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Lifshitz/Schrödinger D-p-branes and dynamical exponents

Harvendra Singh

TL;DR

This work generalizes a double-limit procedure to all black D$p$-brane backgrounds, producing Lifshitz spacetimes with a $p$-dependent dynamical exponent $a_{Lif}=2{p-6\over p-5}$ and, from boosted AdS-Bubble geometries, Schrödinger spacetimes with $a_{Sch}=2/(p-5)$. It reveals a simple mapping between the two nonrelativistic branches, $a_{Lif}=2-a_{Sch}$, realized via exchanging light-cone metric components, and connects their UV/IR structures through a Weyl rescaling that signals running boundary couplings. The paper also analyzes Lifshitz singularities, finite-temperature Lifshitz black holes, and a thermodynamic duality between distinct condensation regimes in DLCQ, suggesting two complementary holographic ensembles. Together, these results extend Lifshitz/Schrödinger realizations to the full D$p$-brane family, provide a tunable exponents framework, and offer insights into nonrelativistic holography and boundary thermodynamics. The inclusion of Kaigorodov-like Schrödinger spaces (e.g., $a=-1$ for D3) and the explicit exponent relations strengthen the potential for modeling quantum critical behavior in strongly coupled systems.

Abstract

We extend our earlier study of special double limits of `boosted' $AdS_5$ black hole solutions to include all black D$p$-branes of type II strings. We find that Lifshitz solutions can be obtained in generality, with varied dynamical exponents, by employing these limits. We then study such double limits for `boosted' D$p$-brane bubble solutions and find that the resulting non-relativistic solutions instead describe Schrödinger like spacetimes, having varied dynamical exponents. We get a simple map between these Lifshitz & Schrödinger solutions and a relationship between two types of dynamical exponents. We also discuss about the singularities of the Lifshitz solutions and an intriguing thermodynamic duality.

Lifshitz/Schrödinger D-p-branes and dynamical exponents

TL;DR

This work generalizes a double-limit procedure to all black D-brane backgrounds, producing Lifshitz spacetimes with a -dependent dynamical exponent and, from boosted AdS-Bubble geometries, Schrödinger spacetimes with . It reveals a simple mapping between the two nonrelativistic branches, , realized via exchanging light-cone metric components, and connects their UV/IR structures through a Weyl rescaling that signals running boundary couplings. The paper also analyzes Lifshitz singularities, finite-temperature Lifshitz black holes, and a thermodynamic duality between distinct condensation regimes in DLCQ, suggesting two complementary holographic ensembles. Together, these results extend Lifshitz/Schrödinger realizations to the full D-brane family, provide a tunable exponents framework, and offer insights into nonrelativistic holography and boundary thermodynamics. The inclusion of Kaigorodov-like Schrödinger spaces (e.g., for D3) and the explicit exponent relations strengthen the potential for modeling quantum critical behavior in strongly coupled systems.

Abstract

We extend our earlier study of special double limits of `boosted' black hole solutions to include all black D-branes of type II strings. We find that Lifshitz solutions can be obtained in generality, with varied dynamical exponents, by employing these limits. We then study such double limits for `boosted' D-brane bubble solutions and find that the resulting non-relativistic solutions instead describe Schrödinger like spacetimes, having varied dynamical exponents. We get a simple map between these Lifshitz & Schrödinger solutions and a relationship between two types of dynamical exponents. We also discuss about the singularities of the Lifshitz solutions and an intriguing thermodynamic duality.

Paper Structure

This paper contains 9 sections, 74 equations, 3 figures, 1 table.

Figures (3)

  • Figure 1: The Lifshitz window appears as the shaded region. It starts at $r_0$ and ends at $r_w \sim W^{2\over{7-p}}$.
  • Figure 2: Depiction of an usual AdS black hole spacetime. There is no Lifshitz like region here.
  • Figure 3: In zero temperature solutions the Lifshitz window (the shaded region) starts at $r=0$ and ends at $r_w$.