octave: Basic Matrix Functions

 
 18.2 Basic Matrix Functions
 ===========================
 
  -- : AA = balance (A)
  -- : AA = balance (A, OPT)
  -- : [DD, AA] = balance (A, OPT)
  -- : [D, P, AA] = balance (A, OPT)
  -- : [CC, DD, AA, BB] = balance (A, B, OPT)
 
      Balance the matrix A to reduce numerical errors in future
      calculations.
 
      Compute ‘AA = DD \ A * DD’ in which AA is a matrix whose row and
      column norms are roughly equal in magnitude, and ‘DD = P * D’, in
      which P is a permutation matrix and D is a diagonal matrix of
      powers of two.  This allows the equilibration to be computed
      without round-off.  Results of eigenvalue calculation are typically
      improved by balancing first.
 
      If two output values are requested, ‘balance’ returns the diagonal
      D and the permutation P separately as vectors.  In this case, ‘DD =
      eye(n)(:,P) * diag (D)’, where n is the matrix size.
 
      If four output values are requested, compute ‘AA = CC*A*DD’ and ‘BB
      = CC*B*DD’, in which AA and BB have nonzero elements of
      approximately the same magnitude and CC and DD are permuted
      diagonal matrices as in DD for the algebraic eigenvalue problem.
 
      The eigenvalue balancing option OPT may be one of:
 
      "noperm", "S"
           Scale only; do not permute.
 
      "noscal", "P"
           Permute only; do not scale.
 
      Algebraic eigenvalue balancing uses standard LAPACK routines.
 
      Generalized eigenvalue problem balancing uses Ward’s algorithm
      (SIAM Journal on Scientific and Statistical Computing, 1981).
 
  -- : BW = bandwidth (A, TYPE)
  -- : [LOWER, UPPER] = bandwidth (A)
      Compute the bandwidth of A.
 
      The TYPE argument is the string "lower" for the lower bandwidth and
      "upper" for the upper bandwidth.  If no TYPE is specified return
      both the lower and upper bandwidth of A.
 
      The lower/upper bandwidth of a matrix is the number of
      subdiagonals/superdiagonals with nonzero entries.
 
      See also: Seeisbanded XREFisbanded, Seeisdiag XREFisdiag,
      Seeistril XREFistril, Seeistriu XREFistriu.
 
  -- : cond (A)
  -- : cond (A, P)
      Compute the P-norm condition number of a matrix with respect to
      inversion.
 
      ‘cond (A)’ is defined as ‘norm (A, P) * norm (inv (A), P)’.
 
      By default, ‘P = 2’ is used which implies a (relatively slow)
      singular value decomposition.  Other possible selections are ‘P =
      1, Inf, "fro"’ which are generally faster.  See ‘norm’ for a full
      discussion of possible P values.
 
      The condition number of a matrix quantifies the sensitivity of the
      matrix inversion operation when small changes are made to matrix
      elements.  Ideally the condition number will be close to 1.  When
      the number is large this indicates small changes (such as underflow
      or round-off error) will produce large changes in the resulting
      output.  In such cases the solution results from numerical
      computing are not likely to be accurate.
 
DONTPRINTYET       See also: Seecondest XREFcondest, Seercond XREFrcond, *noteDONTPRINTYET       See also: Seecondest XREFcondest, Seercond XREFrcond, See
      condeig XREFcondeig, Seenorm XREFnorm, Seesvd XREFsvd.
 
  -- : C = condeig (A)
  -- : [V, LAMBDA, C] = condeig (A)
      Compute condition numbers of a matrix with respect to eigenvalues.
 
      The condition numbers are the reciprocals of the cosines of the
      angles between the left and right eigenvectors; Large values
      indicate that the matrix has multiple distinct eigenvalues.
 
      The input A must be a square numeric matrix.
 
      The outputs are:
 
         • C is a vector of condition numbers for the eigenvalues of A.
 
         • V is the matrix of right eigenvectors of A.  The result is
           equivalent to calling ‘[V, LAMBDA] = eig (A)’.
 
         • LAMBDA is the diagonal matrix of eigenvalues of A.  The result
           is equivalent to calling ‘[V, LAMBDA] = eig (A)’.
 
      Example
 
           a = [1, 2; 3, 4];
           c = condeig (a)
           ⇒ [1.0150; 1.0150]
 
DONTPRINTYET       See also: Seeeig XREFeig, Seecond XREFcond, *notebalance:
DONTPRINTYET       See also: Seeeig XREFeig, Seecond XREFcond, Seebalance

      XREFbalance.
 
  -- : det (A)
  -- : [D, RCOND] = det (A)
      Compute the determinant of A.
 
      Return an estimate of the reciprocal condition number if requested.
 
      Programming Notes: Routines from LAPACK are used for full matrices
      and code from UMFPACK is used for sparse matrices.
 
      The determinant should not be used to check a matrix for
      singularity.  For that, use any of the condition number functions:
      ‘cond’, ‘condest’, ‘rcond’.
 
DONTPRINTYET       See also: Seecond XREFcond, Seecondest XREFcondest, *noteDONTPRINTYET       See also: Seecond XREFcond, Seecondest XREFcondest, See
      rcond XREFrcond.
 
  -- : LAMBDA = eig (A)
  -- : LAMBDA = eig (A, B)
  -- : [V, LAMBDA] = eig (A)
  -- : [V, LAMBDA] = eig (A, B)
  -- : [V, LAMBDA, W] = eig (A)
  -- : [V, LAMBDA, W] = eig (A, B)
  -- : [...] = eig (A, BALANCEOPTION)
  -- : [...] = eig (A, B, ALGORITHM)
  -- : [...] = eig (..., EIGVALOPTION)
      Compute the eigenvalues (LAMBDA) and optionally the right
      eigenvectors (V) and the left eigenvectors (W) of a matrix or a
      pair of matrices.
 
      The flag BALANCEOPTION can be one of:
 
      "balance"
           Preliminary balancing is on.  (default)
 
      "nobalance"
           Disables preliminary balancing.
 
      The flag EIGVALOPTION can be one of:
 
      "matrix"
           Return the eigenvalues in a diagonal matrix.  (default if 2 or
           3 outputs are specified)
 
      "vector"
           Return the eigenvalues in a column vector.  (default if 1
           output is specified, e.g.  LAMBDA = eig (A))
 
      The flag ALGORITHM can be one of:
 
      "chol"
           Uses the Cholesky factorization of B. (default if A is
           symmetric (Hermitian) and B is symmetric (Hermitian) positive
           definite)
 
      "qz"
           Uses the QZ algorithm.  (When A or B are not symmetric always
           the QZ algorithm will be used)
 
                             no flag           chol              qz
      -----------------------------------------------------------------------------
      both are symmetric     "chol"            "chol"            "qz"
      at least one is not    "qz"              "qz"              "qz"
      symmetric
 
      The eigenvalues returned by ‘eig’ are not ordered.
 
      See also: Seeeigs XREFeigs, Seesvd XREFsvd.
 
  -- : G = givens (X, Y)
  -- : [C, S] = givens (X, Y)
      Compute the Givens rotation matrix G.
 
      The Givens matrix is a 2 by 2 orthogonal matrix
 
      ‘G = [C S; -S' C]’
 
      such that
 
      ‘G [X; Y] = [*; 0]’
 
      with X and Y scalars.
 
      If two output arguments are requested, return the factors C and S
      rather than the Givens rotation matrix.
 
      For example:
 
           givens (1, 1)
              ⇒   0.70711   0.70711
                  -0.70711   0.70711
 
      See also: Seeplanerot XREFplanerot.
 
  -- : [G, Y] = planerot (X)
      Given a two-element column vector, return the 2 by 2 orthogonal
      matrix G such that ‘Y = G * X’ and ‘Y(2) = 0’.
 
      See also: Seegivens XREFgivens.
 
  -- : X = inv (A)
  -- : [X, RCOND] = inv (A)
      Compute the inverse of the square matrix A.
 
      Return an estimate of the reciprocal condition number if requested,
      otherwise warn of an ill-conditioned matrix if the reciprocal
      condition number is small.
 
      In general it is best to avoid calculating the inverse of a matrix
      directly.  For example, it is both faster and more accurate to
      solve systems of equations (A*x = b) with ‘Y = A \ b’, rather than
      ‘Y = inv (A) * b’.
 
      If called with a sparse matrix, then in general X will be a full
      matrix requiring significantly more storage.  Avoid forming the
      inverse of a sparse matrix if possible.
 
      See also: Seeldivide XREFldivide, Seerdivide XREFrdivide,
      Seepinv XREFpinv.
 
  -- : X = linsolve (A, B)
  -- : X = linsolve (A, B, OPTS)
  -- : [X, R] = linsolve (...)
      Solve the linear system ‘A*x = b’.
 
      With no options, this function is equivalent to the left division
      operator (‘x = A \ b’) or the matrix-left-divide function
      (‘x = mldivide (A, b)’).
 
      Octave ordinarily examines the properties of the matrix A and
      chooses a solver that best matches the matrix.  By passing a
      structure OPTS to ‘linsolve’ you can inform Octave directly about
      the matrix A.  In this case Octave will skip the matrix examination
      and proceed directly to solving the linear system.
 
      *Warning:* If the matrix A does not have the properties listed in
      the OPTS structure then the result will not be accurate AND no
      warning will be given.  When in doubt, let Octave examine the
      matrix and choose the appropriate solver as this step takes little
      time and the result is cached so that it is only done once per
      linear system.
 
      Possible OPTS fields (set value to true/false):
 
      LT
           A is lower triangular
 
      UT
           A is upper triangular
 
      UHESS
           A is upper Hessenberg (currently makes no difference)
 
      SYM
           A is symmetric or complex Hermitian (currently makes no
           difference)
 
      POSDEF
           A is positive definite
 
      RECT
           A is general rectangular (currently makes no difference)
 
      TRANSA
           Solve ‘A'*x = b’ by ‘transpose (A) \ b’
 
      The optional second output R is the inverse condition number of A
      (zero if matrix is singular).
 
DONTPRINTYET       See also: Seemldivide XREFmldivide, *notematrix_type:
DONTPRINTYET       See also: Seemldivide XREFmldivide, Seematrix_type

      XREFmatrix_type, Seercond XREFrcond.
 
  -- : TYPE = matrix_type (A)
  -- : TYPE = matrix_type (A, "nocompute")
  -- : A = matrix_type (A, TYPE)
  -- : A = matrix_type (A, "upper", PERM)
  -- : A = matrix_type (A, "lower", PERM)
  -- : A = matrix_type (A, "banded", NL, NU)
      Identify the matrix type or mark a matrix as a particular type.
 
      This allows more rapid solutions of linear equations involving A to
      be performed.
 
      Called with a single argument, ‘matrix_type’ returns the type of
      the matrix and caches it for future use.
 
      Called with more than one argument, ‘matrix_type’ allows the type
      of the matrix to be defined.
 
      If the option "nocompute" is given, the function will not attempt
      to guess the type if it is still unknown.  This is useful for
      debugging purposes.
 
      The possible matrix types depend on whether the matrix is full or
      sparse, and can be one of the following
 
      "unknown"
           Remove any previously cached matrix type, and mark type as
           unknown.
 
      "full"
           Mark the matrix as full.
 
      "positive definite"
           Probable full positive definite matrix.
 
      "diagonal"
           Diagonal matrix.  (Sparse matrices only)
 
      "permuted diagonal"
           Permuted Diagonal matrix.  The permutation does not need to be
           specifically indicated, as the structure of the matrix
           explicitly gives this.  (Sparse matrices only)
 
      "upper"
           Upper triangular.  If the optional third argument PERM is
           given, the matrix is assumed to be a permuted upper triangular
           with the permutations defined by the vector PERM.
 
      "lower"
           Lower triangular.  If the optional third argument PERM is
           given, the matrix is assumed to be a permuted lower triangular
           with the permutations defined by the vector PERM.
 
      "banded"
      "banded positive definite"
           Banded matrix with the band size of NL below the diagonal and
           NU above it.  If NL and NU are 1, then the matrix is
           tridiagonal and treated with specialized code.  In addition
           the matrix can be marked as probably a positive definite.
           (Sparse matrices only)
 
      "singular"
           The matrix is assumed to be singular and will be treated with
           a minimum norm solution.
 
      Note that the matrix type will be discovered automatically on the
      first attempt to solve a linear equation involving A.  Therefore
      ‘matrix_type’ is only useful to give Octave hints of the matrix
      type.  Incorrectly defining the matrix type will result in
      incorrect results from solutions of linear equations; it is
      entirely *the responsibility of the user* to correctly identify the
      matrix type.
 
      Also, the test for positive definiteness is a low-cost test for a
      Hermitian matrix with a real positive diagonal.  This does not
      guarantee that the matrix is positive definite, but only that it is
      a probable candidate.  When such a matrix is factorized, a
      Cholesky factorization is first attempted, and if that fails the
      matrix is then treated with an LU factorization.  Once the matrix
      has been factorized, ‘matrix_type’ will return the correct
      classification of the matrix.
 
  -- : norm (A)
  -- : norm (A, P)
  -- : norm (A, P, OPT)
      Compute the p-norm of the matrix A.
 
      If the second argument is not given, ‘p = 2’ is used.
 
      If A is a matrix (or sparse matrix):
 
      P = ‘1’
           1-norm, the largest column sum of the absolute values of A.
 
      P = ‘2’
           Largest singular value of A.
 
      P = ‘Inf’ or "inf"
           Infinity norm, the largest row sum of the absolute values of
           A.
 
      P = "fro"
           Frobenius norm of A, ‘sqrt (sum (diag (A' * A)))’.
 
      other P, ‘P > 1’
           maximum ‘norm (A*x, p)’ such that ‘norm (x, p) == 1’
 
      If A is a vector or a scalar:
 
      P = ‘Inf’ or "inf"
           ‘max (abs (A))’.
 
      P = ‘-Inf’
           ‘min (abs (A))’.
 
      P = "fro"
           Frobenius norm of A, ‘sqrt (sumsq (abs (A)))’.
 
      P = 0
           Hamming norm—the number of nonzero elements.
 
      other P, ‘P > 1’
           p-norm of A, ‘(sum (abs (A) .^ P)) ^ (1/P)’.
 
      other P ‘P < 1’
           the p-pseudonorm defined as above.
 
      If OPT is the value "rows", treat each row as a vector and compute
      its norm.  The result is returned as a column vector.  Similarly,
      if OPT is "columns" or "cols" then compute the norms of each column
      and return a row vector.
 
      See also: Seenormest XREFnormest, Seenormest1 XREFnormest1,
      Seecond XREFcond, Seesvd XREFsvd.
 
  -- : null (A)
  -- : null (A, TOL)
      Return an orthonormal basis of the null space of A.
 
      The dimension of the null space is taken as the number of singular
      values of A not greater than TOL.  If the argument TOL is missing,
      it is computed as
 
           max (size (A)) * max (svd (A)) * eps
 
      See also: Seeorth XREForth.
 
  -- : orth (A)
  -- : orth (A, TOL)
      Return an orthonormal basis of the range space of A.
 
      The dimension of the range space is taken as the number of singular
      values of A greater than TOL.  If the argument TOL is missing, it
      is computed as
 
           max (size (A)) * max (svd (A)) * eps
 
      See also: Seenull XREFnull.
 
  -- : [Y, H] = mgorth (X, V)
      Orthogonalize a given column vector X with respect to a set of
      orthonormal vectors comprising the columns of V using the modified
      Gram-Schmidt method.
 
      On exit, Y is a unit vector such that:
 
             norm (Y) = 1
             V' * Y = 0
             X = [V, Y]*H'
 
  -- : pinv (X)
  -- : pinv (X, TOL)
      Return the Moore-Penrose pseudoinverse of X.
 
      Singular values less than TOL are ignored.
 
      If the second argument is omitted, it is taken to be
 
           tol = max ([rows(X), columns(X)]) * norm (X) * eps
 
      See also: Seeinv XREFinv, Seeldivide XREFldivide.
 
  -- : rank (A)
  -- : rank (A, TOL)
      Compute the rank of matrix A, using the singular value
      decomposition.
 
      The rank is taken to be the number of singular values of A that are
      greater than the specified tolerance TOL.  If the second argument
      is omitted, it is taken to be
 
           tol = max (size (A)) * sigma(1) * eps;
 
      where ‘eps’ is machine precision and ‘sigma(1)’ is the largest
      singular value of A.
 
      The rank of a matrix is the number of linearly independent rows or
      columns and determines how many particular solutions exist to a
      system of equations.  Use ‘null’ for finding the remaining
      homogenous solutions.
 
      Example:
 
           x = [1 2 3
                4 5 6
                7 8 9];
           rank (x)
             ⇒ 2
 
      The number of linearly independent rows is only 2 because the final
      row is a linear combination of -1*row1 + 2*row2.
 
DONTPRINTYET       See also: Seenull XREFnull, Seesprank XREFsprank, *noteDONTPRINTYET       See also: Seenull XREFnull, Seesprank XREFsprank, See
      svd XREFsvd.
 
  -- : C = rcond (A)
      Compute the 1-norm estimate of the reciprocal condition number as
      returned by LAPACK.
 
      If the matrix is well-conditioned then C will be near 1 and if the
      matrix is poorly conditioned it will be close to 0.
 
      The matrix A must not be sparse.  If the matrix is sparse then
      ‘condest (A)’ or ‘rcond (full (A))’ should be used instead.
 
      See also: Seecond XREFcond, Seecondest XREFcondest.
 
  -- : trace (A)
      Compute the trace of A, the sum of the elements along the main
      diagonal.
 
      The implementation is straightforward: ‘sum (diag (A))’.
 
      See also: Seeeig XREFeig.
 
  -- : rref (A)
  -- : rref (A, TOL)
  -- : [R, K] = rref (...)
      Return the reduced row echelon form of A.
 
      TOL defaults to ‘eps * max (size (A)) * norm (A, inf)’.
 
      The optional return argument K contains the vector of "bound
      variables", which are those columns on which elimination has been
      performed.