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Photonuclear Reactions in Lightning Discovered from Detection of Positrons and Neutrons

机译:从闪烁探测中发现的闪电中的光核反应   正电子和中子

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摘要

Lightning and thundercloud are the most dramatic natural particleaccelerators on the Earth. Relativistic electrons accelerated by electricfields therein emit bremsstrahlung gamma rays, which have been detected atground observations, by airborne detectors, and as terrestrial gamma-rayflashes (TGFs) from space. The energy of the gamma rays is sufficiently high topotentially invoke atmospheric photonuclear reactions 14N(gamma, n)13N, whichwould produce neutrons and eventually positrons via beta-plus decay ofgenerated unstable radioactive isotopes, especially 13N. However, no clearobservational evidence for the reaction has been reported to date. Here wereport the first detection of neutron and positron signals from lightning witha ground observation. During a thunderstorm on 6 February 2017 in Japan, aTGF-like intense flash (within 1 ms) was detected at our monitoring sites0.5-1.7 km away from the lightning. The subsequent initial burst quicklysubsided with an exponential decay constant of 40-60 ms, followed by aprolonged line emission at about 0.511 megaelectronvolt (MeV), lasting for aminute. The observed decay timescale and spectral cutoff at about 10 MeV of theinitial emission are well explained with de-excitation gamma rays from thenuclei excited by neutron capture. The centre energy of the prolonged lineemission corresponds to the electron-positron annihilation, and hence is theconclusive indication of positrons produced after the lightning. Our detectionof neutrons and positrons is unequivocal evidence that natural lightningtriggers photonuclear reactions. No other natural event on the Earth is knownto trigger photonuclear reactions. This discovery places lightning as only thesecond known natural channel on the Earth after the atmospheric cosmic-rayinteraction, in which isotopes, such as 13C, 14C, and 15N, are produced.
机译:闪电和雷云是地球上最引人注目的自然粒子加速器。由其中的电场加速的相对论电子发出致辐射的伽马射线,这些射线已由机载探测器在地面观测中检测到,并作为来自太空的地面伽马射线闪光(TGF)。伽马射线的能量足够高,有可能引起大气光核反应14N(γ,n)13N,该反应将产生中子,并最终通过生成的不稳定放射性同位素(尤其是13N)的β加衰变产生正电子。然而,迄今尚无该反应的明确观察证据。在这里,我们首先进行了地面观测,发现了来自闪电的中子和正电子信号。在2017年2月6日的日本雷暴雨中,我们的监测点在距闪电0.5-1.7公里处检测到类似TGF的强烈闪光(1毫秒内)。随后的初始突发迅速消失,其指数衰减常数为40-60 ms,随后以约0.511兆电子伏特(MeV)的延长线发射,持续一分钟。用中子俘获所激发的来自核的去激发伽马射线很好地解释了在初始发射的大约10 MeV处观察到的衰变时间尺度和光谱截止。延长线发射的中心能量对应于电子-正电子an灭,因此是闪电后产生的正电子的结论性指示。我们对中子和正电子的检测是自然闪电触发光核反应的明确证据。已知地球上没有其他自然事件触发光核反应。这一发现将闪电作为大气宇宙射线相互作用之后地球上仅第二个已知的自然通道,在其中产生了同位素,例如13C,14C和15N。

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