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cppsvx(3P)		    Sun Performance Library		    cppsvx(3P)

NAME
       cppsvx  -  use  the  Cholesky factorization A = U**H*U or A = L*L**H to
       compute the solution to a complex system of linear equations  A *  X  =
       B,

SYNOPSIS
       SUBROUTINE CPPSVX(FACT, UPLO, N, NRHS, A, AF, EQUED, S, B, LDB,
	     X, LDX, RCOND, FERR, BERR, WORK, WORK2, INFO)

       CHARACTER * 1 FACT, UPLO, EQUED
       COMPLEX A(*), AF(*), B(LDB,*), X(LDX,*), WORK(*)
       INTEGER N, NRHS, LDB, LDX, INFO
       REAL RCOND
       REAL S(*), FERR(*), BERR(*), WORK2(*)

       SUBROUTINE CPPSVX_64(FACT, UPLO, N, NRHS, A, AF, EQUED, S, B,
	     LDB, X, LDX, RCOND, FERR, BERR, WORK, WORK2, INFO)

       CHARACTER * 1 FACT, UPLO, EQUED
       COMPLEX A(*), AF(*), B(LDB,*), X(LDX,*), WORK(*)
       INTEGER*8 N, NRHS, LDB, LDX, INFO
       REAL RCOND
       REAL S(*), FERR(*), BERR(*), WORK2(*)

   F95 INTERFACE
       SUBROUTINE PPSVX(FACT, UPLO, [N], [NRHS], A, AF, EQUED, S, B,
	      [LDB], X, [LDX], RCOND, FERR, BERR, [WORK], [WORK2], [INFO])

       CHARACTER(LEN=1) :: FACT, UPLO, EQUED
       COMPLEX, DIMENSION(:) :: A, AF, WORK
       COMPLEX, DIMENSION(:,:) :: B, X
       INTEGER :: N, NRHS, LDB, LDX, INFO
       REAL :: RCOND
       REAL, DIMENSION(:) :: S, FERR, BERR, WORK2

       SUBROUTINE PPSVX_64(FACT, UPLO, [N], [NRHS], A, AF, EQUED, S, B,
	      [LDB], X, [LDX], RCOND, FERR, BERR, [WORK], [WORK2], [INFO])

       CHARACTER(LEN=1) :: FACT, UPLO, EQUED
       COMPLEX, DIMENSION(:) :: A, AF, WORK
       COMPLEX, DIMENSION(:,:) :: B, X
       INTEGER(8) :: N, NRHS, LDB, LDX, INFO
       REAL :: RCOND
       REAL, DIMENSION(:) :: S, FERR, BERR, WORK2

   C INTERFACE
       #include <sunperf.h>

       void  cppsvx(char fact, char uplo, int n, int nrhs, complex *a, complex
		 *af, char *equed, float *s, complex *b, int ldb, complex  *x,
		 int ldx, float *rcond, float *ferr, float *berr, int *info);

       void  cppsvx_64(char  fact,  char  uplo, long n, long nrhs, complex *a,
		 complex *af, char *equed, float *s,  complex  *b,  long  ldb,
		 complex *x, long ldx, float *rcond, float *ferr, float *berr,
		 long *info);

PURPOSE
       cppsvx uses the Cholesky factorization A = U**H*U or A = L*L**H to com‐
       pute the solution to a complex system of linear equations
	  A  *	X = B, where A is an N-by-N Hermitian positive definite matrix
       stored in packed format and X and B are N-by-NRHS matrices.

       Error bounds on the solution and a condition  estimate  are  also  pro‐
       vided.

       The following steps are performed:

       1. If FACT = 'E', real scaling factors are computed to equilibrate
	  the system:
	     diag(S) * A * diag(S) * inv(diag(S)) * X = diag(S) * B
	  Whether or not the system will be equilibrated depends on the
	  scaling of the matrix A, but if equilibration is used, A is
	  overwritten by diag(S)*A*diag(S) and B by diag(S)*B.

       2. If FACT = 'N' or 'E', the Cholesky decomposition is used to
	  factor the matrix A (after equilibration if FACT = 'E') as
	     A = U'* U ,  if UPLO = 'U', or
	     A = L * L',  if UPLO = 'L',
	  where U is an upper triangular matrix, L is a lower triangular
	  matrix, and ' indicates conjugate transpose.

       3. If the leading i-by-i principal minor is not positive definite,
	  then the routine returns with INFO = i. Otherwise, the factored
	  form of A is used to estimate the condition number of the matrix
	  A.  If the reciprocal of the condition number is less than machine
	  precision, INFO = N+1 is returned as a warning, but the routine
	  still goes on to solve for X and compute error bounds as
	  described below.

       4. The system of equations is solved for X using the factored form
	  of A.

       5. Iterative refinement is applied to improve the computed solution
	  matrix and calculate error bounds and backward error estimates
	  for it.

       6. If equilibration was used, the matrix X is premultiplied by
	  diag(S) so that it solves the original system before
	  equilibration.

ARGUMENTS
       FACT (input)
		 Specifies whether or not the factored form of the matrix A is
		 supplied on entry, and if not, whether the matrix A should be
		 equilibrated  before  it  is  factored.  = 'F':  On entry, AF
		 contains the factored form of A.  If EQUED = 'Y', the	matrix
		 A  has	 been equilibrated with scaling factors given by S.  A
		 and AF will not be modified.  = 'N':  The matrix  A  will  be
		 copied to AF and factored.
		 =  'E':  The matrix A will be equilibrated if necessary, then
		 copied to AF and factored.

       UPLO (input)
		 = 'U':	 Upper triangle of A is stored;
		 = 'L':	 Lower triangle of A is stored.

       N (input) The number of linear equations, i.e., the order of the matrix
		 A.  N >= 0.

       NRHS (input)
		 The  number  of right hand sides, i.e., the number of columns
		 of the matrices B and X.  NRHS >= 0.

       A (input/output) COMPLEX array, dimension (N*(N+1)/2)
		 On entry, the upper or lower triangle of the Hermitian matrix
		 A,  packed columnwise in a linear array, except if FACT = 'F'
		 and EQUED = 'Y', then A must contain the equilibrated	matrix
		 diag(S)*A*diag(S).   The  j-th	 column	 of A is stored in the
		 array A as follows: if UPLO = 'U', A(i + (j-1)*j/2) =	A(i,j)
		 for  1<=i<=j;	if  UPLO = 'L', A(i + (j-1)*(2n-j)/2) = A(i,j)
		 for j<=i<=n.  See below for further details.  A is not	 modi‐
		 fied  if  FACT = 'F' or 'N', or if FACT = 'E' and EQUED = 'N'
		 on exit.

		 On exit, if FACT = 'E' and EQUED = 'Y', A is  overwritten  by
		 diag(S)*A*diag(S).

       AF (input or output) COMPLEX array, dimension (N*(N+1)/2)
		 If FACT = 'F', then AF is an input argument and on entry con‐
		 tains the triangular factor U or L from the Cholesky  factor‐
		 ization  A = U**H*U or A = L*L**H, in the same storage format
		 as A.	If EQUED .ne. 'N', then AF is the factored form of the
		 equilibrated matrix A.

		 If  FACT  =  'N',  then  AF is an output argument and on exit
		 returns the triangular factor U or L from the	Cholesky  fac‐
		 torization A = U**H*U or A = L*L**H of the original matrix A.

		 If  FACT  =  'E',  then  AF is an output argument and on exit
		 returns the triangular factor U or L from the	Cholesky  fac‐
		 torization  A	=  U**H*U  or  A  = L*L**H of the equilibrated
		 matrix A (see the description of A for the form of the	 equi‐
		 librated matrix).

       EQUED (input or output)
		 Specifies  the	 form  of equilibration that was done.	= 'N':
		 No equilibration (always true if FACT = 'N').
		 = 'Y':	 Equilibration was done, i.e., A has been replaced  by
		 diag(S)  * A * diag(S).  EQUED is an input argument if FACT =
		 'F'; otherwise, it is an output argument.

       S (input or output) REAL array, dimension (N)
		 The scale factors for A; not accessed if EQUED = 'N'.	 S  is
		 an  input  argument  if FACT = 'F'; otherwise, S is an output
		 argument.  If FACT = 'F' and EQUED = 'Y', each element	 of  S
		 must be positive.

       B (input/output) COMPLEX array, dimension (LDB,NRHS)
		 On  entry,  the N-by-NRHS right hand side matrix B.  On exit,
		 if EQUED = 'N', B is not modified; if EQUED = 'Y', B is over‐
		 written by diag(S) * B.

       LDB (input)
		 The leading dimension of the array B.	LDB >= max(1,N).

       X (output) COMPLEX array, dimension (LDX,NRHS)
		 If INFO = 0 or INFO = N+1, the N-by-NRHS solution matrix X to
		 the original system of equations.  Note that if EQUED =  'Y',
		 A and B are modified on exit, and the solution to the equili‐
		 brated system is inv(diag(S))*X.

       LDX (input)
		 The leading dimension of the array X.	LDX >= max(1,N).

       RCOND (output)
		 The estimate of the reciprocal condition number of the matrix
		 A  after  equilibration (if done).  If RCOND is less than the
		 machine precision (in particular, if RCOND = 0),  the	matrix
		 is  singular  to  working precision.  This condition is indi‐
		 cated by a return code of INFO > 0.

       FERR (output) REAL array, dimension (NRHS)
		 The estimated forward error bound for	each  solution	vector
		 X(j) (the j-th column of the solution matrix X).  If XTRUE is
		 the true solution corresponding to X(j), FERR(j) is an	 esti‐
		 mated upper bound for the magnitude of the largest element in
		 (X(j) - XTRUE) divided by the magnitude of the	 largest  ele‐
		 ment  in  X(j).   The estimate is as reliable as the estimate
		 for RCOND, and is almost always a slight overestimate of  the
		 true error.

       BERR (output) REAL array, dimension (NRHS)
		 The  componentwise  relative  backward error of each solution
		 vector X(j) (i.e., the smallest relative change in  any  ele‐
		 ment of A or B that makes X(j) an exact solution).

       WORK (workspace)
		 COMPLEX array, dimension(2*N)

       WORK2 (workspace)
		 REAL array, dimension(N)

       INFO (output)
		 = 0:  successful exit
		 < 0:  if INFO = -i, the i-th argument had an illegal value
		 > 0:  if INFO = i, and i is
		 <= N:	the leading minor of order i of A is not positive def‐
		 inite, so the factorization could not be completed,  and  the
		 solution  has	not  been  computed. RCOND = 0 is returned.  =
		 N+1: U is nonsingular, but RCOND is less than machine	preci‐
		 sion,	meaning	 that the matrix is singular to working preci‐
		 sion.	Nevertheless, the solution and error bounds  are  com‐
		 puted because there are a number of situations where the com‐
		 puted solution can be more accurate than the value  of	 RCOND
		 would suggest.

FURTHER DETAILS
       The  packed storage scheme is illustrated by the following example when
       N = 4, UPLO = 'U':

       Two-dimensional storage of the Hermitian matrix A:

	  a11 a12 a13 a14
	      a22 a23 a24
		  a33 a34     (aij = conjg(aji))
		      a44

       Packed storage of the upper triangle of A:

       A = [ a11, a12, a22, a13, a23, a33, a14, a24, a34, a44 ]

				  6 Mar 2009			    cppsvx(3P)
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