충격! 가로우 감마선 폭발의 위력ㄷㄷㄷㄷㄷㄷㄷ

감마선 폭발의 요인은 극초거성의 붕괴, 블랙홀 충돌, 중성자별의 폭발 3가지가 있지만 펑맨에선 극초거성의 붕괴로 설명했음

극초거성의 질량은 평균적으로 태양의 30배 이상임

태양의 질량 1.989x10^30kg

1.989x10^30x30=5.967e+31kg

반면 가로우의 질량은 100kg도 되지 않아보임

펑퀴들을 위해 100kg으로 잡아준다 해도 극초거성의 질량과는 5.967x10^29(50양6700자)배 차이가 남ㅠㅠ

In 1997 it was established that GRBs occupy the furthest reaches of the Universe and astronomers were immediately faced with the dilemma of how to produce so much energy in such a short period of time. They began with the assumption that GRBs emit their radiation isotropically (equally in all directions) much as a supernova does, but quickly decided that such massive energy production was physically unfeasable. If the radiation was emitted in this way, 3×10⁴⁷ Joules of energy was required in less than a minute (the equivalent of 100,000 supernovae going off simultaneously) for the most energetic bursts!

감마선 폭발은 일반적으로 1분동안 3x10^47줄의 에너지를 방출한다고 함

3x10^47/(5.967x10^29)=5.0276521e+17J

도시 레벨의 강자 핵로우ㄷㄷㄷㄷㄷㄷㄷㄷㄷㄷㄷㄷㄷㄷㄷㄷㄷㄷㄷㄷㄷㄷㄷㄷㄷ

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