Relic Density of Asymmetric Dark Matter in Modified Cosmological Scenarios<xref rid="ctp_70_5_602fn1" ref-type="fn">*</xref><fn id="ctp_70_5_602fn1"><label>*</label><p>Supported by the National Natural Science Foundation of China under Grant Nos. 11365022 and 11765021</p></fn>

Relic Density of Asymmetric Dark Matter in Modified Cosmological Scenarios**

Supported by the National Natural Science Foundation of China under Grant Nos. 11365022 and 11765021

Iminniyaz Hoernisa, Salai Burhan, Lv Guo-Liang

(Color online) Evolution of Y_χ and as a function of the inverse-scaled temperature x for n_D = 6 and n_D = 8. η = 10³ for panels (a), (c) and η = 10⁴ for panels (b), (d). Here Λ = 5 × 10⁻¹², m = 100 GeV, g_χ = 2, g_* = 90, a = 1.31 × 10⁻²⁵ cm³ · s⁻¹, b = 0, x₀ = 25.