activity
20172025
most citedThe Science of the Einstein Telescope

97 citations · 303 across the 12 of their papers we have counts for

collaborators

12 papers

gr-qc2025★ 97 cited

The Science of the Einstein Telescope

Adrian Abac, Raul Abramo, Simone Albanesi +485

Einstein Telescope (ET) is the European project for a gravitational-wave (GW) observatory of third-generation. In this paper we present a comprehensive discussion of its science ob…

gr-qc2024★ 7 cited

Integrability in Perturbed Black Holes: Background Hidden Structures

José Luis Jaramillo, Michele Lenzi, Carlos F. Sopuerta

In this work we investigate the presence of integrable hidden structures in the dynamics of perturbed non-rotating black holes (BHs). This can also be considered as a first step in…

gr-qc2024

Gauge-Independent Metric Reconstruction of Perturbations of Vacuum Spherically-Symmetric Spacetimes

Michele Lenzi, Carlos F. Sopuerta

Perturbation theory of vacuum spherically-symmetric spacetimes (including the cosmological constant) has greatly contributed to the understanding of black holes, relativistic compa…

gr-qc2023★ 12 cited

Black Hole Greybody Factors from Korteweg-de Vries Integrals: Computation

Michele Lenzi, Carlos F. Sopuerta

It has recently been shown that the dynamics of perturbed non-rotating black holes (BHs) admits an infinite number of symmetries that are generated by the flow of the Korteweg-de V…

gr-qc2022★ 15 cited

Black Hole Greybody Factors from Korteweg-de Vries Integrals: Theory

Michele Lenzi, Carlos F. Sopuerta

The dynamics of perturbed non-rotating black holes (BHs) can be described in terms of master equations of the wave type with a potential. In the frequency domain, the master equati…

gr-qc2021★ 1 cited

Master Functions and Equations for Perturbations of Vacuum Spherically-Symmetric Spacetimes

Michele Lenzi, Carlos F. Sopuerta

Perturbation theory of vacuum spherically-symmetric spacetimes is a crucial tool to understand the dynamics of black hole perturbations. Spherical symmetry allows for an expansion…