semiclassical geometry of two-dimensional (CGHS) black holes in the Boulware vacuum. In this state, the expectation value of the stress-energy tensor is singular at the classical horizon. However, when backreaction effects are taken into account, the resulting geometry becomes horizonless and takes the form of a non-symmetric wormhole, featuring a curvature singularity beyond...
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Carlos Barcelo Seron02/07/2025 14:45
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Marc Mars02/07/2025 16:00
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Maxim Chernodub02/07/2025 16:45
Recent first-principles lattice simulations of SU(N) Yang-Mills theory in 3+1 dimensions have revealed that the gluon plasma—a precursor to the quark-gluon plasma believed to have existed in the early Universe—exhibits several unexpected equilibrium properties under extreme conditions: (i) a negative moment of inertia within a certain temperature range; (ii) the formation of a...
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Barausse Enrico03/07/2025 09:00
I will review how non-linearities can allow for screening solar-system
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scales from non-tensorial gravitational polarizations, focusing on the
case of scalar-tensor theories with derivative self-interactions
(K-essence). I will then present fully relativistic simulations in
these theories in 1+1 dimensions (stellar oscillations and collapse)
and 3+1 dimensions (binary neutron stars),... -
Laura Bernard03/07/2025 10:15
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Oscar Dias03/07/2025 11:00
According to the Λ-Cold Dark Matter (ΛCDM) model, a positive cosmological constant explains
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the accelerated expansion of the Universe. We start by constructing a static solution of general
relativity with a positive cosmological constant that consists of two (or more) static black holes
whose gravitational attraction is balanced by the cosmic expansion of the de Sitter background.
Then, we... -
Stefano Liberati03/07/2025 14:00
The standard paradigm of black holes, rooted in Einstein's General Relativity, predicts the existence of singularities. However, the emergence of quantum gravity candidates and new observational technologies have opened the door to exploring regular black holes and black hole mimickers as viable alternatives. These non-singular solutions, which replace the central singularity with a...
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Jose Luis Jaramillo03/07/2025 14:45
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Vagif Tagiev03/07/2025 16:00
This presentation explores the classification of various configurations of
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non-symmetric black hole mimickers, limited by the conditions
of spacetime regularity and geodesic completeness. For physically viable models, test metrics will be presented, and their parameters will
be analyzed in light of observational data from black hole shadow
experiments. Furthermore, scalar perturbations... -
Mikhael Volkov03/07/2025 16:30
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Romain Gervalle03/07/2025 17:00
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Simone Speziale04/07/2025 09:00
I will present a common description of null infinity and physical
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horizons, highlighting the geometric properties they share, and the
origin of the radically different physics they describe. The common
description offers new perspectives on the different symmetry groups
considered at finite distance. I will then show how ambiguities in the
construction of charges from Noether's theorem... -
Marco Astorino04/07/2025 10:15
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Yannick Herfray04/07/2025 11:00
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Pablo Bueno04/07/2025 14:00
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Panagiotis Charalambous04/07/2025 14:45
Exact continuous symmetries play a central role in constraining black hole dynamics. In this talk, I will discuss two examples of non-exact or non-continuous enhanced black hole symmetries that also have physical implications. One is the manifestation of SL(2,R) symmetries within the near-zone region, a region that extends beyond the near-horizon regime and has a non-empty overlap with the far...
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Peter Horvathy04/07/2025 16:00
The displacement of particles hit by a burst of gravitation waves called the Memory Effect, proposed by Braginski, Thorne, Zel'dovich, Polnarev, and others, is studied. The original proposal of Gibbons and Hawking admits only numerical solutions, however ingeneous approximations of the wave profile allow to find analytic solutions.
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Germain Rousseaux
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Scott Robertson
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