English

Higher Spin Mode Stability for STU Black Hole Backgrounds

General Relativity and Quantum Cosmology 2023-12-11 v1 High Energy Physics - Theory

Abstract

This work studies mode stability of an STU black hole with four pairwise equal U(1)\rm{U(1)} charges in four spacetime dimensions. We investigate bosonic perturbations for probe fields of different spins through the transformation technique devised by Whiting in 1989. Finally, we introduce connection relations inspired by the work of ~Duzta\c{s} (2016) to prove the absence of unstable modes that solve the torsion-modified Dirac equation appropriate for this black hole background.

Keywords

Cite

@article{arxiv.2312.04929,
  title  = {Higher Spin Mode Stability for STU Black Hole Backgrounds},
  author = {M. Cvetic and M. A. Liao and M. M. Stetsko},
  journal= {arXiv preprint arXiv:2312.04929},
  year   = {2023}
}

Comments

11 pages + references

R2 v1 2026-06-28T13:44:52.528Z