Figure 1 from EARLY STRUCTURE FORMATION FROM PRIMORDIAL DENSITY FLUCTUATIONS WITH A BLUE, TILTED POWER SPECTRUM

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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 1.

We plot the matter power spectra for the considered cases in the present paper with k_p = 100 h Mpc⁻¹. The black line is for the scale-independent PPS (Equation (1)), whereas the other three lines show the scale-dependent models given by Equation (2) with m_s = 1.5 (blue), 2.0 (green), and 2.5 (red), respectively.

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