# Cubature (Multi-dimensional integration)

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## Contents |

## Cubature

Steven G. Johnson has written a simple C subroutine for **adaptive multidimensional integration** (*cubature*) of **vector-valued integrands** over **hypercubes**, i.e. to compute integrals of the form:

(Of course, it can handle scalar integrands as the special case where is a one-dimensional vector: the dimensionalities of and are independent.) The code, which is distributed as **free software** under the terms of the GNU General Public License (v2 or later), is based on the algorithms described in:

- A. C. Genz and A. A. Malik, "An adaptive algorithm for numeric integration over an N-dimensional rectangular region,"
*J. Comput. Appl. Math.***6**(4), 295–302 (1980). - J. Berntsen, T. O. Espelid, and A. Genz, "An adaptive algorithm for the approximate calculation of multiple integrals,"
*ACM Trans. Math. Soft.***17**(4), 437–451 (1991).

(Note that we do *not* use any of the original DCUHRE code by Genz, which is not under a free/open-source license.) Our code is based in part on code borrowed from the HIntLib numeric-integration library by Rudolf Schürer and (for 1d integrals) from code for Gauss-Kronrod quadrature from the GNU Scientific Library, both of which are free software under the GNU GPL. (Another free-software multi-dimensional integration library, unrelated to our code here but also implementing the Genz–Malik algorithm, is Cuba.)

I am also grateful to Dmitry Turbiner (dturbiner ατ alum.mit.edu), who implemented an initial prototype of the "vectorized" functionality (see below) for evaluating multiple points in a single call (as opposed to multiple functions in a single call), which facilitates parallelization of the integrand evaluation.

## Download

The current version of the code can be downloaded from:

a gzipped tar file. This unpacks to a directory containing a `README`

file with instructions and a stand-alone `cubature.c`

file that you can compile and link into your program, and a header file `cubature.h`

that you `#include`

. (The `cubature.c`

code is small enough that it doesn't seem worthwhile to go to the trouble of installing it as a library.) The `cubature.c`

also contains a little test program which is produced if you compile that file with `-DTEST_INTEGRATOR`

(and is commented out otherwise), as described below.

B. Narasimhan wrote a GNU R interface for these routines, which can be downloaded here: http://cran.r-project.org/web/packages/cubature/index.html.

## Usage

You should compile `cubature.c`

and link it with your program, and `#include`

the header file `cubature.h`

.

The central subroutine you will be calling is:

int adapt_integrate(unsigned fdim, integrand f, void *fdata, unsigned dim, const double *xmin, const double *xmax, unsigned maxEval, double reqAbsError, double reqRelError, double *val, double *err);

This integrates a function F(x), returning a vector of FDIM integrands, where x is a DIM-dimensional vector ranging from XMIN to XMAX (i.e. in a hypercube XMIN_{i} ≤ x_{i} ≤ XMAX_{i}).

MAXEVAL specifies a maximum number of function evaluations (0 for no limit). Otherwise, the integration stops when the estimated |error| is less than REQABSERROR (the absolute error requested), or when the estimated |error| is less than REQRELERROR × |integral value| (the relative error requested). (Either of the error tolerances can be set to zero to ignore it.)

VAL and ERR are arrays of length FDIM, which upon return are the computed integral values and estimated errors, respectively. (The estimated errors are based on an embedded cubature rule of lower order; for smooth functions, this estimate is usually conservative.)

The return value of adapt_integrate is 0 on success and nonzero if there was an error (currently, only out-of-memory situations).

The integrand function F should be a function of the form:

void f(unsigned ndim, const double *x, void *fdata, unsigned fdim, double *fval);

Here, the input is an array X of length NDIM (the point to be evaluated), the output is an array FVAL of length FDIM (the vector of function values at the point X).

The FDATA argument of F is equal to the FDATA argument passed to `adapt_integrate`

—this can be used by the caller to pass any additional information through to F as needed (rather than using global variables, which are not re-entrant). If F does not need any additional data, you can just pass FDATA = `NULL`

and ignore the FDATA argument to F.

### "Vectorized" interface

These integration algorithms evaluate the integrand in "batches" of several points at a time. It is often useful to have access to this information so that your integrand function is not called for one point at a time, but rather for a whole "vector" of many points at once. For example, you may want to evaluate the integrand in parallel at different points. This functionality is available by calling:

int adapt_integrate_v(unsigned fdim, integrand_v f, void *fdata, unsigned dim, const double *xmin, const double *xmax, unsigned maxEval, double reqAbsError, double reqRelError, double *val, double *err);

All of the arguments and the return value are identical to `adapt_integrate`

, above, except that now the integrand `F`

is of type `integrand_v`

, corresponding to a function of a different form. The integrand function F should now be a function of the form:

void f(unsigned ndim, unsigned npts, const double *x, void *fdata, unsigned fdim, double *fval);

Now, X is not a single point, but an array of NPTS points (length NPTS×NDIM), and upon return the values of all FDIM integrands at all NPTS points should be stored in FVAL (length FDIM×NPTS). In particular, `x[i*ndim + j]`

is the `j`

-th coordinate of the `i`

-th point (`i`

<`npts`

and `j`

<`ndim`

), and the `k`

-th function evaluation (`k`

<`fdim`

) for the `i`

-th point is returned in `fval[k*npt + i]`

.

The size of NPTS will vary with the dimensionality of the problem; higher-dimensional problems will have (exponentially) larger NPTS, allowing for the possibility of more parallelism. (However, for sufficiently high dimensions, e.g. >8, a different algorithm like Monte-Carlo integration or sparse grids is likely to be more efficient.) Currently, NPTS is 30 in 1d, 34 in 2d, and 66 in 3d, although the first call to `F`

will have half that many points.

### Example

As a simple example, consider the Gaussian integral of the scalar function over the hypercube [ − 2,2]^{3} in 3 dimensions. You could compute this integral via code that looks like:

#include <stdio.h> #include <math.h> #include "cubature.h" void f(unsigned ndim, const double *x, void *fdata, unsigned fdim, double *fval) { double sigma = *((double *) fdata);// we can pass σ via fdata argumentdouble sum = 0; unsigned i; for (i = 0; i < ndim; ++i) sum += x[i] * x[i];// compute the output value: note that fdim should == 1 from belowfval[0] = exp(-sigma * sum); }

then, later in the program where we call `adapt_integrate`

:

{ double xmin[3] = {-2,-2,-2}, xmax[3] = {2,2,2}, sigma = 0.5, val, err; adapt_integrate(1, f, &sigma, 3, xmin, xmax, 0, 0, 1e-4, &val, &err); printf("Computed integral = %0.10g +/- %g\n", val, err); }

Here, we have specified a relative error tolerance of 10^{ − 4} (and no absolute error tolerance or maximum number of function evaluations). Note also that, to demonstrate the `fdata`

parameter, we have used it to pass the σ value through to our function (rather than hard-coding the value of σ in `f`

or using a global variable).

The output should be:

Computed integral = 13.69609043 +/- 0.00136919

Note that the estimated *relative* error is 0.00136919/13.69609043 = 9.9969×10^{–5}, within our requested tolerance of 10^{ − 4}. The *actual* error in the integral value, as can be determined e.g. by running the integration with a much lower tolerance, is much smaller: the integral is too small by about 0.00002, for an actual relative error of about 1.4×10^{–6}. As mentioned above, for smooth integrands the estimated error is almost always conservative (which means, unfortunately, that the integrator usually does more function evaluations than it needs to).

With the vectorized interface `adapt_integrate_v`

, one would instead do:

void f(unsigned ndim, unsigned npts, const double *x, void *fdata, unsigned fdim, double *fval) { double sigma = *((double *) fdata); unsigned i, j; for (j = 0; j < npts; ++j) {// evaluate the integrand for npts pointsdouble sum = 0; for (i = 0; i < ndim; ++i) sum += x[j*ndim+i] * x[j*ndim+i]; fval[j] = exp(-sigma * sum); } }

### Infinite intervals

Integrals over infinite or semi-infinite intervals is possible by a change of variables. This is best illustrated in one dimension.

To compute an integral over a semi-infinite interval, you can perform the change of variables *x*=1/(1-*t*):

For an infinite interval, you can perform the change of variables *x*=*t*/(1-*t*^{2}):

Note the Jacobian factors multiplying *f*(⋅⋅⋅) in both integrals.

In multiple dimensions, one simply performs this change of variables on each dimension separately, as desired, multiplying the integrand by the corresponding Jacobian factor for each dimension being transformed.

The Jacobian factors diverge as the endpoints are approached. However, in order for your integral to have been finite in the first place it must be true that *f*(*x*) goes to zero at infinity faster than 1/*x*, hence the limit of the integrand multiplied by the Jacobian is zero at the endpoints. In any case, the quadrature/cubature rules currently employed in `cubature.c`

do not evaluate the integrand at the endpoints, so you need not implement special handling for |*t*|=1.

## Test program

To compile a test program, just compile `cubature.c`

while #defining `TEST_INTEGRATOR`

, e.g. (on Unix or GNU/Linux) via:

cc -DTEST_INTEGRATOR -o cubature_test cubature.c -lm

The usage is then:

./cubature_test <dim> <tol> <integrand> <maxeval>

where <dim> = # dimensions, <tol> = relative tolerance, <integrand> is 0–7 for one of eight possible test integrands (see below) and <maxeval> is the maximum number of function evaluations (0 for none, the default).

The different test integrands are:

- 0: a product of cosine functions
- 1: a Gaussian integral of exp(-x^2), remapped to [0,infinity) limits
- 2: volume of a hypersphere (integrating a discontinuous function!)
- 3: a simple polynomial (product of coordinates)
- 4: a Gaussian centered in the middle of the integration volume
- 5: a sum of two Gaussians
- 6: an example function by Tsuda, a product of terms with near poles
- 7: a test integrand by Morokoff and Caflisch, a simple product of dim-th roots of the coordinates (weakly singular at the boundary)

For example:

./cubature_test 3 1e-5 4

integrates the Gaussian function (4) to a desired relative error tolerance of 10^{–5} in 3 dimensions. The output is:

3-dim integral, tolerance = 1e-05 integrand 4: integral = 1, est err = 9.99952e-06, true err = 2.54397e-08 #evals = 82203

Notice that it finds the integral after 82203 function evaluations with an estimated error of about 10^{–5}, but the true error (compared to the exact result) is much smaller (2.5×10^{–8}): the error estimation is typically conservative when applied to smooth functions like this.