English

Hydro-elastic Complementarity in Black Branes at large D

High Energy Physics - Theory 2022-03-07 v3 General Relativity and Quantum Cosmology

Abstract

We obtain the effective theory for the non-linear dynamics of black branes---both neutral and charged, in asymptotically flat or Anti-deSitter spacetimes---to leading order in the inverse-dimensional expansion. We find that black branes evolve as viscous fluids, but when they settle down they are more naturally viewed as solutions of an elastic soap-bubble theory. The two views are complementary: the same variable is regarded in one case as the energy density of the fluid, in the other as the deformation of the elastic membrane. The large-D theory captures finite-wavelength phenomena beyond the conventional reach of hydrodynamics. For asymptotically flat charged black branes (either Reissner-Nordstrom or p-brane-charged black branes) it yields the non-linear evolution of the Gregory-Laflamme instability at large D and its endpoint at stable non-uniform black branes. For Reissner-Nordstrom AdS black branes we find that sound perturbations do not propagate (have purely imaginary frequency) when their wavelength is below a certain charge-dependent value. We also study the polarization of black branes induced by an external electric field.

Keywords

Cite

@article{arxiv.1602.05752,
  title  = {Hydro-elastic Complementarity in Black Branes at large D},
  author = {Roberto Emparan and Keisuke Izumi and Raimon Luna and Ryotaku Suzuki and Kentaro Tanabe},
  journal= {arXiv preprint arXiv:1602.05752},
  year   = {2022}
}

Comments

26 pages. v2: 33 pages. Appendix added with a systematic derivation of the effective equations. v3: 34 pages. Expanded introduction

R2 v1 2026-06-22T12:52:54.551Z