Ilaria Andrei

- B.Sc. in Physics, University of Trento, 2017

Both for studies of cosmic censorship and for practical purposes in gravitational wave astronomy, it is desirable to include future null-infinity in the computational domain. Extending formulations of general relativity known to behave well in the strong-field regime out to infinity with compactification is, however, a subtle game.
Equatorial EMRIs in KBHsSH Spacetimes
Lucas G. Collodel, Daniela D. Doneva, and Stoytcho S. Yazadjiev
arXiv:2108.11658 [gr-qc]
Great COST Advanced School on the physics of dark matter and the hidden sector, at Lund, Sweeden, co-organized by A. Morais. In the photo the Gr@v team members that attended the school with some close collaborators.
Despite the plethora of evidence of the existence and abundance of dark matter we have from large scale cosmological observations, there is still little we know of its properties or its behaviour on small scales. A promising way to test this is through the effects it may have on the gravitational wave signal from black hole binary mergers.
I summarize theoretical findings, astrophysical modeling, and current gravitational-wave evidence of hierarchical stellar-mass black-hole mergers.
P. Cunha was one of the invited speakers of the workshop "Regular black holes in quantum gravity and beyond: from theory to shadow observations", held from October 18-21, 2021.
Are you interested in doing research in topics such as black hole physics/mathematics, gravitational waves, numerical relativity, cosmology and high energy particle physics? Do you have (or are you finishing) a M.Sc. degree in Physics or Maths?
If so, and you would like pursue a PhD at Gr@v, there's a few steps you need to follow.
The warp drive: hyper-fast travel within general relativity
Miguel Alcubierre
Class. Quant. Grav. 11 (1994) L73-L77