Conveners
Session 12
- Chair: Lucien Heurtier
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Robyn Munoz (University of Sussex)19/06/2024, 15:10
We look into whether the spherical collapse model is a good approximation in a numerical relativity cosmological simulation and describe the spacetime’s evolution during nonlinear collapse. In the simulation, we evolve a quasi-spherical structure, where fully nonlinear initial conditions are provided by perturbing the ΛCDM model with the comoving curvature perturbation, defined as a 3D...
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Michael Zantedeschi (Tsung-Dao Lee Institute, Shanghai, China)19/06/2024, 15:30
The essence of the \textit{memory burden} effect is that a load of information carried by a system stabilizes it. This universal effect is especially prominent in systems with a high capacity of information storage, such as black holes and other objects with maximal microstate degeneracy, the entities universally referred to as \textit{saturons}. The phenomenon has several implications. The...
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Ms Anjali Abirami Kugarajh (Gran Sasso Science Institute)19/06/2024, 15:50
Observations of gravitational waves (GW) from mergers of binary black holes has opened up a new door into cosmology. Due to their weak interaction with matter, we hope to observe Primordial GWs among the various signals that are expected from current and future-generation detectors. This offers a new and exciting opportunity to explore the physics of the early Universe. Quantum vacuum...
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Jessica Turner (IPPP, Durham University)19/06/2024, 16:00