activity
20082026
most citedTesting General Relativity with Present and Future Astrophysical Observations

1.5k citations · 5.3k across the 75 of their papers we have counts for

collaborators

76 papers

hep-th2026

Turbulent gravitational wakes

Giulio Taiocchi, Christiana Pantelidou, Miguel Zilhão

We construct turbulent gravitational wakes in asymptotically AdS spacetimes by solving the full non-linear Einstein equations in the characteristic formulation. Specifically, w…

gr-qc2026

Electromagnetic duality degeneracy in dynamical black hole mergers

José Ferreira, Gabriele Bozzola, Carlos A. R. Herdeiro +2

Electromagnetic duality is a symmetry of the source-free Einstein-Maxwell equations that rotates electric and magnetic fields while leaving the stress-energy tensor invariant. We p…

gr-qc2026

Spontaneous spherical symmetry breaking of black holes with resonant hair

José Ferreira, Carlos A. R. Herdeiro, Eugen Radu +1

Black holes with resonant hair are static, spherical, electrically charged solutions of the Einstein-Maxwell-(gauged-)scalar system. Scalar self-interactions are mandatory for thei…

gr-qc2025★ 3 cited

Splitting the Gravitational Atom: Instabilities of Black Holes with Synchronized or Resonant Hair

Jordan Nicoules, José Ferreira, Carlos A. R. Herdeiro +2

Black holes (BHs) with synchronized bosonic hair challenge the Kerr paradigm, linking superradiance from ultralight fields -- creating gravitational atoms -- to bosonic stars acros…

gr-qc2025★ 1 cited

Dancing in the dark: probing Dark Matter through the dynamics of eccentric binary pulsars

Giorgio Nicolini, Andrea Maselli, Miguel Zilhão

We investigate the dynamics of eccentric binary pulsars embedded in dark matter environments. While previous studies have primarily focused on circular orbits in collisionless dark…

gr-qc2025★ 4 cited

Stability and collisions of excited spherical boson stars: glimpses of chains and rings

Marco Brito, Carlos Herdeiro, Eugen Radu +2

Scalar, spherically symmetric, radially excited boson stars were previously shown to be stabilized, against spherical dynamics, by sufficiently strong self-interactions. Here, we f…