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researcher

Antonio J. Iovino

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author3

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • gr-qc2
  • astro-ph.CO1
ORCID 0000-0002-8531-5962

identity via Semantic Scholar / OpenAlex

activity
20232025
most citedWhat is the source of the PTA GW signal?

1 citations · 1 across the 3 of their papers we have counts for

collaborators

3 papers

gr-qc2025

From new physics to a running power law and back again: Minimal refitting techniques for the reconstruction of the gravitational-wave background signal in pulsar timing array data

David Esmyol, Antonio J. Iovino, Kai Schmitz

Pulsar timing array (PTA) collaborations recently presented evidence for a gravitational-wave background (GWB) signal at nanohertz frequencies. In this paper, we introduce new refi…

gr-qc2024

Deciphering the Instability of the Black Hole Ringdown Quasinormal Spectrum

A. Ianniccari, A. J. Iovino, A. Kehagias +4

The spectrum of the quasinormal modes of the gravitational waves emitted during the ringdown phase following the merger of two black holes is of primary importance in gravitational…

astro-ph.CO2023★ 1 cited

What is the source of the PTA GW signal?

John Ellis, Malcolm Fairbairn, Gabriele Franciolini +7

The most conservative interpretation of the nHz stochastic gravitational wave background (SGWB) discovered by NANOGrav and other Pulsar Timing Array (PTA) Collaborations is astroph…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.