activity
20142026
most citedLarge Interferometer For Exoplanets (LIFE): I. Improved exoplanet detection yield estimates for a large mid-infrared space-interferometer mission

203 citations · 413 across the 17 of their papers we have counts for

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Showing 2026Show all

8 papers · 1 filter

astro-ph.HE2026

A binary black hole merger rate comparison within the same metallicity-star formation rate framework

Lumen Boco, Michele Bosi, Cecilia Sgalletta +2

Recent studies have suggested that binary population synthesis models, when coupled with observationally based, metallicity-dependent SFRD, overpredict the observed local BBH merge…

astro-ph.SR2026

The Stellar Winds Atlas II: Black Hole Formation at Solar Metallicity

Amedeo Romagnolo, Floor S. Broekgaarden, Alex C. Gormaz-Matamala +7

Stellar winds are a primary source of uncertainty in predicting the masses of black holes (BHs) from massive stars. At solar metallicity, theoretical models lead to widely divergen…

astro-ph.HE2026

How Common Are Common Envelopes? Quantifying Their Role in Forming Gravitational-Wave Sources

Floor S. Broekgaarden, Ana Lam, Sasha Levina +14

A central goal of gravitational-wave astronomy is to use merging binary black hole (BBH), black hole-neutron star (BHNS), and binary neutron star (BNS) systems as fossils to recons…

astro-ph.HE2026

Can current models predict the local black hole merger rate?

Lumen Boco, Michele Bosi, Cecilia Sgalletta +2

After four observational runs, the Ligo-Virgo-Kagra collaboration estimated a local binary black hole (BBH) merger rate density of $R_{0,\textrm{LVK}}\simeq 14-26\,\textrm{Gpc}^{-3…

astro-ph.HE2026

Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions

Tyler B. Smith, Floor Broekgaarden, Sasha Levina +4

We investigate the role of mass ratio reversal (MRR), in which the initially less massive star in a binary forms the more massive compact object, in shaping the astrophysical binar…

astro-ph.HE2026

The role of accretion efficiency, natal kicks, and angular momentum transport in the formation of the Gaia black holes

Michela Mapelli, Cecilia Sgalletta, Johanna Müller-Horn +5

Gaia has the potential to deliver several tens of new dormant black holes (BHs) with low-mass stellar companions (hereafter, Gaia BHs) in the upcoming fourth data release. Three Ga…

astro-ph.HE2026

From cosmological simulations to binary black hole mergers: The impact of using analytical star formation history models on gravitational-wave source populations

Sasha Levina, Floor Broekgaarden, Lieke van Son +4

Observations of binary black hole (BBH) mergers provide a unique window into the lives of massive stars across cosmic time. Connecting redshift-dependent merger properties to massi…

astro-ph.SR2026

The Stellar Winds Atlas I: Current uncertainties in mass-loss rates

Amedeo Romagnolo, Floor S. Broekgaarden, Konstantinos Antoniadis +1

Stellar winds are a major source of uncertainty in understanding the life and deaths of massive stars. Across studies in the field, prescriptions for stellar winds differ substanti…