Cubature (Multidimensional integration)
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== Cubature ==  == Cubature ==  
  [http://math.mit.edu/~stevenj Steven G. Johnson] has written a simple C subroutine for '''adaptive multidimensional integration''' (''cubature'') of '''vectorvalued integrands''' over '''hypercubes''', i.e. to compute integrals of the form:  +  [http://math.mit.edu/~stevenj Steven G. Johnson] has written a simple C package for '''adaptive multidimensional integration''' (''cubature'') of '''vectorvalued integrands''' over '''hypercubes''', i.e. to compute integrals of the form: 
:<math>\int_{a_1}^{b_1}\int_{a_2}^{b_2}\cdots\int_{a_n}^{b_n} \vec{f}(\vec{x}) d^n\vec{x}</math>  :<math>\int_{a_1}^{b_1}\int_{a_2}^{b_2}\cdots\int_{a_n}^{b_n} \vec{f}(\vec{x}) d^n\vec{x}</math>  
  (Of course, it can handle scalar integrands as the special case where <math>\vec{f}</math> is a onedimensional vector: the dimensionalities of <math>\vec{f}</math> and <math>\vec{x}</math> are independent.) The code, which is distributed as '''free software''' under the terms of the [[w:GNU General Public LicenseGNU General Public License]] (v2 or later), is based on the algorithms described in:  +  (Of course, it can handle scalar integrands as the special case where <math>\vec{f}</math> is a onedimensional vector: the dimensionalities of <math>\vec{f}</math> and <math>\vec{x}</math> are independent.) The integrand can be evaluated for an '''array of points at once''' to enable '''easy parallelization'''. The code, which is distributed as '''free software''' under the terms of the [[w:GNU General Public LicenseGNU General Public License]] (v2 or later), implements two algorithms for adaptive integration. 
+  
+  The first, ''h''adaptive integration (recursively partitioning the integration domain into smaller subdomains, applying the same integration rule to each, until convergence is achieved), is based on the algorithms described in:  
* A. C. Genz and A. A. Malik, "An adaptive algorithm for numeric integration over an Ndimensional rectangular region," ''J. Comput. Appl. Math.'' '''6''' (4), 295–302 (1980).  * A. C. Genz and A. A. Malik, "An adaptive algorithm for numeric integration over an Ndimensional 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).  * 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/opensource license.) Our code is based in part on code borrowed from the [http://mint.sbg.ac.at/HIntLib/ HIntLib numericintegration library] by Rudolf Schürer and (for 1d integrals) from code for GaussKronrod quadrature from the [http://www.gnu.org/software/gsl/ GNU Scientific Library], both of which are free software under the GNU GPL.  +  This algorithm is '''best suited for a moderate number of dimensions''' (say, < 7), and is superseded for highdimensional integrals by other methods (e.g. [[w:Monte Carlo integrationMonte Carlo]] variants or [[w:Sparse gridsparse grids]]). 
+  
+  (Note that we do ''not'' use any of the original DCUHRE code by Genz, which is not under a free/opensource license.) Our code is based in part on code borrowed from the [http://mint.sbg.ac.at/HIntLib/ HIntLib numericintegration library] by Rudolf Schürer and from code for GaussKronrod quadrature (for 1d integrals) from the [http://www.gnu.org/software/gsl/ GNU Scientific Library], both of which are free software under the GNU GPL. (Another freesoftware multidimensional integration library, unrelated to our code here but also implementing the Genz–Malik algorithm among other techniques, is [http://www.feynarts.de/cuba/ Cuba].)  
+  
+  The second, ''p''adaptive integration (repeatedly doubling the degree of the quadrature rules until convergence is achieved), is based on a tensor product of [[w:Clenshaw–Curtis quadratureClenshaw–Curtis quadrature]] rules. This algorithm is often superior to ''h''adaptive integration for [[w:Smooth functionsmooth]] integrands in a few (≤3) dimensions, but is a poor choice in higher dimensions or for nonsmooth integrands.  
+  
+  For the most part, the ''p''adaptive routines below are dropin replacements for the ''h''adaptive routines, with the same arguments etcetera, so you can experiment to see which one works best for your problem. One difference: the ''h''adaptive routines do *not* evaluate the integrand on the boundaries of the integration volume, whereas the ''p''adaptive routines *do* evaluate the integrand at the boundaries. This means that the ''p'' adaptive routines require more care in cases where there are singularities at the boundaries.  
  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).  +  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 an array of points in a single call, which facilitates parallelization of the integrand evaluation. 
== Download ==  == Download ==  
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The current version of the code can be downloaded from:  The current version of the code can be downloaded from:  
  * [http://abinitio.mit.edu/cubature/cubature20101016.tgz cubature20101016.tgz]  +  * [http://abinitio.mit.edu/cubature/cubature1.0.2.tgz cubature1.0.2.tgz] 
  a [[w:gzipgzipped]] [[w:tar (file format)tar]] file. This unpacks to a directory containing a <code>README</code> file with instructions and a standalone <code>cubature.c</code> file that you can compile and link into your program, and a header file <code>cubature.h</code> that you <code>#include</code>. (The <code>cubature.c</code> code is small enough that it doesn't seem worthwhile to go to the trouble of installing it as a library.) The <code>cubature.c</code> also contains a little test program which is produced if you compile that file with <code>DTEST_INTEGRATOR</code> (and is commented out otherwise), as described below.  +  a [[w:gzipgzipped]] [[w:tar (file format)tar]] file. This unpacks to a directory containing a <code>README</code> file with instructions and a standalone <code>hcubature.c</code> or <code>pcubature.c</code> file (along with a couple of private header files) that you can compile and link into your program for hadaptive and padaptive integration, respectively, and a header file <code>cubature.h</code> that you <code>#include</code>. 
  B. Narasimhan wrote a [[w:GNU RGNU R]] interface for these routines, which can be downloaded here: [http://cran.rproject.org/web/packages/cubature/index.html http://cran.rproject.org/web/packages/cubature/index.html].  +  The <code>test.c</code> file contains a little test program which is produced if you compile that file with <code>DHCUBATURE</code> or <code>DPCUBATURE</code> and link with <code>hcubature.c</code> or <code>pcubature.c</code>, respectively, as described below. 
+  
+  B. Narasimhan wrote a [[w:GNU RGNU R]] interface, which can be downloaded here: [http://cran.rproject.org/web/packages/cubature/index.html http://cran.rproject.org/web/packages/cubature/index.html].  
+  
+  A [http://julialang.org/ Julia] interface can be obtained from [https://github.com/stevengj/Cubature.jl Cubature.jl]. A Python [https://github.com/saullocastro/cubature cubature.py interface] written by Saullo Castro is also available.  
== Usage ==  == Usage ==  
  You should compile <code>cubature.c</code> and link it with your program, and <code>#include</code> the header file <code>cubature.h</code>.  +  You should compile <code>hcubature.c</code> and/or <code>pcubature.c</code> and link it with your program, and <code>#include</code> the header file <code>cubature.h</code>. 
+  
+  The central subroutine you will be calling for hadaptive cubature is:  
  The central subroutine you will be calling is:  +  int hcubature(unsigned fdim, integrand f, void *fdata, 
+  unsigned dim, const double *xmin, const double *xmax,  
+  size_t maxEval, double reqAbsError, double reqRelError,  
+  error_norm norm,  
+  double *val, double *err);  
  int adapt_integrate(unsigned fdim, integrand f, void *fdata,  +  or <code>pcubature</code> (same arguments) for padaptive cubature. (See also the vectorized interface below.) 
  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 DIMdimensional vector ranging from XMIN to XMAX (i.e. in a hypercube XMIN<sub>i</sub> ≤ x<sub>i</sub> ≤ XMAX<sub>i</sub>).  This integrates a function F(x), returning a vector of FDIM integrands, where x is a DIMdimensional vector ranging from XMIN to XMAX (i.e. in a hypercube XMIN<sub>i</sub> ≤ x<sub>i</sub> ≤ XMAX<sub>i</sub>).  
  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  +  MAXEVAL specifies a maximum number of function evaluations (0 for no limit). <nowiki>[</nowiki>Note: the actual number of evaluations may somewhat exceed MAXEVAL: MAXEVAL is rounded up to an integer number of subregion evaluations.<nowiki>]</nowiki> 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.)  +  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  +  For vectorvalued integrands (FDIM > 1), NORM specifies the norm that is used to measure the error and determine convergence properties. 
  order; for smooth functions, this estimate is usually conservative.)  +  (The NORM argument is irrelevant for FDIM ≤ 1 and is ignored.) Given vectors ''v'' and ''e'' of estimated integrals and errors therein, respectively, the NORM argument takes on one of the following enumerated constant values: 
  The return value of adapt_integrate is 0 on success and nonzero if there was an error (currently, only outofmemory situations).  +  * <code>ERROR_L1</code>, <code>ERROR_L2</code>, <code>ERROR_LINF</code>: the absolute error is measured as ''e'' and the relative error as ''e''/''v'', where ... is the [[w:Taxicab geometryL<sub>1</sub>]], [[w:Euclidean distanceL<sub>2</sub>]], or [[w:Maximum normL<sub>∞</sub>]] [[w:Norm (mathematics)norm]], respectively. (''x'' in the L<sub>1</sub> norm is the sum of the absolute values of the components, in the L<sub>2</sub> norm is the root mean square of the components, and in the L<sub>∞</sub> norm is the maximum absolute value of the components) 
  The integrand function F should be a function of the form:  +  * <code>ERROR_INDIVIDUAL</code>: Convergence is achieved only when each integrand (each component of v and e) individually satisfies the requested error tolerances. 
  void f(unsigned ndim, const double *x, void *fdata,  +  * <code>ERROR_PAIRED</code>: Like <code>ERROR_INDIVIDUAL</code>, except that the integrands are grouped into consecutive pairs, with the error tolerance applied in an L2 sense to each pair. This option is mainly useful for integrating vectors of complex numbers, where each consecutive pair 
  unsigned fdim, double *fval);  +  of real integrands is the real and imaginary parts of a single complex integrand, and you only care about the error in the complex plane rather than the error in the real and imaginary parts separately. 
  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).  +  <code>VAL</code> and <code>ERR</code> are arrays of length <code>FDIM</code>, 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 FDATA argument of F is equal to the FDATA argument passed to <code>adapt_integrate</code>—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 reentrant). If F does not need any additional data, you can just pass FDATA = <code>NULL</code> and ignore the FDATA argument to F.  +  The return value of <code>hcubature</code> and <code>pcubature</code> is 0 on success and nonzero if there was an error (mainly only outofmemory situations or if the integrand signals an error). For a nonzero return value, the contents of the <code>VAL</code> and <code>ERR</code> arrays are undefined. 
+  
+  The integrand function <code>F</code> should be a function of the form:  
+  
+  int f(unsigned ndim, const double *x, void *fdata,  
+  unsigned fdim, double *fval);  
+  
+  Here, the input is an array <code>X</code> of length <code>NDIM</code> (the point to be evaluated), the output is an array <code>FVAL</code> of length <code>FDIM</code> (the vector of function values at the point <code>X</code>). he return value should be 0 on success or a nonzero value if an error occurred and the integration is to be terminated immediately (<code>hcubature</code> will then return a nonzero error code).  
+  
+  The <code>FDATA</code> argument of <code>F</code> is equal to the <code>FDATA</code> argument passed to <code>hcubature</code>—this can be used by the caller to pass any additional information through to <code>F</code> as needed (rather than using global variables, which are not reentrant). If <code>F</code> does not need any additional data, you can just pass <code>FDATA</code> = <code>NULL</code> and ignore the <code>FDATA</code> argument to <code>F</code>.  
=== "Vectorized" interface ===  === "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:  +  These integration algorithms actually 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,  +  int hcubature_v(unsigned fdim, integrand_v f, void *fdata, 
  unsigned dim, const double *xmin, const double *xmax,  +  unsigned dim, const double *xmin, const double *xmax, 
  unsigned maxEval, double reqAbsError, double reqRelError,  +  unsigned maxEval, double reqAbsError, double reqRelError, 
  double *val, double *err);  +  error_norm norm, double *val, double *err); 
  All of the arguments and the return value are identical to <code>adapt_integrate</code>, above, except that now the integrand <code>F</code> is of type <code>integrand_v</code>, corresponding to a function of a different form. The integrand function F should now be a function of the form:  +  (and similarly for <code>pcubature_v</code>). All of the arguments and the return value are identical to <code>hcubature</code>, above, except that now the integrand <code>F</code> is of type <code>integrand_v</code>, corresponding to a function of a different form. The integrand function <code>F</code> should now be a function of the form: 
  void f(unsigned ndim, unsigned npts, const double *x, void *fdata,  +  int f(unsigned ndim, unsigned npts, const double *x, void *fdata, 
  unsigned fdim, double *fval);  +  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, <code>x[i*ndim + j]</code> is the <code>j</code>th coordinate of the <code>i</code>th point (<code>i</code><<code>npts</code> and <code>j</code><<code>ndim</code>), and the <code>k</code>th function evaluation (<code>k</code><<code>fdim</code>) for the <code>i</code>th point is returned in <code>fval[k*npt + i]</code>.  +  Now, <code>X</code> is not a single point, but an array of <code>NPTS</code> points (length <code>NPTS</code>×<code>NDIM</code>), and upon return the values of all <code>FDIM</code> integrands at all <code>NPTS</code> points should be stored in <code>FVAL</code> (length <code>NPTS</code>×<code>FDIM</code>). In particular, <code>x[i*ndim + j]</code> is the <code>j</code>th coordinate of the <code>i</code>th point (<code>i</code><<code>npts</code> and <code>j</code><<code>ndim</code>), and the <code>k</code>th function evaluation (<code>k</code><<code>fdim</code>) for the <code>i</code>th point is returned in <code>fval[i*fdim + k]</code>. ('''Note''': the <code>fval</code> indexing is changed compared to the <code>adapt_integrate_v</code> interface in previous versions.) 
  The size of NPTS will vary with the dimensionality of the problem; higherdimensional 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 MonteCarlo 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 <code>F</code> will have half that many points.  +  Again, the return value should be 0 on success or nonzero to terminate the integration immediately (e.g. if an error occurred). 
+  
+  The size of <code>NPTS</code> will vary with the dimensionality of the problem; higherdimensional problems will have (exponentially) larger NPTS, allowing for the possibility of more parallelism. Currently, for <code>hcubature_v</code>, <code>NPTS</code> starts at 15 in 1d, 17 in 2d, and 33 in 3d, but as <code>adapt_integrate_v</code> calls your integrand more and more times the value of NPTS will grow. e.g. if you end up requiring several thousand points in total, <code>NPTS</code> may grow to several hundred. We utilize an algorithm from:  
+  
+  * I. Gladwell, "Vectorization of one dimensional quadrature codes," pp. 230–238 in ''Numerical Integration. Recent Developments, Software and Applications'', G. Fairweather and P. M. Keast, eds., NATO ASI Series C203, Dordrecht (1987).  
+  
+  as described in the article "Parallel globally adaptive algorithms for multidimensional integration" by [http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.42.6638 Bull and Freeman] (1994).  
=== Example ===  === Example ===  
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#include "cubature.h"  #include "cubature.h"  
  void f(unsigned ndim, const double *x, void *fdata, unsigned fdim, double *fval) {  +  int f(unsigned ndim, const double *x, void *fdata, unsigned fdim, double *fval) { 
double sigma = *((double *) fdata); ''// we can pass σ via fdata argument''  double sigma = *((double *) fdata); ''// we can pass σ via fdata argument''  
double sum = 0;  double sum = 0;  
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''// compute the output value: note that fdim should == 1 from below''  ''// compute the output value: note that fdim should == 1 from below''  
fval[0] = exp(sigma * sum);  fval[0] = exp(sigma * sum);  
+  return 0; ''// success''  
}  }  
  then, later in the program where we call <code>adapt_integrate</code>:  +  then, later in the program where we call <code>hcubature</code>: 
{  {  
double xmin[3] = {2,2,2}, xmax[3] = {2,2,2}, sigma = 0.5, val, err;  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, 1e4, &val, &err);  +  hcubature(1, f, &sigma, 3, xmin, xmax, 0, 0, 1e4, ERROR_INDIVIDUAL, &val, &err); 
printf("Computed integral = %0.10g +/ %g\n", val, err);  printf("Computed integral = %0.10g +/ %g\n", val, err);  
}  }  
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Note that the estimated ''relative'' error is 0.00136919/13.69609043 = 9.9969×10<sup>–5</sup>, within our requested tolerance of <math>10^{4}</math>. 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<sup>–6</sup>. 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).  Note that the estimated ''relative'' error is 0.00136919/13.69609043 = 9.9969×10<sup>–5</sup>, within our requested tolerance of <math>10^{4}</math>. 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<sup>–6</sup>. 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 <code>adapt_integrate_v</code>, one would instead do:  +  With the vectorized interface <code>hcubature_v</code>, one would instead use: 
  void f(unsigned ndim, unsigned npts, const double *x, void *fdata, unsigned fdim, double *fval) {  +  int f(unsigned ndim, unsigned npts, const double *x, void *fdata, unsigned fdim, double *fval) { 
double sigma = *((double *) fdata);  double sigma = *((double *) fdata);  
unsigned i, j;  unsigned i, j;  
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fval[j] = exp(sigma * sum);  fval[j] = exp(sigma * sum);  
}  }  
+  return 0; ''// success''  
}  }  
+  
+  ===Infinite intervals===  
+  
+  Integrals over infinite or semiinfinite intervals is possible by a [[w:Integration by substitutionchange of variables]]. This is best illustrated in one dimension.  
+  
+  To compute an integral over a semiinfinite interval, you can perform the change of variables ''x''=a+''t''/(1''t''):  
+  :<math>\int_a^\infty f(x) dx = \int_0^1 f\left(a + \frac{t}{1t}\right) \frac{1}{(1t)^2} dt .</math>  
+  For an infinite interval, you can perform the change of variables ''x''=''t''/(1''t''<sup>2</sup>):  
+  :<math>\int_{\infty}^\infty f(x) dx = \int_{1}^1 f\left(\frac{t}{1t^2}\right) \frac{1 + t^2}{(1t^2)^2} dt .</math>  
+  Note the [[w:Jacobian matrixJacobian]] factors multiplying ''f''(⋅⋅⋅) in both integrals, and also that the limits of the ''t'' integrals are different in the two cases.  
+  
+  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, if ''f''(''x'') goes to zero at least as fast as 1/''x''<sup>2</sup>, then the limit of the integrand (including the Jacobian factor) is finite at the endpoints. If your ''f''(''x'') vanishes more slowly than 1/''x''<sup>2</sup> but still faster than 1/''x'', then the integrand blows up at the endpoints but the integral is still finite (it is an integrable singularity), so the code will work (although it may take many function evaluations to converge). If your ''f''(''x'') vanishes only as 1/''x'', then it is not [[w:Absolute convergenceabsolutely convergent]] and much more care is required even to define what you are trying to compute. (In any case, the hadaptive quadrature/cubature rules currently employed in <code>cubature.c</code> do not evaluate the integrand at the endpoints, so you need not implement special handling for ''t''=1.)  
== Test program ==  == Test program ==  
  To compile a test program, just compile <code>cubature.c</code> while #defining <code>TEST_INTEGRATOR</code>, e.g. (on Unix or GNU/Linux) via:  +  To compile a test programs, just compile <code>hcubature.c</code> and/or <code>pcubature.c</code> along with the test program <code>test.c</code>, e.g. (on Unix or GNU/Linux) via: 
  cc DTEST_INTEGRATOR o cubature_test cubature.c lm  +  cc o htest test.c hcubature.c l 
+  cc o ptest DPCUBATURE test.c pcubature.c lm  
The usage is then:  The usage is then:  
  ./cubature_test <dim> <tol> <integrand> <maxeval>  +  ./htest <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).  +  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). Similarly for <code>ptest</code> (which tests the <code>pcubature</code> function). 
The different test integrands are:  The different test integrands are:  
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For example:  For example:  
  ./cubature_test 3 1e5 4  +  ./htest 3 1e5 4 
integrates the Gaussian function (4) to a desired relative error tolerance of 10<sup>–5</sup> in 3 dimensions. The output is:  integrates the Gaussian function (4) to a desired relative error tolerance of 10<sup>–5</sup> in 3 dimensions. The output is: 
Current revision
Contents 
Cubature
Steven G. Johnson has written a simple C package for adaptive multidimensional integration (cubature) of vectorvalued 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 onedimensional vector: the dimensionalities of and are independent.) The integrand can be evaluated for an array of points at once to enable easy parallelization. The code, which is distributed as free software under the terms of the GNU General Public License (v2 or later), implements two algorithms for adaptive integration.
The first, hadaptive integration (recursively partitioning the integration domain into smaller subdomains, applying the same integration rule to each, until convergence is achieved), is based on the algorithms described in:
 A. C. Genz and A. A. Malik, "An adaptive algorithm for numeric integration over an Ndimensional 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).
This algorithm is best suited for a moderate number of dimensions (say, < 7), and is superseded for highdimensional integrals by other methods (e.g. Monte Carlo variants or sparse grids).
(Note that we do not use any of the original DCUHRE code by Genz, which is not under a free/opensource license.) Our code is based in part on code borrowed from the HIntLib numericintegration library by Rudolf Schürer and from code for GaussKronrod quadrature (for 1d integrals) from the GNU Scientific Library, both of which are free software under the GNU GPL. (Another freesoftware multidimensional integration library, unrelated to our code here but also implementing the Genz–Malik algorithm among other techniques, is Cuba.)
The second, padaptive integration (repeatedly doubling the degree of the quadrature rules until convergence is achieved), is based on a tensor product of Clenshaw–Curtis quadrature rules. This algorithm is often superior to hadaptive integration for smooth integrands in a few (≤3) dimensions, but is a poor choice in higher dimensions or for nonsmooth integrands.
For the most part, the padaptive routines below are dropin replacements for the hadaptive routines, with the same arguments etcetera, so you can experiment to see which one works best for your problem. One difference: the hadaptive routines do *not* evaluate the integrand on the boundaries of the integration volume, whereas the padaptive routines *do* evaluate the integrand at the boundaries. This means that the p adaptive routines require more care in cases where there are singularities at the boundaries.
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 an array of points 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 standalone hcubature.c
or pcubature.c
file (along with a couple of private header files) that you can compile and link into your program for hadaptive and padaptive integration, respectively, and a header file cubature.h
that you #include
.
The test.c
file contains a little test program which is produced if you compile that file with DHCUBATURE
or DPCUBATURE
and link with hcubature.c
or pcubature.c
, respectively, as described below.
B. Narasimhan wrote a GNU R interface, which can be downloaded here: http://cran.rproject.org/web/packages/cubature/index.html.
A Julia interface can be obtained from Cubature.jl. A Python cubature.py interface written by Saullo Castro is also available.
Usage
You should compile hcubature.c
and/or pcubature.c
and link it with your program, and #include
the header file cubature.h
.
The central subroutine you will be calling for hadaptive cubature is:
int hcubature(unsigned fdim, integrand f, void *fdata, unsigned dim, const double *xmin, const double *xmax, size_t maxEval, double reqAbsError, double reqRelError, error_norm norm, double *val, double *err);
or pcubature
(same arguments) for padaptive cubature. (See also the vectorized interface below.)
This integrates a function F(x), returning a vector of FDIM integrands, where x is a DIMdimensional 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). [Note: the actual number of evaluations may somewhat exceed MAXEVAL: MAXEVAL is rounded up to an integer number of subregion evaluations.] 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.)
For vectorvalued integrands (FDIM > 1), NORM specifies the norm that is used to measure the error and determine convergence properties. (The NORM argument is irrelevant for FDIM ≤ 1 and is ignored.) Given vectors v and e of estimated integrals and errors therein, respectively, the NORM argument takes on one of the following enumerated constant values:

ERROR_L1
,ERROR_L2
,ERROR_LINF
: the absolute error is measured as e and the relative error as e/v, where ... is the L_{1}, L_{2}, or L_{∞} norm, respectively. (x in the L_{1} norm is the sum of the absolute values of the components, in the L_{2} norm is the root mean square of the components, and in the L_{∞} norm is the maximum absolute value of the components)

ERROR_INDIVIDUAL
: Convergence is achieved only when each integrand (each component of v and e) individually satisfies the requested error tolerances.

ERROR_PAIRED
: LikeERROR_INDIVIDUAL
, except that the integrands are grouped into consecutive pairs, with the error tolerance applied in an L2 sense to each pair. This option is mainly useful for integrating vectors of complex numbers, where each consecutive pair
of real integrands is the real and imaginary parts of a single complex integrand, and you only care about the error in the complex plane rather than the error in the real and imaginary parts separately.
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 hcubature
and pcubature
is 0 on success and nonzero if there was an error (mainly only outofmemory situations or if the integrand signals an error). For a nonzero return value, the contents of the VAL
and ERR
arrays are undefined.
The integrand function F
should be a function of the form:
int 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
). he return value should be 0 on success or a nonzero value if an error occurred and the integration is to be terminated immediately (hcubature
will then return a nonzero error code).
The FDATA
argument of F
is equal to the FDATA
argument passed to hcubature
—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 reentrant). 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 actually 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 hcubature_v(unsigned fdim, integrand_v f, void *fdata, unsigned dim, const double *xmin, const double *xmax, unsigned maxEval, double reqAbsError, double reqRelError, error_norm norm, double *val, double *err);
(and similarly for pcubature_v
). All of the arguments and the return value are identical to hcubature
, 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:
int 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 NPTS
×FDIM
). 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[i*fdim + k]
. (Note: the fval
indexing is changed compared to the adapt_integrate_v
interface in previous versions.)
Again, the return value should be 0 on success or nonzero to terminate the integration immediately (e.g. if an error occurred).
The size of NPTS
will vary with the dimensionality of the problem; higherdimensional problems will have (exponentially) larger NPTS, allowing for the possibility of more parallelism. Currently, for hcubature_v
, NPTS
starts at 15 in 1d, 17 in 2d, and 33 in 3d, but as adapt_integrate_v
calls your integrand more and more times the value of NPTS will grow. e.g. if you end up requiring several thousand points in total, NPTS
may grow to several hundred. We utilize an algorithm from:
 I. Gladwell, "Vectorization of one dimensional quadrature codes," pp. 230–238 in Numerical Integration. Recent Developments, Software and Applications, G. Fairweather and P. M. Keast, eds., NATO ASI Series C203, Dordrecht (1987).
as described in the article "Parallel globally adaptive algorithms for multidimensional integration" by Bull and Freeman (1994).
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" int f(unsigned ndim, const double *x, void *fdata, unsigned fdim, double *fval) { double sigma = *((double *) fdata); // we can pass σ via fdata argument double 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 below fval[0] = exp(sigma * sum); return 0; // success }
then, later in the program where we call hcubature
:
{ double xmin[3] = {2,2,2}, xmax[3] = {2,2,2}, sigma = 0.5, val, err; hcubature(1, f, &sigma, 3, xmin, xmax, 0, 0, 1e4, ERROR_INDIVIDUAL, &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 hardcoding 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 hcubature_v
, one would instead use:
int 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 points double sum = 0; for (i = 0; i < ndim; ++i) sum += x[j*ndim+i] * x[j*ndim+i]; fval[j] = exp(sigma * sum); } return 0; // success }
Infinite intervals
Integrals over infinite or semiinfinite intervals is possible by a change of variables. This is best illustrated in one dimension.
To compute an integral over a semiinfinite interval, you can perform the change of variables x=a+t/(1t):
For an infinite interval, you can perform the change of variables x=t/(1t^{2}):
Note the Jacobian factors multiplying f(⋅⋅⋅) in both integrals, and also that the limits of the t integrals are different in the two cases.
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, if f(x) goes to zero at least as fast as 1/x^{2}, then the limit of the integrand (including the Jacobian factor) is finite at the endpoints. If your f(x) vanishes more slowly than 1/x^{2} but still faster than 1/x, then the integrand blows up at the endpoints but the integral is still finite (it is an integrable singularity), so the code will work (although it may take many function evaluations to converge). If your f(x) vanishes only as 1/x, then it is not absolutely convergent and much more care is required even to define what you are trying to compute. (In any case, the hadaptive 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 programs, just compile hcubature.c
and/or pcubature.c
along with the test program test.c
, e.g. (on Unix or GNU/Linux) via:
cc o htest test.c hcubature.c l cc o ptest DPCUBATURE test.c pcubature.c lm
The usage is then:
./htest <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). Similarly for ptest
(which tests the pcubature
function).
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 dimth roots of the coordinates (weakly singular at the boundary)
For example:
./htest 3 1e5 4
integrates the Gaussian function (4) to a desired relative error tolerance of 10^{–5} in 3 dimensions. The output is:
3dim integral, tolerance = 1e05 integrand 4: integral = 1, est err = 9.99952e06, true err = 2.54397e08 #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.