Strong Gravity News & Events

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Numerical black hole perturbation theory

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Speaker
Lidia Gomes da Silva (QMUL, London)
Event date
Venue
On-site: Room 11.2.21
Event type
Extreme-Mass-Ratio-Inspirals (EMRIs) modelling in time-domain has been anything but trivial due to the challenges associated with resolving the discontinuity emerging from the point-particle model

Detecting environmental effects

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Speaker
Laura Sberna (Albert Einstein Institute, Potsdam)
Event date
Venue
Online only
Event type

Gravitational-wave observations of extreme mass ratio inspirals (EMRIs) hold incredible potential to probe gravity, astrophysical and exotic environments. One of the main effects of astrophysical environments — in particular active galactic nuclei — is the torque exerted by their gaseous disk, which forces EMRIs to “migrate” (mostly) inward like planets.

Primordial Black Holes from Inflation: recent challenges and opportunities in the GW era

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Speaker
Gabriele Franciolini (Sapienza University)
Event date
Venue
Online only
Event type

Primordial black holes (PBHs) might form in the early universe and could comprise a significant fraction of the dark matter. If they are generated due to enhanced scalar perturbations at small scales, their formation is inevitably accompanied by the emission of gravitational waves (GWs) that could be seen by current and future GW experiments.

Black hole binaries in ultralight dark matter environments

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Speaker
Rodrigo Vicente (IFAE, Barcelona)
Event date
Venue
Hybrid: Room 11.2.21 and Zoom
Event type

Ultralight dark matter is an exciting alternative to the standard cold dark matter paradigm, reproducing its large scale predictions, while solving most of its potential tension with small scale observations (like the "cusp-core" and "missing satellites" problems).