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も読めないwww 0006ご冗談でしょう？名無しさん2023/11/26(日) 17:28:24.61ID:XUpixQvU>>4
低学歴「horizonって書いてない！」
1960年代のAIレベルの知能しかないwwww これがセンター8割しか取れない脳障害よ
out of the holeも読めないwww 0007ご冗談でしょう？名無しさん2023/11/26(日) 17:28:26.73ID:??? 新素粒子見つかったと聞いたが？ 0008ご冗談でしょう？名無しさん2023/11/26(日) 17:28:59.39ID:???>>6 地平面跨いでないねぇw 0009ご冗談でしょう？名無しさん2023/11/26(日) 17:29:40.45ID:XUpixQvU そもそもその文の直前でOn the horizonって言ってるからこのout of the holeはthe horizonでしかないんだが やっぱりセンター試験問題文すら読めない脳障害には無理かwwwwwww 0010ご冗談でしょう？名無しさん2023/11/26(日) 17:29:49.87ID:XUpixQvU>>8
そもそもその文の直前でOn the horizonって言ってるからこのout of the holeはthe horizonでしかないんだが やっぱりセンター試験問題文すら読めない脳障害には無理かwwwwwww 0011ご冗談でしょう？名無しさん2023/11/26(日) 17:30:09.62ID:XUpixQvU こーれLisp人工無能の方が賢いまであるwwwww 0012ご冗談でしょう？名無しさん2023/11/26(日) 17:30:20.90ID:XUpixQvU>>8
そもそもその文の直前でOn the horizonって言ってるからこのout of the holeはthe horizonでしかないんだが やっぱりセンター試験問題文すら読めない脳障害には無理かwwwwwww 0013ご冗談でしょう？名無しさん2023/11/26(日) 17:30:35.43ID:XUpixQvU 英文全く読めてないwwwwwwwwwwwww 0014ご冗談でしょう？名無しさん2023/11/26(日) 17:30:51.54ID:XUpixQvU なんでセンター英語すら出来ないガイジが吠えてんの？
そもそもその文の直前でOn the horizonって言ってるからこのout of the holeはthe horizonでしかないんだが やっぱりセンター試験問題文すら読めない脳障害には無理かwwwwwww 0015ご冗談でしょう？名無しさん2023/11/26(日) 17:31:15.06ID:XUpixQvU なんでセンター英語すら出来ないガイジが吠えてんの？
そもそもその文の直前でOn the horizonって言ってるからこのout of the holeはthe horizonでしかないんだが やっぱりセンター試験問題文すら読めない脳障害には無理かwwwwwww 0016ご冗談でしょう？名無しさん2023/11/26(日) 17:31:22.05ID:??? outgoingの概念が理解できないからout of the holeが跨いてるとか言っちゃうんだよなあw https://i.imgur.com/MjKDH77.png0017ご冗談でしょう？名無しさん2023/11/26(日) 17:31:37.52ID:XUpixQvU な？ これがセンター8割しか取れなかったくせに論文読めると思い込んでる脳障害よ 0018ご冗談でしょう？名無しさん2023/11/26(日) 17:31:52.42ID:XUpixQvU>>16
なんでセンター英語すら出来ないガイジが吠えてんの？
そもそもその文の直前でOn the horizonって言ってるからこのout of the holeはthe horizonでしかないんだが やっぱりセンター試験問題文すら読めない脳障害には無理かwwwwwww 0019ご冗談でしょう？名無しさん2023/11/26(日) 17:32:10.39ID:???>>15 一切跨いでなくて草 0020ご冗談でしょう？名無しさん2023/11/26(日) 17:32:32.28ID:XUpixQvU>>19
なんでセンター英語すら出来ないガイジが吠えてんの？
そもそもその文の直前でOn the horizonって言ってるからこのout of the holeはthe horizonでしかないんだが やっぱりセンター試験問題文すら読めない脳障害には無理かwwwwwww 0021ご冗談でしょう？名無しさん2023/11/26(日) 17:32:55.46ID:XUpixQvU>>16 じゃあholeが何なのか言ってみ？ 不可能だからwwww 0022ご冗談でしょう？名無しさん2023/11/26(日) 17:33:13.15ID:???>>16 これがout of the holeだよな 世界の物理学者はこれをわかってるw トンデモくんはこれを分からないからoutgoingで情報消失問題は解決したと主張w 0023ご冗談でしょう？名無しさん2023/11/26(日) 17:33:24.46ID:XUpixQvU>>19 the holeはthe horizonでないなら何なの？ 言ってみ？
絶対に不可能だからwwwwww 0025ご冗談でしょう？名無しさん2023/11/26(日) 17:33:52.32ID:???>>16 out of the holeなのに地平面跨いでなくて草 0026ご冗談でしょう？名無しさん2023/11/26(日) 17:34:32.93ID:XUpixQvU>>25
the holeはthe horizonでないなら何なの？ 言ってみ？
絶対に不可能だからwwwwww 0027ご冗談でしょう？名無しさん2023/11/26(日) 17:34:55.29ID:??? out of the mirrorなのに跨いでないのと同じだなw 0028ご冗談でしょう？名無しさん2023/11/26(日) 17:34:59.10ID:XUpixQvU>>22 その図にholeって書いてないぞ低学歴脳障害 0029ご冗談でしょう？名無しさん2023/11/26(日) 17:35:17.06ID:XUpixQvU>>27 the holeはthe horizonでないなら何なの？ 言ってみ？
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].
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.
https://arxiv.org/pdf/2010.14293.pdf0360ご冗談でしょう？名無しさん2023/12/12(火) 22:25:23.54ID:4AX27uqC 例えば、 Can gravitational waves pass through a black hole? とか "gravitational wave" "event horizon" で検索すれば、わかりやすい回答が色々出てくる。
＞v_phase = -k/ω = -1 + mω_+/ω ＞Note that if mω_+/ω > 1, then v_phase is positive
これは、位相速度が「外向き」になることがあると言っている。 ただし、その前で、
＞v_group = -dk/dω = -1 ＞The group velocity agrees with condition (ii) above.
この(ii)というのは、
＞Equivalently, way (ii) : demand that the radial group velocity of a wave packet, as measured by a physically well-behaved observer, be negative (i.e., signals can travel into the hole, but cannot come out).
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].
＞＞Equivalently, way (ii) : demand that the radial group velocity of a wave packet, as measured by a physically well-behaved observer, be negative (i.e., signals can travel into the hole, but cannot come out).
