Chinese Physics C > 2003, Vol. 27 > Issue(11): 973-977

Very High Energy Gamma Rays from Gamma Ray Bursts

Institute of High Energy Physics, CAS, Beijing 100039, China2 Science College of Southwest Jiaotong University, Chengdu 610031, China

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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 ^－2arriving at the earth.

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[3]	ZHANG Ji-Long,CUI Shu-Wang,DING Lin-Kai,DING Xiao-Hong,FENG Cun-Feng,FENG Zhen-Yong,GAO Xiao-Yu,GENG Qing-Xi,GUO Hong-Wei,HE Hui-Hai,HE Mao,,,,,,. Search for a TeV Gamma Rays Emission from the Shell-like SNP G40.5-0.5 Using the Yangbajing Extend Air Shower Array. Chinese Physics C, 2006, 30(1): 13-17.
[4]	HUANG Xiao-Long,YU Wei-Xiang,LU Han-Lin,ZHOU Chun-Mei,WU Zhen-Dong,HUO Jun-De. Calculation the Absolute γ-Ray Intensities and Their Uncertainties. Chinese Physics C, 2004, 28(6): 588-593.
[5]	ZHOU Chun-Mei,WU Zhen-Dong. Calculation of Absolute Intensities of γ-Rays from α Decay. Chinese Physics C, 2004, 28(10): 1074-1078.
[6]	CHEN Xin,ZHOU Xun-Xiu,HU Hong-Bo,LIU Kun,YANG Qun-Yu,MU Jun. Study on the Optimum Angular Radius of Windows in Searching for TeV GRBs. Chinese Physics C, 2004, 28(10): 1094-1098.
[7]	XU Chun-Xian,ZHANG Yong,HE Hui-Lin,HE Hui-Hai,CHEN Yong-Zhong,JIANG Yin-Lin. Observations of TeV Gamma Ray from the Galactic Plane. Chinese Physics C, 2001, 25(9): 799-806.
[8]	XU XianWu,DING LinKai,CAO PeiYuan,DAI BenZhong,FENG ZhenYong,FU Yu,GUO HongWei,HE Mao,HUANG Qing,HUO AnXiang,JIA HuanYu,LI JinYu,LIU ShaoMin,,,,. Search for TeV Gamma Rays from the Crab Nebula with Tibet Ⅱ/HD AS Array. Chinese Physics C, 2000, 24(6): 473-477.
[9]	Peng Zhaoran,Li Jing,Ma Xinhua,Wang Wei,Zhu Qingqi,Shen Changquan,Jing Cailiu,Deng Yuju,Yuan Yukui,Huo Anxiang. A Very High Energy GLE Event Possibly Associated With the X Solar Flare of 15th June 1991. Chinese Physics C, 1999, 23(11): 1033-1038.
[10]	Xu Chunxian,He Huilin,Chen Yongzhong,He Huihai,Li Huidong,Zhang Yong,Jiang Yinlin. Search for TeV Gamma Ray Bursts From Evaporating Primordial Black Holes. Chinese Physics C, 1999, 23(1): 35-38.
[11]	Ding Linkai,Mu Jun,Wang Hui,Feng Zhenyong,Ren Jingru,Yu Guangce,Zhou Wende,Meng Xianru,Meng Lie,Zhang Chunsheng,,,,,,. Search for 10TeV Gamma-Ray Bursts. Chinese Physics C, 1997, 21(8): 673-679.
[12]	Bai Ge,Li Jiarong. Studing the Screened Potential of the Quark in QGP by the Kinetic Equation. Chinese Physics C, 1996, 20(9): 801-811.
[13]	Huo Anxiang,Kuang Haohuai. A Model for Enhancement of the Flux of Very High EnergyParticles During Large Solar Flares. Chinese Physics C, 1996, 20(12): 1068-1072.
[14]	Jia Huanyu,Cao Zhen,Zhang Huimin. The Study of Meteorological Effects on TeV Cosmic Ray Flux. Chinese Physics C, 1994, 18(9): 788-793.
[15]	HUO An-Xiang,DAI Yi-Fang,YUAN Yu-Kui. VERY HIGH-ENERGY PARTICLE EMISSION FROM THE SOLAR COSMIC RAY FLARES. Chinese Physics C, 1990, 14(9): 862-864.
[16]	CHEN Ke-Zhong,TAN Zhen-Qiang,LI Qing-Run. HIGH ENERGY DEUTERON-DEUTERON SCATTERING. Chinese Physics C, 1984, 8(1): 69-74.
[17]	ZHANG Gui-Shan,ZHANG Huan-Qiao. MONTE CARLO CALCULATION OF THE EFFICIENCIES OF THE LEAD GLASS DETECTORS FOR HIGH-ENERGY GAMMA RAYS. Chinese Physics C, 1983, 7(3): 370-378.
[18]	ZHANG HUAN-QIAO,DING SHENG-YUE,LIU ZU-HUA,ZHANG GUI-SHAN,LIU ZHAO-MING,TANG XIO-WEI,LI HUAN-TIE. EXPERIMETAL SEARCH FOR HIGH ENERGY γ RAYS IN THE SPONTANEOUTANEOUS FISSIONS OF²⁵²Cf. Chinese Physics C, 1982, 6(4): 491-494.
[19]	HO YU-KUN. NEUTRON CAPTURE GAMMA RAY SPECTRA AT LOW ENERGY. Chinese Physics C, 1981, 5(6): 732-740.
[20]	CHIANG HUAN-CHING,LI YANG-KUO. BACK-WARD POTENTIAL SCATTERING AT HIGH ENERGIES. Chinese Physics C, 1978, 2(5): 411-416.

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MA Xin-Hua, ZHOU Xun-Xiu, WU Mei and ZHU Qing-Qi. Very High Energy Gamma Rays from Gamma Ray Bursts[J]. Chinese Physics C, 2003, 27(11): 973-977.

MA Xin-Hua, ZHOU Xun-Xiu, WU Mei and ZHU Qing-Qi. Very High Energy Gamma Rays from Gamma Ray Bursts[J]. Chinese Physics C, 2003, 27(11): 973-977. shu

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Received: 2003-04-29
Revised: 1900-01-01

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沈阳化工大学材料科学与工程学院沈阳 110142

Very High Energy Gamma Rays from Gamma Ray Bursts

Corresponding author:MA Xin-Hua,

Institute of High Energy Physics, CAS, Beijing 100039, China2 Science College of Southwest Jiaotong University, Chengdu 610031, China

Received Date:2003-04-29
Accepted Date:1900-01-01
Available Online:2003-11-05

Abstract: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^－2arriving at the earth.