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(10) The outer horizon corresponds to ∆ = 0 which givesr+ =M + √ M2− (a2 +g2 +Q2)

KERR-NEWMAN SPACETIME The Kerr-Newman metric is given in the form of the following line element in Boyer-Lindquist coordinates (t,r,θ,φ ): ds2 =− (∆−a2 sin2θ ρ2 ) dt2− 2ωω2dtdφ +ω2dφ2 +ρ2dθ2 + ρ2 ∆dr2, (1) where ∆ =r2 +a2− 2Mr +G2 =M2(S2 +R · 1973

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Gravitational Radiation from Binaries: A Pedagogical Introduction

gr-qc · 2019-08-07 · conditional · novelty 3.0

A pedagogical review of inspiral-to-plunge gravitational waves that extends the Ori-Thorne transition calculation to charged black holes and tabulates wave frequency, duration, cycles, amplitude, and signal-to-noise ratio.

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  • Gravitational Radiation from Binaries: A Pedagogical Introduction gr-qc · 2019-08-07 · conditional · none · ref 2

    A pedagogical review of inspiral-to-plunge gravitational waves that extends the Ori-Thorne transition calculation to charged black holes and tabulates wave frequency, duration, cycles, amplitude, and signal-to-noise ratio.