nIFTy galaxy cluster simulations – I. Dark matter and non-radiative models

nIFTy galaxy cluster simulations – I. Dark matter and non-radiative models

We have simulated the formation of a galaxy cluster in a Ʌ cold dark matter universe using 13 different codes modelling only gravity and non-radiative hydrodynamics (RAMSES, ART, AREPO, HYDRA and nine incarnations of GADGET). This range of codes includes particle-based, moving and fixed mesh codes a...

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Bibliographic Details
Main Authors: Sembolini, Federico, Yepes, Gustavo, Pearce, Frazer R., Knebe, Alexander, Kay, Scott T., Power, Chris, Cui, Weiguang, Beck, Alexander M., Borgani, Stefano, Dalla Vecchia, Claudio, Davé, Romeel, Elahi, Pascal Jahan, February, Sean, Huang, Shuiyao, Hobbs, Alex, Katz, Neal, Lau, Erwin, McCarthy, Ian G., Murante, Giuseppe, Nagai, Daisuke, Nelson, Kaylea, Newton, Richard D. A., Perret, Valentin, Puchwein, Ewald, Read, Justin I., Saro, Alexandro, Schaye, Joop, Teyssier, Romain, Thacker, Robert J.
Format: Article
Published: Oxford University Press 2016
Subjects:
Methods: numerical - galaxies: haloes - cosmology: theory - dark matter
Online Access:https://eprints.nottingham.ac.uk/36360/

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