## Decay of weakly charged solutions for the spherically symmetric Maxwell-Charged-Scalar-Field equations on a Reissner-Nordstr\"{o}m exterior space-time. (arXiv:1804.04297v1 [gr-qc])

We consider the Cauchy problem for the (non-linear) Maxwell-Charged-Scalar-Field equations with spherically symmetric initial data, on a fixed sub-extremal Reissner-Nordstr\"{o}m exterior space-time. We prove that the solutions are bounded and decay at an inverse polynomial rate towards time-like infinity and along the black hole event horizon, provided the charge of the Maxwell equation is sufficiently small. This condition is in particular satisfied for small data in energy space that enjoy a sufficient decay towards the asymptotically flat end. Some of the decay estimates we prove are arbitrarily close to the conjectured optimal rate in the limit where the charge tends to \$0\$, following the heuristics of Hod and Piran, arXiv:gr-qc/9712041. Our result can also be interpreted as a step towards the stability of Reissner-Nordstr\"{o}m black holes for the gravity coupled Einstein-Maxwell-Charged-Scalar-Field model. This problem is closely connected to the understanding of strong cosmic c查看全文

## Solidot 文章翻译

 你的名字 留空匿名提交 你的Email或网站 用户可以联系你 标题 简单描述 内容 We consider the Cauchy problem for the (non-linear) Maxwell-Charged-Scalar-Field equations with spherically symmetric initial data, on a fixed sub-extremal Reissner-Nordstr\"{o}m exterior space-time. We prove that the solutions are bounded and decay at an inverse polynomial rate towards time-like infinity and along the black hole event horizon, provided the charge of the Maxwell equation is sufficiently small. This condition is in particular satisfied for small data in energy space that enjoy a sufficient decay towards the asymptotically flat end. Some of the decay estimates we prove are arbitrarily close to the conjectured optimal rate in the limit where the charge tends to \$0\$, following the heuristics of Hod and Piran, arXiv:gr-qc/9712041. Our result can also be interpreted as a step towards the stability of Reissner-Nordstr\"{o}m black holes for the gravity coupled Einstein-Maxwell-Charged-Scalar-Field model. This problem is closely connected to the understanding of strong cosmic c