Commit 47bf3682 authored by Batson Iii, John's avatar Batson Iii, John
Browse files

more conversion

parent 5018ff6f
# Sphinx build info version 1
# This file hashes the configuration used when building these files. When it is not found, a full rebuild will be done.
config: 9839cddfb01ced1be595bc80712a022f
tags: 645f666f9bcd5a90fca523b33c5a78b7
<!DOCTYPE html>
<html class="writer-html5" lang="en" >
<head>
<meta charset="utf-8">
<meta name="viewport" content="width=device-width, initial-scale=1.0">
<title>MAVRIC: Monaco with Automated Variance Reduction using Importance Calculations &mdash; SCALE test documentation 0.0.1 documentation</title>
<link rel="stylesheet" href="_static/css/theme.css" type="text/css" />
<link rel="stylesheet" href="_static/pygments.css" type="text/css" />
<link rel="stylesheet" href="_static/custom.css" type="text/css" />
<!--[if lt IE 9]>
<script src="_static/js/html5shiv.min.js"></script>
<![endif]-->
<script type="text/javascript" id="documentation_options" data-url_root="./" src="_static/documentation_options.js"></script>
<script src="_static/jquery.js"></script>
<script src="_static/underscore.js"></script>
<script src="_static/doctools.js"></script>
<script src="_static/language_data.js"></script>
<script async="async" src="https://cdnjs.cloudflare.com/ajax/libs/mathjax/2.7.5/latest.js?config=TeX-AMS-MML_HTMLorMML"></script>
<script type="text/javascript" src="_static/js/theme.js"></script>
<link rel="index" title="Index" href="genindex.html" />
<link rel="search" title="Search" href="search.html" />
<link rel="prev" title="Welcome to SCALE test documentation!" href="index.html" />
</head>
<body class="wy-body-for-nav">
<div class="wy-grid-for-nav">
<nav data-toggle="wy-nav-shift" class="wy-nav-side">
<div class="wy-side-scroll">
<div class="wy-side-nav-search" >
<a href="index.html" class="icon icon-home" alt="Documentation Home"> SCALE test documentation
</a>
<div role="search">
<form id="rtd-search-form" class="wy-form" action="search.html" method="get">
<input type="text" name="q" placeholder="Search docs" />
<input type="hidden" name="check_keywords" value="yes" />
<input type="hidden" name="area" value="default" />
</form>
</div>
</div>
<div class="wy-menu wy-menu-vertical" data-spy="affix" role="navigation" aria-label="main navigation">
<p class="caption"><span class="caption-text">Radiation Shielding</span></p>
<ul class="current">
<li class="toctree-l1 current"><a class="current reference internal" href="#">MAVRIC: Monaco with Automated Variance Reduction using Importance Calculations</a><ul>
<li class="toctree-l2"><a class="reference internal" href="#introduction">Introduction</a></li>
<li class="toctree-l2"><a class="reference internal" href="#cadis-methodology">CADIS Methodology</a><ul>
<li class="toctree-l3"><a class="reference internal" href="#overview-of-cadis">Overview of CADIS</a></li>
<li class="toctree-l3"><a class="reference internal" href="#multiple-sources-with-cadis">Multiple sources with CADIS</a></li>
<li class="toctree-l3"><a class="reference internal" href="#multiple-tallies-with-cadis">Multiple tallies with CADIS</a></li>
<li class="toctree-l3"><a class="reference internal" href="#forward-weighted-cadis">Forward-weighted CADIS</a></li>
</ul>
</li>
<li class="toctree-l2"><a class="reference internal" href="#mavric-implementation-of-cadis">MAVRIC Implementation of CADIS</a><ul>
<li class="toctree-l3"><a class="reference internal" href="#denovo">Denovo</a></li>
<li class="toctree-l3"><a class="reference internal" href="#monaco">Monaco</a></li>
<li class="toctree-l3"><a class="reference internal" href="#running-mavric">Running MAVRIC</a></li>
</ul>
</li>
<li class="toctree-l2"><a class="reference internal" href="#mavric-input">MAVRIC input</a><ul>
<li class="toctree-l3"><a class="reference internal" href="#composition-block">Composition block</a></li>
<li class="toctree-l3"><a class="reference internal" href="#sggp-geometry-blocks">SGGP geometry blocks</a></li>
<li class="toctree-l3"><a class="reference internal" href="#other-blocks-shared-with-monaco">Other blocks shared with Monaco</a></li>
<li class="toctree-l3"><a class="reference internal" href="#importance-map-block">Importance map block</a><ul>
<li class="toctree-l4"><a class="reference internal" href="#constructing-a-mesh-for-the-sn-calculation">Constructing a mesh for the S<sub>N</sub> calculation</a></li>
<li class="toctree-l4"><a class="reference internal" href="#macromaterials-for-sn-geometries">Macromaterials for S<sub>N</sub> geometries</a></li>
</ul>
</li>
</ul>
</li>
</ul>
</li>
</ul>
</div>
</div>
</nav>
<section data-toggle="wy-nav-shift" class="wy-nav-content-wrap">
<nav class="wy-nav-top" aria-label="top navigation">
<i data-toggle="wy-nav-top" class="fa fa-bars"></i>
<a href="index.html">SCALE test documentation</a>
</nav>
<div class="wy-nav-content">
<div class="rst-content">
<div role="navigation" aria-label="breadcrumbs navigation">
<ul class="wy-breadcrumbs">
<li><a href="index.html" class="icon icon-home"></a> &raquo;</li>
<li>MAVRIC: Monaco with Automated Variance Reduction using Importance Calculations</li>
<li class="wy-breadcrumbs-aside">
<a href="_sources/MAVRIC.rst.txt" rel="nofollow"> View page source</a>
</li>
</ul>
<hr/>
</div>
<div role="main" class="document" itemscope="itemscope" itemtype="http://schema.org/Article">
<div itemprop="articleBody">
<div class="section" id="mavric-monaco-with-automated-variance-reduction-using-importance-calculations">
<span id="mavric"></span><h1>MAVRIC: Monaco with Automated Variance Reduction using Importance Calculations<a class="headerlink" href="#mavric-monaco-with-automated-variance-reduction-using-importance-calculations" title="Permalink to this headline"></a></h1>
<p><em>D. E. Peplow and C. Celik</em></p>
<div class="section" id="introduction">
<h2>Introduction<a class="headerlink" href="#introduction" title="Permalink to this headline"></a></h2>
<p>Monte Carlo particle transport calculations for deep penetration problems can require very long run times in order to achieve an acceptable level of statistical uncertainty in the final answers. Discrete-ordinates codes can be faster but have limitations relative to the discretization of space, energy, and direction. Monte Carlo calculations can be modified (biased) to produce results with the same variance in less time if an approximate answer or some other additional information is already known about the problem. If an importance can be assigned to different particles based on how much they will contribute to the final answer, more time can be spent on important particles with less time devoted to unimportant particles. One of the best ways to bias a Monte Carlo code for a particular tally is to form an importance map from the adjoint flux based on that tally. Unfortunately, determining the exact adjoint flux could be just as difficult as computing the original problem itself. However, an approximate adjoint can still be very useful in biasing the Monte Carlo solution <a class="bibtex reference internal" href="#wagner-acceleration-1997" id="id1">[Wag97]</a>. Discrete ordinates can be used to quickly compute that approximate adjoint. Together, Monte Carlo and discrete ordinates can be used to find solutions to thick shielding problems in reasonable times.</p>
<p>The MAVRIC (Monaco with Automated Variance Reduction using Importance Calculations) sequence is based on the CADIS (Consistent Adjoint Driven Importance Sampling) and FW-CADIS (Forward-Weighted CADIS) methodologies <a class="bibtex reference internal" href="#wagner-automated-1998" id="id2">[WH98]</a> <a class="bibtex reference internal" href="#wagner-automated-2002" id="id3">[Wag02]</a> <a class="bibtex reference internal" href="#haghighat-monte-2003" id="id4">[HW03]</a> <a class="bibtex reference internal" href="#wagner-forward-weighted-2007" id="id5">[WBP07]</a> MAVRIC automatically performs a three-dimensional, discrete-ordinates calculation using Denovo to compute the adjoint flux as a function of position and energy. This adjoint flux information is then used to construct an importance map (i.e., target weights for weight windows) and a biased source distribution that work together—particles are born with a weight matching the target weight of the cell into which they are born. The fixed-source Monte Carlo radiation transport Monaco then uses the importance map for biasing during particle transport and the biased source distribution as its source. During transport, the particle weight is compared with the importance map after each particle interaction and whenever a particle crosses into a new importance cell in the map.</p>
<p>For problems that do not require variance reduction to complete in a reasonable time, execution of MAVRIC without the importance map calculation provides an easy way to run Monaco. For problems that do require variance reduction to complete in a reasonable time, MAVRIC removes the burden of setting weight windows from the user and performs it automatically with a minimal amount of additional input. Note that the MAVRIC sequence can be used with the final Monaco calculation as either a multigroup (MG) or a continuous-energy (CE) calculation.</p>
<p>Monaco has a wide variety of tally options: it can calculate fluxes (by group) at a point in space, over any geometrical region, or for a user-defined, three-dimensional, rectangular grid. These tallies can also integrate the fluxes with either standard response functions from the cross section library or user-defined response functions. All of these tallies are available in the MAVRIC sequence.</p>
<p>While originally designed for CADIS, the MAVRIC sequence is also capable of creating importance maps using both forward and adjoint deterministic estimates. The FW-CADIS method can be used for optimizing several tallies at once, a mesh tally over a large region, or a mesh tally over the entire problem. Several other methods for producing importance maps are also available in MAVRIC and are explored in Appendix C.</p>
</div>
<div class="section" id="cadis-methodology">
<h2>CADIS Methodology<a class="headerlink" href="#cadis-methodology" title="Permalink to this headline"></a></h2>
<p>MAVRIC is an implementation of CADIS (Consistent Adjoint Driven Importance Sampling) using the Denovo SN and Monaco Monte Carlo functional modules. Source biasing and a mesh-based importance map, overlaying the physical geometry, are the basic methods of variance reduction. In order to make the best use of an importance map, the map must be made consistent with the source biasing. If the source biasing is inconsistent with the weight windows that will be used during the transport process, source particles will undergo Russian roulette or splitting immediately, wasting computational time and negating the intent of the biasing.</p>
<div class="section" id="overview-of-cadis">
<h3>Overview of CADIS<a class="headerlink" href="#overview-of-cadis" title="Permalink to this headline"></a></h3>
<p>CADIS has been well described in the literature, so only a
brief overview is given here. Consider a class source-detector problem
described by a unit source with emission probability distribution
function <span class="math notranslate nohighlight">\(q\left(\overrightarrow{r},E \right)\)</span> and a detector
response function <span class="math notranslate nohighlight">\(\sigma_{d}\left(\overrightarrow{r},E \right)\)</span>.
To determine the total detector response, <em>R</em>, the forward scalar flux
<span class="math notranslate nohighlight">\(\phi\left(\overrightarrow{r},E \right)\)</span> must be known. The
response is found by integrating the product of the detector response
function and the flux over the detector volume <span class="math notranslate nohighlight">\(V_{d}\)</span>.</p>
<div class="math notranslate nohighlight" id="equation-mavric-1">
<span class="eqno">(1)<a class="headerlink" href="#equation-mavric-1" title="Permalink to this equation"></a></span>\[R = \int_{V_{d}}^{}{\int_{E}^{}{\sigma_{d}\left( \overrightarrow{r},E \right)}}\phi\left(\overrightarrow{r},E \right)\textit{dE dV.}\]</div>
<p>Alternatively, if the adjoint scalar flux,
<span class="math notranslate nohighlight">\(\phi^{+}\left(\overrightarrow{r},E \right)\)</span>, is known from the
corresponding adjoint problem with adjoint source
<span class="math notranslate nohighlight">\(q^{+}\left(\overrightarrow{r},E \right) = \sigma_{d}\left(\overrightarrow{r},E \right)\)</span>,
then the total detector response could be found by integrating the
product of the forward source and the adjoint flux over the source
volume, <span class="math notranslate nohighlight">\(V_{s}\)</span>.</p>
<div class="math notranslate nohighlight" id="equation-mavric-2">
<span class="eqno">(2)<a class="headerlink" href="#equation-mavric-2" title="Permalink to this equation"></a></span>\[R = \int_{V_{s}}^{}{\int_{E}^{}{q\left(\overrightarrow{r},E \right)}}\phi^{+}\left( \overrightarrow{r},E \right)\textit{dE dV.}\]</div>
<p>Unfortunately, the exact adjoint flux may be just as difficult to
determine as the forward flux, but an approximation of the adjoint flux
can still be used to form an importance map and a biased source
distribution for use in the forward Monte Carlo calculation.</p>
<p>Wagner<sup>1</sup> showed that if an estimate of the adjoint scalar flux
for the corresponding adjoint problem could be found, then an estimate
of the response <em>R</em> could be made using Eq. . The adjoint source for the
adjoint problem is typically separable and corresponds to the detector
response and spatial area of tally to be optimized:
<span class="math notranslate nohighlight">\(q^{+}\left(\overrightarrow{r},E \right) = \sigma_{d}\left(E \right)g\left( \overrightarrow{r} \right)\)</span>,
where <span class="math notranslate nohighlight">\(\sigma_{d}\left( E \right)\)</span> is a flux-to-dose conversion
factor and <span class="math notranslate nohighlight">\(g\left( \overrightarrow{r} \right)\)</span> is 1 in the tally
volume and 0 otherwise. Then, from the adjoint flux
<span class="math notranslate nohighlight">\(\phi^{+}\left( \overrightarrow{r},E \right)\)</span> and response
estimate <em>R</em>, a biased source distribution,
<span class="math notranslate nohighlight">\(\widehat{q}\left( \overrightarrow{r},E \right)\)</span>, for source
sampling of the form</p>
<div class="math notranslate nohighlight" id="equation-mavric-3">
<span class="eqno">(3)<a class="headerlink" href="#equation-mavric-3" title="Permalink to this equation"></a></span>\[\widehat{q}\left(\overrightarrow{r},E \right) = \frac{1}{R}q\left(\overrightarrow{r},E\right)\phi^{+}\left( \overrightarrow{r},E \right)\]</div>
<p>and weight window target values,
<span class="math notranslate nohighlight">\(\overline{w}\left( \overrightarrow{r},E \right)\)</span>, for particle
transport of the form</p>
<div class="math notranslate nohighlight" id="equation-mavric-4">
<span class="eqno">(4)<a class="headerlink" href="#equation-mavric-4" title="Permalink to this equation"></a></span>\[\overline{w}\left( \overrightarrow{r},E \right) = \frac{R}{\phi^{+}\left( \overrightarrow{r},E \right)}\]</div>
<p>could be constructed, which minimize the variance in the forward Monte
Carlo calculation of <em>R</em>.</p>
<p>When a particle is sampled from the biased source distribution
<span class="math notranslate nohighlight">\(\widehat{q}\left( \overrightarrow{r},E \right)\)</span>, to preserve a
fair game, its initial weight is set to</p>
<div class="math notranslate nohighlight" id="equation-mavric-5">
<span class="eqno">(5)<a class="headerlink" href="#equation-mavric-5" title="Permalink to this equation"></a></span>\[w_{0}\left(\overrightarrow{r},E \right) = \frac{q\left(\overrightarrow{r},E \right)}{\widehat{q}\left( \overrightarrow{r},E \right)} = \frac{R}{\phi^{+}\left( \overrightarrow{r},E \right)}\,\]</div>
<p>which exactly matches the target weight for that particle’s position and
energy. This is the “consistent” part of CADIS—source particles are born
with a weight matching the weight window of the region/energy they are
born into. The source biasing and the weight windows work together.</p>
<p>CADIS has been applied to many problems—including reactor ex-core
detectors, well-logging instruments, cask shielding studies, and
independent spent fuel storage facility models—and has demonstrated very
significant speed-ups in calculation time compared to analog
simulations.</p>
</div>
<div class="section" id="multiple-sources-with-cadis">
<h3>Multiple sources with CADIS<a class="headerlink" href="#multiple-sources-with-cadis" title="Permalink to this headline"></a></h3>
<p>For a typical Monte Carlo calculation with multiple sources (each with a
probability distribution function
<span class="math notranslate nohighlight">\(q_{i}\left( \overrightarrow{r},E \right)\)</span> and a strength
<span class="math notranslate nohighlight">\(S_{i}\)</span>, giving a total source strength of
<span class="math notranslate nohighlight">\(S = \sum_{}^{}S_{i}\)</span>), the source is sampled in two steps. First,
the specific source <em>i</em> is sampled with probability
<span class="math notranslate nohighlight">\(p\left( i \right) = \ S_{i}/S\)</span>, and then the particle is sampled
from the specific source distribution
<span class="math notranslate nohighlight">\(q_{i}\left( \overrightarrow{r},E \right)\)</span>.</p>
<p>The source sampling can be biased at both levels: which source to sample
from and how to sample each source. For example, the specific source can
be sampled using some arbitrary distribution,
<span class="math notranslate nohighlight">\(\widehat{p}\left( i \right)\)</span>, and then the individual sources can
be sampled using distributions
<span class="math notranslate nohighlight">\({\widehat{q}}_{i}\left( \overrightarrow{r},E \right)\)</span>. Particles
would then have a birth weight of</p>
<div class="math notranslate nohighlight" id="equation-mavric-6">
<span class="eqno">(6)<a class="headerlink" href="#equation-mavric-6" title="Permalink to this equation"></a></span>\[w_{0} \equiv \ \left(\frac{p\left( i \right)}{\widehat{p}\left( i \right)} \right)\left(\frac{q_{i}\left( \overrightarrow{r},E \right)}{{\widehat{q}}_{i}\left( \overrightarrow{r},E \right)} \right)\text{.}\]</div>
<p>For CADIS, a biased multiple source needs to be developed so that the
birth weights of sampled particles still match the target weights of the
importance map. For a problem with multiple sources (each with a
distribution <span class="math notranslate nohighlight">\(q_{i}\left( \overrightarrow{r},E \right)\)</span> and a
strength <span class="math notranslate nohighlight">\(S_{i}\)</span>), the goal of the Monte Carlo calculation is to
compute some response <span class="math notranslate nohighlight">\(R\)</span> for a response function
<span class="math notranslate nohighlight">\(\sigma_{d}\left( \overrightarrow{r},E \right)\)</span> at a given
detector.</p>
<div class="math notranslate nohighlight" id="equation-mavric-7">
<span class="eqno">(7)<a class="headerlink" href="#equation-mavric-7" title="Permalink to this equation"></a></span>\[R = \ \int_{V}^{}{\int_{E}^{}{\sigma_{d}\left( \overrightarrow{r},E \right)\text{ϕ}\left( \overrightarrow{r},E \right)\textit{dE dV.}}}\]</div>
<p>Note that the flux <span class="math notranslate nohighlight">\(\phi\left( \overrightarrow{r},E \right)\)</span> has
contributions from each source. The response, <span class="math notranslate nohighlight">\(R_{i}\)</span>, from each
specific source (<span class="math notranslate nohighlight">\(S_{i}\)</span> with
<span class="math notranslate nohighlight">\(q_{i}\left( \overrightarrow{r},E \right)\)</span>) can be expressed using
just the flux from that source,
<span class="math notranslate nohighlight">\(\phi_{i}\left( \overrightarrow{r},E \right)\)</span>, as</p>
<div class="math notranslate nohighlight" id="equation-mavric-8">
<span class="eqno">(8)<a class="headerlink" href="#equation-mavric-8" title="Permalink to this equation"></a></span>\[R_{i} = \ \int_{V}^{}{\int_{E}^{}{\sigma_{d}\left(\overrightarrow{r},E \right)\ \phi_{i}\left(\overrightarrow{r},E \right)\textit{dE dV .}}}\]</div>
<p>The total response is then found as <span class="math notranslate nohighlight">\(R = \sum_{i}^{}R_{i}\)</span>.</p>
<p>For the adjoint problem, using the adjoint source of
<span class="math notranslate nohighlight">\(q^{+}\left( \overrightarrow{r},E \right) = \sigma_{d}\left( \overrightarrow{r},E \right)\)</span>,
the response <span class="math notranslate nohighlight">\(R\)</span> can also be calculated as</p>
<div class="math notranslate nohighlight" id="equation-mavric-9">
<span class="eqno">(9)<a class="headerlink" href="#equation-mavric-9" title="Permalink to this equation"></a></span>\[R = \ \int_{V}^{}{\int_{E}^{}{\left\lbrack \sum_{i}^{}{S_{i}q_{i}\left( \overrightarrow{r},E \right)} \right\rbrack\ \phi^{+}\left( \overrightarrow{r},E \right)\textit{dE dV}}},\]</div>
<p>with response contribution from each specific source being</p>
<div class="math notranslate nohighlight" id="equation-mavric-10">
<span class="eqno">(10)<a class="headerlink" href="#equation-mavric-10" title="Permalink to this equation"></a></span>\[R_{i} = \ \int_{V}^{}{\int_{E}^{}{\ {S_{i}q_{i}\left( \overrightarrow{r},E \right)\text{ϕ}}^{+}\left( \overrightarrow{r}, E \right)\textit{dE dV.}}}\]</div>
<p>The target weights
<span class="math notranslate nohighlight">\(\overline{w}\left( \overrightarrow{r},E \right)\)</span> of the
importance map are found using</p>
<div class="math notranslate nohighlight" id="equation-mavric-11">
<span class="eqno">(11)<a class="headerlink" href="#equation-mavric-11" title="Permalink to this equation"></a></span>\[\overline{w}\left( \overrightarrow{r},E \right) = \frac{R/S}{\text{ϕ}^{+}\left( \overrightarrow{r},E \right)\ }.\]</div>
<p>Each biased source
<span class="math notranslate nohighlight">\({\widehat{q}}_{i}\left( \overrightarrow{r},E \right)\)</span> pdf is
found using</p>
<div class="math notranslate nohighlight" id="equation-mavric-12">
<span class="eqno">(12)<a class="headerlink" href="#equation-mavric-12" title="Permalink to this equation"></a></span>\[{\widehat{q}}_{i}\left(\overrightarrow{r},E \right) = \frac{S_{i}}{R_{i}}{q_{i}\left( \overrightarrow{r},E \right)\text{ϕ}}^{+}\left( \overrightarrow{r}, E \right)\ ,\]</div>
<p>and the biased distribution used to select an individual source is
<span class="math notranslate nohighlight">\(\widehat{p}\left( i \right) = \ R_{i}/\sum_{}^{}{R_{i} = R_{i}/R}\)</span>.</p>
<p>When using the biased distribution used to select an individual source,
<span class="math notranslate nohighlight">\(\widehat{p}\left( i \right)\)</span>, and the biased source distribution,
<span class="math notranslate nohighlight">\({\widehat{q}}_{i}\left( \overrightarrow{r},E \right)\)</span>, the birth
weight of the sampled particle will be</p>
<div class="math notranslate nohighlight" id="equation-mavric-13">
<span class="eqno">(13)<a class="headerlink" href="#equation-mavric-13" title="Permalink to this equation"></a></span>\[\begin{split} \begin{matrix}
w_{0} &amp; \equiv &amp; \left( \frac{p\left( i \right)}{\widehat{p}\left( i \right)} \right)\left( \frac{q_{i}\left( \overrightarrow{r}, E \right)}{{\widehat{q}}_{i}\left(\overrightarrow{r},E \right)} \right) \\ &amp; = &amp; \ \left( \frac{\frac{S_{i}}{S}}{\frac{R_{i}}{R}} \right) \left( \frac{q_{i}\left( \overrightarrow{r},E \right)}{\frac{S_{i}}{R_{i}}{q_{i}\left( \overrightarrow{r},E \right)\text{ϕ}}^{+}\left( \overrightarrow{r},E \right)} \right) \\
&amp; = &amp; \frac{R/S}{\text{ϕ}^{+}\left( \overrightarrow{r},E \right)\ }, \\
\end{matrix}\end{split}\]</div>
<p>which matches the target weight,
<span class="math notranslate nohighlight">\(\overline{w}\left( \overrightarrow{r},E \right)\)</span>.</p>
</div>
<div class="section" id="multiple-tallies-with-cadis">
<h3>Multiple tallies with CADIS<a class="headerlink" href="#multiple-tallies-with-cadis" title="Permalink to this headline"></a></h3>
<p>The CADIS methodology works quite well for classic source/detector problems. The statistical uncertainty of the tally that serves as the adjoint source is greatly reduced since the Monte Carlo transport is optimized to spend more simulation time on those particles that contribute to the tally, at the expense of tracking particles in other parts of phase space. However, more recently, Monte Carlo has been applied to problems where multiple tallies need to all be found with low statistical uncertainties. The extension of this idea is the mesh tally—where each voxel is a tally where the user desires low statistical uncertainties. For these problems, the user must accept a total simulation time that is controlled by the tally with the slowest convergence and simulation results where the tallies have a wide range of relative uncertainties.</p>
<p>The obvious way around this problem is to create a separate problem for each tally and use CADIS to optimize each. Each simulation can then be run until the tally reaches the level of acceptable uncertainty. For more than a few tallies, this approach becomes complicated and time-consuming for the user. For large mesh tallies, this approach is not reasonable.</p>
<p>Another approach to treat several tallies, if they are in close proximity to each other, or a mesh tally covering a small portion of the physical problem is to use the CADIS methodology with the adjoint source near the middle of the tallies to be optimized. Since particles in the forward Monte Carlo simulation are optimized to reach the location of the adjoint source, all the tallies surrounding that adjoint source should converge quickly. The drawback to this approach is the difficult question of “how close.” If the tallies are too far apart, certain energies or regions that are needed for one tally may be of low importance for getting particles to the central adjoint source. This may under-predict the flux or dose at the tally sites far from the adjoint source.</p>
<p>MAVRIC has the capability to have multiple adjoint sources with this problem in mind. For several tallies that are far from each other, multiple adjoint sources could be used. In the forward Monte Carlo, particles would be drawn to one of those adjoint sources. The difficulty with this approach is that typically the tally that is closest to the true physical source converges faster than the other tallies—showing the closest adjoint source seems to attract more particles than the others. Assigning more strength to the adjoint source further from the true physical source helps, but finding the correct strengths so that all of the tallies converge to the same relative uncertainty in one simulation is an iterative process for the user.</p>
</div>
<div class="section" id="forward-weighted-cadis">
<h3>Forward-weighted CADIS<a class="headerlink" href="#forward-weighted-cadis" title="Permalink to this headline"></a></h3>
<p>In order to converge several tallies to the same relative uncertainty in
one simulation, the adjoint source corresponding to each of those
tallies needs to be weighted inversely by the expected tally value. In
order to calculate the dose rate at two points—say one near a reactor
and one far from a reactor—in one simulation, then the total adjoint
source used to develop the weight windows and biased source needs to
have two parts. The adjoint source far from the reactor needs to have
more strength than the adjoint source near the reactor by a factor equal
to the ratio of the expected near dose rate to the expected far dose
rate.</p>
<p>This concept can be extended to mesh tallies as well. Instead of using a
uniform adjoint source strength over the entire mesh tally volume, each
voxel of the adjoint source should be weighted inversely by the expected
forward tally value for that voxel. Areas of low flux or low dose rate
would have more adjoint source strength than areas of high flux or high
dose rate.</p>
<p>An estimate of the expected tally results can be found by using a quick
discrete-ordinates calculation. This leads to an extension of the CADIS
method: forward-weighted CADIS (FW-CADIS).**Error! Bookmark not
defined.** First, a forward S<sub>N</sub> calculation is performed to
estimate the expected tally results. A total adjoint source is
constructed where the adjoint source corresponding to each tally is
weighted inversely by those forward tally estimates. Then the standard
CADIS approach is used—an importance map (target weight windows) and a
biased source are made using the adjoint flux computed from the adjoint
S<sub>N</sub> calculation.</p>
<p>For example, if the goal is to calculate a detector response function
<span class="math notranslate nohighlight">\(\sigma_{d}\left( E \right)\)</span> (such as dose rate using
flux-to-dose-rate conversion factors) over a volume (defined by
<span class="math notranslate nohighlight">\(g\left( \overrightarrow{r} \right)\)</span>) corresponding to mesh tally,
then instead of simply using
<span class="math notranslate nohighlight">\(q^{+}\left( \overrightarrow{r},E \right) = \sigma_{d}\left( E \right)\ g(\overrightarrow{r})\)</span>,
the adjoint source would be</p>
<div class="math notranslate nohighlight" id="equation-mavric-14">
<span class="eqno">(14)<a class="headerlink" href="#equation-mavric-14" title="Permalink to this equation"></a></span>\[ q^{+}\left( \overrightarrow{r},E \right) = \frac{\sigma_{d}\left( E \right)\text{g}\left( \overrightarrow{r} \right)}{\int_{}^{}{\sigma_{d}\left( E \right)\text{ϕ}\left( \overrightarrow{r},E \right)}\textit{dE}}\ ,\]</div>
<p>where <span class="math notranslate nohighlight">\(\phi\left( \overrightarrow{r},E \right)\)</span> is an estimate of
the forward flux and the energy integral is over the voxel at <span class="math notranslate nohighlight">\(\overrightarrow{r}\)</span>.
The adjoint source is nonzero only where the mesh tally is defined
(<span class="math notranslate nohighlight">\(g\left( \overrightarrow{r} \right)\)</span>), and its strength is
inversely proportional to the forward estimate of dose rate.</p>
<p>The relative uncertainty of a tally is controlled by two components:
first, the number of tracks contributing to the tally and, second, the
shape of the distribution of scores contributing to that tally. In the
Monte Carlo game, the number of simulated particles,
<span class="math notranslate nohighlight">\(m\left( \overrightarrow{r},E \right)\)</span>, can be related to the true
physical particle density, <span class="math notranslate nohighlight">\(n\left( \overrightarrow{r},E \right),\)</span>
by the average Monte Carlo weight of scoring particles,
<span class="math notranslate nohighlight">\(\overline{w}\left( \overrightarrow{r},E \right)\)</span>, by</p>
<div class="math notranslate nohighlight" id="equation-mavric-15">
<span class="eqno">(15)<a class="headerlink" href="#equation-mavric-15" title="Permalink to this equation"></a></span>\[n\left( \overrightarrow{r},E \right) = \ \overline{w}\left( \overrightarrow{r},E \right)\text{m}\left( \overrightarrow{r},E \right).\]</div>
<p>In a typical Monte Carlo calculation, tallies are made by adding some
score, multiplied by the current particle weight, to an accumulator. To
calculate a similar quantity related to the Monte Carlo particle density
would be very close to calculating any other quantity but without
including the particle weight. The goal of FW-CADIS is to make the Monte
Carlo particle density, <span class="math notranslate nohighlight">\(m\left( \overrightarrow{r},E \right)\)</span>,
uniform over the tally areas, so an importance map needs to be developed
that represents the importance to achieving uniform Monte Carlo particle
density. By attempting to keep the Monte Carlo particle density more
uniform, more uniform relative errors for the tallies should be
realized.</p>
<p>Two options for forward weighting are possible. For tallies over some
area where the entire group-wise flux is needed with low relative
uncertainties, the adjoint source should be weighted inversely by the
forward flux, <span class="math notranslate nohighlight">\(\phi\left( \overrightarrow{r},E \right)\)</span>. The other
option, for a tally where only an energy-integrated quantity is desired,
is to weight the adjoint inversely by that energy-integrated
quantity,<span class="math notranslate nohighlight">\(\int_{}^{}{\sigma_{d}\left( E \right)\text{ϕ}\left( \overrightarrow{r},E \right)}\text{\ dE}\)</span>.
For a tally where the total flux is desired, then the response in the
adjoint source is simply <span class="math notranslate nohighlight">\(\sigma_{d}\left( E \right) = 1\)</span>.</p>
<p>To optimize the forward Monte Carlo simulation for the calculation of
some quantity at multiple tally locations or across a mesh tally, the
adjoint source needs to be weighted by the estimate of that quantity.
For a tally defined by its spatial location
<span class="math notranslate nohighlight">\(g\left( \overrightarrow{r} \right)\)</span> and its optional response
<span class="math notranslate nohighlight">\(\sigma_{d}\left( E \right)\)</span>, the standard adjoint source would be
<span class="math notranslate nohighlight">\(q^{+}\left( \overrightarrow{r},E \right) = \sigma_{d}\left( E \right)\text{g}\left( \overrightarrow{r} \right)\)</span>.
The forward-weighted adjoint source,
<span class="math notranslate nohighlight">\(q^{+}\left( \overrightarrow{r},E \right)\)</span>, depending on what
quantity is to be optimized, is listed below.</p>
<table class="docutils align-default">
<colgroup>
<col style="width: 40%" />
<col style="width: 60%" />
</colgroup>
<thead>
<tr class="row-odd"><th class="head"><p><strong>For the calculation of</strong></p></th>
<th class="head"><p><strong>Adjoint source</strong></p></th>
</tr>
</thead>
<tbody>
<tr class="row-even"><td><p>Energy and spatially dependent flux. <span class="math notranslate nohighlight">\(\phi\left(\overrightarrow{r},E \right)\)</span></p></td>
<td><div class="math notranslate nohighlight">
\[\frac{g\left( \overrightarrow{r}\right)}{\phi\left(\overrightarrow{r},E \right)}\]</div>
</td>
</tr>
<tr class="row-odd"><td><p>Spatially dependent total flux. <span class="math notranslate nohighlight">\(\int_{}^{}{\phi\left( \overrightarrow{r},E \right)}\textit{dE}\)</span></p></td>
<td><div class="math notranslate nohighlight">
\[\frac{g\left( \overrightarrow{r}\right)}{\int_{}^{}{\phi\left( \overrightarrow{r},E \right)}\textit{dE}}\]</div>
</td>
</tr>
<tr class="row-even"><td><p>Spatially dependent total response. <span class="math notranslate nohighlight">\(\int_{}^{}{\sigma_{d}\left( E \right)\text{ϕ}\left(\overrightarrow{r},E\right)}\textit{dE}\)</span></p></td>
<td><div class="math notranslate nohighlight">
\[\frac{\sigma_{d}\left( E \right)\text{g}\left( \overrightarrow{r} \right)}{\int_{}^{}{\sigma_{d}\left( E \right)\text{ϕ}\left( \overrightarrow{r},E \right)}\textit{dE}}\]</div>
</td>
</tr>
</tbody>
</table>
<p>The bottom line of FW-CADIS is that in order to calculate a quantity at
multiple tally locations (or across a mesh tally) with more uniform
relative uncertainties, an adjoint source needs to be developed for an
objective function that keeps some non-physical quantity—related to the
Monte Carlo particle density and similar in form to the desired
quantity—constant. FW-CADIS uses the solution of a forward
discrete-ordinates calculation to properly weight the adjoint source.
After that, the standard CADIS approach is used.</p>
</div>
</div>
<div class="section" id="mavric-implementation-of-cadis">
<h2>MAVRIC Implementation of CADIS<a class="headerlink" href="#mavric-implementation-of-cadis" title="Permalink to this headline"></a></h2>
<p>With MAVRIC, as with other shielding codes, the user defines the problem as a set of physical models—the material compositions, the geometry, the source, and the detectors (locations and response functions)—as well as some mathematical parameters on how to solve the problem (number of histories, etc.). For the variance reduction portion of MAVRIC, the only additional inputs required are (1) the mesh planes to use in the discrete-ordinates calculation(s) and (2) the adjoint source description—basically the location and the response of each tally to optimize in the forward Monte Carlo calculation. MAVRIC takes this information and constructs a Denovo adjoint problem. (The adjoint source is weighted by a Denovo forward flux or response estimate for FW-CADIS applications.) MAVRIC then uses the CADIS methodology: it combines the adjoint flux from the Denovo calculation with the source description and creates the importance map (weight window targets) and the mesh-based biased source. Monaco is then run using the CADIS biased source distribution and the weight window targets.</p>
<div class="section" id="denovo">
<h3>Denovo<a class="headerlink" href="#denovo" title="Permalink to this headline"></a></h3>
<p>Denovo is a parallel three-dimensional SN code that is used to generate adjoint (and, for FW-CADIS, forward) scalar fluxes for the CADIS methods in MAVRIC. For use in MAVRIC/CADIS, it is highly desirable that the SN code be fast, positive, and robust. The phase-space shape of the forward and adjoint fluxes, as opposed to a highly accurate solution, is the most important quality for Monte Carlo weight-window generation. Accordingly, Denovo provides a step-characteristics spatial differencing option that produces positive scalar fluxes as long as the source (volume plus in-scatter) is positive. Denovo uses an orthogonal, nonuniform mesh that is ideal for CADIS applications because of the speed and robustness of calculations on this mesh type.</p>
<p>Denovo uses the highly robust GMRES (Generalized Minimum Residual) Krylov method to solve the SN equations in each group. GMRES has been shown to be more robust and efficient than traditional source (fixed-point) iteration. The in-group discrete SN equations are defined as</p>
<div class="math notranslate nohighlight" id="equation-mavric-16">
<span class="eqno">(16)<a class="headerlink" href="#equation-mavric-16" title="Permalink to this equation"></a></span>\[\mathbf{L}\psi = \mathbf{\text{MS}}\phi + q\]</div>
<p>where <strong>L</strong> is the differential transport operator, <strong>M</strong> is the
moment-to-discrete operator, <strong>S</strong> is the matrix of scattering
cross-section moments, <em>q</em> is the external and in-scatter source,
<span class="math notranslate nohighlight">\(\phi\)</span> is the vector of angular flux moments, and <span class="math notranslate nohighlight">\(\psi\)</span> is
the vector of angular fluxes at discrete angles. Applying the operator
<strong>D</strong>, where <span class="math notranslate nohighlight">\(\phi = \mathbf{D}\psi\)</span>, and rearranging terms casts
the in-group equations in the form of a traditional linear system,
<span class="math notranslate nohighlight">\(\mathbf{A}x = b\)</span>,</p>
<blockquote>
<div><div class="math notranslate nohighlight" id="equation-mavric-17">
<span class="eqno">(17)<a class="headerlink" href="#equation-mavric-17" title="Permalink to this equation"></a></span>\[\left( \mathbf{I} - \mathbf{D}\mathbf{L}^{- 1}\mathbf{\text{MS}} \right) = \mathbf{D}\mathbf{L}^{- 1}q .\]</div>
</div></blockquote>
<p>The operation <span class="math notranslate nohighlight">\(\mathbf{L}^{- 1}\nu\)</span>, where <span class="math notranslate nohighlight">\(\nu\)</span> is an
iteration vector, is performed using a traditional wave-front solve
(transport sweep). The parallel implementation of the Denovo wave-front
solver uses the well-known Koch-Baker-Alcouffe (KBA) algorithm, which is
a two-dimensional block‑spatial decomposition of a three-dimensional
orthogonal mesh <a class="bibtex reference internal" href="#baker-sn-1998" id="id6">[BK98]</a>. The Trilinos package is used for the GMRES
implementation <a class="bibtex reference internal" href="#willenbring-trilinos-2003" id="id7">[WH03]</a> Denovo stores the mesh-based scalar fluxes in a
double precision binary file (<a href="#id8"><span class="problematic" id="id9">*</span></a>.dff) called a Denovo flux file. Past
versions of SCALE/Denovo used the TORT <a class="bibtex reference internal" href="#rhoades-tort-1997" id="id10">[RS97]</a> *.varscl file format
(DOORS package <a class="bibtex reference internal" href="#rhoades-doors-1998" id="id11">[RC98]</a>), but this was limited to single precision. Since
the rest of the MAVRIC sequence has not yet been parallelized, Denovo is
currently used only in serial mode within MAVRIC.</p>
</div>
<div class="section" id="monaco">
<h3>Monaco<a class="headerlink" href="#monaco" title="Permalink to this headline"></a></h3>
<p>The forward Monte Carlo transport is performed using Monaco, a
fixed-source, shielding code that uses the SCALE General Geometry
Package (SGGP, the same as used by the criticality code KENO-VI) and the
standard SCALE material information processor. Monaco can use either MG
or CE cross section libraries. Monaco was originally based on the MORSE
Monte Carlo code but has been extensively modified to modernize the
coding, incorporate more flexibility in terms of sources/tallies, and
read a user-friendly block/keyword style input.</p>
<p>Much of the input to MAVRIC is the same as Monaco. More details can be
found in the Monaco chapter of the SCALE manual.</p>
</div>
<div class="section" id="running-mavric">
<h3>Running MAVRIC<a class="headerlink" href="#running-mavric" title="Permalink to this headline"></a></h3>
<p>The objective of a SCALE sequence is to execute several codes, passing
the output from one to the input of the next, in order to perform some
analysis—things that users typically had to do in the past. MAVRIC does
this for difficult shielding problems by running approximate
discrete-ordinates calculations, constructing an importance map and
biased source for one or more tallies that the user wants to optimize in
the Monte Carlo calculation, and then using those in a forward Monaco
Monte Carlo calculation. MAVRIC also prepares the forward and adjoint
cross sections when needed. The steps of a MAVRIC sequence are listed in
<a class="reference internal" href="#mavric-sequence"><span class="std std-numref">Table 1</span></a>. The user can instruct MAVRIC to run this whole sequence of
steps or just some subset of the steps—in order to verify the
intermediate steps or to reuse previously calculated quantities in a new
analyses.</p>
<p>The MAVRIC sequence can be stopped after key points by using the
“parm= <em>parameter</em> ” operator on the “=mavric” command line, which is
the first line of the input file. The various parameters are listed in
Table <a class="reference internal" href="#mavric-param"><span class="std std-numref">Table 2</span></a>. These parameters allow the user to perform checks and make
changes to the importance map calculation before the actual Monte Carlo
calculation in Monaco.</p>
<p>MAVRIC also allows the sequence to start at several different points. If
an importance map and biased source have already been computed, they can
be used directly. If the adjoint scalar fluxes are known, they can
quickly be used to create the importance map and biased source and then
begin the forward Monte Carlo. All of the different combinations of
starting MAVRIC with some previously calculated quantities are listed in
the following section detailing the input options.</p>
<p>When using MG cross-section libraries that do not have flux-to-dose-rate
conversion factors, use “parm=nodose” to prevent the cross section
processing codes from trying to move these values into the working
library.</p>
<p>MAVRIC creates many files that use the base problem name from the output
file. For an output file called “c:path1path2\<em>outputName</em>.out” or
“/home/path1/path2/ <em>outputName</em>.inp”, spaces in the output name will
cause trouble and should not be used.</p>
<table class="colwidths-given docutils align-center" id="mavric-sequence">
<caption><span class="caption-number">Table 1 </span><span class="caption-text">Steps in the MAVRIC sequence</span><a class="headerlink" href="#mavric-sequence" title="Permalink to this table"></a></caption>
<colgroup>
<col style="width: 50%" />
<col style="width: 50%" />
</colgroup>
<tbody>
<tr class="row-odd"><td><p><strong>Cross section calculation</strong></p></td>
<td><p>XSProc is used to calculate the forward cross sections for Monaco</p></td>
</tr>
<tr class="row-even"><td><p><strong>Forward Denovo (optional)</strong></p></td>
<td></td>
</tr>
<tr class="row-odd"><td><p>Cross section calculation</p></td>
<td><p>XSProc is used to calculate the forward cross sections for Denovo</p></td>
</tr>
<tr class="row-even"><td><p>Forward flux calculation</p></td>
<td><p>Denovo calculates the estimate of the forward flux</p></td>
</tr>
<tr class="row-odd"><td><p><strong>Adjoint Denovo (optional)</strong></p></td>
<td></td>
</tr>
<tr class="row-even"><td><p>Cross section calculation</p></td>
<td><p>XSProc is used to calculate the adjoint cross sections for Denovo</p></td>
</tr>
<tr class="row-odd"><td><p>Adjoint flux calculation</p></td>
<td><p>Denovo calculates the estimate of the adjoint flux</p></td>
</tr>
<tr class="row-even"><td><p><strong>CADIS (optional)</strong></p></td>
<td><p>The scalar flux file from Denovo is then used to create the biased source distribution and transport weight windows</p></td>
</tr>
<tr class="row-odd"><td><p><strong>Monte Carlo calculation</strong></p></td>
<td><p>Monaco uses the biased source distribution and transport weight windows to calculate the various tallies</p></td>
</tr>
</tbody>
</table>
<table class="colwidths-given docutils align-center" id="mavric-param">
<caption><span class="caption-number">Table 2 </span><span class="caption-text">Parameters for the MAVRIC command line (“parm=…”)</span><a class="headerlink" href="#mavric-param" title="Permalink to this table"></a></caption>
<colgroup>
<col style="width: 50%" />
<col style="width: 50%" />
</colgroup>
<thead>
<tr class="row-odd"><th class="head"><p>Parameter</p></th>
<th class="head"><p>MAVRIC will stop after</p></th>
</tr>
</thead>
<tbody>
<tr class="row-even"><td><p>check</p></td>