Strong Gravity
The group's research on strong gravity involves finding analytical and numerical solutions of Einstein's theory of general relativity, and many of its extensions, either in vacuum or coupled to various types of matter. For our latest developments/activities in this area, please see the listing at the end of this article.
The prime examples of (relativistic) strong gravitational systems are Black Holes. They are truly unifying objects of all physics. The understanding of their formation and dynamics requires the laws of all four fundamental forces, and their physics is relevant not only for astrophysics and cosmology but for a variety of topics within high energy physics.
See here a movie made by the COST action `Black holes in a violent universe', in which our group participates, for a visual overview of different types of black holes.
Latest Strong Gravity News & Events
The optical appearance of some regular compact objects
Discussion of the paper "Primordial black hole capture, gravitational wave beats, and the nuclear equation of state", by Thomas W. Baumgarte, and Stuart L. Shapiro
Primordial black hole capture, gravitational wave beats, and the nuclear equation of state
Thomas W. Baumgarte, Stuart L. Shapiro
Hairy black holes induced by nonlinear superadiant instability
Hairy black holes induced by nonlinear superadiant instability
Cheng-Yong Zhang, Qian Chen, Yuxuan Liu, Yu Tian, Bin Wang
arXiv:2309.05045 [gr-qc]
Confinement of exotic energy
By solving the Einstein's field equations, we derive several
configurations of compact objects with a nucleus of exotic energy in a
static and spherically symmetric spacetime. In this talk I describe the
derivation and several properties of the configurations, including the
fact that in some of these objects can be reached a compacity as close to