activity
20092026
most citedNeutrino-driven winds from neutron star merger remnants

482 citations · 828 across the 19 of their papers we have counts for

collaborators

21 papers

astro-ph.HE2026

The MARTINI platform II. Tracing r-process nucleosynthesis in neutron star mergers with long-lived remnants

Eleonora Loffredo, Diego Vescovi, Albino Perego +2

Binary neutron star (BNS) mergers are among the primary sites of the rapid neutron-capture (r-)process. In mergers with long-lived remnants, sustained neutrino irradiation raises t…

astro-ph.HE2026

A Hybrid Neural Network Emulator for M1 Neutrino Reaction Rates in Binary Neutron Star Merger Simulations

Yi Qiu, David Radice, Raffaele Ferrari +1

We present a neural network emulator for the bns_nurates library, which computes neutrino reaction rates used in binary neutron star merger simulations. Following a hybrid strategy…

astro-ph.HE2026

Binary Neutron Star Merger Simulations with Microphysical Equation of State using Spritz

Fatemeh Hossein Nouri, Jay V. Kalinani, Bruno Giacomazzo +2

We present the first binary neutron star merger simulations performed with the general-relativistic magnetohydrodynamics (GRMHD) Spritz code employing a finite-temperature tabulate…

astro-ph.HE2026

Multipolar Neutrino Radiation in Binary Neutron Star Mergers: Angular Structure, Rotational Variability, and Implications for Electron Fraction

Kutay Arınç Çokluk, Albino Perego, Federico Maria Guercilena +1

The angular structure and temporal variability of neutrino emission from binary neutron star mergers are characterized using fully general-relativistic simulations with energy-inte…

astro-ph.HE2026★ 1 cited

Exploring Composition Mixing in Kilonova Ejecta with Ray-by-ray Simulations

Ruocheng Zhai, David Radice, Fabio Magistrelli +2

Binary neutron star merger (BNSM) ejecta are considered a primary repository of -process nucleosynthesis and a source of the observed heavy-element abundances. We implement comp…

astro-ph.HE2025★ 2 cited

Impact of in situ nuclear networks and atomic opacities on neutron star merger ejecta dynamics, nucleosynthesis, and kilonovae

Fabio Magistrelli, Sebastiano Bernuzzi, Albino Perego +2

Modeling binary neutron star merger (BNSM) ejecta evolution requires simulations involving hydrodynamics, nuclear reactions, and radiative processes. The impact of nuclear burning…

astro-ph.HE2025★ 4 cited

Impact of Neutrino Flavor Conversions on Neutron Star Merger Dynamics, Ejecta, Nucleosynthesis, and Multi-Messenger Signals

Yi Qiu, David Radice, Sherwood Richers +3

We present numerical relativity simulations of binary neutron star mergers incorporating neutrino flavor transformations triggered by fast flavor instability, quantum many-body eff…

gr-qc2025

Remnant properties of binary neutron star mergers undergoing prompt collapse

Arnab Dhani, Alessandro Camilletti, David Radice +4

We study the properties of remnants formed in prompt-collapse binary neutron star mergers. We consider non-spinning binaries over a range of total masses and mass ratios across a s…

gr-qc2025

Direct Measurement of the Accretion Disk Formed in Prompt Collapse Mergers with Future Gravitational-Wave Observatories

Arnab Dhani, Alessandro Camilletti, Alessio Ludovico De Santis +6

The production site of heavy r-process elements, such as Gold and Uranium, is uncertain. Neutron star mergers are the only astrophysical phenomenon in which we have witnessed their…

astro-ph.HE2025

Ni production in long-lived binary neutron star merger remnants

Maximilian Jacobi, Fabio Magistrelli, Eleonora Loffredo +5

We investigate the nucleosynthesis and kilonova emission based on numerical-relativity binary neutron star merger simulations that incorporate a two-moment neutrino-transport schem…

gr-qc2025★ 97 cited

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.HE2024★ 7 cited

Open-source library for performance-portable neutrino reaction rates: Application to neutron star mergers

Leonardo Chiesa, Maitraya Bhattacharyya, Filippo Mazzini +3

A realistic and detailed description of neutrinos in binary neutron star (BNS) mergers is essential to build reliable models of such systems. To this end, we present BNS_NURATES, a…

astro-ph.HE2024★ 13 cited

Long-lived neutron-star remnants from asymmetric binary neutron star mergers: element formation, kilonova signals and gravitational waves

Sebastiano Bernuzzi, Fabio Magistrelli, Maximilian Jacobi +3

We present 3D general-relativistic neutrino-radiation hydrodynamics simulations of two asymmetric binary neutron star mergers producing long-lived neutron stars remnants and spanni…

astro-ph.HE2024★ 9 cited

Element formation in radiation-hydrodynamics simulations of kilonovae

Fabio Magistrelli, Sebastiano Bernuzzi, Albino Perego +1

Understanding the details of -process nucleosynthesis in binary neutron star mergers (BNSM) ejecta is key to interpreting kilonova observations and identifying the role of BNSMs…

astro-ph.HE2024★ 13 cited

Geometric and thermodynamic characterization of binary neutron star accretion discs

Alessandro Camilletti, Albino Perego, Federico Maria Guercilena +2

Accretion disks formed in binary neutron star mergers play a central role in many astrophysical processes of interest, including the launching of relativistic jets or the ejection…

astro-ph.HE2024★ 25 cited

Bayesian inference of multimessenger astrophysical data: Joint and coherent inference of gravitational waves and kilonovae

Matteo Breschi, Rossella Gamba, Gregorio Carullo +4

We present a Bayesian framework for joint and coherent analyses of multimessenger binary neutron star signals. The method, implemented in our bajes infrastructure, incorporates a j…

astro-ph.HE2023★ 6 cited

Did a Kilonova Set Off in Our Galactic Backyard 3.5 Myr ago?

Leonardo Chiesa, Albino Perego, Federico Maria Guercilena

The recent detection of the live isotopes and in deep ocean sediments dating back to the past 3-4 Myr poses a serious challenge to the identificati…

astro-ph.HE2019★ 72 cited

Light-curve models of black hole - neutron star mergers: steps towards a multi-messenger parameter estimation

C. Barbieri, O. S. Salafia, A. Perego +2

In the new era of gravitational wave (GW) and multi-messenger astrophysics, the detection of a GW signal from the coalescence of a black hole - neutron star (BHNS) binary remains a…

astro-ph.HE2014★ 482 cited

Neutrino-driven winds from neutron star merger remnants

Albino Perego, Stephan Rosswog, Ruben Cabezon +4

We present a detailed, 3D hydrodynamics study of the neutrino-driven winds that emerge from the remnant of a NS merger. Our simulations are performed with the Newtonian, Eulerian c…

astro-ph.HE2010★ 1 cited

A path to radio-loudness through gas-poor galaxy mergers and the role of retrograde accretion

M. Dotti, M. Colpi, L. Maraschi +2

In this proceeding we explore a pathway to radio-loudness under the hypothesis that retrograde accretion onto giant spinning black holes leads to the launch of powerful jets, as se…

astro-ph.CO2009★ 96 cited

Mass and spin coevolution during the alignment of a black hole in a warped accretion disc

A. Perego, M. Dotti, M. Colpi +1

In this paper, we explore the gravitomagnetic interaction of a black hole (BH) with a misaligned accretion disc to study BH spin precession and alignment jointly with BH mass and s…