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From the 1 of 8 linked papers with an AI index.

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8 papers

physics.flu-dyn2026

Exploring 2D turbulent properties in anisotropic and disordered Fourier space: Insights into inverse cascades and universal superdiffusion from randomly sampled triadic interaction

Francesco Carbone, Sergio Servidio

The study examines how anisotropic and randomly sampled resonant triads in Fourier space influence two‑dimensional turbulence, demonstrating that the reduced model reproduces the c…

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…

astro-ph.HE2025

Supermassive black-hole imaging with a self-consistent electron-temperature prescription

Alejandro Cruz-Osorio, Claudio Meringolo, Christian M. Fromm +5

The recent 230 GHz observations by the Event Horizon Telescope have resolved the innermost structure of the M87 galaxy, revealing a ring-like feature consistent with thermal synchr…

physics.plasm-ph2025

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…

gr-qc2025

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…