共查询到19条相似文献,搜索用时 31 毫秒
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宇宙线发现100年来,人们对其成分、产生和加速机制、及其传播效应进行了广泛的研究,并获得了丰富的天体物理信息,但其起源至今仍然不清楚。一般认为相对低能的宇宙线起源于银河系内,极高能宇宙线起源于河外,而作为宇宙中最明亮的河外天体,活动星系核很可能是河外宇宙线源。随着多信使观测时代的到来,我们拥有了前所未有的从整体上去理解高能伽马射线和河外极高能宇宙线最好机遇。本文将简要地回顾和讨论活动星系核与高能宇宙线起源之间的关系,并对我国即将建成的高海拔宇宙线观测站(LHAASO)研究预期进行展望。 相似文献
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宇宙线发现100年来,人们对其成分、产生和加速机制、及其传播效应进行了广泛的研究,并获得了丰富的天体物理信息,但其起源至今仍然不清楚。一般认为相对低能的宇宙线起源于银河系内,极高能宇宙线起源于河外,而作为宇宙中最明亮的河外天体,活动星系核很可能是河外宇宙线源。随着多信使观测时代的到来,我们拥有了前所未有的从整体上去理解高能伽马射线和河外极高能宇宙线最好机遇。本文将简要地回顾和讨论活动星系核与高能宇宙线起源之间的关系,并对我国即将建成的高海拔宇宙线观测站(LHAASO)研究预期进行展望。 相似文献
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<正>对地球上的人类而言,来自遥远宇宙的高能信使包括质子、光子、中微子和引力波。由于质子携带一个单位的正电荷,它在宇宙空间的长途跋涉会受到磁场的影响而改变方向,使得我们很难追踪到它的起源之地。极高能的质子也会和宇宙的微波背景辐射发生反应,从而损失能量和它所携带的原始信息,这一现象就是著名的Greisen-ZatsepinKuzmin (GZK)截断效应, 相似文献
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<正>宇宙线是来自地球之外的高能带电粒子,约99%为原子核,1%为电子。此外,在传播过程中,宇宙线通过与星际介质作用,产生少量次级核子及反质子、正电子等次级宇宙线粒子。宇宙线的发现始于1912年,迄今为止观测到的宇宙线粒子的最高能量已达到3×1020电子伏特,是最大的粒子加速器LHC 相似文献
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宇宙线是来自地球之外的高能带电粒子,约99%为原子核,1%为电子。此外,在传播过程中,宇宙线通过与星际介质作用,产生少量次级核子及反质子、正电子等次级宇宙线粒子。宇宙线的发现始于1912年,迄今为止观测到的宇宙线粒子的最高能量已达到3×1020电子伏特,是最大的粒子加速器LHC (large hadron collider)所能加速粒子能量的千万倍。但宇宙线的起源至今仍是未知之谜①。近些年研究表明,高能宇宙线应来自于宇宙中的天体,因而宇宙线研究属天体物理和粒子物理的交叉学科②。 相似文献
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DING Lin-Kai 《中国物理C(英文版)》1990,14(6):486-489
The inelasticity of p-air and A-air interactions of superhigh energy cosmic rays is analysed and the influence of the nuclear collision geometry is investigated. 相似文献
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ZHANG Nai-Jian WANG Cheng-Rui HE Mao CAO Pei-Yuan LI Jin-Yu ZOU Bao-Tang WANG Guang-Jun WEI Chao 《中国物理C(英文版)》1989,13(11):961-966
A part of K4(1984—1985) Fe emulsion chambers exposed at Mt.Kanbala (5500m,atmospheric depth 520g/cm2)by China-Japan Emulsion Chamber Collaboration has been analyzed with systematic scanning and measurement.The distribution of the starting of the starting point depths of the observed showers is given.The zenith angle distribution,vertical intensity,energy spectrum and attenuation length of hadrons in air and in iron are presented.Our results are compared with the recent data given by other experiments,and they are consistent with each other approximately. 相似文献
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In this paper a kind of fireball model for subquark stratum is proposed, which can be used to explain the cosmic ray experiments for superhigh energy range, e. g., the mean multiplicity of secondary particles increases as S increases average transversal momentum ⊥> increases as S increases …etc. It can also give predictions which can be verified experimentally. This means that the information of the existence of subquark can be probed in the experiments on superhigh energy cosmic ray. Furthermore, this also means that some new phenomena observed in the experiments. on superhigh energy cosmiq ray provide. probably this kind of information. 相似文献
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Within the framework of the Glauber theory, we divide the many particle systeminto two subsystems formed. by the "valence" particles and "sea" particles respective-ly. Then the multiple scattering amplitudes can be divided into "sea","sea","sea","valence", "valence","sea", and "valence","valence" multiple scattering amplitude.For the calculations of these different amplitudes different effective approximatemethods are proposed, Finally, for "sea"."sea". "sea""valence", "valence" "sea"and "valence"."valence" processes, we obatain the respective S-matrices which phy-sically clear and convenient in calculation. 相似文献
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JIANG Yin-Lin YUAN Yu-Kui LI Yan-Guo CHEN Duan-Bao ZHENG Rong-Ting SONG Jian-Ning 《中国物理C(英文版)》1986,10(1):9-14
The exploring results of the possibility on detecting cosmic ray particles by acoustic way are reported. It shows that the ultrasonic background noise is very complicated and there are some individual and transient ultrasonic signals in the natural wide water. The mechanism producing these signals may be the sound radiation of the microbubbles in water. There is no evidence for the possible correlation between these signals and cosmic ray particles. The threshold energy of acoustic detection of EAS core is above 3﹒1016eV at sealevel and the threshold energy of acoustic detection of the local showers produced by cosmic ray particles is above 1014eV 相似文献
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The charge dispersion of fragments in high energy p+Cu,Kr and Xe reactions are calculated by statistical model and Monte Carlo technique.The corresponding data are reproduced quite well.It is shown that the charge dispersions are all nearly gaussian.The mass dependence of the most probable fragment charge reflects the rest target memory effect. 相似文献
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由于天体粒子物理涉及的研究领域太宽,本文拟以宇宙线总的能谱特征为线索,分段介绍各能区的研究前沿,总结有关宇宙线的起源、传播和成分的理论模型和相应的观测实验进展,并简要介绍相关的高能领域,例如γ暴(GRB),中微子,暗物质,超对称(SUSY),大统一理论(GUT)。这些理论在某种程度上暗示着极高能宇宙线的产生机制,并可能意味着需要新的超出标准粒子物理模型的理论来解释GZK截断(GZK Cutoff)的疑难问题。对高能天体物理的研究可以拓宽人类对早期宇宙的认识,为新物理理论模型提供检验的证据,为人类认识自然提供了另一扇窗口。 相似文献
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本文叙述利用场强为6200高斯的磁云室,对级联簇射中的能量大于30兆电子伏的电子在铝中直接产生电子对的平均总截面进行了测量。实验上总共找到真正由电子产生的电子三岔8.1个,相应于三岔产生的平均自由路程为672±585厘米或平均总截面为(0.25±0.22)×10-25厘米2。在数据处理中,对假三岔数目的除去作了应有的适当考虑。此外对Bhabha及Murota等的总截面公式也作了适合于于我们实验具体情况的修正,并算出总截面值,最后将它同实验值作了比较。结果我们认为实验上测得的值和Murota等的总截面值较为接近,但也不与Bhabha的截面值矛盾。 相似文献