2–4 juil. 2025
Tours
Fuseau horaire Europe/Paris

Liste des Contributions

22 sur 22 affichés
Exporter en PDF
  1. Harvey Reall
    02/07/2025 10:15
  2. Eric Gourgoulhon
    02/07/2025 11:00
  3. Jose Navarro Salas
    02/07/2025 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...

    Go to contribution page
  4. Carlos Barcelo Seron
    02/07/2025 14:45
  5. Marc Mars
    02/07/2025 16:00
  6. Maxim Chernodub
    02/07/2025 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...

    Go to contribution page
  7. Barausse Enrico
    03/07/2025 09:00

    I will review how non-linearities can allow for screening solar-system
    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),...

    Go to contribution page
  8. Laura Bernard
    03/07/2025 10:15
  9. Oscar Dias
    03/07/2025 11:00

    According to the Λ-Cold Dark Matter (ΛCDM) model, a positive cosmological constant explains
    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...

    Go to contribution page
  10. Stefano Liberati
    03/07/2025 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...

    Go to contribution page
  11. Jose Luis Jaramillo
    03/07/2025 14:45
  12. Vagif Tagiev
    03/07/2025 16:00

    This presentation explores the classification of various configurations of
    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...

    Go to contribution page
  13. Mikhael Volkov
    03/07/2025 16:30
  14. Romain Gervalle
    03/07/2025 17:00
  15. Simone Speziale
    04/07/2025 09:00

    I will present a common description of null infinity and physical
    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...

    Go to contribution page
  16. Marco Astorino
    04/07/2025 10:15
  17. Yannick Herfray
    04/07/2025 11:00
  18. Pablo Bueno
    04/07/2025 14:00
  19. Panagiotis Charalambous
    04/07/2025 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...

    Go to contribution page
  20. Peter Horvathy
    04/07/2025 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.

    Go to contribution page
  21. Germain Rousseaux
  22. Scott Robertson