English

Gravitino and other spin-3/2 quasinormal modes in Schwarzschild-AdS spacetime

High Energy Physics - Theory 2014-02-12 v2 General Relativity and Quantum Cosmology

Abstract

We investigate quasinormal mode frequencies ωn\omega_n of gravitinos and generic massive spin-3/2 fields in a Schwarzschild-AdSD_D background in spacetime dimension D>3D>3, in the black brane (large black hole) limit appropriate to many applications of the AdS/CFT correspondence. First, we find asymptotic formulas for ωn\omega_n in the limit of large overtone number nn. Asymptotically, ωnnΔω+O(lnn)+O(n0)\omega_n \simeq n \Delta\omega + O(\ln n) + O(n^0), where Δω\Delta\omega is a known constant, and here we compute the O(lnn)O(\ln n) and O(n0)O(n^0) corrections to the leading O(n)O(n) behavior. Then we compare to numerical calculations of exact quasinormal mode frequencies. Along the way, we also improve the reach and accuracy of an earlier, similar analysis of spin-1/2 fields.

Keywords

Cite

@article{arxiv.1311.6409,
  title  = {Gravitino and other spin-3/2 quasinormal modes in Schwarzschild-AdS spacetime},
  author = {Peter Arnold and Phillip Szepietowski and Diana Vaman},
  journal= {arXiv preprint arXiv:1311.6409},
  year   = {2014}
}

Comments

31 pages, 3 figures [change from v1: very minor changes to text, and some references added]