The awakening of the gravitational astronomy era, together with the ever increasing precision of electromagnetic observations, motivates scrutinizing models of alternative compact objects and their phenomenology. As a contribution to this effort, Gr@v researchers will be guest editors of a Focus issue of Classical and Quantum gravity on hairy black holes.
Abstract: The talk is devided into two parts: I will talk about the current status and the prospects of relativistic geodesy and a very interesting project related to this that is called „geoQ“.
Abstract: In this talk, I will first discuss the challenges one faces when trying to explain the observed late-time acceleration of our Universe, due to the obstacles which the yet unkown physics of dark energy and dark matter place when we try to understand the true theory of gravity at large scales. In this context, I will further explain how model-independent observables have the potential to reveal whether gravity is truly modified at large scales, and will describe a fundamental, underlying relation between large-scale modifications of gravity and the (non-trivial) propagation of gravitational waves, as well as its observational implications for cosmology and astrophysics.
The kick off meeting of the RISE network StronGrHEP, took place on May 12th-13th 2016, in the Institut d'Astrophysique de Paris. Photo: the coordinates of the five European nodes, C. Herdeiro, E. Barausse, U. Sperhake, V. Cardoso and L. Gualtieri by the statue of the great Urbain Le Verrier.
The ceremony for distinguising the recipients of the 2015 Gulbenkian Prizes for Stimulus of Research, took place on March 9th 2016, at the Gulbenkian Foundation, in Lisbon. Pedro Cunha was awarded one of the prizes for his project on "Black Hole Shadows".
Abstract: I will present our results of a series of numerical relativity simulations of dynamical nonrotating black holes surrounded by self-gravitating scalar fields. In the non-charged case, even in the non-linear regime, quasistationary configurations of scalar fields are formed around black holes.
Our group coordinated the "Numerical Relativity and High Energy Physics" IRSES network (2012-2015). Here is a list of the global network meetings organized: