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From the 1 of 5 linked papers with an AI index.

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5 papers

astro-ph.GA2026

Perturber-Driven Dynamics of Supermassive Black Hole Binaries in Galaxy Merger

Julian Chan, Alessia Gualandris, Walter Dehnen +1

The paper uses high‑resolution N‑body simulations of a major galaxy merger to test how massive perturbers in the host galaxy affect the eccentricity scatter of supermassive black h…

astro-ph.GA2026

Scaling Relations for Binary Black Hole Merger Times from Cosmological Initial Conditions

Thibaut L. Francois, Alessia Gualandris, Walter Dehnen

Recent evidence from Pulsar Timing Arrays (PTAs) for a nanohertz gravitational wave background is broadly consistent with theoretical expectations from a population of massive blac…

astro-ph.GA2026

Converging on the eccentricity of massive black hole binaries in galactic mergers

Alessia Gualandris, Justin Read, Federica Fastidio +4

Binaries of supermassive black holes (MBHBs) represent the primary sources of the gravitational wave background (GWB) detectable by Pulsar Timing Arrays (PTAs). The eccentricity wi…

astro-ph.GA2025

Black hole dragging: a new mechanism for forming nuclear star clusters in giant elliptical galaxies

Nader Khonji, Alessia Gualandris, Justin I. Read +1

It has long been thought that nuclear star clusters (NSCs) cannot co-exist with the most massive supermassive black holes (SMBHs), since SMBH mergers - unavoidable for the most mas…

astro-ph.GA2025

Realistic consecutive galaxy mergers form eccentric PTA sources

Federica Fastidio, Elisa Bortolas, Alessia Gualandris +3

Results from pulsar timing arrays (PTAs) show evidence of a gravitational wave background (GWB) consistent with a population of unresolved supermassive black hole binaries (BHBs).…