高能物理与核物理
高能物理與覈物理
고능물리여핵물리
HIGH ENERGY PHYSICS AND NUCLEAR PHYSICS
2003年
11期
973-977
,共5页
马欣华%周勋秀%吴枚%朱清棋
馬訢華%週勛秀%吳枚%硃清棋
마흔화%주훈수%오매%주청기
γ暴%宇宙线%火球模型
γ暴%宇宙線%火毬模型
γ폭%우주선%화구모형
gamma ray burst%cosmic ray%fireball model
以膨胀火球模型解释来自γ暴的甚高能γ射线,其中考虑了高能γ射线产生效率,相对论效应以及宇宙背景辐射等因素. 计算表明,大于10GeV的γ射线的喷射可能在火球膨胀开始后约10-5s发生,其到达地面时的通量可达10-4-10-6cm-2.
以膨脹火毬模型解釋來自γ暴的甚高能γ射線,其中攷慮瞭高能γ射線產生效率,相對論效應以及宇宙揹景輻射等因素. 計算錶明,大于10GeV的γ射線的噴射可能在火毬膨脹開始後約10-5s髮生,其到達地麵時的通量可達10-4-10-6cm-2.
이팽창화구모형해석래자γ폭적심고능γ사선,기중고필료고능γ사선산생효솔,상대론효응이급우주배경복사등인소. 계산표명,대우10GeV적γ사선적분사가능재화구팽창개시후약10-5s발생,기도체지면시적통량가체10-4-10-6cm-2.
Very high energy gamma rays from gamma ray bursts are explained by the expanding fireball model. The high energy gamma ray generation efficiency, the relativistic effect, and the absorption in cosmic background radiation are taken into account. It is shown that the ejection of gamma rays with the energies higher than 10GeV may happen at the very beginning of the fireball expansion~10-5s with a fluence up to 10-4-10-6cm-2 arriving at the earth.