1999
DOI: 10.2172/767449
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The Physical Models and Statistical Procedures Used in the RACER Monte Carlo Code

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Cited by 8 publications
(6 citation statements)
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“…The energy hash table methods also provide simple means of speeding up simulations that can be relatively cheap from a memory perspective. However, as the speedup with respect to the global unionized 10 Speedup values are relative to the same optimization schemes run in serial. 11 Speedup values are relative to the single-nuclide energy grid binary search run with 8 threads.…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…The energy hash table methods also provide simple means of speeding up simulations that can be relatively cheap from a memory perspective. However, as the speedup with respect to the global unionized 10 Speedup values are relative to the same optimization schemes run in serial. 11 Speedup values are relative to the single-nuclide energy grid binary search run with 8 threads.…”
Section: Discussionmentioning
confidence: 99%
“…The unionized energy grid treatment [9] is one method which has been shown to significantly cut down simulation runtime relative to the individual nuclide energy grid method just described. This algorithm, which can be traced at least as far back as its implementation in RACER [10] and RCP01 [11] and was recently reintroduced in the Serpent code [12], calls for the construction of a grid containing the union of all of the energy points from the individual grids of every nuclide in the problem. Then, the individual reaction cross sections for each nuclide are stored on this same grid.…”
Section: Introductionmentioning
confidence: 99%
“…Since each volume element allows for analytic sampling, all we need is a way to carry samples across its boundaries in case the sampled distance exceeds them. This method is known as regular tracking [SBB*99] or surface tracking [Lep10] and works as follows.…”
Section: Distance Samplingmentioning
confidence: 99%
“…For LWR applications in particular this means that coolant temperature cannot be adjusted, even though the distribution is passed into the tracking routine. Various solutions successfully implemented in other Monte Carlo codes are currently being evaluated for compatibility with Serpent, including direct tabular interpolation (Sutton et al, 1999) and functional expansion (Pavlou and Ji, 2014) of temperature-dependent S(a; b) data. The incapability to model self-shielding effects in the unresolved resonance region becomes an issue in fast spectrum systems, and the extension of TMS to probability table sampling is currently being studied.…”
Section: Future Plansmentioning
confidence: 99%