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sppsvx(3P)		    Sun Performance Library		    sppsvx(3P)

NAME
       sppsvx  -  use  the  Cholesky factorization A = U**T*U or A = L*L**T to
       compute the solution to a real system of linear equations  A * X = B,

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

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

       SUBROUTINE SPPSVX_64(FACT, UPLO, N, NRHS, A, AF, EQUED, S, B,
	     LDB, X, LDX, RCOND, FERR, BERR, WORK, WORK2, INFO)

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

   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
       INTEGER :: N, NRHS, LDB, LDX, INFO
       INTEGER, DIMENSION(:) :: WORK2
       REAL :: RCOND
       REAL, DIMENSION(:) :: A, AF, S, FERR, BERR, WORK
       REAL, DIMENSION(:,:) :: B, X

       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
       INTEGER(8) :: N, NRHS, LDB, LDX, INFO
       INTEGER(8), DIMENSION(:) :: WORK2
       REAL :: RCOND
       REAL, DIMENSION(:) :: A, AF, S, FERR, BERR, WORK
       REAL, DIMENSION(:,:) :: B, X

   C INTERFACE
       #include <sunperf.h>

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

       void sppsvx_64(char fact, char uplo, long n, long nrhs, float *a, float
		 *af,  char  *equed,  float  *s, float *b, long ldb, float *x,
		 long ldx,  float  *rcond,  float  *ferr,  float  *berr,  long
		 *info);

PURPOSE
       sppsvx uses the Cholesky factorization A = U**T*U or A = L*L**T to com‐
       pute the solution to a real system of linear equations
	  A * X = B, where A is an N-by-N symmetric 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**T* U,  if UPLO = 'U', or
	     A = L * L**T,  if UPLO = 'L',
	  where U is an upper triangular matrix and L is a lower triangular
	  matrix.

       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) REAL array, dimension (N*(N+1)/2)
		 On entry, the upper or lower triangle of the symmetric 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) REAL 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'*U or A = L*L', 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'*U or A = L*L' 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'*U or A = L*L' of the equilibrated matrix  A
		 (see  the  description	 of A for the form of the equilibrated
		 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) REAL 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) REAL 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)
		 REAL array, dimension (3*N)

       WORK2 (workspace)
		 INTEGER 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 symmetric 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			    sppsvx(3P)
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