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Davide Gerosa

Researcher at University of Birmingham

Publications -  120
Citations -  6286

Davide Gerosa is an academic researcher from University of Birmingham. The author has contributed to research in topics: Gravitational wave & Binary black hole. The author has an hindex of 36, co-authored 100 publications receiving 4506 citations. Previous affiliations of Davide Gerosa include University of Cambridge & University of Mississippi.

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Testing general relativity with present and future astrophysical observations

Emanuele Berti, +64 more
TL;DR: In this article, a catalog of modified theories of gravity for which strong-field predictions have been computed and contrasted to Einstein's theory is presented, and the current understanding of the structure and dynamics of compact objects in these theories is summarized.
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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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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'.
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Evolutionary roads leading to low effective spins, high black hole masses, and O1/O2 rates for LIGO/Virgo binary black holes

TL;DR: In this article, the authors proposed three models of angular momentum transport in massive stars: a mildly efficient transport by meridional currents, an efficient transport implemented in the MESA code, and a very efficient transport to calculate natal BH spins.
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Are merging black holes born from stellar collapse or previous mergers

TL;DR: In this paper, the authors construct simple, observationally motivated populations of black hole binaries, and use Bayesian model selection to show that measurements of the masses, luminosity distance (or redshift), and effective spin of a black hole binary can indeed distinguish between these different formation scenarios.