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EARLY STRUCTURE FORMATION FROM PRIMORDIAL DENSITY FLUCTUATIONS WITH A BLUE, TILTED POWER SPECTRUM

  • Authors: Shingo Hirano, Nick Zhu, Naoki Yoshida, David Spergel, and Harold W. Yorke

2015 The Astrophysical Journal 814 18.

  • Provider: AAS Journals

Caption: Figure 2.

We compare the halo mass functions at z = 100 for three PPS models. We set the normalization parameter to σ8 = 2.5 here. The lines show the Press–Schechter mass functions, while the symbols show the results of our cosmological simulations with a volume of 60 h−1 comoving kilo-parsec on a side. We run the Friend of Friend (FOF) halo finder with linking length b = 0.2 to obtain the halo mass functions.

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