activity
20192026
most citedThe effect of the metallicity-specific star formation history on double compact object mergers

298 citations · 1.6k across the 44 of their papers we have counts for

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Showing 2024Show all

5 papers · 1 filter

astro-ph.HE2024

Not just winds: why models find binary black hole formation is metallicity dependent, while binary neutron star formation is not

L. A. C. van Son, S. K. Roy, I. Mandel +6

Both detailed and rapid population studies alike predict that binary black hole (BHBH) formation is orders of magnitude more efficient at low metallicity than high metallicity, whi…

astro-ph.IM2024★ 14 cited

Streamlining and standardizing software citations with The Software Citation Station

Tom Wagg, Floor S. Broekgaarden, Phil R. Van-Lane

Software is crucial for the advancement of science, especially in the context of rapidly growing datasets that increasingly require algorithm and pipeline development to process da…

astro-ph.HE2024

Investigating the Cosmological Rate of Compact Object Mergers from Isolated Massive Binary Stars

Adam Boesky, Floor S. Broekgaarden, Edo Berger

Gravitational wave detectors are observing compact object mergers from increasingly far distances, revealing the redshift evolution of the binary black hole (BBH) -- and soon the b…

astro-ph.HE2024

The Binary Black Hole Merger Rate Deviates From the Cosmic Star Formation Rate: A Tug of War Between Metallicity and Delay Times

Adam Boesky, Floor S. Broekgaarden, Edo Berger

Gravitational-wave detectors are now making it possible to investigate how the merger rate of binary black holes (BBHs) evolves with redshift. In this study, we examine whether the…

astro-ph.HE2024

Beyond the far side: Observing black hole mergers beyond the pair-instability mass gap with next-generation gravitational wave detectors

Gabriele Franciolini, Konstantinos Kritos, Luca Reali +2

Stellar evolution predicts the existence of a mass gap for black hole remnants produced by pair-instability supernova dynamics, whose lower and upper edges are very uncertain. We s…