22–26 Jul 2024
Europe/Lisbon timezone

Session

Parallel session 6 (Black Holes Beyond GR)

23 Jul 2024, 14:30

Conveners

Parallel session 6 (Black Holes Beyond GR)

  • Session convener: Miguel Zilhão

Presentation materials

There are no materials yet.

  1. Marco Calza (University of Trento)
    23/07/2024, 14:30

    The literature is flourishing in exotic and theoretical black hole solutions realized in the framework of general relativity or modified gravity theories to cure the singularity affecting the vacuum solutions of general relativity.
    On the other hand, the Schwarzschild solution is the standard lore when computing constraints on primordial black hole abundance arising from the isotropic diffuse...

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  2. Pablo Bueno
    23/07/2024, 14:45

    I will show via an explicit construction how an infinite tower of higher-curvature corrections generically leads to the resolution of the Schwarzschild singularity in any spacetime dimension D≥5. The theories we consider have two key properties that ensure the results are general and robust: (1) they provide a basis for (vacuum) gravitational effective field theory in five and...

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  3. Breno L. Giacchini (Charles University)
    23/07/2024, 15:00

    Higher-derivative terms are relevant in several approaches to quantum gravity. For instance, they occur in the perturbative quantization of Einstein gravity, and they can be used to construct (super-)renormalizable quantum gravity models. In this talk, we discuss the problem of whether higher derivatives could already resolve black hole singularities at classical level. To this end, we present...

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  4. ANGEL RINCON RIVERO (Universidad de Alicante)
    23/07/2024, 15:15

    In this talk, we will study the shadow, the greybody bounding, and the QNMs of a non-singular black hole in 4-dimensional spacetime in the context of scale-dependent gravity. Our focus is on determining constraints on the scale-dependent parameter, which serves as a descriptor for the scale-dependent solution with respect to the classically observed shadow radius. We also perform an analytical...

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  5. David Lopes
    23/07/2024, 15:30

    The evolution of the event horizon in the merger of a large black hole and a small compact object can be studied exactly in the extreme mass ratio regime by tracing back a specific set of null geodesics. While this type of analysis has already been conducted for various scenarios in General Relativity, a similar study in modified theories of gravity is still missing. We study how higher-order...

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  6. Farid Thaalba
    23/07/2024, 15:45

    Many modified theories of gravity that deviate from general relativity (GR) in the vicinity of black holes or neutron stars lack a well-posed initial value problem formulation. Numerical considerations play a crucial role in solving the modified equations. Nonetheless, performing numerical simulations is only possible when the equations are well-posed. In this talk, I will focus on a single...

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