Published 2015 | Version v1
Journal article

Effects of Stopping Ions and LET Fluctuations on Soft Error Rate Prediction

  • 1. Vanderbilt University, Nashville, TN (United States)
  • 2. Sandia National Laboratory (SNL-NM), Albuquerque, NM (United States)
  • 3. Dynetics, Inc., Huntsville, AL (United States)
  • 4. Intel Corp, Santa Clara, CA (United States)

Description

Variability in energy deposition from stopping ions and LET fluctuations is quantified for specific radiation environments. When compared to predictions using average LET via CREME96, LET fluctuations lead to an order-of-magnitude difference in effective flux and a nearly 4x decrease in predicted soft error rate (SER) in an example calculation performed on a commercial 65 nm SRAM. The large LET fluctuations reported here will be even greater for the smaller sensitive volumes that are characteristic of highly scaled technologies. End-of-range effects of stopping ions do not lead to significant inaccuracies in radiation environments with low solar activity unless the sensitivevolume thickness is 100 μm or greater. In contrast, end-of-range effects for stopping ions lead to significant inaccuracies for sensitive- volume thicknesses less than 10 μm in radiation environments with high solar activity.

Availability note (English)

Available from https://www.osti.gov/pages/servlets/purl/1427234; https://www.osti.gov/pages/biblio/1427234; DOE Accepted Manuscript full text, or the publishers Best Available Version will be available free of charge after the embargo period

Additional details

Publishing Information

Journal Title
IEEE Transactions on Nuclear Science
Journal Volume
62
Journal Issue
5
Journal Page Range
p. 2181-2186
ISSN
0018-9499

INIS

Country of Publication
United States
Country of Input or Organization
United States
INIS RN
50031515
Subject category
S42: ENGINEERING;
Descriptors DEI
ENERGY ABSORPTION; ENERGY LOSSES; ERRORS; FLUCTUATIONS; FORECASTING; IONS; SOLAR ACTIVITY
Descriptors DEC
ABSORPTION; CHARGED PARTICLES; LOSSES; SORPTION; STELLAR ACTIVITY; VARIATIONS

Optional Information