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

Non-linear tides and Gauss-Bonnet scalarization, L. Annulli, C. A. R. Herdeiro, Phys. Lett. B 845 (2023) 138137, arXiv:2307.10368 [gr-qc].

Publication type
Regular Articles
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 Piercing of a solitonic boson star by a black hole, Z. Zhong, V. Cardoso, T. Ikeda, M. Zilhão; arXiv:2307.02548 [gr-qc].

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Regular Articles
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Spherically symmetric elastic bodies in general relativity, A. Alho, J. Natário, P. Pani, G. Raposo; arXiv:2307.03146 [gr-qc].

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Regular Articles
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Self-interacting dipolar boson stars and their dynamics, P. Ildefonso, M. Zilhão. C. Herdeiro, E. Radu, N. M. Santos; Phys. Rev. D 108 (2023) 064011, arXiv:2307.00044 [gr-qc].

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Regular Articles
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Scale invariant elastic stars in General Relativity, A. Alho, J. Natário, P. Pani, G. Raposo; arXiv:2306.16584 [gr-qc].

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Regular Articles
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Latest Strong Gravity News & Events

Cosmological tests on non-metricity based theories of gravity​

Gr@v Seminars - Banner
Speaker
José Ferreira (University of Aveiro and CIDMA)
Event date
Venue
Hybrid: Room 11.2.21 and Zoom
Event type
In this seminar, we study and present constraints for two cosmological models based on non-metric theories of gravity, referred to as f(Q) gravity, using both current datasets and forecast Standard Siren events.
The first model is the most general f(Q) model that replicates a ΛCDM background, with deviatio