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多物理场建模有助于沿着CMOS技术的缩放趋势研究大气宇宙射线对单粒子翻转敏感性的影响。

Multi-physics modelling contributions to investigate the atmospheric cosmic rays on the single event upset sensitivity along the scaling trend of CMOS technologies.

作者信息

Hubert G, Regis D, Cheminet A, Gatti M, Lacoste V

机构信息

The French Aerospace Lab, ONERA, Toulouse 31055, France

Thales Systèmes Aéroportés, Pessac 33600, France.

出版信息

Radiat Prot Dosimetry. 2014 Oct;161(1-4):290-4. doi: 10.1093/rpd/ncu003. Epub 2014 Feb 4.

Abstract

Particles originating from primary cosmic radiation, which hit the Earth's atmosphere give rise to a complex field of secondary particles. These particles include neutrons, protons, muons, pions, etc. Since the 1980s it has been known that terrestrial cosmic rays can penetrate the natural shielding of buildings, equipment and circuit package and induce soft errors in integrated circuits. Recently, research has shown that commercial static random access memories are now so small and sufficiently sensitive that single event upsets (SEUs) may be induced from the electronic stopping of a proton. With continued advancements in process size, this downward trend in sensitivity is expected to continue. Then, muon soft errors have been predicted for nano-electronics. This paper describes the effects in the specific cases such as neutron-, proton- and muon-induced SEU observed in complementary metal-oxide semiconductor. The results will allow investigating the technology node sensitivity along the scaling trend.

摘要

源自初级宇宙辐射的粒子撞击地球大气层后会产生一个由次级粒子构成的复杂场。这些粒子包括中子、质子、μ子、π介子等。自20世纪80年代以来,人们就知道地面宇宙射线能够穿透建筑物、设备和电路封装的天然屏蔽层,并在集成电路中引发软错误。最近的研究表明,如今商用静态随机存取存储器体积如此之小且灵敏度足够高,以至于质子的电子阻止作用可能会引发单粒子翻转(SEU)。随着工艺尺寸的不断进步,这种灵敏度下降的趋势预计还会持续。于是,人们预测纳米电子学中会出现μ子软错误。本文描述了在互补金属氧化物半导体中观察到的中子、质子和μ子诱发单粒子翻转等特定情况下的影响。这些结果将有助于研究沿缩放趋势的技术节点灵敏度。

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