Boundedness and Decay for the Teukolsky System of Spin $$\pm \,2$$ on Reissner–Nordström Spacetime: The Case $$|Q| \ll M$$

Author:

Giorgi ElenaORCID

Publisher

Springer Science and Business Media LLC

Subject

Mathematical Physics,Nuclear and High Energy Physics,Statistical and Nonlinear Physics

Reference50 articles.

1. Andersson, L., Bäckdahl, T., Blue, P., Ma, S.: Stability for linearized gravity on the Kerr spacetime (2019). arXiv preprint arXiv:1903.03859

2. Angelopoulos, Y., Aretakis, S., Gajic, D.: A vectorfield approach to almost-sharp decay for the wave equation on spherically symmetric, stationary spacetimes. (2016). arXiv preprint arXiv:1612.01565

3. Angelopoulos, Y., Aretakis, S., Gajic, D.: Late-time asymptotics for the wave equation on spherically symmetric, stationary spacetimes (2016). arXiv preprint arXiv:1612.01566

4. Andersson, L., Blue, P.: Hidden symmetries and decay for the wave equation on the Kerr spacetime. Ann. Math. (2) 182(3), 787–853 (2015)

5. Andersson, L., Blue, P.: Uniform energy bound and asymptotics for the Maxwell field on a slowly rotating Kerr black hole exterior. J. Hyperbolic Differ. Equ. 12(4), 689–743 (2015)

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