高维旋转黑洞的不稳定性与新相
高能物理 - 理论
2010-01-07 v2 广义相对论与量子宇宙学
摘要
已有猜想认为，高维旋转黑洞在旋转足够大时会变得不稳定，并且在失稳阈值处会出现具有收缩视界的新型黑洞。我们通过数值搜索找到了单自旋Myers-Perry黑洞的稳态轴对称扰动，这些扰动标志着不稳定性的开始和新型黑洞相的出现。我们还发现了旋转黑弦和黑膜的新的超旋转Gregory-Laflamme不稳定性。
引用
@article{arxiv.0907.2248,
title = {Instability and new phases of higher-dimensional rotating black holes},
author = {Oscar J. C. Dias and Pau Figueras and Ricardo Monteiro and Jorge E. Santos and Roberto Emparan},
journal= {arXiv preprint arXiv:0907.2248},
year = {2010}
}
备注
5 pages, 5 figures. The instability of the black hole is argued to appear at the second zero mode. The first zero mode is not associated to a new branch of black hole solutions