Simulation technologies for cosmic ray neutron-induced soft errors: Models and simulation systems

Journal Article · Tue Jun 01 04:00:00 EDT 1999 · IEEE Transactions on Nuclear Science

DOI:https://doi.org/10.1109/23.774176· OSTI ID:6381112

Tosaka, Y; Kanata, H; Itakura, T; Satoh, S ^[1]

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1. Fujitsu Labs., Ltd., Atsugi (Japan). ULSI Technology Lab.

The authors review two types of simulators for the analysis of cosmic ray neutron-induced soft errors (SE's). One of them is the neutron-induced soft error simulator (NISES). A recently proposed nuclear reaction theory forms the foundation for the nuclear reaction database used in NISES. The other simulator, the simplified simulator MBGR, is based on a modified version of the burst generation rate (BGR) model. Both simulators accurately simulate neutron-induced SE rates (SER's). MBGR actually provides an easier and quicker estimation of neutron-induced SER's than NISES. On the other hand, NISES covers more applications; it simulates neutron-induced charge collection, multiple-bit SE, and [alpha]-induced SE analysis.

• OSTI ID: 6381112
• Journal Information: IEEE Transactions on Nuclear Science, Journal Name: IEEE Transactions on Nuclear Science Vol. 46:3Pt3; ISSN 0018-9499; ISSN IETNAE
• Country of Publication: United States
• Language: English

Related Subjects

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Instruments
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46 INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY
BARYONS
COSMIC NEUTRONS
COSMIC RADIATION
DIGITAL SYSTEMS
ELECTRONIC EQUIPMENT
ELEMENTARY PARTICLES
EQUIPMENT
ERRORS
FERMIONS
HADRONS
IONIZING RADIATIONS
MATHEMATICAL MODELS
NEUTRONS
NUCLEONS
PHYSICAL RADIATION EFFECTS
RADIATION EFFECTS
RADIATIONS
SECONDARY COSMIC RADIATION