Note that if mω+/ω > 1, then vphase is positive. It turns out that the energy flow down the hole, while always inward as seen locally, is determined by vphase for an observer at infinity. If mω+/ω > 1, energy flows out of the hole and the corresponding scattering wave mode is amplified, or “superradiantly scattered” (cf. Press and Teukolsky 1972, Misner 1972, and Zel’dovich 1972). A detailed discussion of electromagnetic and gravitational superradiance, including numerical values, will be given in a later paper in this series.
Note that if mω+/ω > 1, then vphase is positive. It turns out that the energy flow down the hole, while always inward as seen locally, is determined by vphase for an observer at infinity. If mω+/ω > 1, energy flows out of the hole and the corresponding scattering wave mode is amplified, or “superradiantly scattered” (cf. Press and Teukolsky 1972, Misner 1972, and Zel’dovich 1972). A detailed discussion of electromagnetic and gravitational superradiance, including numerical values, will be given in a later paper in this series.
Note that if mω+/ω > 1, then vphase is positive. It turns out that the energy flow down the hole, while always inward as seen locally, is determined by vphase for an observer at infinity. If mω+/ω > 1, energy flows out of the hole and the corresponding scattering wave mode is amplified, or “superradiantly scattered” (cf. Press and Teukolsky 1972, Misner 1972, and Zel’dovich 1972). A detailed discussion of electromagnetic and gravitational superradiance, including numerical values, will be given in a later paper in this series.
Note that if mω+/ω > 1, then vphase is positive. It turns out that the energy flow down the hole, while always inward as seen locally, is determined by vphase for an observer at infinity. If mω+/ω > 1, energy flows out of the hole and the corresponding scattering wave mode is amplified, or “superradiantly scattered” (cf. Press and Teukolsky 1972, Misner 1972, and Zel’dovich 1972). A detailed discussion of electromagnetic and gravitational superradiance, including numerical values, will be given in a later paper in this series.
Note that if mω+/ω > 1, then vphase is positive. It turns out that the energy flow down the hole, while always inward as seen locally, is determined by vphase for an observer at infinity. If mω+/ω > 1, energy flows out of the hole and the corresponding scattering wave mode is amplified, or “superradiantly scattered” (cf. Press and Teukolsky 1972, Misner 1972, and Zel’dovich 1972). A detailed discussion of electromagnetic and gravitational superradiance, including numerical values, will be given in a later paper in this series.
Note that if mω+/ω > 1, then vphase is positive. It turns out that the energy flow down the hole, while always inward as seen locally, is determined by vphase for an observer at infinity. If mω+/ω > 1, energy flows out of the hole and the corresponding scattering wave mode is amplified, or “superradiantly scattered” (cf. Press and Teukolsky 1972, Misner 1972, and Zel’dovich 1972). A detailed discussion of electromagnetic and gravitational superradiance, including numerical values, will be given in a later paper in this series.