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It is shown that highly-charged Reissner-Nordstr\"om black holes in the charge interval $8/9<{(Q/M)}^2<1$ are stable to charged scalar perturbations.
C. Flammer, Spheroidal Wave Functions
1957
Earlier work this paper cites.
M. Abramowitz and I. A. Stegun, Handbook of Mathematical Functions
1970
Earlier work this paper cites.
W. H. Press and S. A. Teukolsky, Nature 238
1973
Earlier work this paper cites.
J. D. Bekenstein, Phys. Rev. D 7
1973
Earlier work this paper cites.
J. B. Hartle and D. C. Wilkins, Commun. Math. Phys. 38
1974
Earlier work this paper cites.
Ya. B. Zel’dovich, Pis‘ma Zh. Eksp. Teor. Fiz. 14
1978
Earlier work this paper cites.
S. Chandrasekhar, The Mathematical Theory of Black Holes
1983
Earlier work this paper cites.
A. Ronveaux, Heun’s differential equations
1995
Cited alongside, same era.
S. Hod and T. Piran, Phys. Rev. D 58
1998
Cited alongside, same era.
S. Hod, Class. Quant. Grav. 23
2006
Cited alongside, same era.
T. Hartman, W. Song, and A. Strominger, JHEP 1003:118 (2010)
2010
Cited alongside, same era.
2010
Cited alongside, same era.
T. Damour, N. Deruelle and R. Ruffini, Lett. Nuovo Cimento 15
2011
Cited alongside, same era.
2012
Later among the works it cites.
The stability of extremal
2012
Later among the works it cites.
2013
Later among the works it cites.
2014
Later among the works it cites.
S. Hod, Submitted for publication in Class. Quant. Grav. (2014)
2014
Later among the works it cites.
V. Cardoso, O. J. C. Dias, J. P. S. Lemos and S. Yoshida, Phys. Rev. D 70
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We use natural units in which G = c = ℏ = 1 G=c=\hbar=1
Cited in the paper.
It has recently been shown [ 6 ] that the upper bound ( 1
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We shall assume, without loss of generality, that Q ≥ 0 Q\geq 0
Cited in the paper.
A superradiant instability which is expected to be analogous to the superradiant instability of the Kerr black hole described above
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Note that μ \mu and q q stand for μ / ℏ \mu/\hbar and q / ℏ q/\hbar , respectively. Hence, these field parameters have the dimensions of ( ( length OPEN ) − 1 )^{-1}
Cited in the paper.
We shall henceforth omit the harmonic indexes l l and m m for brevity
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2014
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