activity
20202026
most citedCosmological coupling of nonsingular black holes

34 citations · 91 across the 13 of their papers we have counts for

collaborators

13 papers

gr-qc2026

Cosmologically Coupled Black Holes with Regular Horizons

Mariano Cadoni, Leonardo de Lima, Mirko Pitzalis +2

We present the most general and exact solution of Einstein's gravity sourced by an anisotropic fluid describing the cosmological embedding (CE) of a static and spherically-symmetri…

gr-qc2025

Stable Wormholes in Conformal Gravity

Mariano Cadoni, Leonardo Modesto, Mirko Pitzalis +1

We present a class of Lorentzian traversable wormholes in conformal gravity, constructed via Weyl rescaling of Minkowski spacetime. As a result, these wormholes are solutions of ev…

gr-qc2025

Deriving the paradox: original derivation of Hawking radiation

Mariano Cadoni, Salvatore Mignemi, Mirko Pitzalis +1

We revisit Hawking's original derivation of the evaporation process in a non-stationary spacetime, presenting it in a clear and pedagogical manner, with a focus on the spherical co…

physics.ed-ph2025★ 1 cited

The Role of Conceptual Problem Solving in Learning Physics: A Study in a General Relativity University Course

Matteo Tuveri, Andrea Pierfrancesco Sanna, Mariano Cadoni

Effective physics learning, especially in complex topics, requires balancing mathematical formalism with conceptual understanding. Conceptual problem-solving involves connecting ma…

gr-qc2024

Apparent horizons in cosmologically-embedded black holes

Mariano Cadoni, Mirko Pitzalis, Andrea Pierfrancesco Sanna

We present exact solutions for the cosmological embedding of a broad class of non-singular black holes, demonstrating that these objects exhibit an apparent horizon. The evolution…

gr-qc2024★ 1 cited

Effective Quantum Spacetimes from Functional Renormalization Group

Alfio Bonanno, Mariano Cadoni, Mirko Pitzalis +1

Using the Functional Renormalization Group approach we construct effective quantum spacetime geometries by self-consistently deforming the classical Schwarzschild-de Sitter black-h…

gr-qc2024

Nucleation of de Sitter from the anti de Sitter spacetime in scalar field models

Mariano Cadoni, Mirko Pitzalis, Andrea P. Sanna

We show that, in the framework of Einstein-scalar gravity, the gravitational coupling can drive the nucleation of the de Sitter (dS) spacetime from an anti de Sitter (AdS) one. Thi…

gr-qc2024

Cosmological coupling of local gravitational systems

Mariano Cadoni, Mirko Pitzalis, Davi C. Rodrigues +1

We investigate the cosmological coupling of spherical, local astrophysical systems. We derive a general formula quantifying the cosmological coupling of the Misner-Sharp mass of th…

gr-qc2023

Scalar stars and lumps with (A)dS core

Mariano Cadoni, Mauro Oi, Mirko Pitzalis +1

We explore the possibility of embedding regular compact objects with (anti) de Sitter ((A)dS) core as solutions of Einstein's gravity minimally coupled to a real scalar field. We c…

gr-qc2023★ 22 cited

Quasi-local masses and cosmological coupling of black holes and mimickers

Mariano Cadoni, Riccardo Murgia, Mirko Pitzalis +1

Motivated by the recent heated debate on whether the masses of local objects, such as compact stars or black holes (BHs), may be affected by the large-scale, cosmological dynamics,…

gr-qc2023★ 34 cited

Cosmological coupling of nonsingular black holes

M. Cadoni, A. P. Sanna, M. Pitzalis +4

We show that -- in the framework of general relativity (GR) -- if black holes (BHs) are singularity-free objects, they couple to the large-scale cosmological dynamics. We find that…

gr-qc2022★ 31 cited

Are nonsingular black holes with super-Planckian hair ruled out by S2 star data?

M. Cadoni, M. De Laurentis, I. De Martino +3

We propose a novel nonsingular black-hole spacetime representing a strong deformation of the Schwarzschild solution with mass by an additional hair , which may be hierarc…

gr-qc2020★ 2 cited

Long-Range Quantum Gravity

M. Cadoni, M. Tuveri, A. P. Sanna

It is a tantalising possibility that quantum gravity (QG) states remaining coherent at astrophysical, galactic and cosmological scales could exist and that they could play a crucia…