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20212026
most citedExtreme Gravitational Interactions in the Problem of Three Black Holes in General Relativity

8 citations · 16 across the 6 of their papers we have counts for

collaborators

6 papers

physics.plasm-ph2026

Plasma turbulence driven by wave-hole interaction

Gabriele Celebre, Mario Imbrogno, Sergio Servidio +1

Wave-obstacle diffraction is, par excellence, an example of transition to nonlinearity, generating turbulence and complexity in fluids. We present an idealized kinetic plasma regim…

astro-ph.HE2026

Particle-acceleration mechanisms in multispecies relativistic plasmas

Claudio Meringolo, Mario Imbrogno, Alejandro Cruz-Osorio +2

While collisionless plasmas are ubiquitously present near astrophysical compact objects, the impact that their composition has on the high-energy emission is presently unknown. We…

gr-qc2025★ 2 cited

Measuring the properties of homogeneous turbulence in curved spacetimes

Rita Megale, Alejandro Cruz-Osorio, Giuseppe Ficarra +5

Turbulence in curved spacetimes in general, and in the vicinity of black holes (BHs) in particular, represents a poorly understood phenomenon that is often analysed employing techn…

physics.plasm-ph2025★ 6 cited

Turbulence and Magnetic Reconnection in Relativistic Multispecies Plasmas

Mario Imbrogno, Claudio Meringolo, Alejandro Cruz-Osorio +3

Simulations of relativistic plasmas traditionally focus on the dynamics of two-species mixtures of charged particles under the influence of external magnetic fields and those gener…

physics.plasm-ph2024

Long-living Equilibria in Kinetic Astrophysical Plasma Turbulence

Mario Imbrogno, Claudio Meringolo, Sergio Servidio +3

Turbulence in classical fluids is characterized by persistent structures that emerge from the chaotic landscape. We investigate the analogous process in fully kinetic plasma turbul…

gr-qc2021★ 8 cited

Extreme Gravitational Interactions in the Problem of Three Black Holes in General Relativity

Mario Imbrogno, Claudio Meringolo, Sergio Servidio

We study the three-body problem going from Newtonian mechanics to general relativity. In the classical case, we model the interactions in a typical chaotic configuration, identifyi…