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Bence Kocsis

Researcher at Eötvös Loránd University

Publications -  169
Citations -  9850

Bence Kocsis is an academic researcher from Eötvös Loránd University. The author has contributed to research in topics: Gravitational wave & Supermassive black hole. The author has an hindex of 52, co-authored 159 publications receiving 8039 citations. Previous affiliations of Bence Kocsis include Princeton University & University of Oxford.

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Gravitational waves from scattering of stellar-mass black holes in galactic nuclei

TL;DR: In this paper, the authors follow the evolution of a multimass system of BHs and stars by numerically integrating the Fokker-Planck energy diffusion equations for a variety of binary BH mass distributions.
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Black holes, gravitational waves and fundamental physics: a roadmap.

Leor Barack, +205 more
TL;DR: A comprehensive overview of the state of the art in the relevant fields of research, summarize important open problems, and lay out a roadmap for future progress can be found in this article, where the authors present a concise, yet comprehensive overview.
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Rapid and Bright Stellar-mass Binary Black Hole Mergers in Active Galactic Nuclei

TL;DR: In this article, the authors examined the fate of binary black hole binaries in active galactic nuclei, which get trapped in the inner region of the accretion disk around the central supermassive black hole and showed that binary black holes can migrate into and then rapidly merge within the disk well within a Salpeter time.
Journal ArticleDOI

Black holes, gravitational waves and fundamental physics: a roadmap

Leor Barack, +231 more
TL;DR: A comprehensive overview of the state of the art in the relevant fields of research, summarize important open problems, and lay out a roadmap for future progress can be found in this article, which is an initiative taken within the framework of the European Action on 'Black holes, Gravitational waves and Fundamental Physics'.
Journal ArticleDOI

Rapid and Bright Stellar-mass Binary Black Hole Mergers in Active Galactic Nuclei

TL;DR: In this article, the authors examined the fate of binary black hole binaries in active galactic nuclei, which get trapped in the inner region of the accretion disk around the central supermassive black hole and showed that binary black holes can migrate into and then rapidly merge within the disk well within a Salpeter time.