Speaker
Description
We investigate the linear stability of static, spherically symmetric dyonic black hole solutions carrying both electric and magnetic charges in the U(1) gauge-invariant scalar-vector-tensor theory [1]. In the limit of vanishing magnetic charge, our framework reproduces the results of previous studies [2,3]. With appropriate choices of the interaction functions, it also encompasses the theoretical setup considered in Ref. [4]. On the other hand, the recently discovered dyonic hairy black hole solutions [5] are not covered by the frameworks developed in the previous studies and can therefore be analyzed for the first time within our framework. In particular, we focus on higher-order interactions and clarify the effects of the magnetic charge on the stability conditions.
[1] L. Heisenberg, JCAP 10, 054 (2018), arXiv:1801.01523 [gr-qc].
[2] L. Heisenberg, R. Kase, and S. Tsujikawa, Phys. Rev. D 97, 124043 (2018), arXiv:1804.00535 [gr-qc].
[3] C. Zhang and R. Kase, Phys. Rev. D 110, 044047 (2024), arXiv:2404.11910 [gr-qc].
[4] K. Taniguchi, S. Nishimura, N. Tsukamoto, and R. Kase, Phys. Rev. D 112, 124043 (2025), arXiv:2504.21279 [gr-qc].
[5] M. Kitagawa, N. Tsukamoto, and R. Kase, arXiv:2603.04884 [gr-qc].