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.
out of the hole
自殺しとけ脳障害 0077ご冗談でしょう？名無しさん2023/11/26(日) 17:50:35.09ID:??? out of the hole(horizon)が地平面を跨ぐという英語弱者の解釈する人って… 0078ご冗談でしょう？名無しさん2023/11/26(日) 17:52:46.71ID:??? こういうout of the holeを地平面跨いでると勘違いしちゃったかぁ https://i.imgur.com/ZL6MseA.jpg0079ご冗談でしょう？名無しさん2023/11/26(日) 17:55:49.17ID:??? トンデモ理論の根拠が英語ミスとか流石にしょぼすぎ 0080ご冗談でしょう？名無しさん2023/11/26(日) 17:59:36.45ID:XUpixQvU>>77-79 英語弱者はお前だけ 摂動あるなら地平面が動く 0081ご冗談でしょう？名無しさん2023/11/26(日) 18:00:47.93ID:XUpixQvU>>77-79 そもそも無毛定理が破れてるのは常識なのでその時点で英語弱者すぎるwwwwww
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
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. 0133ご冗談でしょう？名無しさん2023/11/26(日) 18:22:45.52ID:XUpixQvU>>111 そもそも無毛定理が破れてるのは常識なのでその時点で英語弱者すぎるwwwwww
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
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.
The uniqueness of the modes’ frequencies and damping times is directly related to the ‘‘no-hair’’ theorem of general relativistic black holes, and thus a reliable detection and accurate identification of QNMs could provide the ‘‘smoking gun’’ for black holes and an important test of general relativity in the strong-field regime [3].
