Eliminated another initialization error and tweaked rdf-adf example
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@ -133,7 +133,7 @@ arguments are specified.
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The first ADF value for a bin is calculated from the histogram count by
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dividing by the total number of triples satisfying the criteria,
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so that the integral of the ADF w.r.t. angle is one i.e. the ADF
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so that the integral of the ADF w.r.t. angle is 1, i.e. the ADF
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is a probability density function.
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The second ADF value is reported as a cumulative sum of
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@ -147,9 +147,15 @@ number radial distribution function.
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The {ordinate} optional keyword determines
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whether the bins are of uniform angular size from zero
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to 180 ({degree}), zero to Pi ({radian}), or the
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cosine of the angle uniform in the range \[-1,1\] ({cosine}).
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Regardless of which is chosen, the first ADF will be normalized
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so that the integral w.r.t. the ordinate is one.
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cosine of the angle uniform in the range \[-1,1\] ({cosine}).
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{cosine} has the advantage of eliminating the {acos()} function
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call, which speeds up the compute by 2-3x, and it is also preferred
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on physical grounds, because the for uniformly distributed particles
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in 3D, the angular probability density w.r.t dtheta is
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sin(theta)/2, while for d(cos(theta)), it is 1/2,
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Regardless of which ordinate is chosen, the first column of ADF
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values is normalized w.r.t. the range of that ordinate, so that
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the integral is 1.
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The simplest way to output the results of the compute adf calculation
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to a file is to use the "fix ave/time"_fix_ave_time.html command, for
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@ -177,7 +183,7 @@ the angle in degrees or radians, or the cosine of the angle. Each
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subsequent pair of columns gives the first and second kinds of ADF
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for a specific set of ({itypeN},{jtypeN},{ktypeN}). The values
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in the first ADF column are normalized numbers >= 0.0,
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whose integral w.r.t. the ordinate is one,
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whose integral w.r.t. the ordinate is 1,
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i.e. the first ADF is a normalized probability distribution.
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The values in the second ADF column are also numbers >= 0.0.
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They are the cumulative density distribution of angles per atom.
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