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) The allowed region in the (a,Λ) plane for different n_D and standard cosmology when the Dark Matter relic density Ω h² = 0.1199. Here m = 100 GeV, g_χ = 2 and g_* = 90, x₀ = 25, η = 10³. The three dot-dashed (red) line is the limiting cross section, which corresponds to the Fermi-LAT bounds for channel and the thick (red) line is for channel.^[27]