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Filaments of the Slime Mold Cosmic Web and How They Affect Galaxy Evolution

We present a novel approach for identifying cosmic web filaments within the DisPerSE structure identification framework, using cosmic density field estimates from the Monte Carlo Physarum Machine (MCPM), inspired by the slime mold organism. We apply our method to the IllustrisTNG (TNG100) cosmologic...

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Xehetasun bibliografikoak
Egile Nagusiak: Farhanul Hasan, Joseph N. Burchett, Douglas Hellinger, Oskar Elek, Daisuke Nagai, S. M. Faber, Joel R. Primack, David C. Koo, Nir Mandelker, Joanna Woo
Formatua: Artigo
Hizkuntza:Inglês
Argitaratua: IOP Publishing 2024-01-01
Saila:The Astrophysical Journal
Gaiak:
Sarrera elektronikoa:https://doi.org/10.3847/1538-4357/ad4ee2
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