Holographic flows to IR Lifshitz spacetimes
Abstract
Recently we studied `vanishing' horizon limits of `boosted' black D3-brane geometry hsnr. The type IIB solutions obtained by taking these special double limits were found to describe nonrelativistic Lifshitz spacetimes at zero temperature. In the present work we study these limits for TsT black-hole solutions which include B-field. The new Galilean solutions describe a holographic RG flow from Schr\"odinger (a=2) spacetime in UV to a Lifshitz universe (a=3) in the IR.
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