TBA
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.
Spontaneous spherical symmetry breaking of black holes with resonant hair, J. Ferreira, C. A. R. Herdeiro, E. Radu, M. Zilhão; arXiv:2604.22437 [gr-qc].
Detection of a second jet within the nuclear core of Mrk 501, S. Britzen, H. Olivares, Gopal-Krishna, F. Jaron, I. N. Pashchenko, E. Kun, F. K. Schinzel, J. Becerra González, D. Paneque, N. R. MacDonald; Monthly Notices of the Royal Astronomical Society (2026) stag291.
Phase Structure of Scalarized Black Holes in Einstein-Scalar-Gauss-Bonnet Gravity, C. Herdeiro, H. Huang, J. Kunz, M. Lai, E. Radu, D. Zou; arXiv:2603.24164 [gr-qc].
The two shadows of a single black hole: Vacuum birefringence phenomena within Einstein-Nonlinear-Electrodynamics, M. A. A. de Paula, H. C. D. Lima, P. V. P. Cunha, C. A. R. Herdeiro, L. C. B. Crispino; arXiv:2603.17007 [gr-qc]
The imitation game (r)evolutions: Q-star effective shadow from GRMHD analysis, V. Jaramillo, L. Meneses, H. R. Olivares Sánchez, C. Herdeiro, D. Núñez, Shuang-Yong Zhou; arXiv:2603.16995 [gr-qc]
I will discuss the first 3D-general relativistic magnetohydrodynamic (GRMHD) simulation of sustained accretion onto a horizonless singularity in which matter falls onto the central object rather than being accumulated outside of it or expelled in outflows.
Inspired by noncommutative geometry in string theory, we introduce extended derivatives in black hole physics by incorporating a real antisymmetric rank-2 tensor, exhibiting similarities with certain string-theoretic fields.
In this talk, I describe in detail how one might understand the termination of the event horizon of a black hole in terms of of quasiregular singularity characterized by points possessing two future-directed light cones and two past-directed light cones (in fact this spacetime is conformal to a region of the 1+1 trousers spacetime).
Gr@v is hosting the visits of Yasha Shnir, long time group collaborator, under an FCT mobility grant, and Mario Luciano Navarro, Ph.D. student from Valencia in the spring 2026. In the photo Yasha and Mario enjoy a bit of sunshine after the weekly group lunch.