Linear waves in the interior of extremal black holes I
arXiv:1509.06568 · doi:10.1007/s00220-016-2800-y
Abstract
We consider solutions to the linear wave equation in the interior region of extremal Reissner-Nordström black holes. We show that, under suitable assumptions on the initial data, the solutions can be extended continuously beyond the Cauchy horizon and moreover, that their local energy is finite. This result is in contrast with previously established results for subextremal Reissner-Nordström black holes, where the local energy was shown to generically blow up at the Cauchy horizon.
46 pages, 2 figures
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- Time-Translation Invariance of Scattering Maps and Blue-Shift Instabilities on Kerr Black Hole Spacetimes
- Late-time asymptotics for the wave equation on extremal Reissner-Nordström backgrounds
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- Rough initial data and the strength of the blue-shift instability on cosmological black holes with
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