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From the 1 of 7 linked papers with an AI index.

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7 papers

astro-ph.IM2026

Assessing the Impact of Instrumental Requirements on the Scientific Performance of the Einstein Telescope

Ulyana Dupletsa, Francesco Iacovelli, Mikhail Korobko +23

The paper evaluates how different design choices and noise characteristics of the Einstein Telescope affect its ability to detect and analyze various gravitational‑wave sources, us…

astro-ph.HE2026

The impact of stellar binaries and star cluster dynamics on pair-instability supernovae

Francesco Gabrielli, Cristiano Ugolini, Lavinia Paiella +12

Pair-instability supernovae (PISNe) are among the most luminous transients in the Universe. However, they have never been confidently observed. Solving this puzzle would have key i…

gr-qc2026

Comparing astrophysical models to gravitational-wave data in the observable space

Alexandre Toubiana, Davide Gerosa, Matthew Mould +9

Comparing population-synthesis models to the results of hierarchical Bayesian inference in gravitational-wave astronomy requires a careful understanding of the domain of validity o…

astro-ph.GA2025

Assembling GW231123 in star clusters through the combination of stellar binary evolution and hierarchical mergers

Lavinia Paiella, Cristiano Ugolini, Mario Spera +2

GW231123 is the most massive binary black hole (BBH) merger detected to date by the LIGO-Virgo-KAGRA collaboration. With at least one black hole (BH) in the upper-mass gap and both…

gr-qc2025

The Science of the Einstein Telescope

Adrian Abac, Raul Abramo, Simone Albanesi +485

Einstein Telescope (ET) is the European project for a gravitational-wave (GW) observatory of third-generation. In this paper we present a comprehensive discussion of its science ob…

astro-ph.SR2025

Enhanced Mass Loss of Very Massive Stars: Impact on the Evolution, Binary Processes, and Remnant Mass Spectrum

Kendall G. Shepherd, Guglielmo Costa, Cristiano Ugolini +7

Very massive stars (VMS) play a fundamental role in astrophysics due to their winds and supernovae (SN), and their role as massive black hole (BH) progenitors. However, their origi…