activity
20202026
most citedRelativistic perturbation theory for black-hole boson clouds

35 citations · 108 across the 21 of their papers we have counts for

collaborators

21 papers

gr-qc2026

Revisiting environmental effects on black hole quasibound-state spectra with relativistic perturbation theory

Yin-Da Guo, Qi-Xuan Xu, Richard Brito +1

We present a relativistic framework for computing corrections to the eigenfrequency spectrum of a massive scalar field in perturbed black-hole spacetimes, including first-order shi…

gr-qc2026

Dynamical quasinormal mode excitation II: propagation and convergence in Schwarzschild

Marina De Amicis, Enrico Cannizzaro, Gregorio Carullo +2

We study the dynamical excitation of quasinormal modes (QNMs) during the plunge of a particle into a Schwarzschild black hole, building on the framework of Phys. Rev. D 113 (2026)…

hep-ph2026

Simulating Axion Electrodynamics in Magnetized Plasmas: Energy transfer in the inhomogeneous and strongly varying limit

Fabrizio Corelli, Estanis Utrilla Ginés, Enrico Cannizzaro +2

In this work we study the electromagnetic response induced by axions in a magnetized plasma, focusing specifically on characterizing energy transfer and energy losses from the ambi…

gr-qc2026

Post-Minkowskian expansion of the Prompt Response in a Schwarzschild background

Marina De Amicis, Enrico Cannizzaro

We study the early-time component of the Green's function of a Schwarzschild black hole, traveling on the curved light cone and usually denoted as the prompt response. Working in a…

gr-qc2025

Excitation of scalar quasi-normal modes from boson clouds

Enrico Cannizzaro, Marco Palleschi, Laura Sberna +2

Massive scalar fields on black hole backgrounds generally admit two families of modes: quasi-bound states (QBS) and quasinormal modes (QNM). We demonstrate the orthogonality betwee…

gr-qc2025★ 14 cited

Dynamical quasinormal mode excitation

Marina De Amicis, Enrico Cannizzaro, Gregorio Carullo +1

We study the dynamical excitation of quasinormal modes (QNMs) through the plunge, merger and ringdown of an extreme-mass-ratio-inspiral into a Schwarzschild black hole, for generic…

astro-ph.GA2025★ 6 cited

In the grip of the disk: dragging the companion through an AGN

Thomas F. M. Spieksma, Enrico Cannizzaro

Active galactic nuclei (AGN) have been proposed as environments that can facilitate the capture of extreme-mass-ratio binaries and accelerate their inspiral beyond the rate expecte…

hep-ph2025

Axion dissipation in conductive media and neutron star superradiance

Thomas F. M. Spieksma, Enrico Cannizzaro

In axion electrodynamics, magnetic fields enable axion-photon mixing. Recent proposals suggest that rotating, conductive plasmas in neutron star magnetospheres could trigger axion…

hep-ph2024

Beyond The Standard Model electrodynamics in the time domain

Fabrizio Corelli, Enrico Cannizzaro, Andrea Caputo +1

Many motivated extensions of the standard model include new light bosons, such as axions and dark photons, which can mix with the ordinary photon. This latter, when in a dilute pla…

astro-ph.HE2024

Tidal deformability of black holes surrounded by thin accretion disks

Enrico Cannizzaro, Valerio De Luca, Paolo Pani

The tidal Love numbers of self-gravitating compact objects describe their response to external tidal perturbations, such as those from a companion in a binary system, offering valu…

gr-qc2024

Impact of a plasma on the relaxation of black holes

Enrico Cannizzaro, Thomas F. M. Spieksma, Vitor Cardoso +1

Our universe is permeated with interstellar plasma, which prevents propagation of low-frequency electromagnetic waves. Here, we show that two dramatic consequences arise out of suc…

hep-ph2024

Phenomenology of ultralight bosons around compact objects: in-medium suppression

Enrico Cannizzaro, Thomas F. M. Spieksma

Mixing between ultralight bosons and the Standard Model photon may allow access to the hitherto invisible Universe. In the presence of plasma, photons are dressed with an effective…

gr-qc2023

Extreme mass-ratio inspirals as probes of fundamental dipoles

Jacopo Lestingi, Enrico Cannizzaro, Paolo Pani

Even if globally neutral, in various scenarios compact objects can have a nonvanishing dipole moment. Examples include neutron stars with magnetic dipoles, black-hole microstates i…

gr-qc2023★ 35 cited

Relativistic perturbation theory for black-hole boson clouds

Enrico Cannizzaro, Laura Sberna, Stephen R. Green +1

We develop a relativistic perturbation theory for scalar clouds around rotating black holes. We first introduce a relativistic product and corresponding orthogonality relation betw…

gr-qc2023★ 1 cited

Novel tests of gravity using nano-Hertz stochastic gravitational-wave background signals

Enrico Cannizzaro, Gabriele Franciolini, Paolo Pani

Gravity theories that modify General Relativity in the slow-motion regime can introduce nonperturbative corrections to the stochastic gravitational-wave background~(SGWB) from supe…

gr-qc2023

Superradiance: Axionic Couplings and Plasma Effects

Thomas F. M. Spieksma, Enrico Cannizzaro, Taishi Ikeda +2

Spinning black holes can transfer a significant fraction of their energy to ultralight bosonic fields via superradiance, condensing them in a co-rotating structure or "cloud". This…

gr-qc2023

Nonlinear photon-plasma interaction and the black hole superradiant instability

Enrico Cannizzaro, Fabrizio Corelli, Paolo Pani

Electromagnetic field confinement due to plasma near accreting black holes can trigger superradiant instabilities at the linear level, limiting the spin of black holes and providin…

hep-ph2022★ 13 cited

Dark photon superradiance quenched by dark matter

Enrico Cannizzaro, Laura Sberna, Andrea Caputo +1

Black-hole superradiance has been used to place very strong bounds on a variety of models of ultralight bosons such as axions, new light scalars, and dark photons. It is common lor…

gr-qc2022★ 9 cited

Superradiant instabilities by accretion disks in scalar-tensor theories

Giuseppe Lingetti, Enrico Cannizzaro, Paolo Pani

We study the superradiant instability in scalar-tensor theories of gravitation, where matter outside a black hole provides an effective mass to the scalar degree of freedom of the…

gr-qc2021

Plasma-photon interaction in curved spacetime II: collisions, thermal corrections, and superradiant instabilities

Enrico Cannizzaro, Andrea Caputo, Laura Sberna +1

Motivated by electromagnetic-field confinement due to plasma near accreting black holes, we continue our exploration of the linear dynamics of an electromagnetic field propagating…

gr-qc2020★ 30 cited

Plasma-photon interaction in curved spacetime I: formalism and quasibound states around nonspinning black holes

Enrico Cannizzaro, Andrea Caputo, Laura Sberna +1

We investigate the linear dynamics of an electromagnetic field propagating in curved spacetime in the presence of plasma. The dynamical equations are generically more involved and…