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In this work we calculate pulsar kick velocity of magnetized neutron starcomposed of degenerate quark matter core with non-Fermi liquid (NFL)correction. Both the leading order (LO) and next to leading order (NLO)corrections to the kick velocity have been incorporated. In addition, the NFLcorrections to the specific heat of magnetized quark matter have beenpresented. This has been taken into account to calculate the kick velocity ofthe neutron star. Results show significant departure from the normal Fermiliquid estimates. The relation between radius and temperature has been shownwith kick velocity of $100\, km/s$ with and without NFL corrections.

Modifications to the pulsar kick velocity due to magnetic interactions in dense plasma