Theoretical Challenges in Galaxy Formation
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1,105 citations
518 citations
Cites background from "Theoretical Challenges in Galaxy Fo..."
...While this framework has been broadly successful at reproducing many key observed characteristics of the galaxy population at a range of cosmic epochs, the physical understanding of most of these small-scale feedback processes remains coarse and heuristic (see Naab & Ostriker 2017, for a review)....
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257 citations
161 citations
Cites background from "Theoretical Challenges in Galaxy Fo..."
...…2005; Heckman & Thompson 2017, for reviews) and believed to be essential to distribution of the gas and metals in galaxies and the circumgalactic/intergalactic medium (CGM/IGM) and hence to regulating cosmic star formation history (see Somerville & Davé 2015; Naab & Ostriker 2017, for reviews)....
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151 citations
References
7,060 citations
6,206 citations
"Theoretical Challenges in Galaxy Fo..." refers methods in this paper
...The Lagrangian particle based SPH method (Gingold & Monaghan (1977), Lucy (1977), see also Springel (2010b) and Somerville & Davé (2015) for recent reviews) is relatively simple to implement and due to its adaptive spatial resolution and good conservation properties has been very popular for…...
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6,196 citations
"Theoretical Challenges in Galaxy Fo..." refers methods in this paper
...The newly developed moving mesh code AREPO (Springel 2010a) similarly suffers from numerical diffusion but combines advantages of the Lagrangian and Eulerian approaches and performs much better than traditional SPH codes like GADGET on mixing problems with a high convergence rate (Sijacki et al. 2012, Springel 2010b)....
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...The recent GIZMO implementation is based on the GADGET framework and shows some significant improvements on idealised test problems, in particular for low Mach number gas (Hopkins 2015)....
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...…recent SPH work on cosmological galaxy formation is based on derivatives of either the GASOLINE (Wadsley, Stadel & Quinn 2004) code or the GADGET (Springel 2005) code and include updated implementations to treat the mixing problem better (see e.g. Hopkins et al. 2014; Hu et al. 2014; Read &…...
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...Bottom middle: SPH (GADGET ) simulation of Aumer et al. (2013)....
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...Most of the recent SPH work on cosmological galaxy formation is based on derivatives of either the GASOLINE (Wadsley, Stadel & Quinn 2004) code or the GADGET (Springel 2005) code and include updated implementations to treat the mixing problem better (see e.g. Hopkins et al. 2014; Hu et al. 2014; Read & Hayfield 2012; Schaller et al. 2015; Schaye et al. 2015; Wadsley, Veeravalli & Couchman 2008 and references therein)....
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5,508 citations
"Theoretical Challenges in Galaxy Fo..." refers methods in this paper
...The Lagrangian particle based SPH method (Gingold & Monaghan (1977), Lucy (1977), see also Springel (2010b) and Somerville & Davé (2015) for recent reviews) is relatively simple to implement and due to its adaptive spatial resolution and good conservation properties has been very popular for…...
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5,299 citations