16 KiB
Exercise 5
The following integral is to be evaluated comparing different Monte Carlo techniques.
\begin{figure} \hypertarget{fig:exp}{% \centering \begin{tikzpicture} \definecolor{cyclamen}{RGB}{146, 24, 43} % Integral \filldraw [cyclamen!15!white, domain=0:5, variable=\x] (0,0) -- plot({\x},{exp(\x/5)}) -- (5,0) -- cycle; \draw [cyclamen] (5,0) -- (5,2.7182818); \node [below] at (5,0) {1}; % Axis \draw [thick, <-] (0,4) -- (0,0); \draw [thick, ->] (-2,0) -- (7,0); \node [below right] at (7,0) {$x$}; \node [above left] at (0,4) {$e^{x}$}; % Plot \draw [domain=-2:7, smooth, variable=\x, cyclamen, ultra thick] plot ({\x},{exp(\x/5)}); % Equation \node [above] at (2.5, 2.5) {$I = \int\limits_0^1 dx , e^x$}; \end{tikzpicture} \caption{Plot of the integral to be evaluated.} } \end{figure}
whose exact value is 1.7182818285...
The three most popular Monte Carlo (MC) methods where applied: plain MC, Miser
and Vegas. Besides being commonly used, these were chosen for also being
implemented in the GSL libraries gsl_monte_plain
, gsl_monte_miser
and
gsl_monte_vegas
, respectively.
Plain Monte Carlo
When an integral I
over a $n-$dimensional space \Omega
of volume V
of a
function f
has to be evaluated, that is:
I = \int\limits_{\Omega} dx \, f(x)
\with V = \int\limits_{\Omega} dx
the simplest MC method approach is to sample N
points x_i
in V
and
approximate I
as:
I \approx I_N = \frac{V}{N} \sum_{i=1}^N f(x_i) = V \cdot \avg{f}
If x_i
are uniformly distributed I_N \rightarrow I
for $N \rightarrow +
\infty$ by the law of large numbers, whereas the sample variance can be
estimated as:
\sigma^2_f = \frac{1}{N - 1}
\sum_{i = 1}^N \left( f(x_i) - \avg{f} \right)^2
\et
\sigma^2_I = \frac{V^2}{N^2} \sum_{i = 1}^N
\sigma^2_f = \frac{V^2}{N} \sigma^2_f
Thus, the error decreases as 1/\sqrt{N}
.
Unlike in deterministic methods, the error estimate is not a strict bound:
random sampling may not cover all the important features of the integrand and
this can result in an underestimation of the error.
In this case f(x) = e^{x}
and \Omega = [0,1]
, hence V = 1
.
Since the distance from I
of I_N
is related to N
, the accuracy of the
method lies in how many points are generated, namely how many function calls
are executed when the iterative method is implemented. In @fig:plain-mc-iter
and @fig:miser-iter, results obtained with the plain MC method are shown in
red. In @tbl:plain-mc-res, some of them are listed: the estimated integrals
I^{\text{oss}}
are compared to the expected value I
and the differences
between them are given.
calls I^{\text{oss}}
\sigma
diff
\num{5e5} 1.7166435813 0.0006955691 0.0016382472
\num{5e6} 1.7181231109 0.0002200309 0.0001587176
\num{5e7} 1.7183387184 0.0000695809 0.0000568899
Table: Some MC results with three different numbers of function calls. Differences between computed and exact values are given in diff. {#tbl:plain-mc-res}
As can be seen, \sigma
is always of the same order of magnitude of diff,
except for very low numbers of function calls. Even with \num{5e7} calls,
I^{\text{oss}}
still differs from I
at the fifth decimal place, meaning
that this method shows a really slow convergence.
The \sigma
dependence on the number C
of function calls was checked with a
least square minimization by modeling the data with the function:
\sigma = \frac{a}{x^b}
As can be seen in @fig:err_fit, the obtained result confirmes the expected value
of b^{\text{exp}} = 0.5
, having found b \sim 0.499
.
Given this dependence, for an error of 10^{-n}
, a number \propto 10^{2n}
of
function calls is needed. To compute an integral within double precision, an
impossibly large number of \sigma \sim 10^{32}
calls is needed, which makes
this method unpractical for high-precision applications.
Stratified sampling
In statistics, stratified sampling is a method of sampling from a population
partitioned into subpopulations. Stratification, indeed, is the process of
dividing the primary sample into subgroups (strata) before sampling
within each stratum.
Given a sample \{x_j\}_i
of the $i$-th strata, its mean \bar{x}_i
and
variance {\sigma^2_x}_i
, are given by
\bar{x}_i = \frac{1}{n_i} \sum_j x_j
and from:
\sigma_i^2 = \frac{1}{n_i - 1} \sum_j \left( x_j - \bar{x}_i \right)^2
\thus
{\sigma^2_x}_i = \frac{1}{n_i^2} \sum_j \sigma_i^2 = \frac{\sigma_i^2}{n_i}
where:
j
runs over the pointsx_j
of the samplen_i
is the size of the sample\sigma_i^2
is the variance associated to every point of the $i$-th stratum.
An estimation of the mean \bar{x}
and variance \sigma_x^2
for the whole
population are then given by the stratified sampling as follows:
\bar{x} = \frac{1}{N} \sum_i N_i \bar{x}_i \et
\sigma_x^2 = \sum_i \left( \frac{N_i}{N} \right)^2 {\sigma_x}^2_i
= \sum_i \left( \frac{N_i}{N} \right)^2 \frac{\sigma^2_i}{n_i}
where:
i
runs over the strata,N_i
is the weight of the $i$-th stratumN
is the sum of all strata weights.
In practical terms, it can produce a weighted mean that has less variability
than the arithmetic mean of a simple random sample of the whole population. In
fact, if measurements within strata have lower standard deviation, the final
result will have a smaller error in estimation with respect to the one otherwise
obtained with simple sampling.
For this reason, stratified sampling is used as a method of variance reduction
when MC methods are used to estimate population statistics from a known
population. For examples, see [@ridder17].
MISER
The MISER technique aims at reducing the integration error through the use of
recursive stratified sampling.
As stated before, according to the law of large numbers, for a large number of
extracted points, the estimation of the integral I
can be computed as:
I= V \cdot \avg{f}
Since V
is known (in this case, V = 1
), it is sufficient to estimate
\avg{f}
.
Consider two disjoint regions a
and b
, such that a \cup b = \Omega
, in
which n_a
and n_b
points are respectively uniformly sampled. Given the
Monte Carlo estimates of the means \avg{f}_a
and \avg{f}_b
of those points
and their variances \sigma_a^2
and \sigma_b^2
, if the weights N_a
and
N_b
of \avg{f}_a
and \avg{f}_b
are chosen unitary, then the variance
\sigma^2
of the combined estimate \avg{f}
:
\avg{f} = \frac{1}{2} \left( \avg{f}_a + \avg{f}_b \right)
is given by:
\sigma^2 = \frac{\sigma_a^2}{4n_a} + \frac{\sigma_b^2}{4n_b}
It can be shown that this variance is minimized by distributing the points such that:
\frac{n_a}{n_a + n_b} = \frac{\sigma_a}{\sigma_a + \sigma_b}
Hence, the smallest error estimate is obtained by allocating sample points in
proportion to the standard deviation of the function in each sub-region.
The whole integral estimate and its variance are therefore given by:
I = V \cdot \avg{f} \et \sigma_I^2 = V^2 \cdot \sigma^2
When implemented, MISER is in fact a recursive method. First, all the possible
bisections of \Omega
are tested and the one which minimizes the combined
variance of the two sub-regions is selected. In order to speed up the
algorithm, the variance in the sub-regions is estimated with a fraction of the
total number of available points (function calls), in GSL it default to 0.1.
The remaining points are allocated to the sub-regions using the formula for
n_a
and n_b
, once the variances are computed.
This procedure is then repeated recursively for each of the two half-regions
from the best bisection. When the allocated calls for a region running out
(less than 512 in GSL), the method falls back to a plain Monte Carlo.
The final individual values and their error estimates are then combined upwards
to give an overall result and an estimate of its error [@sayah19].
Results for this particular sample are shown in black in @fig:miser-iter and some of them are listed in @tbl:miser-res. Except for the first very little number of calls, the improvement with respect to the Plain MC technique (in red) is appreciable.
calls I^{\text{oss}}
\sigma
diff
\num{5e5} 1.7182850738 0.0000021829 0.0000032453
\num{5e6} 1.7182819143 0.0000001024 0.0000000858
\num{5e7} 1.7182818221 0.0000000049 0.0000000064
Table: MISER results with different numbers of function calls. Differences between computed and exact values are given in diff. {#tbl:miser-res}
The convergence is much faster than a plain MC: at 500'000 function calls, the estimate agrees with the exact integral to the fifth decimal place. Once again, the standard deviation and the difference share the same magnitude.
Importance sampling
In Monte Carlo methods, importance sampling is a technique which samples points
from distribution whose shape is close to the integrand f
itself. In this way
the points cluster in the regions that make the largest contribution to the
integral \int f(x)dx
and consequently decrease the variance.
In a plain MC the points are sampled uniformly, so their probability density is given by
g(x) = \frac{1}{V} \quad \forall x \in \Omega
and the integral can be written as
I = \int_\Omega dx f(x) = V \int_\Omega f(x) \frac{1}{V}dx
\approx V \avg{f}
More generally, consider a distribution h(x)
and similarly do
I
= \int_\Omega dx f(x)
= \int_\Omega dx \, \frac{f(x)}{h(x)} \, h(x)
= \Exp \left[ \frac{f}{h}, h \right]
where \Exp[X, h]
is the expected value of X
wrt h
.
Also note that h
has to vanish outside \Omega
for this to hold.
As anticipated, to reduce the variance h
must be close to f
.
Assuming they are proportional, h(x) = \alpha |f(x)|
, it follows
that:
\Exp \left[ \frac{f}{h}, h \right] = \frac{1}{\alpha}
\et
\Var \left[ \frac{f}{h}, h \right] = 0
For the expected value to give the original I
, the proportionality constant
must be taken to be I^{-1}
, meaning:
h(z) = \frac{1}{I}\, |f(z)|
The sampling from this h
would produce a perfect result with zero variance.
Of course, this is nonsense: if I
is known in advance, there would be no need
to do a Monte Carlo integration to begin with. Nonetheless, this example serves
to prove how variance reduction is achieved by sampling from an approximation
of the integrand.
In conclusion, since certain values of x
have more impact on $\Exp[f/h, h]$
than others, these "important" values must be emphasized by sampling them more
frequently. As a consequence, the estimator variance will be reduced.
VEGAS
The VEGAS algorithm [@lepage78] of G. P. Lepage is based on importance
sampling. As stated before, it is in practice impossible to sample points from
the best distribution h(x)
: only a good approximation can be achieved. The
VEGAS algorithm attempts this by building a histogram of the function f
in
different subregions with an iterative method, namely:
-
a fixed number of points (function calls) is generated uniformly in the whole region;
-
the volume
V
is divided intoN
intervals of width $\Delta x_i = \Delta x , \forall , i$, whereN
is limited by the computer storage space available and must be held constant from iteration to iteration. (In GSL this default toN = 50
); -
each interval is then divided into
m_i + 1
subintervals, where:m_i = K \frac{\bar{f}_i \Delta x_i}{\sum_j \bar{f}_j \Delta x_j}
where
j
runs over all the intervals and\bar{f}_i
is the average value off
in the interval. Hence,m_i
is therefore a measure of the "importance" of the interval with respect to the others: the higher\bar{f}_i
, the higherm_i
. The constantK
is called stiffness. It is defaults 1.5 in GSL; -
as it is desirable to restore the number of intervals to its original value
N
, groups of the new intervals must be merged into larger intervals, the number of subintervals in each group being constant. The net effect is to alter the intervals sizes, while keeping the total number constant, so that the smallest intervals occur wheref
is largest; -
the function is integrated with a plain MC method in each interval and the sum of the integrals is taken as the $j$-th estimate of
I
. Its error is given the sum of the variances in each interval. -
the new grid is used and further refined in subsequent iterations. By default, the number of iterations 5 in GSL.
The final estimate of the integral I
and its error
\sigma_I
are made based on weighted average:
\avg{I} = \sigma_I^2 \sum_i \frac{I_i}{\sigma_i^2}
\with
\frac{1}{\sigma_I^2} = \sum_i \frac{1}{\sigma_i^2}
where I_i
and \sigma_i
are are the integral and standard deviation
estimated in each iteration.
The reliability of the result is asserted by a chi-squared per degree of
freedom \chi_r^2
, which should be close to 1 for a good estimation. At a
given iteration i
, the \chi^2_i
is computed as follows:
\chi^2_i = \sum_{j \le i}
\frac{(I_j - \avg{I})^2}{\sigma_j^2}
While performing the iterations, if the value of \chi_r^2
exceed 1.5, the
routine stops since is not making progress.
Clearly, a better estimation is achieved with a greater number of function calls. For this particular sample, the most accurate results are shown in @fig:vegas-iter and some of them are listed in @tbl:vegas-res.
calls I^{\text{oss}}
\sigma
diff \chi_r^2
\num{5e5} 1.7182818281 0.0000000012 0.0000000004 1.457
\num{5e6} 1.7182818284 0.0000000000 0.0000000001 0.632
\num{5e7} 1.7182818285 0.0000000000 0.0000000000 0.884
Table: Some VEGAS results with different numbers of function calls. {#tbl:vegas-res}
As can be appreciated in @fig:vegas-iter, the VEGAS algorithm manages to compute the
integral value more accurately compared to MISER. The \chi_r^2
turns out to
be close enough to 1 to guarantee a good estimation of I
, goodness which is
also confirmed by the very small difference shown in @tbl:vegas-res.
In fact, with a number of \num{5e7} function calls, the difference is
smaller than \num{1e-10}.
In conclusion, between a plain Monte Carlo technique, stratified sampling and importance sampling, the last turned out to be the most powerful mean to obtain a good estimation of the integrand.