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 Publications

General relativistic quasi-spherical accretion in a dark matter halo, R. Ranjbar, H. R. Olivares-Sánchez; arXiv:2502.12072 [astro-ph.HE]

Publication type
Regular Articles
Read more

Bondi-like Accretion Flow Dynamics: The Role of Gravitational Potential, R. Ranjbar, H. R. Olivares-Sánchez, S. Abbassi; arXiv:2502.12101 [astro-ph.HE]

Publication type
Regular Articles
Read more

Spinning generalizations of Majumdar-Papapetrou multi-black hole spacetimes: light rings, lensing and shadows, Z. S. Moreira, C. A. R. Herdeiro, L. C. B. Crispino; arXiv:2502.01759 [gr-qc].

Publication type
Regular Articles
Read more

The persistent shadow of the supermassive black hole of M87 II. Model comparisons and theoretical interpretations, K. Akiyama et al. (w/ H. Olivares); Astron. Astrophys. 693 (2025) A265

Publication type
Regular Articles
Read more

Bifurcations in Bosonic Stars: chains and rings from spherical solutions, C. Liang, C. A. R. Herdeiro, E. Radu; arXiv:2501.05342 [gr-qc]

Publication type
Regular Articles
Read more

Latest Strong Gravity News & Events

TBA

Speaker
Manuel Mariano (U. Aveiro)
Event date
Venue
Hybrid: Room Sousa Pinto and Zoom
Ends on
Event type

An Overview of the magnetized advective flows around black holes

GGD - Gr@V seminar
Speaker
Samik Mitra (Indian Institute of Technology Guwahati)
Event date
Venue
Online only
Event type

One of the most efficient energy sources in the universe is the matter accretion onto compact objects, such as black holes (BHs) and neutron stars (NSs). Since magnetic fields are ubiquitous everywhere, the accretion flow is expected to be magnetized in nature, where the large-scale magnetic fields inside the disks are commonly rooted either from the companion star or the interstellar medium.