Eigen
3.4.90 (git rev 67eeba6e720c5745abc77ae6c92ce0a44aa7b7ae)

Manipulating and solving sparse problems involves various modules which are summarized below:
Module  Header file  Contents 

SparseCore  #include <Eigen/SparseCore>
 SparseMatrix and SparseVector classes, matrix assembly, basic sparse linear algebra (including sparse triangular solvers) 
SparseCholesky  #include <Eigen/SparseCholesky>
 Direct sparse LLT and LDLT Cholesky factorization to solve sparse selfadjoint positive definite problems 
SparseLU  #include<Eigen/SparseLU>
 Sparse LU factorization to solve general square sparse systems 
SparseQR  #include<Eigen/SparseQR>
 Sparse QR factorization for solving sparse linear leastsquares problems 
IterativeLinearSolvers  #include <Eigen/IterativeLinearSolvers>
 Iterative solvers to solve large general linear square problems (including selfadjoint positive definite problems) 
Sparse  #include <Eigen/Sparse>
 Includes all the above modules 
In many applications (e.g., finite element methods) it is common to deal with very large matrices where only a few coefficients are different from zero. In such cases, memory consumption can be reduced and performance increased by using a specialized representation storing only the nonzero coefficients. Such a matrix is called a sparse matrix.
The SparseMatrix class
The class SparseMatrix is the main sparse matrix representation of Eigen's sparse module; it offers high performance and low memory usage. It implements a more versatile variant of the widelyused Compressed Column (or Row) Storage scheme. It consists of four compact arrays:
Values:
stores the coefficient values of the nonzeros.InnerIndices:
stores the row (resp. column) indices of the nonzeros.OuterStarts:
stores for each column (resp. row) the index of the first nonzero in the previous two arrays.InnerNNZs:
stores the number of nonzeros of each column (resp. row). The word inner
refers to an inner vector that is a column for a columnmajor matrix, or a row for a rowmajor matrix. The word outer
refers to the other direction.This storage scheme is better explained on an example. The following matrix
0  3  0  0  0 
22  0  0  0  17 
7  5  0  1  0 
0  0  0  0  0 
0  0  14  0  8 
and one of its possible sparse, column major representation:
Values:  22  7  _  3  5  14  _  _  1  _  17  8 
InnerIndices:  1  2  _  0  2  4  _  _  2  _  1  4 
OuterStarts:  0  3  5  8  10  12 
InnerNNZs:  2  2  1  1  2 
Currently the elements of a given inner vector are guaranteed to be always sorted by increasing inner indices. The "_"
indicates available free space to quickly insert new elements. Assuming no reallocation is needed, the insertion of a random element is therefore in O(nnz_j)
where nnz_j
is the number of nonzeros of the respective inner vector. On the other hand, inserting elements with increasing inner indices in a given inner vector is much more efficient since this only requires to increase the respective InnerNNZs
entry that is a O(1)
operation.
The case where no empty space is available is a special case, and is referred as the compressed mode. It corresponds to the widely used Compressed Column (or Row) Storage schemes (CCS or CRS). Any SparseMatrix can be turned to this form by calling the SparseMatrix::makeCompressed() function. In this case, one can remark that the InnerNNZs
array is redundant with OuterStarts
because we have the equality: InnerNNZs[j] == OuterStarts[j+1]  OuterStarts[j]
. Therefore, in practice a call to SparseMatrix::makeCompressed() frees this buffer.
It is worth noting that most of our wrappers to external libraries requires compressed matrices as inputs.
The results of Eigen's operations always produces compressed sparse matrices. On the other hand, the insertion of a new element into a SparseMatrix converts this later to the uncompressed mode.
Here is the previous matrix represented in compressed mode:
Values:  22  7  3  5  14  1  17  8 
InnerIndices:  1  2  0  2  4  2  1  4 
OuterStarts:  0  2  4  5  6  8 
A SparseVector is a special case of a SparseMatrix where only the Values
and InnerIndices
arrays are stored. There is no notion of compressed/uncompressed mode for a SparseVector.
Before describing each individual class, let's start with the following typical example: solving the Laplace equation \( \Delta u = 0 \) on a regular 2D grid using a finite difference scheme and Dirichlet boundary conditions. Such problem can be mathematically expressed as a linear problem of the form \( Ax=b \) where \( x \) is the vector of m
unknowns (in our case, the values of the pixels), \( b \) is the right hand side vector resulting from the boundary conditions, and \( A \) is an \( m \times m \) matrix containing only a few nonzero elements resulting from the discretization of the Laplacian operator.
#include <Eigen/Sparse>
#include <vector>
#include <iostream>
typedef Eigen::Triplet<double> T;
int main(int argc, char** argv)
{
if(argc!=2) {
std::cerr << "Error: expected one and only one argument.\n";
return 1;
}
int n = 300; // size of the image
int m = n*n; // number of unknowns (=number of pixels)
// Assembly:
std::vector<T> coefficients; // list of nonzeros coefficients
Eigen::VectorXd b(m); // the right hand sidevector resulting from the constraints
buildProblem(coefficients, b, n);
SpMat A(m,m);
A.setFromTriplets(coefficients.begin(), coefficients.end());
// Solving:
Eigen::SimplicialCholesky<SpMat> chol(A); // performs a Cholesky factorization of A
Eigen::VectorXd x = chol.solve(b); // use the factorization to solve for the given right hand side
// Export the result to a file:
saveAsBitmap(x, n, argv[1]);
return 0;
}
Definition: SimplicialCholesky.h:514 A small structure to hold a non zero as a triplet (i,j,value). Definition: SparseUtil.h:163 
In this example, we start by defining a columnmajor sparse matrix type of double SparseMatrix<double>
, and a triplet list of the same scalar type Triplet<double>
. A triplet is a simple object representing a nonzero entry as the triplet: row
index, column
index, value
.
In the main function, we declare a list coefficients
of triplets (as a std vector) and the right hand side vector \( b \) which are filled by the buildProblem function. The raw and flat list of nonzero entries is then converted to a true SparseMatrix object A
. Note that the elements of the list do not have to be sorted, and possible duplicate entries will be summed up.
The last step consists of effectively solving the assembled problem. Since the resulting matrix A
is symmetric by construction, we can perform a direct Cholesky factorization via the SimplicialLDLT class which behaves like its LDLT counterpart for dense objects.
The resulting vector x
contains the pixel values as a 1D array which is saved to a jpeg file shown on the right of the code above.
Describing the buildProblem and save functions is out of the scope of this tutorial. They are given here for the curious and reproducibility purpose.
Matrix and vector properties
The SparseMatrix and SparseVector classes take three template arguments: the scalar type (e.g., double) the storage order (ColMajor or RowMajor, the default is ColMajor) the inner index type (default is int
).
As for dense Matrix objects, constructors takes the size of the object. Here are some examples:
In the rest of the tutorial, mat
and vec
represent any sparsematrix and sparsevector objects, respectively.
The dimensions of a matrix can be queried using the following functions:
Standard dimensions  mat.rows()
mat.cols()
 vec.size()

Sizes along the inner/outer dimensions  mat.innerSize()
mat.outerSize()
 
Number of non zero coefficients  mat.nonZeros()
 vec.nonZeros()

Iterating over the nonzero coefficients
Random access to the elements of a sparse object can be done through the coeffRef(i,j)
function. However, this function involves a quite expensive binary search. In most cases, one only wants to iterate over the nonzeros elements. This is achieved by a standard loop over the outer dimension, and then by iterating over the nonzeros of the current inner vector via an InnerIterator. Thus, the nonzero entries have to be visited in the same order than the storage order. Here is an example:
SparseMatrix<double> mat(rows,cols);
for (int k=0; k<mat.outerSize(); ++k)
for (SparseMatrix<double>::InnerIterator it(mat,k); it; ++it)
{
it.value();
it.row(); // row index
it.col(); // col index (here it is equal to k)
it.index(); // inner index, here it is equal to it.row()
}
 SparseVector<double> vec(size);
for (SparseVector<double>::InnerIterator it(vec); it; ++it)
{
it.value(); // == vec[ it.index() ]
it.index();
}

For a writable expression, the referenced value can be modified using the valueRef() function. If the type of the sparse matrix or vector depends on a template parameter, then the typename
keyword is required to indicate that InnerIterator
denotes a type; see The template and typename keywords in C++ for details.
Because of the special storage scheme of a SparseMatrix, special care has to be taken when adding new nonzero entries. For instance, the cost of a single purely random insertion into a SparseMatrix is O(nnz)
, where nnz
is the current number of nonzero coefficients.
The simplest way to create a sparse matrix while guaranteeing good performance is thus to first build a list of socalled triplets, and then convert it to a SparseMatrix.
Here is a typical usage example:
The std::vector
of triplets might contain the elements in arbitrary order, and might even contain duplicated elements that will be summed up by setFromTriplets(). See the SparseMatrix::setFromTriplets() function and class Triplet for more details.
In some cases, however, slightly higher performance, and lower memory consumption can be reached by directly inserting the nonzeros into the destination matrix. A typical scenario of this approach is illustrated below:
operator[](int j)
returning the reserve size of the jth
inner vector (e.g., via a VectorXi
or std::vector<int>
). If only a rought estimate of the number of nonzeros per innervector can be obtained, it is highly recommended to overestimate it rather than the opposite. If this line is omitted, then the first insertion of a new element will reserve room for 2 elements per inner vector.jth
column is not full and contains nonzeros whose innerindices are smaller than i
. In this case, this operation boils down to trivial O(1) operation.insert(i,j)
the element i
, j
must not already exists, otherwise use the coeffRef(i,j)
method that will allow to, e.g., accumulate values. This method first performs a binary search and finally calls insert(i,j)
if the element does not already exist. It is more flexible than insert()
but also more costly.Because of their special storage format, sparse matrices cannot offer the same level of flexibility than dense matrices. In Eigen's sparse module we chose to expose only the subset of the dense matrix API which can be efficiently implemented. In the following sm denotes a sparse matrix, sv a sparse vector, dm a dense matrix, and dv a dense vector.
Sparse expressions support most of the unary and binary coefficient wise operations:
However, a strong restriction is that the storage orders must match. For instance, in the following example:
sm1, sm2, and sm3 must all be rowmajor or all columnmajor. On the other hand, there is no restriction on the target matrix sm4. For instance, this means that for computing \( A^T + A \), the matrix \( A^T \) must be evaluated into a temporary matrix of compatible storage order:
Binary coefficient wise operators can also mix sparse and dense expressions:
Performancewise, the adding/subtracting sparse and dense matrices is better performed in two steps. For instance, instead of doing dm2 = sm1 + dm1
, better write:
This version has the advantage to fully exploit the higher performance of dense storage (no indirection, SIMD, etc.), and to pay the cost of slow sparse evaluation on the few nonzeros of the sparse matrix only.
Sparse expressions also support transposition:
However, there is no transposeInPlace()
method.
Eigen supports various kind of sparse matrix products which are summarize below:
selfadjointView()
: prune()
functions: Regarding readaccess, sparse matrices expose the same API than for dense matrices to access to submatrices such as blocks, columns, and rows. See Block operations for a detailed introduction. However, for performance reasons, writing to a subsparsematrix is much more limited, and currently only contiguous sets of columns (resp. rows) of a columnmajor (resp. rowmajor) SparseMatrix are writable. Moreover, this information has to be known at compiletime, leaving out methods such as block(...)
and corner*(...)
. The available API for writeaccess to a SparseMatrix are summarized below:
In addition, sparse matrices expose the SparseMatrixBase::innerVector()
and SparseMatrixBase::innerVectors()
methods, which are aliases to the col
/middleCols
methods for a columnmajor storage, and to the row
/middleRows
methods for a rowmajor storage.
Just as with dense matrices, the triangularView()
function can be used to address a triangular part of the matrix, and perform triangular solves with a dense right hand side:
The selfadjointView()
function permits various operations:
Please, refer to the Quick Reference guide for the list of supported operations. The list of linear solvers available is here.