Strong Gravity News & Events
Hybrid metric-Palatini gravity: applications to cosmology and astrophysics
In this work, we study cosmological and astrophysical applications of the recently proposed generalized hybrid metric-Palatini gravity theory, which combines features of both the metric and th
Quasinormal modes of neutron stars in R^2 gravity
Spontaneous Scalarization in general Scalar-Vector-Tensor theory
Tidal effect on scalar cloud
Visit of Nelson Eiró, Aichen Li and Ruyong Li
Nelson Eiró visited Gr@v just before successfully defending his M.Sc. thesis on "Strong lensing of light and shadow of a Black Hole surrounded by a heavy accretion disk", at IST-Lisbon, supervised by C. Herdeiro and P. Cunha. This visit coincided with the beginning of a long term visit by Aichen and Ruyong Li, both graduates from Beijing University of Technology.
Visit of Nico Sanchis-Gual and Nuno Santos
Nico Sanchis-Gual and Nuno Santos visited Gr@v. Nico gave a seminar on "Non-linear dynamics of spinning bosonic stars: formation and stability". Nuno, an IST graduate, will join Gr@v as a PhD student in 2020, having been the top ranked candidate in the 2019 Individual FCT grant call in the Physics panel.
COST Workshop - "Astrometry and gravitation - A dynamical view of the sky"
In the framework of the COST action MW-Gaia, related with the Gaia (ESA) mission, for which Gr@v member Sonia Anton serves as MC member, a 3-days workshop on "Astrometry and gravitation - A dynamical view of the sky" is being organised on 4-6 December 2019, at the Observatoire de la Côte d’Azur, Mont Gros site, Nice, France. More info here.
Nonlinear eigenmodes of asymptotically anti de Sitter space-times
I present a review on combined numerical and analytical efforts to construct "geon"-type solutions of the Einstein equations. Geons are time periodic - hence non-radiating - and spatially localized objects.
Non-linear dynamics of spinning bosonic stars: formation and stability
Spherical boson and Proca stars have been extensively studied in the non-linear regime, but no numerical simulations of rotating bosonic stars have been performed.