activity
20162026
most citedStability of the fundamental quasinormal mode in time-domain observations against small perturbations

99 citations · 285 across the 18 of their papers we have counts for

collaborators

20 papers

gr-qc2026

Gravitational quantum friction and the information-loss problem

Francesco Del Porro, Francesco Di Filippo

We study the gravitational collapse of a shell, modeled as a coherent state of quantum matter. Without adding any physics beyond semiclassical gravity, we show that the universal g…

gr-qc2026

Semiclassical regularity of compact trapped regions: From dynamical horizons to inner extremality

Raúl Carballo-Rubio, Francesco Di Filippo, Stefano Liberati +1

In eternal black-hole spacetimes, inner horizons are Cauchy horizons and are generically unstable. For non-extremal inner horizons, this includes both the classical mass-inflation…

gr-qc2025

Macroscopic backreaction of the trace anomaly on classical vacuum backgrounds

Raúl Carballo-Rubio, Francesco Di Filippo, Shinji Mukohyama +1

We study the backreaction of quantum fields in the Boulware vacuum state on the Schwarzschild geometry, using the Riegert--Mottola--Vaulin renormalized stress-energy tensor derived…

gr-qc2025

Imprints of quantum vacuum fluctuations on the gravitational field of a spherical mass

Raúl Carballo-Rubio, Francesco Di Filippo, Shinji Mukohyama +1

The Schwarzschild geometry, describing the gravitational field of a spherical mass in classical vacuum, is one of the most famous vacuum solutions of the Einstein field equations.…

gr-qc2024★ 9 cited

Can light-rings self-gravitate?

Francesco Di Filippo, Luciano Rezzolla

In a spherically symmetric and static spacetime of a compact object, such as that of a Schwarzschild black hole, the light-ring is a 2-sphere where photons experience the only poss…

gr-qc2024★ 5 cited

Fully extremal black holes: a black hole graveyard?

Francesco Di Filippo, Stefano Liberati, Matt Visser

While the standard point of view is that the ultimate endpoint of black hole evolution is determined by Hawking evaporation, there is a growing evidence that classical and semi-cla…