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The {\it dark matter} seem to be an inevitable ingredient of the total matterconfiguration in the Universe and the knowledge how the {\it dark matter}affects the properties of superconductors is of vital importance for theexperiments aimed at its direct detection. The homogeneous magnetic fieldacting perpendicularly to the surface of (2+1) dimensional s-wave holographicsuperconductor in the theory with {\it dark matter} sector has been modeled bythe additional $U(1)$-gauge field representing dark matter and coupled to theMaxwell one. As expected the free energy for the vortex configuration turns outto be negative. Importantly its value is lower in the presence of {\it darkmatter} sector. This feature can explain why in the Early Universe first theweb of {\it dark matter} appeared and next on these gratings the ordinarymatter forming cluster of galaxies has formed.

Holographic vortices in the presence of dark matter sector