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Probing Small-scale Dark Matter Clumping with the Large-scale 21 cm Power Spectrum

  • Authors: Sudipta Sikder, Hyunbae Park, Rennan Barkana, Naoki Yoshida, Anastasia Fialkov

Sudipta Sikder et al 2026 The Astrophysical Journal Letters 1000 .

  • Provider: AAS Journals

Caption: Figure 4.

Testing convergence with respect to the size of our large-scale grid. We show the 21 cm power spectrum of CDM as a function of k at z = 20, 30, and 40, for three box sizes: 1536, 768, and 384 Mpc on a side, corresponding to 5123, 2563, and 1283 pixels, respectively. The curves go down to k = 0.01, 0.02, and 0.04 Mpc−1, respectively. We note that the precise output redshifts that we use from the numerical simulations are 19.46, 30.00, and 39.89 (which we loosely refer to as 20, 30, and 40).

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