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20242026
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astro-ph.GA2026

Emulating the complex galactic-scale orbital dynamics of LISA massive black hole pairs with normalizing flows

Pedro R. Capelo, Carlos Moreno Martinez, Nodens Koren +6

The paper introduces a machine‑learning emulator based on conditional normalizing flows to rapidly predict the orbital decay of massive black hole pairs in galaxy merger remnants,…

astro-ph.GA2026

Unveiling the properties of galaxy cores excavated by supermassive black hole binaries with SHARP

E. Bortolas, E. Portaluri, E. Dalla Bonta' +3

Massive black hole (MBH) binaries form as a result of galaxy mergers and can coalesce into a single MBH by emitting gravitational waves detectable by LISA and pulsar timing array c…

astro-ph.GA2026

A new era for Dual AGN science with SHARP

P. Severgnini, C. Vignali, A. De Rosa +21

The search for and the characterization of ultra-compact dual active galactic nuclei (AGN) are among the hottest topics of current extragalactic astrophysics. These systems involve…

astro-ph.GA2026

The LISA Astrophysics MBHcatalogues Project: A comparison of predictions of simulated massive black hole binaries

David Izquierdo-Villalba, Melanie Habouzit, Matteo Bonetti +67

In the hierarchical paradigm of galaxy formation, central massive black holes (MBHs) are expected to coalesce after the merger of their host galaxies. One of the main goals of the…

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).…