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We investigate deformations of Gauss-Bonnet-Lifshitz holography in $(n+1)$dimensional spacetime. Marginally relevant operators are dynamically generatedby a momentum scale $\Lambda \sim 0$ and correspond to slightly deformedGauss-Bonnet-Lifshitz spacetimes via a holographic picture. To admit(non-trivial) sub-leading orders of the asymptotic solution for the marginalmode, we find that the value of the dynamical critical exponent $z$ isrestricted by $z= n-1-2(n-2) \tilde{\alpha}$, where $\tilde{\alpha}$ is the(rescaled) Gauss-Bonnet coupling constant. The generic black hole solution,which is characterized by the horizon flux of the vector field and$\tilde{\alpha}$, is obtained in the bulk, and we explore its thermodynamicproperties for various values of $n$ and $\tilde{\alpha}$.

Deformations of Lifshitz holography with the Gauss-Bonnet term in ($n+1$) dimensions