Dataset from "Isolated or Dynamical? Tracing Black Hole Binary Formation through the Population of Gravitational-Wave Sources"
Authors/Creators
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1.
Gran Sasso Science Institute
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2.
University of Cagliari
Description
Simulation data from the publication "Isolated or Dynamical? Tracing Black Hole Binary Formation through the Population of Gravitational-Wave Sources" by Arca Sedda et al
Each zipped directory contains merger rate density profiles and mock catalogues of BBH mergers formed from isolated binary evolution in galactic fields or dynamical interactions in young, globular, and nuclear clusters. The structure of the files is described in the B-POP main page (https://github.com/marcasedda/BPOP)
Notes
MAS acknowledges funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No.~101025436 (project GRACE-BH) and from the MERAC Foundation through the 2023 MERAC prize. MAS and MB acknowledge the ACME project which has received funding from the European Union's Horizon Europe Research and Innovation programme under Grant Agreement No.~101131928. This material is based upon work supported by NSF's LIGO Laboratory which is a major facility fully funded by the National Science Foundation. The authors are grateful for computational resources provided by the LIGO Lab (CIT, LHO, LLO) and supported by the National Science Foundation Grants PHY-0757058 and PHY-0823459.
Files
Files
(622.3 MB)
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md5:1c29d5e130280b34e2fce1938d5f4115
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md5:ddfbedcb6a05b7674f357025bc4c552f
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md5:c15b09f64f045d4f287abde2570fb9b3
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md5:1a849c4c84414f86684f1d96949cd1ab
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md5:5b0d5f8d6e69790cbfb40130a03bd441
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md5:404e92c8bd84f15bc21ab8f8331ebd0a
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md5:67388aba42d9179d0185a0cfc92e5c6c
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md5:1e9ab597b4760fb1f91e5e225ffa0367
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71.1 MB | Download |