Strong Gravity News & Events

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Prospects for multi-probe cosmology as gravity and inflation probes

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Speaker
Jose Fonseca (Instituto de Astrofísica e Ciências do Espaço)
Event date
Venue
Hybrid Sala Sousa Pinto (Math dpt) and Zoom
Event type

The next decade will see an overwhelming number of cosmological surveys coming online. The Square Kilometre Array Observatory (SKAO) will, among several other science cases, map the distribution of cold neutral Hydrogen in the Universe using its spin-flip transition emission line at rest of 21cm or 1.4GHz and a novel technique called Intensity Mapping (IM).

Meeting with a scientist

 

Gr@v member Miguel Zilhão was the guest for the activity "Meeting with a scientist", organized by the outreach centre Fábrica.The audience was a group of 4th grade students from the Primary Schools of Glória and São Jacinto. They were all very curious about the Universe and asked a lot of interesting questions.

 

 

Discussion of the paper "Fuzzball Shadows: Emergent Horizons from Microstructure", by Fabio Bacchini, et al.

Speaker
Luís F. M. A. M. Reis (UFRN, Brasil)
Event date
Venue
Sala 11.2.21 and online
Ends on
Event type

Fuzzball Shadows: Emergent Horizons from Microstructure

Fabio Bacchini, Daniel R. Mayerson, Bart Ripperda, Jordy Davelaar, Héctor Olivares, Thomas Hertog and Bert Vercnocke

arXiv:2103.12075[gr-qc]

Research grant in Strong Gravity for M.Sc. holders

A call for one 1-year research grant in Strong Gravity for M.Sc. holders enrolled in a doctoral programme at Aveiro University, within the research grant “Gravitational waves and black holes as ultralight dark matter particle detectors", CERN/FIS-PAR/0024/2021, is open from 20 March to 10 April 2023.  See attached document for details (in Portuguese) or the Euraxess announcement (in English) here.

Challenging black-hole spectroscopy: quasinormal modes, spectral instabilities and the pseudospectrum

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Speaker
Kyriakos Destounis (Sapienza University of Rome - INFN - IAAT Tuebingen)
Event date
Venue
Online (only)
Event type

Black hole spectroscopy is a powerful tool to probe the Kerr nature of astrophysical compact objects and their environment.