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The computational complexity of sparse operations is proportional to nnz, the number of nonzero elements in the matrix. Computational complexity also depends linearly on the row size m and column size n of the matrix, but is independent of the product m*n, the total number of zero and nonzero elements.
The complexity of fairly complicated operations, such as the solution of sparse linear equations, involves factors like ordering and fill-in, which are discussed in the previous section. In general, however, the computer time required for a sparse matrix operation is proportional to the number of arithmetic operations on nonzero quantities.
Sparse matrices propagate through computations according to these rules:
Functions that accept a matrix and return a scalar or constant-size vector always produce output in full storage format. For example, the size function always returns a full vector, whether its input is full or sparse.
Functions that accept scalars or vectors and return matrices, such as zeros, ones, rand, and eye, always return full results. This is necessary to avoid introducing sparsity unexpectedly. The sparse analog of zeros(m,n) is simply sparse(m,n). The sparse analogs of rand and eye are sprand and speye, respectively. There is no sparse analog for the function ones.
Unary functions that accept a matrix and return a matrix or vector preserve the storage class of the operand. If S is a sparse matrix, then chol(S) is also a sparse matrix, and diag(S) is a sparse vector. Columnwise functions such as max and sum also return sparse vectors, even though these vectors can be entirely nonzero. Important exceptions to this rule are the sparse and full functions.
Binary operators yield sparse results if both operands are sparse, and full results if both are full. For mixed operands, the result is full unless the operation preserves sparsity. If S is sparse and F is full, then S+F, S*F, and F\S are full, while S.*F and S&F are sparse. In some cases, the result might be sparse even though the matrix has few zero elements.
Matrix concatenation using either the cat function or square brackets produces sparse results for mixed operands.
Submatrix indexing on the right side of an assignment preserves the storage format of the operand unless the result is a scalar. T = S(i,j) produces a sparse result if S is sparse and either i or j is a vector. It produces a full scalar if both i and j are scalars. Submatrix indexing on the left, as in T(i,j) = S, does not change the storage format of the matrix on the left.
A permutation of the rows and columns of a sparse matrix S can be represented in two ways:
A permutation matrix P acts on the rows of S as P*S or on the columns as S*P'.
A permutation vector p, which is a full vector containing a permutation of 1:n, acts on the rows of S as S(p,:), or on the columns as S(:,p).
For example, the statements
p = [1 3 4 2 5] I = eye(5,5); P = I(p,:); e = ones(4,1); S = diag(11:11:55) + diag(e,1) + diag(e,-1)
p = 1 3 4 2 5 P = 1 0 0 0 0 0 0 1 0 0 0 0 0 1 0 0 1 0 0 0 0 0 0 0 1 S = 11 1 0 0 0 1 22 1 0 0 0 1 33 1 0 0 0 1 44 1 0 0 0 1 55
You can now try some permutations using the permutation vector p and the permutation matrix P. For example, the statements S(p,:) and P*S produce
ans = 11 1 0 0 0 0 1 33 1 0 0 0 1 44 1 1 22 1 0 0 0 0 0 1 55
Similarly, S(:,p) and S*P' produce
ans = 11 0 0 1 0 1 1 0 22 0 0 33 1 1 0 0 1 44 0 1 0 0 1 0 55
If P is a sparse matrix, then both representations use storage proportional to n and you can apply either to S in time proportional to nnz(S). The vector representation is slightly more compact and efficient, so the various sparse matrix permutation routines all return full row vectors with the exception of the pivoting permutation in LU (triangular) factorization, which returns a matrix compatible with the full LU factorization.
To convert between the two representations, let I = speye(n) be an identity matrix of the appropriate size. Then,
P = I(p,:) P' = I(:,p) p = (1:n)*P' p = (P*(1:n)')'
The inverse of P is simply R = P'. You can compute the inverse of p with r(p) = 1:n.
r(p) = 1:5 r = 1 4 2 3 5
Reordering the columns of a matrix can often make its LU or QR factors sparser. Reordering the rows and columns can often make its Cholesky factors sparser. The simplest such reordering is to sort the columns by nonzero count. This is sometimes a good reordering for matrices with very irregular structures, especially if there is great variation in the nonzero counts of rows or columns.
The function p = colperm(S) computes this column-count permutation. The colperm code has only a single line.
[ignore,p] = sort(sum(spones(S)));
This line performs these steps:
The reverse Cuthill-McKee ordering is intended to reduce the profile or bandwidth of the matrix. It is not guaranteed to find the smallest possible bandwidth, but it usually does. The function symrcm(A) actually operates on the nonzero structure of the symmetric matrix A + A', but the result is also useful for asymmetric matrices. This ordering is useful for matrices that come from one-dimensional problems or problems that are in some sense "long and thin."
The degree of a node in a graph is the number of connections to that node. This is the same as the number of off-diagonal nonzero elements in the corresponding row of the adjacency matrix. The approximate minimum degree algorithm generates an ordering based on how these degrees are altered during Gaussian elimination or Cholesky factorization. It is a complicated and powerful algorithm that usually leads to sparser factors than most other orderings, including column count and reverse Cuthill-McKee. Because the keeping track of the degree of each node is very time-consuming, the approximate minimum degree algorithm uses an approximation to the degree, rather than the exact degree.
The following MATLAB® functions implement the approximate minimum degree algorithm:
symamd — Use with symmetric matrices.
colamd — Use with nonsymmetric matrices and symmetric matrices of the form A*A' or A'*A.
See Reordering and Factorization for an example using symamd.
You can change various parameters associated with details of the algorithms using the spparms function.
If S is a sparse matrix, the following command returns three sparse matrices L, U, and P such that P*S = L*U.
[L,U,P] = lu(S)
lu obtains the factors by Gaussian elimination with partial pivoting. The permutation matrix P has only n nonzero elements. As with dense matrices, the statement [L,U] = lu(S) returns a permuted unit lower triangular matrix and an upper triangular matrix whose product is S. By itself, lu(S) returns L and U in a single matrix without the pivot information.
The three-output syntax
[L,U,P] = lu(S)
selects P via numerical partial pivoting, but does not pivot to improve sparsity in the LU factors. On the other hand, the four-output syntax
selects P via threshold partial pivoting, and selects P and Q to improve sparsity in the LU factors.
You can control pivoting in sparse matrices using
where thresh is a pivot threshold in [0,1]. Pivoting occurs when the diagonal entry in a column has magnitude less than thresh times the magnitude of any sub-diagonal entry in that column. thresh = 0 forces diagonal pivoting. thresh = 1 is the default. (The default for thresh is 0.1 for the four-output syntax).
When you call lu with three or less outputs, MATLAB automatically allocates the memory necessary to hold the sparse L and U factors during the factorization. Except for the four-output syntax, MATLAB does not use any symbolic LU prefactorization to determine the memory requirements and set up the data structures in advance.
If you obtain a good column permutation p that reduces fill-in, perhaps from symrcm or colamd, then computing lu(S(:,p)) takes less time and storage than computing lu(S).
Create a sparse matrix using the Bucky ball example.
B = bucky;
B has exactly three nonzero elements in each row and column.
Create two permutations, r and m using symrcm and symamd respectively.
r = symrcm(B); m = symamd(B);
The two permutations are the symmetric reverse Cuthill-McKee ordering and the symmetric approximate minimum degree ordering.
Create spy plots to show the three adjacency matrices of the Bucky Ball graph with these three different numberings. The local, pentagon-based structure of the original numbering is not evident in the others.
figure subplot(1,3,1) spy(B) title('Original') subplot(1,3,2) spy(B(r,r)) title('Reverse Cuthill-McKee') subplot(1,3,3) spy(B(m,m)) title('Approx Min Degree')
The reverse Cuthill-McKee ordering, r, reduces the bandwidth and concentrates all the nonzero elements near the diagonal. The approximate minimum degree ordering, m, produces a fractal-like structure with large blocks of zeros.
To see the fill-in generated in the LU factorization of the Bucky ball, use speye, the sparse identity matrix, to insert -3s on the diagonal of B.
B = B - 3*speye(size(B));
Since each row sum is now zero, this new B is actually singular, but it is still instructive to compute its LU factorization. When called with only one output argument, lu returns the two triangular factors, L and U, in a single sparse matrix. The number of nonzeros in that matrix is a measure of the time and storage required to solve linear systems involving B.
Here are the nonzero counts for the three permutations being considered.
lu(B) (Original): 1022
lu(B(r,r)) (Reverse Cuthill-McKee): 968
lu(B(m,m)) (Approximate minimum degree): 636
Even though this is a small example, the results are typical. The original numbering scheme leads to the most fill-in. The fill-in for the reverse Cuthill-McKee ordering is concentrated within the band, but it is almost as extensive as the first two orderings. For the approximate minimum degree ordering, the relatively large blocks of zeros are preserved during the elimination and the amount of fill-in is significantly less than that generated by the other orderings.
The spy plots below reflect the characteristics of each reordering.
figure subplot(1,3,1) spy(lu(B)) title('Original') subplot(1,3,2) spy(lu(B(r,r))) title('Reverse Cuthill-McKee') subplot(1,3,3) spy(lu(B(m,m))) title('Approx Min Degree')
If S is a symmetric (or Hermitian), positive definite, sparse matrix, the statement below returns a sparse, upper triangular matrix R so that R'*R = S.
R = chol(S)
chol does not automatically pivot for sparsity, but you can compute approximate minimum degree and profile limiting permutations for use with chol(S(p,p)).
Since the Cholesky algorithm does not use pivoting for sparsity and does not require pivoting for numerical stability, chol does a quick calculation of the amount of memory required and allocates all the memory at the start of the factorization. You can use symbfact, which uses the same algorithm as chol, to calculate how much memory is allocated.
MATLAB computes the complete QR factorization of a sparse matrix S with
[Q,R] = qr(S)
[Q,R,E] = qr(S)
but this is often impractical. The unitary matrix Q often fails to have a high proportion of zero elements. A more practical alternative, sometimes known as "the Q-less QR factorization," is available.
With one sparse input argument and one output argument
R = qr(S)
returns just the upper triangular portion of the QR factorization. The matrix R provides a Cholesky factorization for the matrix associated with the normal equations:
R'*R = S'*S
However, the loss of numerical information inherent in the computation of S'*S is avoided.
With two input arguments having the same number of rows, and two output arguments, the statement
[C,R] = qr(S,B)
applies the orthogonal transformations to B, producing C = Q'*B without computing Q.
The Q-less QR factorization allows the solution of sparse least squares problems
with two steps
[c,R] = qr(A,b) x = R\c
If A is sparse, but not square, MATLAB uses these steps for the linear equation solving backslash operator:
x = A\b
It is also possible to solve a sequence of least squares linear systems with different right-hand sides, b, that are not necessarily known when R = qr(A) is computed. The approach solves the "semi-normal equations"
R'*R*x = A'*b
x = R\(R'\(A'*b))
and then employs one step of iterative refinement to reduce round off error:
r = b - A*x e = R\(R'\(A'*r)) x = x + e
The ilu and ichol functions provide approximate, incomplete factorizations, which are useful as preconditioners for sparse iterative methods.
The ilu function produces three incomplete lower-upper (ILU) factorizations: the zero-fill ILU (ILU(0)), a Crout version of ILU (ILUC(tau)), and ILU with threshold dropping and pivoting (ILUTP(tau)). The ILU(0) never pivots and the resulting factors only have nonzeros in positions where the input matrix had nonzeros. Both ILUC(tau) and ILUTP(tau), however, do threshold-based dropping with the user-defined drop tolerance tau.
A = gallery('neumann', 1600) + speye(1600); nnz(A) ans = 7840 nnz(lu(A)) ans = 126478
shows that A has 7840 nonzeros, and its complete LU factorization has 126478 nonzeros. On the other hand, the following code shows the different ILU outputs:
[L,U] = ilu(A); nnz(L)+nnz(U)-size(A,1); ans = 7840 norm(A-(L*U).*spones(A),'fro')./norm(A,'fro') ans = 4.8874e-017 opts.type = 'ilutp'; opts.droptol = 1e-4; [L,U,P] = ilu(A, opts); nnz(L)+nnz(U)-size(A,1) ans = 31147 norm(P*A - L*U,'fro')./norm(A,'fro') ans = 9.9224e-005 opts.type = ‘crout'; nnz(L)+nnz(U)-size(A,1) ans = 31083 norm(P*A-L*U,'fro')./norm(A,'fro') ans = 9.7344e-005
These calculations show that the zero-fill factors have 7840 nonzeros, the ILUTP(1e-4) factors have 31147 nonzeros, and the ILUC(1e-4) factors have 31083 nonzeros. Also, the relative error of the product of the zero-fill factors is essentially zero on the pattern of A. Finally, the relative error in the factorizations produced with threshold dropping is on the same order of the drop tolerance, although this is not guaranteed to occur. See the ilu reference page for more options and details.
The ichol function provides zero-fill incomplete Cholesky factorizations (IC(0)) as well as threshold-based dropping incomplete Cholesky factorizations (ICT(tau)) of symmetric, positive definite sparse matrices. These factorizations are the analogs of the incomplete LU factorizations above and have many of the same characteristics. For example:
A = delsq(numgrid('S',200)); nnz(A) ans = 195228 nnz(chol(A,'lower')) ans = 7762589
shows that A has 195228 nonzeros, and its complete Cholesky factorization without reordering has 7762589 nonzeros. By contrast:
L = ichol(A); nnz(L) ans = 117216 norm(A-(L*L').*spones(A),'fro')./norm(A,'fro') ans = 3.5805e-017 opts.type = 'ict'; opts.droptol = 1e-4; L = ichol(A,opts); nnz(L) ans = 1166754 norm(A-L*L','fro')./norm(A,'fro') ans = 2.3997e-004
IC(0) has nonzeros only in the pattern of the lower triangle of A, and on the pattern of A, the product of the factors matches. Also, the ICT(1e-4) factors are considerably sparser than the complete Cholesky factor, and the relative error between A and L*L' is on the same order of the drop tolerance. It is important to note that unlike the factors provided by chol, the default factors provided by ichol are lower triangular. See the ichol reference page for more information.
There are two different classes of methods for solving systems of simultaneous linear equations:
Direct methods are usually variants of Gaussian elimination. These methods involve the individual matrix elements directly, through matrix operations such as LU or Cholesky factorization. MATLAB implements direct methods through the matrix division operators / and \, which you can use to solve linear systems.
Iterative methods produce only an approximate solution after a finite number of steps. These methods involve the coefficient matrix only indirectly, through a matrix-vector product or an abstract linear operator. Iterative methods are usually applied only to sparse matrices.
Direct methods are usually faster and more generally applicable than indirect methods, if there is enough storage available to carry them out. Iterative methods are usually applicable to restricted cases of equations and depend on properties like diagonal dominance or the existence of an underlying differential operator. Direct methods are implemented in the core of the MATLAB software and are made as efficient as possible for general classes of matrices. Iterative methods are usually implemented in MATLAB-language files and can use the direct solution of subproblems or preconditioners.
Using a Different Preordering. If A is not diagonal, banded, triangular, or a permutation of a triangular matrix, backslash (\) reorders the indices of A to reduce the amount of fill-in—that is, the number of nonzero entries that are added to the sparse factorization matrices. The new ordering, called a preordering, is performed before the factorization of A. In some cases, you might be able to provide a better preordering than the one used by the backslash algorithm.
To use a different preordering, first turn off both of the automatic preorderings that backslash might perform by default, using the function spparms as follows:
defaultParms = spparms('autoamd',0); spparms('autommd',0);
Now, assuming you have created a permutation vector p that specifies a preordering of the indices of A, apply backslash to the matrix A(:,p), whose columns are the columns of A, permuted according to the vector p.
x = A (:,p) \ b; x(p) = x; spparms(defaultParms);
The command spparms(defaultParms) restores the controls to their prior state, in case you use A\b later without specifying an appropriate preordering.
Eleven functions are available that implement iterative methods for sparse systems of simultaneous linear systems.
Functions for Iterative Methods for Sparse Systems
Biconjugate gradient stabilized
|bicgstabl||Biconjugate gradient stabilized (l)|
Conjugate gradient squared
Generalized minimum residual
Preconditioned conjugate gradient
|tfqmr||Transpose-free quasiminimal residual|
These methods are designed to solve Ax = b or minimize the norm of b – Ax. For the Preconditioned Conjugate Gradient method, pcg, A must be a symmetric, positive definite matrix. minres and symmlq can be used on symmetric indefinite matrices. For lsqr, the matrix need not be square. The other seven can handle nonsymmetric, square matrices and each method has a distinct benefit.
All eleven methods can make use of preconditioners. The linear system
is replaced by the equivalent system
The preconditioner M is chosen to accelerate convergence of the iterative method. In many cases, the preconditioners occur naturally in the mathematical model. A partial differential equation with variable coefficients can be approximated by one with constant coefficients, for example. Incomplete matrix factorizations can be used in the absence of natural preconditioners.
The five-point finite difference approximation to Laplace's equation on a square, two-dimensional domain provides an example. The following statements use the preconditioned conjugate gradient method preconditioner M = L*L', where L is the zero-fill incomplete Cholesky factor of A.
A = delsq(numgrid('S',50)); b = ones(size(A,1),1); tol = 1e-3; maxit = 100; L = ichol(A); [x,flag,err,iter,res] = pcg(A,b,tol,maxit,L,L');
Twenty-one iterations are required to achieve the prescribed accuracy. On the other hand, using a different preconditioner may yield better results. For example, using ichol to construct a modified incomplete Cholesky, the prescribed accuracy is met after only 15 iterations:
L = ichol(A,struct('type','nofill','michol','on')); [x,flag,err,iter,res] = pcg(A,b,tol,maxit,L,L');
Two functions are available that compute a few specified eigenvalues or singular values. svds is based on eigs.
Functions to Compute a Few Eigenvalues or Singular Values
Few singular values
These functions are most frequently used with sparse matrices, but they can be used with full matrices or even with linear operators defined in MATLAB code.
[V,lambda] = eigs(A,k,sigma)
finds the k eigenvalues and corresponding eigenvectors of the matrix A that are nearest the "shift" sigma. If sigma is omitted, the eigenvalues largest in magnitude are found. If sigma is zero, the eigenvalues smallest in magnitude are found. A second matrix, B, can be included for the generalized eigenvalue problem: Aυ = λBυ.
[U,S,V] = svds(A,k)
finds the k largest singular values of A and
[U,S,V] = svds(A,k,0)
finds the k smallest singular values.
This example shows how to find the smallest eigenvalue and eigenvector of a sparse matrix.
Set up the five-point Laplacian difference operator on a 65-by-65 grid in an L-shaped, two-dimensional domain.
L = numgrid('L',65); A = delsq(L);
Determine the order and number of nonzero elements.
ans = 2945 2945 ans = 14473
A is a matrix of order 2945 with 14,473 nonzero elements.
Compute the smallest eigenvalue and eigenvector.
[v,d] = eigs(A,1,0);
Distribute the components of the eigenvector over the appropriate grid points and produce a contour plot of the result.
L(L>0) = full(v(L(L>0))); x = -1:1/32:1; contour(x,x,L,15) axis square
The numerical techniques used in eigs and svds are described in .
This section describes some limitations of the sparse matrix storage format and their impact on matrix creation, manipulation, and operations.
The best way to create a sparse matrix is to use the sparse function. If you do not have prior knowledge of the nonzero indices or their values, it is much more efficient to create the vectors containing these values, and then create the sparse matrix.
Preallocating the memory for a sparse matrix and filling it in an elementwise manner causes a significant amount of overhead in indexing into the sparse array:
S1 = spalloc(1000,1000,100000); tic; for n = 1:100000 i = ceil(1000*rand(1,1)); j = ceil(1000*rand(1,1)); S1(i,j) = rand(1,1); end toc Elapsed time is 26.281000 seconds.
Whereas constructing the vectors of indices and values eliminates the need to index into the sparse array, and thus is significantly faster:
i = ceil(1000*rand(100000,1)); j = ceil(1000*rand(100000,1)); v = zeros(size(i)); for n = 1:100000 v(n) = rand(1,1); end tic; S2 = sparse(i,j,v,1000,1000); toc Elapsed time is 0.078000 seconds.
Sparse matrices are stored in a column-major format. In some cases, accessing the matrix by columns may be more efficient than accessing by rows. To do this, you can transpose the matrix, perform operations on the columns, and then retranspose the result:
S = sparse(10000,10000,1); for n = 1:1000 A = S(100,:)' + S(200,:)'; A = A'; end;
The time required to transpose the matrix is negligible. Note that the sparse matrix memory requirements could prevent you from transposing a sparse matrix having a large number of rows. This might occur even when the number of nonzero values is small.
Using linear indexing to access or assign an element in a large sparse matrix will fail if the linear index exceeds intmax. To access an element whose linear index is greater than intmax, use array indexing:
S = spalloc(216^2, 216^2, 2) S(1) = 1 S(end) = 1 S(216^2,216^2) = 1