activity
20152018
most citedSpin orientations of merging black holes formed from the evolution of stellar binaries

231 citations · 380 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2018★ 83 cited

Impact of inter-correlated initial binary parameters on double black hole and neutron star mergers

J. Klencki, M. Moe, W. Gladysz +3

The distributions of the initial main-sequence binary parameters are one of the key ingredients in obtaining evolutionary predictions for compact binary (BH-BH / BH-NS / NS-NS) mer…

astro-ph.HE2018★ 231 cited

Spin orientations of merging black holes formed from the evolution of stellar binaries

Davide Gerosa, Emanuele Berti, Richard O'Shaughnessy +4

We study the expected spin misalignments of merging binary black holes (BHs) formed in isolation by combining state-of-the-art population-synthesis models with efficient post-Newto…

astro-ph.GA2017★ 8 cited

The Contribution Of Outer HI Disks To The Merging Binary Black Hole Population

Sukanya Chakrabarti, Philip Chang, Richard O'Shaughnessy +5

We investigate the contribution of outer HI disks to the observable population of merging black hole binaries. Like dwarf galaxies, the outer HI disks of spirals have low star form…

astro-ph.SR2016

Constraints on the formation of double neutron stars from the observed eccentricities and current limits on merger rates

Martyna Chruslinska, Krzysztof Belczynski, Tomasz Bulik +1

We employ population synthesis method to model the double neutron star (DNS) population and test various possibilities on natal kick velocities gained by neutron stars after their…

astro-ph.HE2016★ 17 cited

Dynamical formation of Black Hole Low-Mass X-Ray Binaries in the field - an alternative to common envelope

Jakub Klencki, Grzegorz Wiktorowicz, Wojciech Gładysz +1

Very wide binaries (> 500 AU) are subject to numerous encounters with flying-by stars in the Galactic field and can be perturbated into highly eccentric orbits (e ~ 0.99). For such…

gr-qc2015★ 41 cited

A Model of the Stochastic Gravitational-Wave Background due to Core Collapse to Black Holes

K. Crocker, V. Mandic, T. Regimbau +5

Superposition of gravitational waves generated by astrophysical sources is expected to give rise to the stochastic gravitational-wave background. We focus on the background generat…