PROGRAMS RCN MOD36 / HF MOD8 / RCN2 (Mod 36)
COMPUTATION OF ATOMIC RADIAL WAVEFUNCTIONS
Robert D. Cowan
Los Alamos National Laboratory
August 1993 (revised June 1994)
CONTENTS
I. SUMMARY OF PROGRAMS
A. Introduction 2
B. Program RCN Mod36 2
C. Program HF Mod8 3
D. Program RCN2 3
E. Computing times 4
II. PROGRAM RCN36
A. Program outline 5
B. Input 8
C. Calculational procedure 13
D. Input/output units 15
E. Output 15
F. Hartree-Fock calculations 16
G. Calculation of continuum functions 18
H. Vinti integrals 18
I. Correlation potential 19
J. Frozen-orbital options 20
K. Negative-ion calculations 20
L. Dielectronic recombination calculations 22
M. Storage requirements 23
N. Conversion to other computers 23
III. PROGRAM HF8
A. Outline 24
B. Input 25
C. Input/output units 26
D. Storage requirements 26
E. Miscellaneous 27
IV. PROGRAM RCN2
A. Outline 27
B. Input 28
C. Calculational procedure 31
D. Input/output units 34
E. Output 34
F. Plane-wave-Born calculations in RCG 34
G. Photoionization and autoionization calculations in RCG 36
H. Storage requirements 36
I. Conversion to other computers 36
V. PROGRAM USAGE AND EXAMPLE
A. Execution 37
B. Sample input and output 38
C. Command-file methods 39
D. Sample monitor screen output
I. SUMMARY OF PROGRAMS
A. Introduction
This is a set of three FORTRAN 77 programs used on 64-bit-
word CRAY or CDC CYBER 205 computers for the self-consistent-field
calculation of atomic radial wavefunctions, and of various radial
integrals involved in the calculation of atomic energy levels and
spectra. RCN and RCN2 are easily adaptable to VAX, IBM RISC, SUN,
Macintosh, and similar 32-bit-word computers because of the
following coding features:
(1) IMPLICIT REAL*8 (A-H,O-Z) statements have been included
in all program units, so that floating-point variables will be double
precision for 32-bit computers. (These statements can be commented
out if necessary on 64-bit machines.)
(2) Generic names have been used for intrinsic functions,
with arguments that are never numbers, but rather are variables
defined by statements, such as HALF=0.5 or TWO=2.0, so that
conversion to double precision will be automatically performed on
32-bit machines.
(3) Named common blocks of a given name have the same length
in all subroutines. In all cases, there are an even number of
integer storage spaces if followed by a floating-point variable.
The programs can be run in a chain in any of the following
four combinations:
RCN
RCN/RCN2
RCN/HF
RCN/HF/RCN2
The primary input information is always to RCN, and each
program automatically provides input information to the succeeding
program of the chain. Details of the programs will be described
later; here we outline only the basic purpose of each program.
NOTE: The program RCN Mod36 still contains the possibility
of feeding information into HF. However, unlike in pre-1981
versions, RCN can itself calculate Hartree-Fock wavefunctions.
Therefore the program HF is no longer used, and is not supplied;
the pertinent option in RCN has been retained for use by anyone
desiring wavefunctions on the logarithmic radial mesh used by HF.
B. Program RCN Mod36
Program RCN calculates single-configuration radial
wavefunctions Pnl(r) for a spherically symmetrized atom via any
one of the four following homogeneous-differential-equation
approximations to the Hartree-Fock method.
(1) Hartree (H);
(2) Hartree-Fock-Slater, with any desired value of the
coefficient for Slater's approximate exchange term, and either
without (HFS) or with (HFSL) Latter's tail cutoff in the central-
field potential-energy function;
(3) Hartree-plus-statistical-exchange (HX);
(4) Hartree-Slater (HS).
(5) RCN can also be used for true Hartree-Fock (HF)
calculations, either for the spherically symmetrized atom (center-
of-gravity energy of the configuration), or for the energy of a
specific LS term of the configuration (LSD-HF) provided there
exists only one LS term having that value of LS.
Normally the HX method or the center-of-gravity HF method is
the only one used.
In addition to the radial wavefunctions, also calculated for
each configuration are various radial integrals (ármñ, Fk, Gk, z),
and the total energy of the atom (Eav) including approximate
relativistic and correlation energy corrections. Relativistic
terms can be included in the potential function of the
differential equation (HXR or HFR) to give approximate
relativistic corrections to the radial wavefunctions, as well as
improved relativistic energy corrections in heavy atoms (important
for outer orbitals only if Z > 50, and for inner orbitals if Z > 20).
Similarly, a correlation term can be included in order to make the
potential function more negative, and thereby help to bind
negative ions. Options are available to provide radial
wavefunctions as input to either program RCN2 or program HF8.
C. Program HF Mod8
Program HF8 calculates single-configuration Hartree-Fock
radial wavefunctions corresponding to either the center-of-gravity
energy of the configuration, or to any specified LS term of the
configuration (provided the LS value of interest appears only once
in that configuration). Radial integrals, Eav, and relativistic
and correlation corrections are calculated as in RCN. Except for
a universal control card, input is entirely from RCN; output
wavefunctions provide input to RCN2. Relativistic terms can be
included in the HF equations if desired (HFR). Inasmuch as RCN
can be used to compute HF or HFR wavefunctions, program HF8 is of
little utility; in contrast to RCN, HF8 does have the advantage
that off-diagonal Lagrangian parameters are included to ensure
orthogonality between radial functions of the same l but different
n (provided the two orbitals have unequal occupation numbers), but
it cannot handle one-electron configurations nor any single-
subshell configuration nlw, and it cannot be used to compute
unbound (continuum) functions.
D. Program RCN2
Program RCN2 accepts radial wavefunctions (for one or more
different configurations of one or more atoms or ions) from either
RCN or HF, and for each atom calculates various two-configuration
radial integrals: overlap integrals á Pnl|Pn'l'ñ, configuration-
interaction Coulomb integrals Rk and spin-orbit integrals znln'l',
and radial electric-dipole and electric-quadrupole integrals. In
its most commonly used option, it automatically computes all
quantities required for calculating energy levels and spectra of
an atom, and writes a file containing this information in exactly
the form required for input to program RCG, which performs these
calculations. For plane-wave-Born calculations in RCG,
calculation of radial multipole integrals in RCN2 is replaced by
calculation of radial integrals of spherical Bessel functions.
For the theory behind all of the above programs, see Robert
D. Cowan, The Theory of Atomic Structure and Spectra (University
of California Press, Berkeley, 1981), Chap. 7, and Secs. 8-1, 16-
1, and 18-13 -- hereafter referred to as TASS.
E. Computing Times
Approximate computing times for RCN and HF on CRAY-1
computers are as listed below. Times on a CRAY-YMP would be two
or three times shorter. Times on the CYBER 205 would be about the
same as listed below; times on the CDC 7600 or IBM 360/95 or
370/195 would be about 3 times longer; times on the CDC 6600 or
SUN Sparcstation would be about 10 times longer; times on the
Macintosh Centris 650 would be about 15 times longer; times on the
VAX 8200, CDC 6500, or IBM 7094 would be about 40 times longer;
and times on the VAX 11/780 would be about 100 times longer.
Time (sec)
--------------------------------------------
RCN RCN + HF8
------------------- ---------------------
Config. HX HXR HF HFR HXa+ HF HXRb+ HFR
Ar I 3p6 2 2 1 1 1 + 1 1 + 1
Kr I 4p6 3 3 3 3 2 + 2 1 + 3
Xe I 5p6 4 4 5 3 + 4 1 + 5
Dy I 4f10 6s2 6 7 10 4 + 6 2 + 8
Rn I 6p6 6 7 13 4 + 9 2 + 11
U I 5f3 6d 7s2 7 9 17 5 + 18 3 + 30
-------------
aTime for SCF calc (TOLEND = 5´10-8) + ZETA1
bTime for SCF calc (TOLEND = 5´10-2) only
Computing time for RCN2 is usually only a small fraction of
the RCN or HF time. However, if there are a large number of
configurations on the TAPE2N input file to RCN2 (say, > 20) and the
configurations in question are the ones with high serial number,
read and rewind times can be uncomfortably long, especially if the
file is on a tape rather than a disk unit.
II. PROGRAM RCN36
A. Program outline
This is a FORTRAN 77 program for the calculation of radial
wavefunctions Pnl(r) of a spherically symmetrized atom,
corresponding to the center-of-gravity energy Eav of an electron
configuration
(n1l1)w1 (n2l2)w2 ...Ê(nqlq)wq . (1)
Computed from these radial wavefunctions are the Coulomb integrals
Fk and Gk and the spin-orbit integrals znl , along with radial
integrals required to give kinetic and electron-nuclear energies,
and rough relativistic and correlation corrections to both the
one-electron binding energies and the total electronic binding
energy Eav .
The program was originally (January 1964) based on the SHARE
program 1417 (ML HFSS) described by Herman and Skillman, Atomic
Structure Calculations (Prentice-Hall, 1963), and this reference
may be used for a description of the radial integration mesh and
basic numerical methods used in RCN. However, except for the
subroutine CROSYM and part of SCHEQ, the original program has been
changed beyond recognition [including notational changes from
SNL(M,I) and SNLO(I) to PNL(I,M) and PNLO(I), and a redefinition
of NNLZ from 100n+10l+const. to 100n+l]. Options are still
available for making calculations via the Hartree-Fock-Slater
approximation used by Herman and Skillman either with or without
Latter's tail cutoff in the one-electron potential, using either
Slater's original exchange coefficient 3/2 or Kohn and Sham's
modified value of 1 (or any other value). However, these
approximations are all considered to be unsatisfactory; a much
better option utilizes the Hartree-plus-statistical-exchange (HX)
approximation described in my book TASS, which should be consulted
for theoretical discussions. Still further options are the HS
approximation of Lindgren and Rosen [Int. J. Quant. Chem. S5, 411
(1971); Phys. Scripta 6, 109 (1972), or TASS], and full Hartree-
Fock calculations. Hartree-Fock is the preferred option.
Normally, all radial functions are iterated to self-
consistency. However, on configurations other than the first one,
any desired number of inner orbitals can be held fixed (frozen-
core approximation; see discussion below concerning the variable
IBB1, and Secs. II-J and II-K).
The program is all in FORTRAN 77, and consists of a main
program and thirty-odd subprograms.
RCN36 is the main program, and mostly just decides whether a
normal calculation is to be performed, or one pertinent to
dielectronic-recombination.
RCN is the main subroutine. It handles all input (for normal
calculations) and some output, controls the self-consistent-field
iteration, and does portions of the detailed calculation.
ANALYZ and SETCFG interpret the configuration-definition
input and estimate initial values of the one-electron eigenvalues.
DIEL and ANALYZ1 are subroutines used to reduce handwork
involved in setting up dielectronic-recombination runs; details
are discussed in Sec. II-L.
SCHEQ integrates the one-electron radial wave equation, and
controls the iteration on the one-electron eigenvalue E=EE(M) to
give a radial wavefunction Pnl(r)ºrRnl(r)=PNLO(I)=PNL(I,M) that
satisfies the boundary conditions at r=0 and ¥. It also properly
normalizes the function for either a bound electron (E < 0) or a
free electron (E > 0); it will not handle the case E=0. The
normalization for a free electron is likely to be inaccurate if E >
0.1 rydberg (because of too coarse an integration mesh) unless
EMX/10 < E < EMX and very large dimensions are used for PNL, R, and
other variables (see remarks below regarding continuum-
wavefunction calculations--Sec. II-G). Appropriate small non-zero
values of EMX also make possible calculation of Pnl for large n
(about 15 to 40) by bringing into use the full 1801-point mesh
instead of the 641-point mesh used when EMX=0; too large a value
of EMX (or too large n) will result in convergence failure because
even the 1801-point mesh will not extend to large enough radii.
OUTPT handles most of the printed output (in part, via calls
to POWER, ZETA1, and SLI1) and the wavefunction output to disk
file 2 or (via a call to HFWRTP) to disk file 7, which provides
input to program RCN2 or HF8, respectively.
SUBCOR calculates a modified free-electron correlation energy
for a specified electron density.
CROSYM solves a system of linear equations to provide a value
of
AZ = [ Pnl(r)/r**(l+1) ] at r=0 . (2)
POWER computes values of ármñ for -3 £ m £ 6 (except m=5) for
each orbital.
ZETA1 computes spin-orbit parameter values znl from the
central-potential formula
1 dV
znl = Integral(0 to inf.) [ Pnl**2(r) - -- dr ] , (3)
r dr
and also via the Blume-Watson method [Proc. Roy. Soc. (London)
A270, 127 (1962), A271, 565 (1963)]; the latter method gives much
more accurate values and so provides the numbers used in practice.
Also computed and printed are the one-electron kinetic-plus-
nuclear energy Inl , and the relativistic mass-velocity and Darwin
corrections. (Actually, Inl is computed in RCN3S, and only
printed in ZETA1.)
SLI1 computes and prints all Slater integrals Fk and Gk (in
units of both rydbergs and cm-1); it also computes overlap
integrals and calls RCN3S.
RCN3S prints the overlap integrals, and calculates (from the
Fk and Gk, with the aid of subroutine S3J0SQ) and prints the
Coulomb interaction energy between each pair of electrons. It
then calculates correlation-energy corrections, and (using values
of Inl from ZETA1) calculates and prints one-electron binding
energies and the total binding energy of the atom (see TASS for
equations). It also prints those single-configuration parameter
values Eav, Fk(ii), zi, Fk(ij), and Gk(ij) required for the
calculation of atomic energy levels; the total binding energy Eav
is given in rydbergs, whereas all other parameter values are in kK
(units of 1000 cm-1).
S3J0SQ calculates the value of
( j1 j2 j3 ) where ( j1 j2 j3 )
( 0 0 0 ) ( m1 m2 m3 )
is a 3-j symbol; though not used here, for other purposes there
exists also a function routine S3J.
FCTRL calculates the factorial of an integer A, required by
S3J0SQ and S3J.
HFWRTP interpolates values of each wavefunction from the
(periodically doubled) linear mesh used by RCN to points on the
logarithmic mesh used by HF8, and writes on tape 7 these
wavefunctions and other input data for a Hartree-Fock calculation
via program HF8.
HFPOT calculates for a given orbital the Hartree-Fock
potential (excluding the classical-potential terms, which are
calculated in the main subroutine), written in the form of an
effective homogeneous-equation local-potential function. (This is
necessary because RCN is basically a homogeneous-equation program.
The singularities that are present in the potential at zeroes of
the orbital in question are smoothed out by means of a linear
interpolation from the second mesh point below to the second mesh
point above each zero.)
QUAD2 calculates the classical potential via a Simpson's-rule
quadrature.
QUAD5 is a general-purpose five-interval quadrature routine.
QUADK is used by HFPOT for the evaluation of Hartree's Yk
function.
ZETABW evaluates spin-orbit parameters via the Blume-Watson
method, using function routines SM, SN, ZK, VK, and DYK patterned
after those in HF8.
S6J evaluates the 6-j symbol
( j1 j2 j3 )
( )
( l1 l2 l3 )
with the aid of a function routine DELSQ .
CLOCK is a subroutine used to call a CPU-time system-routine
SECOND, which contains sections appropriate to a CRAY, VAX or
Macintosh, SUN, and IBM RISC; SECOND may be replaced by a dummy
do-nothing routine if desired.
PHSHIFT is a subroutine that for continuum orbitals computes
and prints the phase shift of the (distorted-wave) continuum
function relative to the phase of a pure (non-relativistic)
Coulomb function. (This phase shift does not become quite
constant at large r, indicating some inaccuracy in numerical
integration of the differential equation. Because of this, and
because of omission in each phase of a term consisting of the
argument of a complex gamma function, only the phase shift is
significant, not the distorted-wave and Coulomb phases
individually.)
VINTI computes values of the Vinti integrals and associated
weighting factors and sum (see Sec. II-H).
EBREIT, BRTINT , and S3J are used for evaluation of
approximate Breit magnetic and retardation energies, if IREL=2.
The approximation is poor and inclusion of this option seems to
provide no improvement between theory and experiment; if one
wishes to save storage space, he can change the dimensions of the
approximate small-component relativistic wavefunction
QNL(KMSHQ,KOQ) from (1801,20) to (1,1), in which case the Breit
energies will not be computed even with IREL=2.
B. Input
For simplicity in the following, terminology will be used in
places that dates from the time when computer input consisted of
punched cards: The word "card" may be used to refer to a line of
an input file or FORTRAN source file, and the word "deck" to refer
to an input file--set of cards--or portion thereof. Characters
"punched" in specific columns of these cards are, of course, to be
typed into the corresponding columns of the input line.
Statements that various information is "printed" means that
information is written to the output print file 9, but in many
cases only if certain print options are in effect.
Normal input, read in subroutine RCN, consists of a control
"card," and one configuration "card" for each configuration to be
computed (not necessarily all of the same element nor ion stage)--
additional cards are required if an LS-term HF calculation is to
be done; see Sec. II-F. Normally, the control card is nearly
universal and is seldom changed from one run to the next, except
to switch from non-relativistic (HF) to relativistic (HFR)
calculations, or to include or delete correlation corrections in
the effective central-field potential function.
(1) Control card: this is read at statement 200 of the main
subroutine, and contains the following quantities.
normal value
-------------------------------------
RCN36 RCN36 + HF8
--------------- ----------------
cols format variable HX HF HX+HF HF only
----- ------ -------- ------ ----- ------ -------
1 I1 ITPOW 2 2 2 0
2 I1 IPTVU 0 0 0 0
3 I1 IPTEB 0 0 0 0
4-5 I2 NORBPT -9 -9 -9 -9
6 I1 IZHXBW 0 0 0 0
7-8 I2 IPHFWF 0 0 0 0
9-10 I2 IHF 0 2 1 1
11-13 I3 IBB 0 0 0 0
14-15 F2.1 TOLSTB 1.0 1.0 1.0 1.0
16-20 E5.1 TOLKM2 2.0 2.0 2.0 2.0
21-30 E10.1 TOLEND 5.E-08 5.E-08 5.E-08 5.E-02a
31-40 E10.1 THRESH 1.E-11 1.E-11 1.E-11 1.E-05a
41-42 I2 KUTD -2 -2 -2 -2
43-44 I2 KUT1 0 0 0 0
45 I1 IVINTI 0 0 0 0
46 I1 IRELb 0 0 0 0
47-48 I2 MAXIT 90 90 90 90
49-50 I2 NPR 0 0 0 0
51-55 F5.5 EXF10 1.0 1.0 1.0 1.0
56-60 F5.5 EXFM1 0.65 0.65 0.65 0.65
61-65 F5.5 EMXc 0.0 0.0 0.0 0.0
66-70 F5.5 CORRFd 1.0 1.0 1.0 1.0
71-75 I5 IW6e -6 -6 -6 -6
_____________________________
aUse 5.E-08 and 1.E-11 if IREL=0, and HX relativistic energy
corrections to Eav are desired.
bUse IREL=1 for HXR or HFR; use IREL=2 to include Breit energies.
cSee notes regarding continuum-wavefunction calculations, p. 5 and
Sec. II-G.
dSee Sec. II-I below.
eUse IW6=0 if output to the monitor screen is not desired on the
progress of the calculation. The value used here for IW6 is
automatically carried through to subsequent programs RCN2,
RCG, and RCE.
The first seven quantities and NPR control the amount of
printed output, as follows:
ITPOW: =1 or >2, print SCF iteration information (NITER, DELT,
ALFM); this information is sent to the
monitor screen if IW6 < 0.
>1, call POWER to print
ITPVU: >0, print Fk and Gk
>1, print Coulomb interaction energies
>2, print wavefunction overlap integrals
>3, print HFS potentials (RU, RUEE, etc)
>4, print HX or HF potentials (Vnl)
>5, in SCHEQ, print relativistic contribution to potential
IPTEB: >0, print EE, JJJ, R(JJJ), AZ
>1, print Ekin , etc
NORBPT: <0, do not print wavefunctions
>0, print first two and last NORBPT wavefunctions at
every fifth mesh point
>5, print continuum wavefunctions at every mesh point
(for configurations 1, 5, 10, 15, ... only,
if 0 < NORBPT < 6)
any, write on tape 2 or 7 the last |NORBPT|
wavefunctions (at least 2; if |NORBPT|=9,
write all wavefunctions)
IZHXBW: >0, in HF8, calculate and print all quantities using
the (HX) input wavefunctions (primarily to give
zeta calculated by the Blume-Watson method;
of no great use, as the Blume-Watson method is
now used in RCN as well as in HF8)
IPHFWF: >0, in HF8, print the last |IHFWF| wavefunctions at
every mesh point
<0, same, except print at only every fourth mesh point
9 or -9, print all wavefunctions
IHF: =0, signifies an RCN calculation only (hence, do not load HF8)
=1, RCN output wavefunctions are for input to HF8
(via tape 7, rather than for RCN2 (via tape 2);
if IREL > 1, RCN calculation of radial integrals
is skipped; if IREL=0 and TOLEND < 1.E-4, only
ZETA1 is called (to calculate relativistic
energy correction for Eav in HF8)
=2, carry out a Hartree-Fock calculation within RCN
NPR: not 0, diagnostic potentials and diagnostic wavefunctions
are printed during the course of the RCN SCF
iteration
The significance of the other input quantities is as follows.
IBB not 0 sets the outer boundary of the atom at mesh point IBB;
do not use this option, as it is not completely debugged.
TOLEND is the maximum permissible value of DELTA (the
absolute value of the change in RU) for ending the SCF iteration
(see the main program, statements number 530-550 and 700-780).
THRESH is the maximum permissible fractional change in the
value of the eigenvalue E to end the eigenvalue iteration (SCHEQ,
statements 805 and 205).
MAXIT is the maximum allowable number of SCF iterations; if
convergence has not been reached within MAXIT cycles, the
calculation is continued for 4 more cycles with diagnostic
printout produced via NPR > 0 (RCN, 710-729).
EXF10 is the coefficient of Slater's exchange term for an HFS
calculation with no tail cutoff (KUT=1) or with tail cutoff
(KUT=0) (RCN 411-417). EXF10=1.5 is Slater's original value and
EXF10=1.0 is Kohn and Sham's modified value.
EXFM1, CAO, and CA1 are values of k1, k3, and k2,
respectively, for KUT=-1 in an HX calculation [Phys. Rev.163, 54
(1967), Eqs. (13)-(14) or TASS, Eqs. (7.49)-(7.50)]. Provided
IHF=0, EXFM1=0.0 will give a Hartree calculation for KUT=-1, and
KUT=-2 gives an HS calculation. (CAO and CA1 are no longer read
in from the control card, but simply set to 0.5 and 0.7,
respectively, in the code.)
If IREL=0, relativistic terms are omitted from the
differential equations (HX or HF); if IREL > 0, these terms are
included (HXR or HFR). If IREL > 1, approximate Breit magnetic and
retardation energies will be included, provided the dimensions of
QNL are the same as those of PNL. If IREL > 3, some diagnostic
printouts will occur.
Other quantities will be discussed later.
(2) Configuration card: This is read at statement 210 of
subroutine RCN and contains the following information.
cols format variable significance
----- ------ -------- --------------------------------------------
1 I1 NHFTRM Number of LS terms for which HF calculations
are to be made
2-5 I4 IZ Atomic number (fixed point)
6-8 I3 IBB1 For this configuration only, overrides the
value IBB read from the control card,
provided IBB1 > KO, the storage dimension
for the maximum number of orbitals. If
0.LE.IBB1.LE.KO, then the input value is
interpreted as a quantity N1SCF, and IBB1 is
set to zero. All radial functions with
serial number equal to or less than N1SCF
are held frozen at their form in the
preceding configuration; see examples
in Secs. II-J and K.
9-10 I2 NSPECT 1+degree of ionization (1=neutral, 2=singly
ionized, 3=doubly ionized, etc.)
11-28 3A6 CONF BCD configuration label (eg, Ca I 4s 3d),
for identification purposes only. (For
clarity of RCN2 and RCG output, columns
11-16 should contain the element and ion
stage, and the configuration label should
be restricted to columns 17-24).
29-32 2I2 IALFMIN Iteration control variables (normally left
blank)
IALFMAX --if IALFMIN is non-blank, then so also
must be IALFMAX. (Each must consist of two
non-blank digits, and represents a value in
percent.)
33-35 A3 NLBCD8(1) Orbital specification (eg, " 4s", "12d",
etc.)
36-37 A2 WWNL8(1) Occupation number (0^ means 0, ^^ or 1^
means 1, 2^ means 2, etc, where ^
signifies a blank)
. . .
. . .
. . .
68-70 A3 NLBCD8(8) Orbital specification
71-72 A2 WWNL8(8) Occupation number (default value is 1)
73-74 I2 KUT For this configuration only, KUT.NE.0 overrides
the value of KUT1 from the control card.
(See examples in Sec. II-K.)
75-80 F6.5 EE8 Eigenvalue (kinetic energy in rydbergs) of
the outermost orbital for a free electron.
(EE8 must be greater than 0; the last-
punched value of NLBCD8 must be "99s",
"99p", "99d", etc, and the corresponding
value of WWNL8 must beÊblank or one.)
The above column-number restrictions for the variables in
columns 11 to 80 may be adhered to if desired, but actually a
blank-delimited, semi-free-form format is permissible, as follows:
(a) The CONF field begins in column 11 and extends to at
least column 16, but terminates at column 28 or whenever three
successive blanks occur-- whichever happens first.
(b) The IALFMIN/IALFMAX field, if present at all, appears
next--two successive non-blank digits if only IALFMAX is present,
four successive non-blank digits if IALFMIN and IALFMAX are both
present. Floating-point control variables are calculated via
ALFMIN=0.01*IALFMIN
ALFMAX=0.01*IALFMAX ,
default values being 0.20 and 1.00, respectively.
(c) The subshell nl values and occupation numbers come next-
-any number of subshells up to eight, each with format A3,A2 (or
A2,A2 is OK if n < 10).
(d) KUT (1 or -1) and/or EE8 (any number of digits, with
decimal point) come last, in either order, default values being 0
and 0.0 .
Thus, beginning with column 11, one has almost complete
freedom as to the columns in which information is to be typed.
For example, for ionized copper plus a free p electron (denoted by
using n=99) with kinetic energy of 13.6268 Ry, the nominal formats
given in the above table would require
29 1Cu I d10 13.6p 3d1099p 13.627
but actually any one of the following is equally valid:
29 1Cu I d10 13.6p 3d1099p 13.627
29 1Cu I d10 13.6p 3d10 99p 13.6268
29 1Cu I d10 13.6p 3d10 99p 13.626793
This semi-free-form flexibility is provided by reading columns 11-
80 with format A70 , and then interpreting this information by
means of subroutine ANALYZ (or ANALYZ1, when subroutine DIEL is
used).
C. Calculational Procedure
After reading the control card, the following is done for
each configuration card:
(a) If IZ > 0 but columns 11-16 are blank (first
configuration card only), the output from IZ completed
configurations done on previous runs is skipped over on tape2n, so
that results for configurations in the present run will be added
on to those done previously.
If IZ=0, go back and read a new control card. (This feature
makes it possible, for example, to make both HF and HFR
calculations in a single run.)
If IZ < 0, write EOF on tape 2 (and on tape7 if IHF0), and
exit.
If IZ > 0 and columns 11-16 are not all blank, this is a
genuine configuration card, and a calculation is made as follows:
(b) Calculate the number of electrons in the atom from
N = IZ + 1 - NSPECT .
Set up the heaviest noble-gas core (ground configuration of He,
Ne, Ar, Kr, Xe, Rn, or Z=118) having no more than N electrons.
Modify or add to this core according to any values of NLBCD8/WWNL8
punched on the configuration card, so as to obtain the final
desired configuration, Eq. (1). [Note that any orbital in the
noble-gas core modified via NLBCD8/WWNL8 with WWNL8=0 is deleted
completely from the final configuration unless it is one of the
frozen-core orbitals, in which case the orbital is retained with
zero occupation number.] Estimate a value of the eigenvalue for
each orbital (unless EE8 is non-zero, in which case this value is
used for the outermost orbital.) [Decoding of WWNL8 (subroutine
SETCFG, statements 230-233) and of NLBCD8 (statements 237-242) is
done partly via table look-up.]
In setting up each configuration card, it is worth noting
that the spectrum number punched in columns 9-10 of the card is
used only to find the noble-gas configuration from which to start
in setting up the desired final configuration. Fictitious numbers
sometimes can be used to simplify the card punching. For example,
the following two cards will produce exactly the same results for
neutral germanium:
32 1Ge I 4p 4d 3d10 4s2 4p 4d
32 -3Ge I 4p 4d 4p 4d
The former starts with Ar I 3p6 and adds on 14 more electrons; the
latter starts with Kr I 4p6, changes 4p6 to 4p1, and adds on 4d1.
(c) A radial integration mesh is set up in terms of a
universal mesh X(I), scaled via R(I)=C*X(I) , where
C=0.88534138/Z1/3 (RCN, 290-295).
(d) A suitable starting atomic potential RU(I) for the
current value of Z is obtained by scaling a universal input
potential RU0 (Herman and Skillman's function U for argon, first
configuration only) or the final SCF potential from the preceding
configuration (RCN, statements 270-290).
(e) A SCF iteration is carried out by repeatedly (up to
MAXIT times): calling SCHEQ to integrate the differential equation
to obtain a radial function PNL(I,M) for each orbital M;
recalculating the potential RU from the PNL; comparing the PNL
and/or RU with values from the preceding cycle, and revising as
appropriate.
An HX or HF calculation is started by first making an HFS
calculation (KUT=0) for at least two cycles to obtain approximate
wavefunctions (required for the calculation of HX or HF potential
functions for use in the differential equation), and then
automatically switching to HX or HF (KUT=-1) when DELTA < TOLKM2
(RCN, statements 730-735). [To calculate via HFS only, make
TOLKM2=0 on the control card; to calculate for two or more values
of KUT in succession (in the order +1, 0, -1, -2), make
TOLKM2=TOLEND on the control card, KUT1=1 (or 0, if KUT=1 is not
desired), and KUTD=0 if KUT=0 is not desired (see RCN, statements
990-end).] On other than the first configuration, the initial HFS
calculation can be skipped and the HX or HF calculation started
immediately by setting KUT=-1 on the configuration card, provided
all orbitals in the new configuration are present also (in the
same order) in the preceding configuration; for examples, see Sec.
II-K.
Stabilization of the SCF iteration is via RU on early cycles
(RCN, statements 600-660), and on the PNL on later cycles (454-
490). The control involves quantities ALF(M), recomputed each
cycle within the range ALFMIN to ALFMAX (normally 0.2 to 1.0). If
convergence is not obtained on a run, rerun it with ITPOW=1 or 3
to print values of DELTA (unless IW6 < 0, in which case this
information is already available on the monitor-screen output).
If the SCF iteration seems to be progressing satisfactorily (DELTA
changing more or less monotonically toward zero), but not
satisfying the criterion |DELTA| < TOLEND in MAXIT cycles, MAXIT
and/or IALFMIN can be increased on the control card. If the SCF
iteration should fail to converge because of oscillatory instabil-
ities (very unlikely), three things can be tried: (1) decrease
the values of IALFMIN and IALFMAX read in on the configuration
card; (2) increase the value of TOLEND on the control card; (3) in
the FORTRAN statement just before statement 708 of RCN, increase
the number "5.E-06", which is an upper bound on the fractional
change allowed in the tail of each wavefunction.
(f) Using the final SCF radial wavefunctions PNL, various
one-electron radial integrals (eg, kinetic energy and electron-
nuclear potential energy) are computed, the subroutines POWER,
ZETA1, SLI1, and RCN3S are called, and output is written on a BCD
output print unit 9 (external name OUT36); also, provided there
exists no asterisk anywhere in columns 11-16 of the configuration
card, then wavefunctions and other information are written on
output file tape2n for use by the computer program RCN2, or (if
IHF=1) HFWRTP is called to convert from a linear to a logarithmic
mesh and write tape7 for use by program HF8 (see subroutine OUTPT,
statements 989-990) .
(g) If the values of TOLKM2, TOLEND, KUT, and KUTD so
indicate, additional calculations are automatically made for the
same configuration, but with different values of KUT [see under
(e) above].
D. Input/output units
Data input and printed output are via files 10 and 9
(external names IN36 and OUT36), respectively. In addition,
binary file 2 (external name TAPE2N) or 7 is used for output
wavefunctions (input to RCN2 or HF8, respectively), and binary
file 4 is used for temporary scratch storage. If IW6 < 0, then the
progress of the SCF iteration for each configuration is sent to
the monitor screen via unit 6.
E. Output
The amount of printed output is controlled by the quantities
ITPOW, IPTVU, IPTEB, IHF, and NPR punched on the control card, in
ways described under "Input," Sec. II-B. If NORBPT > 0 , the first
two and the last NORBPT radial wavefunctions are printed out. For
each function, the value is printed at every fifth mesh point in a
two-column format (mesh points 1, 11, 21, 31, × × × in the first
column, and mesh points 6, 16, 26, 36, × × × in the second column);
the radius is printed only at mesh points 1, 11, etc. (If IREL=2
and subroutine EBREIT is in use, then the small-component
relativistic function QNL at points 1, 11, 21, × × × is printed in
place of PNL at points 6, 16, 26,Ê× × ×) If NORBPT > 5, continuum
wavefunctions are printed in the above manner, and also at every
mesh point in a ten-column format.
Coulomb interaction energies between two electrons, and one-
electron and total binding energies (without corrections, and with
relativistic and/or correlation corrections) are printed out on
the final page; all values are in rydbergs, except that spin-orbit
parameters are given in both rydbergs and cm-1.
The final line of each listing (except for timing
information) contains the configuration identification CONF, the
number of parameters required for an energy-level calculation in
the single-configuration approximation, and a list of the
parameter values together with an integer code number:
0: Eav = total binding energy, including corrections
(in rydbergs)
1: Fk(lili) (in units of 1000 cm-1)
2: zi "
3: Fk(lilj) "
4: Gk(lilj) "
The order of the parameters is the same as that required as input
to program RCG.
Finally, provided there is no asterisk in columns 11-16 of
the configuration card (columns 1-6 of the element/configuration
variable CONF) and IHF=0 or 2, then in subroutine OUTPT (statement
989) most of the important output information is written on file
2. This information includes a configuration serial number ("1"
for the first configuration, and automatically made one greater
for each succeeding configuration), the atomic number IZ and
ionization stage ION (0=neutral), and a number of wavefunctions
which for the first configuration of given IZ and ION is
determined by NORBPT, and which for later configurations is such
as to delete any wavefunctions deleted from the the first
configuration. (The purpose here is to delete most inner closed-
subshell wavefunctions, which are not needed by RCN2, so as to
decrease required disk read/write and storage requirements in
RCN2. Note, however, that if inner-subshell excitations are
involved in a set of configurations, then it is essential that
|NORBPT| be large enough that the inner-subshell orbital in
question is written onto unit 2 for all configurations--otherwise
RCN2 will put out diagnostic remarks to the effect that orbital
so-and-so could not be found, and RCN2 output will be incorrect!
To be safe in all cases, one can always use |NORBPT|=9.)
If IHF=1, then wavefunctions and other information required
to start a Hartree-Fock calculation via program HF8 are written on
unit 7 instead of on unit 2. Most radial integrals are not
computed in RCN--only the call of ZETA1 to calculate a
relativistic energy correction for carryover to HF8; if IREL > 0 ,
HF8 calculates its own relativistic energy, and time can be saved
by using TOLEND equal about 0.05, so that the RCN SCF iteration is
not carried out to final convergence.
F. Hartree-Fock calculations
If IHF > 0 , then a Hartree-Fock (HF) calculation (rather
than HFS, HX, or HS) is to be carried out--either through the use
of program HF8 (IHF=1), or self-contained within program RCN
(IHF=2).
In either case, it is possible to calculate radial
wavefunctions that minimize the energy of a particular LS term
instead of the center-of-gravity energy of the configuration, and
the added input to RCN is identical in the two cases. This option
is called by placing a non-zero value of NHFTRM (number of HF
terms) in column one of the configuration card, and following the
configuration card by NHFTRM LS-term cards (or sets of cards)
containing the following information for the ith LS term:
cols format variable significance
---- ------ -------- ------------------------------------------
1-7 A7 T1HF(I) Unused identification information (eg, the
configuration "pd", "p4 d", etc)
8-10 A3 T2HF(I) LS term identification (eg, "3P " for 3P,
etc.)
11-15 I5 NFG Number of Slater integrals (Fk and Gk)
involved in the diagonal energy-matrix
element for this LS term (excluding Eav)
21-29 F9.8 CFG(1,I) Coefficient fk or gk of the jth Fk or Gk in
the matrix element (relative to Eav)
30 A1 FG(1,I) "F" or "G", as appropriate
31 I1 KFG(1,I) Value of k
33-35 A3 IFG(1,I) Orbital codes; eg, " 3p" and " 3d" for
37-39 A3 JFG(1,I) F2(3p,3d) or Gk(3p,3d).
For legibility, column 32 may contain
a left parenthesis, column 36 a comma, and
column 40 a right parenthesis.
41-60 Same as 21-40 for the second Fk or Gk
71-80 Same as 21-40 for the third Fk or Gk
If more than three Slater integrals are involved in the expression
for the energy of this LS term (relative to Eav), then the
remaining coefficients and integral names are punched four to a
card in columns 1-20, 21-40, 41-60, and 61-80. (If a HF
calculation for the center-of-gravity energy is desired in
addition to one or more calculations for specific LS terms, this
can be done by faking an LS-term card with T2HF=C-G, NFG=1,
CFG(1,I)=0.0, IFG and JFG equal any two orbitals of the
configuration.) For IHF=1, none of this information is used in
RCN, but is simply passed on unchanged to program HF8; for IHF=2,
this information is used in subroutine HFPOT, and in SLI1
(statements 650-700).
The required values of fk and gk can in many cases be
obtained from tables in J. C. Slater, Quantum Theory of Atomic
Structure (McGraw-Hill, New York, 1960), Vol. II, App. 21.
Alternatively, they can be computed with the aid of program RCG,
using the option ICPC > 4 (see RCG writeup, or subroutine PFGD,
statements 499-900). This option will write the above information
out on file 11, except that the first two characters of IFG and
JFG will be the serial numbers of the orbitals in the RCG
calculation, and will have to be changed to the appropriate
principal quantum numbers before use as input to RCN.
G. Calculation of continuum functions
A continuum wavefunction is computed when the last orbital
defined on the configuration card is singly occupied, has a
"principal quantum number" of 99 (ie, has NLBCD8="99s", "99p",
"99d", etc), and a positive eigenvalue (kinetic energy) EE8 (in
rydbergs) has been included on the card.
In columns 61-65 of the control card, a quantity EMX may be
punched with a value approximately equal to the largest value of
EE8 contained on any of the configuration cards; if EMX is left
zero, RCN will automatically search the input file, and by default
set EMX equal to the largest value of EE8 found. The action of
EMX > 0 is firstly to set the size (MESH) of the integration mesh to
KMSH, the dimension of R, PNL, etc (instead of to 641), and
secondly to change the radial integration mesh that is set up:
instead of
del R = R(I) - R(I-1)
being doubled at mesh points 41, 81, 121, 161, ..., no further
doubling is done after del R becomes > 0.40/SQRT(EMX) . This ensures
that the mesh interval will not become so large but what there
will still be about 10 mesh points within each half-wavelength of
the continuum function, even at large R.
It is of course necessary that the dimension of the
integration mesh be great enough (hence the use of MESH=1801), or
that EMX be small enough, so that sufficiently large radii can be
reached for accurate asymptotic normalization--the value of "F"
printed via format 97 of SCHEQ should not differ from unity by
more than about 0.05 or 0.1 .
Small non-zero values of EMX can also be used to handle
large-n bound functions (n equal about 15 to perhaps 40), which
extend to radii too large for the normal 641-point integration
mesh. Use of too large a value of n or an inappropriate value of
EMX usually causes eigenvalue-iteration convergence failures or
causes execution to bomb on an overflow.
H. Vinti integrals
If the quantity IVINTI read from column 45 of the control
card is non-zero, the subroutine VINTI is called from subroutine
RCN just before statement 850:
IVINTI = 0 no call of subroutine VINTI
IVINTI > 0 Vinti integrals calculated and printed
IVINTI > 1 some debugging information printed
For any two orbitals nili and njlj with lj = li - 1, the Vinti
integral [J.P. Vinti, Phys.Rev. 56, 1120 (1939)] is defined as
( dPj Pj )
J(i,j) = Int(0 to Inf.) ( Pi --- - li -- ) dr (4)
( dr r )
In a treatment of specific mass shift, this integral is weighted
by a factor
2 li wi wj
Wij = -------------- (5)
(4li+2)(4lj+2)
The information printed is
J(i,j) J2(i,j) Wij * J2(i,j)
for each (i,j), and also the sum over i and j of
Wij * [J(i,j)]**2
I. Correlation Potential
The quantity CORRF read from columns 66-70 of the control
card is used as a multiplying factor for a theoretical approximate
correlation potential.
CORRF = 0.0 effectively deletes the potential
(equivalent to past versions of RCN)
CORRF = 1.0 is the theoretically correct value, and is the
suggested standard for future use
CORRF > 1.0 exaggerates the correlation potential.
Physically unreal values greater than unity may be needed for
negative-ion calculations. For example,
CORRF = 0.0 is adequate to bind Hg- 5d9 6s2 6p2 ;
CORRF = 1.0 is adequate to bind Hg- 5d10 6s 6p2 ,
F- 2p43s2, and F- 2p43p2 ;
CORRF = 1.5 is needed to (barely) bind F- 2p4 3s3p ;
CORRF = 2.0 is needed to (barely) bind Hg- 5d10 6s2 6p .
It is worth commenting on relationships between the output-
listing quantities EE (eigenvalue of the Schroedinger equation),
EPSFG (one-electron binding energy calculated from the kinetic
energy and the Slater Fk and Gk integrals), and EPSFGC (same,
except with added perturbation correlation energy correction).
For HF (or HFR) calculations with CORRF=0, EE is equal to
EPSFG--this is basically Koopmans' theorem. With CORRF=1, EE is
more negative than EPSFG, but is equal to EPSFGC, as is to be
expected. With CORRF > 1 , EE is more negative even than EPSFGC,
and in fact the latter may become positive (in which case SCHEQ
may mistakenly treat the radial wavefunction as if it were a
continuum function and produce completely incorrect normalization)
As a function of CORRF, the total binding energy of the atom
excluding the perturbation correlation correction is a variational
minimum for CORRF=0, but the total binding energy including the
correlation correction (which is the total energy passed on to
RCN2 and RCG) is a variational minimum for CORRF=1. It thus seems
appropriate to consider CORRF=1 (rather than CORRF=0) to be the
standard value. This results in more-contracted radial wave-
functions and hence in somewhat larger values (usually by only 1
or 2%) of the Slater integrals Fk and Gk; these values are already
too large even for CORRF=0, but this can be compensated for by
using slightly smaller values of the scale factors in RCN2.
J. Frozen-orbital options
If the quantity IBB1 read from columns 6 to 8 of the
configuration card is no larger than the dimensional parameter KO
(currently KO=20) for storing radial wavefunctions, then this
quantity is instead interpreted as N1SCF (and IBB1 set to zero).
The first N1SCF orbitals of this configuration are then held fixed
at their form in the preceding configuration. If desired, all
orbitals can be frozen. For example, with input
13 1Al I 3s2 3p
13 5 1Al I 3s 3p2 ,
all five orbitals of the configuration 3s3p2 (including 1s, 2s,
and 2p as well as 3s and 3p) will be held fixed at the form they
had in 3s23p.
Also, an orbital with zero occupancy can be retained if its
serial number is no greater than N1SCF. For example, with input
13 1Al I 3s2 3p
13 4 1Al I 3s0 3p3
13 4 1Al I 3s 3p2 ,
the orbitals 1s, 2s, and 2p of 3p3, and the orbitals 1s, 2s, 2p
and 3s of 3s3p2, will all be the same as the corresponding
orbitals of 3s23p. Further examples are discussed in the
following section.
K. Negative-ion calculations
In principle, if some value of CORRF can be found that will
bind the electrons of a negative ion in the HF (or HFR) method,
then it should be straightforward to make a calculation. In
practice, the procedure can be tricky and may require several
trial-and-error attempts. As an example, we consider the
following set-up which has been found to work for
F- 2p43s2 + 2p43p2 - 2p43s3p (with CORRF = 1.5 and IREL = 1).
9 9F I* 3S 2P4 3S 1S2 2S2 2P4 (a)
9 1 9F -* 3S2 2P4 3S2 1S2 2S2 2P4 (b)
9 9F - 3S2 2P4 3S2 1S2 2S2 2P4 -1 (c)
9 1 9F I* 3S03P P4 3S0 3P 1S2 2S2 2P4 (d)
9 1 9F - 3P2 2P4 3S0 3P2 1S2 2S2 2P4 -1 (e)
9 1 9F -* 3S 3P P4 3S 3P 1S2 2S2 2P4 -1 (f)
9 9F - 3S 3P P4 3S 3P 1S2 2S2 2P4 -1 (g)
In all configurations, NSPECT (column 10) has been taken as
9 so that the code will not set up any noble-gas core to start with
(and therefore the 1S2 and 2S2 have to be explicitly provided
everywhere). The calculation starts [configuration (a)] with a
neutral fluorine case that includes a 3s electron to provide a
starting wavefunction for (b) and (c). In (b), a calculation
(initially via a couple of HFSL cycles and then changing
automatically to HFR) is made for F- 2p43s2, with the 3s orbital
fixed at the form obtained in case (a) by including the 1 in
column 8. Then in (c), the 3s orbital is allowed to vary freely;
by including the variable KUT=-1 , the calculation begins
immediately via the HFR method, without initially backing up to
HFSL, which would have wrecked the convergence.
In (d), we go back to neutral fluorine (and, initially, HFSL)
in order to introduce a 3p orbital, holding fixed the F- 3s
orbital (with zero occupancy) for later use. In (e) we go to F-
3p2, starting immediately with HFR (KUT=-1); it proved to be
unnecessary to include here an intermediary calculation analogous
to (b), presumably because the 3p electron in (d)--unlike the 3s
electron in (a)--does not much penetrate the core, so that the 1s,
2s, and 2p HFR orbitals in (d) already provide adequate starting
functions for (e).
In (f) we make a first calculation for F- 2p43s3p, using as
starting point the 3s function from (c) and the 3p (and other)
functions from (e), but holding 3s fixed while the 3p and other
functions are allowed to vary from their forms in 2p43p2.
Finally, in (g) the 3s function is allowed to vary freely to
obtain the final 2p43s3p result. [It proved not to be possible to
delete (f), presumably because introduction of the 3s affected the
core orbitals too much to allow everything to vary
simultaneously].
Several additional remarks are appropriate:
(1) Asterisks have been included within columns 11 to 16 of
four of the configuration cards, so that results for only the
three fully relaxed F- calculations will be passed on to RCN2 and
RCG (see Sec. II-C(f), page 15).
(2) Use of IREL=1 (rather than zero) provides an additional
small attractive potential, which helps to bind negative ions;
this will of course be more helpful in heavy atoms than in
something as light as fluorine.
(3) Numerous attempts were made to make a calculation for
2p43s3d, none of them successful. This is not surprising: In
fluorine, a 3d orbital is essentially hydrogenic, with very little
core penetration; the correlation formulation used in RCN depends
entirely on wavefunction overlap with other orbitals, so that the
correlation potential for 3d is very small. (Physically, 3d may
be bound via polarization of the core, but the correlation
algorithm used here does not adequately mimic polarization).
(4) Final results should be obtained using a value of
CORRF=1 if possible, or if not, then as small a value as will give
convergence. If on early attempts a value CORRF=2 (say) is used
in order to help ensure success, then an estimate of the smallest
possible value of CORRF can be made as follows: For the most
weakly bound orbital, note on the final page of the output listing
the values of EE (eigenvalue) and ECT (in the column following the
column labeled N*RC). Unit decrease in CORRF will decrease the
magnitude of EE by approximately the magnitude of ECT; thus if the
magnitude of EE is only about one-third the magnitude of ECT, then
it is safe to try a new run in which CORRF is decreased by no more
than about one third of a unit--in the present example, from 2.0
to about 1.7.
As an illustration of the sensitivity of Coulomb integrals to
the value of CORRF, in the case of F- 2p43p2, decreasing CORRF
from 2.3 to 1.0 decreased the 2p-3p Coulomb integrals by about
20%; for F- 2p43s3p, a decrease from 2.3 to 1.5 decreased the
inter-subshell integrals by 30 to 50%.
L. Dielectronic recombination calculations
RCN input for making dielectronic-recombination calculations
in RCG requires knowing the kinetic energies of the free electrons
that can be captured into the autoionizing configuration of
interest. This requires making preliminary RCN calculations for
the autoionizing configuration and for the ion configuration(s)
involved to get the kinetic energy (by differencing total binding
energies), as well as figuring out by hand the possible value(s)
of the angular momentum of the free electron. This hand work can
be eliminated and final RCN input constructed automatically by
using the subroutine DIEL of RCN36. To do this, the RCN input
file IN36 is constructed so as to contain only the exit card with
-1 in columns 4-5, and input to DIEL is set up in a separate file
named INDIEL (internal file 12). This latter file contains:
(1) the usual RCN control card;
(2) a card for the ground configuration of the ion (it being
assumed that this is the initial configuration for electron
capture), and one for each excited configuration of the ion that
the captured atom might autoionize into (a maximum of 5 ion
configurations, total);
(3) a card for each of the singly excited configurations
that the doubly excited configuration might decay to radiatively
so as to produce a system stable against autoionization;
(4) a card for the doubly excited (autoionizing)
configuration (program dimensions allow more than one such
configuration, but if more than one is used, the RCG output print
of individual-level autoionization rates must be interpreted with
care and the overall dielectronic-recombination-rate number is
incorrect);
(5) the usual "-1" exit card.
Further sets of cards (2)-(5) for other doubly excited
configurations may be included if desired, provided that in all
sets the radiative-decay configurations have the same parity.
(But unlike normal RCN input, all such cards will be utilized--not
just the cards in front of the first exit card!) Note also that
in this INDIEL file, each configuration card must contain
explicitly any orbital (even though full or empty) that is listed
as other than the final (outermost) orbital on any other
configuration! Also, the value used for NSPECT for the ion
configurations (2) must be different from that used for the "atom"
configurations (3)-(4).
RCN36 will then first call DIEL to find kinetic energies,
determine orbital angular momenta for the free electrons, and set
up complete input for the final RCN run--which will then be
carried out automatically in the normal way.
M. Storage requirements
Memory storage requirements for 20 orbitals and an
integration mesh of 561 points (adequate for n up to about 10) or
1801 points (needed for continuum functions or large n) is, on the
CRAY-1, about as follows (number of 64-bit words, octal):
561 1801
------------ -----------
no QNL QNL no QNL QNL
------ ---- ------ ---
FORTRAN code (2 to 4 instrs. per word) 27K 27K 27K 27K
Utility/library 46K 46K 46K 46K
Data storage 61K 106K 221K 327K
---- ---- ---- ----
Total (excluding I/O buffers 156K 203K 316K 424K
On a Macintosh Centris, the minimum RAM for execution is about 1.5
Mbytes with QNL and 1801-point mesh.
Storage requirements can be reduced in various ways,
depending on the kinds of calculations one is interested in. The
parameter KO can be reduced if one is interested only in atoms
involving fewer than 20 orbitals, and KMSH can be reduced to, say,
521 if one is not interested in continuum or large-n bound
orbitals. If the option IREL=2 is not desired (and, in fact, the
Breit magnetic and retardation corrections seem to provide no
increase in accuracy even for very high Z), then KMSHQ and KOQ can
each be reduced to 1 and routines EBREIT, BRTINT, and S3J can be
discarded. If RCN is used only to provide input to HF8 (IHF=1),
the subroutines POWER, SLI1, RCN3S, S3J0SQ, FCTR, and all routines
from HFPOT on may be discarded. If IHF=1 and IREL > 0, then
subroutine ZETA1 may be discarded as well.
N. Conversion to other computers
Conversion problems to other computers having a FORTRAN 77
compiler should be minor except for the following:
The SCF iteration must be carried out to very tight tolerance
if one wishes to compute meaningful excitation energies by
differencing values of Eav for two configurations, because many
significant figures are lost in this difference (about 6 or 7
significant figures for an actinide). This means that most
calculations must be done with a precision of 9 or more
significant figures. On machines using 60- or 64-bit basic
floating-point word lengths, this is no problem. On VAX or IBM
32-bit machines (about 7 significant figures), it is necessary to
compile using 64-bit floating-point numbers--preferably using, if
available, a large-exponent-range option (10±350 rather than
10±38) such as the VAX G_FLOATING compiler option. This means
using basically double-precision floating-point numbers. To
simplify converting back and forth between CRAY and VAX-type
machines, the following program modifications have been
incorporated, as mentioned earlier:
(1) PROGRAM cards have been included both with and without
file-definition names included, and there have also been included
file-name definitions via OPEN statements. On CRAY and CYBER
machines, the simple PROGRAM card can be commented out and III in
the main program set to 2, which causes the OPEN statements to be
bypassed. On VAX-type computers, the file-definition PROGRAM card
is the one to be commented out, and III set to 1 to define all
file names via OPEN statements. (On VAX machines, III may
alternatively be set to zero, in which case some file names are
set by typing them in interactively.)
(2) In all subroutines there are included IMPLICIT REAL*8(A-
H,O-Z) statements, which may be commented out if necessary for 64-
bit machines.
(3) Generic library subroutine names (e.g., MAX in place of
AMAX1 or DMAX1) have been used so that the compiler will
automatically use the single-precision or double-precision
version, depending on the type of the argument variables. In all
argument lists, constants have been replaced by variable names;
the variable being given a value in a replacement statement such
as
TWO=2.0,
so that in the 32-bit-machine case it will automatically be
converted to double precision.
III. PROGRAM HF8
A. Outline
This is a FORTRAN IV program based on the well-known program
of C. Froese-Fischer [Can. J. Phys. 41, 1895 (1963); Report ANL-
7404 (1968); Comp. Phys. Commun. 1, 151 (1969)]. It has been
extensively modified, to accept input from RCN and with the multi-
configuration option removed, by D. C. Griffin (Thesis, Purdue
University, (1970). Further modifications make possible inclusion
of relativistic terms in the differential equation if IREL > 0
(TASS) and incorporate a new method of stabilizing the SCF
iteration [R. D. Cowan and J. B. Mann, J. Comput. Phys. 16, 160
(1974) or TASS, Eq. (7.27).]
Because RCN contains a built-in Hartree-Fock capability,
program HF8 is not of great interest (and it is in any case not
useable for calculation of continuum or large-n bound functions
because it employs a logarithmic radial mesh that becomes much too
coarse at large radii). Nevertheless, we describe it here in case
one wishes to use it for comparison purposes.
The program consists of a main program and 42 subprograms, of
which only a few of the more important ones will be described.
HFMOD8 is the main program, and does little except read a
control card and call various subroutines.
DATA reads the input information that RCN has written on unit
7, and sets up calculations accordingly.
SCF controls the self-consistent-field iteration for a given
configuration (or for a given LS term of a given configuration).
One iteration cycle consists of two parts: (1) A considerable
number of calculations are made for different orbitals, in an
order that depends on which orbital appears to be farthest from
self consistency; (2) each orbital is recalculated once in the
order from innermost to outermost subshell. (The iteration cycle
in RCN consists of only this second phase, and hence convergence
requires many more overall SCF cycles to reach self consistency;
the total number of orbital calculations is, however,
approximately the same in RCN as in HF8.)
SOLVE controls the iteration on the orbital eigenvalue to
obtain a normalized radial function having positive initial slope
and the correct number of nodes (=n-l-1).
HXWRTP converts the wavefunctions from the HF8 logarithmic
mesh to the linear mesh used by RCN and RCN2, and writes results
on unit 2 in the form required as input to RCN2.
B. Input
Most of the input has already been discussed in the RCN
section of this writeup. Here we need describe only the HF
control card (actually, two cards):
cols format variable normal value
----- ------ -------- ------------
1-10 E10.2 WFTOL 1.E-07
13-15 I3 NITER 15
38-40 F3.1 ACMIN (default=0.2)
43-45 I3 ISCACC 0
48-50 I3 ISEND 0
53-55 I3 IGRANG 0
61-65 F5.0 TIMPM (default=280 sec)
68-70 I3 IPRINT 0
76-80 F5.3 HXFAC 0.95
1-5 I5 NSLV 51
6-10 I5 ITERSL 0
11-15 F5.3 QNRNG 0.5
16-20 F5.3 FACHL 0.65
26-30 I5 IRCN 0
WFTOL is the maximum allowable absolute change in any
wavefunction (at any mesh point) from one SCF cycle to the next
before ending the iteration.
NITER is the maximum allowable number of SCF cycles. (If
exceeded before WFTOL is satisfied, the calculation is ended and
no output written on unit 2 for this case).
ACMIN is the minimum allowed value of the acceleration factor
(amount of trial function included in the trial function for the
next cycle).
If ISCACC=0, the acceleration factor ACC(M) for the mth
orbital will be automatically modified (between the limits ACMIN.LE.
ACC(M).LE.0.994) in an attempt to speed the SCF convergence. (Note
that ACC in HF8 is equal to 1-ALF of RCN.)
ISEND0 deletes portion (1) of the calculation described
under subroutine SCF.
IGRANG.NE.0 excludes the off-diagonal Lagrangian multipliers
eij that enforce orthogonality between orbitals of like l but
different n (and different occupation number).
TIMPM is the maximum computational time (in seconds) allowed
for RCN and HF8 before exiting from HF8 to load RCN2.
If IPRINT.NE.0, eigenvalue-iteration information is printed
(for only the outermost two orbitals, if IPRINT=1).
HXFAC determines the magnitude of the term that modifies the
inhomogeneous differential equation to make it approximately
homogeneous in order to eliminate convergence difficulties (J.
Comput. Phys. paper mentioned above). If HXFAC > 0 and the atom is
less than three-fold ionized, this modification is used for the
outermost two orbitals if they are singly occupied.
IRCN accomplishes the same thing as the variable IZHXBW of
RCN.
The remaining quantities on the second control card deal with
calls of subroutines SOLVE1 and SLVTST (at the end of SCF, if
ITERSL0 and the above HXFAC is in effect for the outermost
orbital) to make a diagnostic calculation of the shape of the
normalization curve.
(Several variables not listed above are read from the control
card, but are no longer used in the code.)
C. Input/output units
Control-card input is via unit 5, and printed output is via
unit 6. Input from RCN is via unit 7, and wavefunction output to
RCN2 is via unit 2. Printed output is in a rather different
format from that of RCN, but is basically the same in scope.
D. Storage requirements
Storage requirements for an integration mesh of 200 points
(561 in HXWRTP) and up to 20 orbitals is, on the CDC 7600 (60-bit
words, octal):
FORTRAN code 22K
Utility/library 32K
Data storage 70K
----
Total 144K (plus I/O buffers)
E. Miscellaneous
If no diagnostic norm curves are to be computed (ITERSL=0),
then subroutines SOLVE1 and SLVTST may be discarded. In any case,
the code sections in SLVTST and HXPOT having to do with microfilm
plotting (involving library subroutine PLOJB) should be deleted or
replaced with whatever analogous plotting routine may be
available.
The program HF8 was designed to handle only inhomogeneous
differential equations, which excludes all configurations for
which there are no exchange terms (namely, all single-subshell
configurations--the most important cases being one-electron atoms,
and s2 configurations of helium-like ions). This is no great
limitation, even if RCN is used in the HX mode, for the following
reasons. (a) For hydrogenic (one-electron) ions, HX gives the
equivalent of Hartree-Fock results; (b) even when nominally using
the HF8 option (IHF=1) for He-like (two-electron) configurations,
RCN writes HX results on tape2 for single-subshell configurations
(1s2, 2s2, 2p2, ..., HX results being identical with HF in these
cases), and makes HF8 calculations only for two-subshell
configurations (1s2s, 1s2p, etc). However, if RCN2 is to be used,
the single-subshell configurations must all come before the two-
subshell configurations, and of course the HX convergence criteria
TOLEND and THRESH must be small.
IV. PROGRAM RCN2
A. Outline
This is a FORTRAN 77 program for the CRAY-1 or CDC CYBER
205 computer, or for VAX, Sun, IBM RISC, or Macintosh and similar
computers. It reads information from the output disk unit 2 of
RCN or HF8, calculates configuration-interaction radial Coulomb
integrals Rk and electric dipole and quadrupole reduced matrix
elements
P(k)ll' = < l || r(k) || l > (k=1 or 2)
or analogous matrix elements of spherical Bessel functions, scales
all energy-level-structure parameters Fk, Gk, Rk, and zeta, and
writes on unit 11 a complete file of input data for making energy-
level and spectrum calculations via program RCG. [Note: For HF
wavefunctions, RCN2 output is useful mainly for center-of-gravity
(not LS-term-dependent) calculations; nominally, RCG assumes c-g
results exclusively.]
The program consists of a main program and nine subroutines.
MAIN reads control cards and calls various subroutines
accordingly.
OVER computes an overlap integral between two specified
radial wavefunctions from the same or from different
configurations.
ZETA2 computes single-configuration or configuration-
interaction spin-orbit parameters [using the simple central-field
formula (3)]. The former are computed by ZETA1 of RCN, and the
latter are usually so small as to be negligible, so in practice
this subroutine is almost never used.
DIP computes electric dipole and quadrupole integrals
P(k)ll' or matrix elements of spherical Bessel functions.
SLI2 computes configuration-interaction radial integrals
Rk(l1l2,l3l4).
G5INP is a master program that calls SLI2 and DIP as
appropriate, and prepares the input file for RCG. (Note: The name
"G5INP" refers to the preparation of input for RCG Mod5, which is
now a misnomer since the current version of RCG is Mod 11.)
S3J calculates the 3-j symbol
( j1 j2 j3Ê)
( m1 m2 m3 )
S3J0SQ calculates values of
( j1 j2 j3 )
( 0 0 0 )
FCTRL calculates the factorial of an argument A for use by
S3J and S3J0SQ.
SBESS evaluates the spherical Bessel function of specified
order for a given radius and wavenumber.
B. Input
Input consists of radial wavefunctions and other information
written on unit 2 (in a file named TAPE2N) by program RCN or by
program HF8, and of one control card for each calculation being
made. The control card is read as a string of 80 BCD characters
at statement 200 of MAIN, and then is decoded according to a
format appropriate to subroutines other than G5INP. The first
three characters (columns 1-3 on the control card) specify the
subroutine to be called and columns 11-20 (format 2I5) specify the
serial numbers of the two configurations from which wavefunctions
are to be selected; the orbitals themselves are specified in
columns 21-30 [format 2(2X,A3) for OVER, ZETA2, and DIP] or
columns 21-40 [format 4(2X,A3) for SLI2]. The main program RCN2
usually is no longer used to call the subroutines OVER, DIP, and
SLI2 directly, but only via G5INP. Hence we shall not describe
these options further, but consider only the case in which the
first 3 characters of the data card are "G5I".
In this case, control is transferred to subroutine G5INP,
which decodes the control card according to a new format
(statement 100):
cols format variable normal value
----- ------ ----------- ------------------------------------
1-5 A3,2X ----- g5inp
6-7 A2 NCK blank (or as desired for RCG input)
8 I1 IOVFACT 0
9-10 I2 NOCET blank (or 1 to produce input for RCE)
11 I1 NSCONF(3,1) 0 (or as desired for RCG input)
12-13 I2 NSCONF(3,2) 0 (or as desired for RCG input)
14-20 F7.4 EAV11 0.0 (or as desired for RCG input)
21 I1 IABG 0 (or as desired for RCG input)
22-49 3A8,A4 OPTION blank (or as desired for RCG input)
50 I1 IQUAD 0 (non-zero for E2 spectra)
51-60 5I2 IFACT 9999999999, 8099808080, 9399939393, etc
61-65 A5 DMIN blank (or as desired for RCG input)
66-70 A5 IPRINT blank (or as desired for RCG input)
71 A1 IENGYD blank (or as desired for RCG input)
72 A1 ISPECC blank (or as desired for RCG input)
73 I1 ICON 2
74 I1 ISLI 2 (0 for more printout)
75 I1 IDIP 9 (0 for plane-wave-Born calcns., 5, 6,
7, or 8 for photoionization calcns.)
76-80 F5.0 ALF blank (0.0)
IOVFACT if non-zero multiplies Rk values or radial multipole
integrals or both by the product of overlap integrals for all
spectator electrons for the subshells included in the RCN2 output,
according as IOVFACT is 1, 2, or greater than 2, respectively.
NOCSET is normally zero, but if not (normally +1), the RCG
input file OUT2ING will be set up to provide input files for RCE.
Any punches in columns 6-7, 22-49, and 61-72 are unused in
RCN2, and are simply transferred unchanged to the same columns of
the RCG input control card; likewise, punches in columns 11, 12-
13, and 21 are transferred unchanged to columns 15 and 19-21. (See
the description of this control card in Sec. IV(4)(A) of the RCG
program writeup). For a modification of these remarks when column
33 contains a number greater than 4, see Sec. IV-F of this writeup
(page 34).
EAV11 is the value desired for the center-of gravity energy
Eav of the first configuration (in units of 1000 cm-1). It merely
shifts the energy scale of all energy levels calculated by RCG.
If IABG > 0, it is a signal that the effective-operator
parameters alpha, beta, gamma are to be included in the RCG
calculation. Values of these parameters cannot easily be computed
theoretically; hence, RCN2 simply leaves room at the proper places
on the single-configuration parameters cards of the RCG input
file, where empirical parameter values can be inserted by hand
(except that the number ALF punched in columns 76-80 of the G5INP
control card will be punched for alpha).
IQUAD (column 50) causes electric-quadrupole radial integrals
to be computed for configurations of the first, second, or both
parities according as IQUAD=1, 2, or 3, respectively; the value of
IQUAD is also transferred unchanged to column 50 of the RCG
control card.
All this provides a means of controlling within RCN2 the
various RCG options in a chained RCN/RCN2/RCG or RCN/HF8/RCN2/RCG
run.
The values of IFACT(5) are converted to floating point and
divided by 100 to provide scale factors FACT(5); if IFACT=01 or
99, FACT is set to 0.001 or 1.00, respectively. The values of
FACT(5) are fudge factors to be applied to the theoretical values
of the parameters Fk(li,li), zetai, Fk(li,lj), Gk(li,lj), and
Rk(lilj,l'il'j), respectively, to give scaled-down parameters for
input to RCG. It is known empirically that computed energy-level
intervals will agree better with experiment if the Coulomb
parameter values are 5 to 30% smaller than theoretical. Values of
FACT of 0.85, 0.95, 0.85, 0.85, 0.85 are assumed by the code if
zeroes are read in. Values of 0.90, 1.00, 0.90, 0.90, 0.90 are about
right for HF calculations on about 5- or 10-fold ionized atoms.
The first and the last three values should be more like 0.80 for
most neutral atoms (except about 0.70 for lanthanides and
actinides), and should be 0.92 to 0.95 for very highly ionized
atoms. (All values should be about 0.05 smaller if HX calculations
are used instead of HF.)
ICON = 1 the RCG-input control and config. cards are not
punched
> 1 the number of subshells set up on the configuration
cards is limited to no more than ICON if possible
ISLI = 0 print maximum SLI2 output
= 1 omit page restore and most printout
= 2 omit all but final punched card image (except that
parameter values are printed unscaled as well as
scaled)
= 3 omit all printout
IDIP = 1 do not punch dipole cards
= 5 configuration-interaction radial matrix elements
between a bound and a continuum configuration are
set to zero if the two configurations have the same
total energy; otherwise, as for IDIP=9
= 6 configuration-interaction matrix elements involving
a continuum electron are set to zero except for
core bound-bound interactions in the case of two
continuum configurations for which the free
electrons have the same angular momenta and kinetic
energies
= 7 values of Rk and dipole integrals in Rydberg series
will be modified appropriately for pseudo-discrete
calculations. [Each Rydberg-series configuration
is given an effective-energy-width weighting
factor DE, which is unity for successive-n discrete
configurations, greater than one for non-
successive-n discrete configurations, and an
effective width in rydbergs for continuum config-
urations. Rk values are weighted by the square
root of delE1 * delE2, and discrete-continuum
dipole integrals are weighted by the square root
of delE2--see the RCG writeup, Sec. XI(B).]
= 8 modifications will automatically be made for simple
photoionization calculations in RCG. [The value of
NSCONF(3,2) on the RCG control card is set to -8,
and all Rk involving a continuum configuration are
set to zero--see the RCG writeup, Sec. XI(A)]
= 9 values of Eav, Rk, and dipole integrals involving
continuum functions will be modified appropriately
for perturbation calculation of autoionization
transition probabilities in program RCG. [The
continuum Eav are changed to large negative values,
and the continuum-continuum Rk and discrete-
continuum dipole integrals are set to zero--see the
RCG writeup, Sec. XII]. The value IDIP=9 can be
used as a universal value for runs not involving
continuum configurations.
C. Calculational procedure
In order for G5INP to properly prepare input decks for RCG,
it is necessary that the pertinent configurations be arranged on
unit 2 in a specific order, and hence that the input configuration
cards for RCN also be arranged in this order:
(a) All configurations of given IZ and ION that are to be
included in one RCG calculation must be arranged in succession.
Usually the lowest-energy configuration is chosen as the first
one; all configurations of this same parity follow, and then come
all configurations of the opposite parity (if any). Within a
given parity, all configurations that are members of a single
Rydberg series (eg, 3p5 3d, 3p5 4d, 3p5 5d,...) should preferably
be placed in succession. Each input configuration card for RCN
should be punched so that all orbitals (other than the outer,
most-weakly-bound, singly occupied orbital) are arranged in order
of increasing n, and for given n in order of increasing l; if
orbitals are not arranged this way, G5INP attempts to rearrange
things so, but the code is not bug-proof. [Note the exception to
this order in the negative-ion example of Sec. II-K, necessitated
by the fact that only the "inner" (ie, first-listed) orbitals can
be held frozen.]
(b) In multi-configuration runs involving excitations out of
inner subshells, RCN2 may incorrectly give zero for certain radial
dipole integrals unless the configurations are arranged in such an
order that the different nl values of the outermost excited
electron first appear in the same order in each parity; for
example, if the even parity configurations are
2s2 2p2
2s2 2p 3p
2s 2p2 3s
2s 2p2 3d
(outer electrons in the order 3p, 3s, 3d), then for the second
parity the order should be
2s 2p2 3p
2s2 2p 3s
2s2 2p 3d .
If the first-parity configuration 2s 2p2 3s is omitted, then the
second-parity order should be
2s 2p2 3p
2s2 2p 3d
2s2 2p 3s .
This caveat can probably be ignored if ICON on the G5INP control
card is set to two.
(c) G5INP will process sets of configurations in groups such
that each group ends when (a) G5INP has already found two parities
for a given ion and encounters on unit 2 the first parity again,
or (b) it encounters a different element or ionization stage. For
example, if A, B, C, D, and E represent five sets of consecutive
configurations, all configurations of a given set belonging to the
same ion and parity, and of the following sort (ION = degree of
ionization):
set Z ION parity
--- -- --- -----------
A 12 9 even
B 12 9 odd
C 12 9 even
D 14 9 even or odd
E 14 7 even or odd
then A and B will be processed together (including calculation of
radial dipole integrals), but C, D, and E will each be processed
individually. If for some reason one had desired that A and B
also be processed individually (or that the set C be processed as
two separate subsets), this could have been accomplished by
separating A and B (or the two subsets of C) by, say, the set E or
by some single dummy configuration with Z12 and/or ION9.
The calculational procedure is as follows:
(1) Disk unit 2 ("tape2n") is searched to find a group of
consecutive configurations of the type described above--all having
the same Z and same ION, and of at most two non-interleaved
parities. (With current dimensions, the maximum number of
configurations in any one group is 90.)
(2) The configurations of the first parity are copied onto
disk unit 31, and those of the second parity (if any) are copied
onto unit 32. (This is done to reduce disk search times after
rewinding in the case of configuration sets D, E, ××× far from the
beginning of the file on disk unit 2.)
(3) All subshells lw that are full (w=4l+2) in all
configurations of the group are ignored. The remaining subshells
in the various configurations are ascertained, and arranged
according to the requirements of RCG.
(4) The RCG control card is "punched" (ie, written on file
11--external name "out2ine"); this card contains the total number
of subshells and the number of configurations of each parity
[NSCONF(2,K)], among other things.
(5) The l and w values are punched for each configuration.
[The configuration label and total binding energy (in units of
1000 cm-1) are also punched, though this information is not used
by RCG.]
(6) The single-configuration parameter values VPAR supplied
by RCN (via disk 2) are rearranged if necessary [see the remark in
Sec. C(a) above], scaled by the factors FACT, and punched. [First
parity only]
(7) Parameter values Rk for all possible configuration
interactions are computed with the aid of calls to SLI2, and
punched. [First parity]
(8) If the value of IQUAD so indicates, values of the
electric quadrupole reduced matrix element P(2)ll' [or of the
appropriate spherical Bessel function, if IGEN (column 33 of the
G5INP control card) ³ 5] are computed via calls to DIP and punched.
[First parity]
(9) If configurations of both parities are present, (6)-(8)
are repeated for the second parity, and then values of the
electric dipole reduced matrix element [or of the spherical Bessel
function] are computed via calls to DIP and punched.
(10) A card with "-99999999." in columns 21-30 is punched to
provide the "end" card for an RCG calculation. (If the value of
NCMAX is non-zero, a similar card with fives instead of nines is
punched first.)
(11) Disk unit 2 is searched to see if there exist
additional configurations. If so, items (2)-(10) are repeated for
each remaining group of configurations. [If the new group of
configurations is identical with the preceding set so far as the
liwi are concerned, then ICTC=1 is punched in column 78 of the RCG
control card and step (5) above omitted, so that RCG will not
waste time repeating the calculation of quantum numbers and
angular matrix elements--see the RCG writeup, SEC. IV(4)(A).]
(12) When unit 2 has been exhausted, a return is made to the
main program, and a new RCN2 control card is read and processed.
(This feature could, for example, be used to run RCG with two
different sets of scale factors by including two G5INP control
cards.) A final "control card" containing a negative number in
columns 8-10 results in an exit from RCN2 (after writing to file
11 an RCG exit card--a card with a negative number in columns 1-
5).
Note: The identification labeling that RCN2 provides on the
configuration-interaction-parameter cards consists of whatever
appears in columns 17-25 of the two RCN configuration-definition
cards involved. For maximum legibility, it is suggested that
these latter cards contain (insofar as possible) the element and
ion stage in columns 11-16 and the configuration label in columns
17-25 (or, even better, in columns 17-24, because of some eight-
character limitations in labeling in RCE).
D. Input/output units
Data input and output are via units 10 and 9 (external names
IN2 and OUT2), respectively. In addition, disk unit 2 (external
name TAPE2N) is used for input wavefunctions from RCN or HF8, and
unit 11 (external name OUT2ING) is used for the output file that
will be the input file for RCG. Disk units 31 and 32 are used for
scratch storage in the manner described earlier.
E. Output
Output includes the ASCII file OUT2ING on unit 11 ready to
be used directly as input to program RCG. Such a file may be used
without change (except for the name change to ING11) or it may be
modified by hand in various obvious ways. For example, the print
options in columns 66-70 of the RCG control card may be modified;
if one wishes to add or delete calculation of magnetic dipole
spectra, that can be done simply by changing column 49
appropriately; if configurations of both parity were included in
the RCN/RCN2 run but one wishes to include only the first parity
in the RCG calculation, it is only necessary to insert zeroes in
columns 16-20 of the control card, and delete all configuration-
definition and parameter-value cards for the second parity, and
remove all electric dipole cards; if one wishes to make the RCG
calculation in the JJ- rather than LS-coupling representation,
column 5 of the control card can be changed from 1 to 2; etc.
Parameter values in file OUT2ING are always in kK (units
of 1000 cm-1). Decimal points are usually omitted to provide an
extra column to obtain an additional significant figure; values
are read in RCG (subroutine ENERGY) with a format such that the
implied decimal point lies between columns 5 and 6 of the 10-digit
parameter field. (Note: The tenth digit is not actually part of
the parameter value, but is rather a code number that indicates
the type of parameter--see Sec. X of the RCG writeup.)
In addition to the file 11 output, all information in this
file is also printed via the output file 9 (OUT2), as is some
additional detail regarding the calculation of the Rk and the
P(k)ll' .
F. Plane-wave-Born calculations in RCG
Input for plane-wave-Born collision-strength calculations
via program RCG is prepared when column 33 of the G5INP control card
of RCN2 is greater than 4. In this case, certain columns of the
control card are interpreted differently from the manner indicated
in Sec. IV-B:
cols format variable normal value
----- ------ -------- -------------------------------
23-25 I3 NBIGKS 41 or blank (default=41)
26-27 I2 NENRGS blank (default=21)
33 I1 IGEN 9 (or as desired for RCG input)
34 I1 IRNQ (default=0)
35 I1 IRXQ (default=IRNQ)
36 I1 IRND (default=1)
37 I1 IRXD (default=IRND)
50 I1 IQUAD
73 I1 ICON 0
75 I1 IDIP 0
After interpretation of the above information, columns 22-29 are
in effect reset to blanks, and then columns 22-50 transferred
directly on to the RCG control card just as when column 33 is less
than 5; ICON and IDIP are also ultimately reset to zero.
The amount of printed output in RCG for IGEN > 4 is smaller
the larger the value of IGEN; the value IGEN=9 is recommended. The
effect within RCN2 is the same for any value IGEN > 4, and is to
cause matrix element
< l || jt(Kr) C(t) || l' >
of the spherical Bessel function jt(Kr) to be computed in DIP
instead of the electric multipole reduced matrix element
< l || rt C(t) || l' > ;
see TASS, Secs. 18-12 and 18-13 for details. Calculations will be
made for
t = IRNQ, IRNQ+2, ... , IRXQ
in the case of parity-conserving excitations (called for by
IQUAD0 in the usual fashion), and/or for
t = IRND, IRND+2, ... , IRXD
in the case of parity-changing excitations, at NBIGKS different
values of the momentum transfer K. The values of IRNQ and IRXQ
must be even integers covering the range of values of t needed
for all parity-conserving excitations included in the present
calculation, as specified by NCK(1) [default=1 when IGEN > 4] and
NCK(2); similarly, ICND and IRXD are odd integers covering the
range needed for all parity-changing excitations. [Note: For
intra-configuration excitations, calculations are made
(incorrectly in some cases, just as for electric quadrupole
radiative transitions) for a given partially filled subshell only
if there exists no other less-tightly-bound, non-s, partially
occupied orbital.]
The values of K are equally spaced on a logarithmic scale,
covering an energy-transfer range from 10-3 Ry to 4.4*XMAX*ENMAX,
where ENMAX is the difference between the highest and lowest
values of Eav [or is the value of VPAR(2) if there is only one
configuration present]. Values of collision strength are to be
computed in RCG at NERGS values of X=E/(delE) on a logarithmic mesh
from XMIN to XMAX, where E is the kinetic energy of the impacting
electron, DE is the excitation energy, and
1.01 if ICON=0
1.1 if ICON=1
XMIN = ICON if ICON=2 to 8
10 if ICON=9
100 if IDIP=0
20 if IDIP=1
XMAX = 100*IDIP if IDIP=2 to 8
1000 if IDIP=9
G. Photoionization and autoionization calculations in RCG
Calculation of photoionization cross sections can be carried
out in RCG in various ways. The value of IDIP in column 75 of the
RCN2 G5INP control card needs to be chosen appropriate to the
method to be used in RCG. In one method (appropriate only if all
configuration interactions involving continuum configurations may
be neglected), IDIP should be eight. In another method (in which
all interactions are to be retained, with no necessity for
handwork in the preparation of input to RCG), IDIP should be equal
to seven; the kinetic energies of the free electron in the various
continuum configurations then need to be chosen judiciously, and
RCN2 will modify the various Rk and radial multipole integrals in
a manner appropriate to the energy spacings between successive
configurations of each Rydberg series.
If detailed autoionization calculations (by perturbation
methods) are to be made in RCG, then IDIP should be nine. In this
case, RCN2 will modify Eav for continuum configurations to
appropriate large negative values, and will set to zero all
continuum-continuum Rk and all radial multipole integrals
involving a continuum configuration.
See Sec. IVB above--for further details, see the RCG program
writeup.
H. Storage requirements
Storage requirements for up to 90 configurations of given IZ
and ION, 20 orbitals per configuration (so far as the information
written on unit 2 is concerned), and 561 or 1801 mesh points are,
for the CRAY-1, about as follows (number of 64-bit words, octal):
FORTRAN code (2 to 4 instructions/word) 16K 16K
Utility/library 46K 46K
Data storage 130K 234K
---- ----
Total (excluding I/O buffer) 214K 320K
On a Macintosh Centris, execution requires a minimum RAM of about
1.5 Mbytes.
I. Conversion to other computers
Conversion problems to other computers should be minor,
in the same manner discussed for program RCN36 (Sec. II-N).
Except for the calculation of values of delEav, double-precision
calculations are probably not really necessary, but floating-
point variables have to be defined consistently with RCN because
of the binary information passed from RCN to RCN2 via TAPE2N.)
If plane-wave-Born calculations are of no interest,
subroutine SBESS can be deleted and the dimension KBGKS reduced to
unity, thus reducing data storage requirements by about 14K octal
words.
V. PROGRAM USAGE AND EXAMPLE
A. Execution
At Los ALamos, an RCN/RCN2 calculational session might go as
follows:
(1) Assuming that one is going to be running on a CRAY, get
RCN and RCN2 executable files, and sample IN36 and IN2 input
files, from the common file system (CFS): These are present in
the directory /045706 with names rcn.out, rcn2.out, etc., and,
for rcg11 runs, rcg.out, tape72, tape73, and tape74.
(2) Edit any desired changes into the RCN control card (eg,
change to desired values of IREL, CORRF, IW6, etc.).
(3) Following the control card, type in the desired
configuration cards, followed by an exit card (-1 in columns 4-5).
(4) Make any desired changes in the RCN2 G5INP control card.
(5) Execute RCN and then RCN2.
(6) Ship desired output (OUT36 and OUT2) to the printer,
save any desired files on the common file system, and destroy
unwanted files (such as TAPE2N and TAPE4). The name of the RCN2
output file OUT2ING can be changed to ING11, ready for use as
input to an RCG calculation.
The source programs rcn.f, rcn2.f, and rcg.f are available on
the cfs, and are also available by anonymous ftp:
The three source files (SUN versions) and various sample input data
files have been placed in a public ftp directory
ftp/pub/cowan
on the Los Alamos t4 network, and can be accessed by anyone
having an FTP facility, in the following way:
type ftp t4.lanl.gov
When asked for sign-on name, use anonymous
(with no blank spaces, only a return after the word "anonymous",)
and for password use your e-mail address.
Then type cd pub/cowan
ls (to list file names)
and get each file in turn by typing
get (file name)
or type mget *
and then answer y for each file presented by the interactive query.
Use control-D or bye to exit from ftp.
For use on a CRAY, VAX, or IBM, in each of the three programs
modify the timing routine SUBROUTINE SECONDS by commenting out the
SUN section and uncommenting the appropriate section.
For a first RCG calculation, use ing11k (renamed ing11)
as input in order to calculate binary files TAPE72, TAPE73, and TAPE74
for subsequent RCG calculations; this input file contains all cfp
decks that can be used in RCG with the dimensions provided. The file
CFP includes additional cfp decks (for f5, f6, f7, f8, f9, and f10),
but these can be used in RCG only if numerous dimensions are increased
appropriately, as described by comment cards in the RCG source
program, lines 75 to 95; the file rcglg.f is such a large-dimension
version.
B. Sample input and output
Sample RCN36 and RCN2 input files, and output from execution
of the two programs follows.
Sample RCN input file, in36
333 9 2 10 0.2 5.e-08 1.e-11-2 190 1.0 0.65 0.0 0.0 -6
1 1H I 1s 1s
19 6K VI 3s2 3p2 3s2 3p2
19 6K VI 3p4 3p4
19 6K VI 3p 3d 3s2 3p 3d
-1
29 1Cu I 1s2 4s 1s2 3d10 4s
29 1Cu I 1s 4s .1p 1s 3d10 4s 99p 0.1
29 1Cu I 1s 4s 1.p 1s 3d10 4s 99p 1.0
-1
10 1Ne I 2p6 2p6
10 1Ne I 2p5 3d 2p5 3d
10 1Ne I 2p5 4d 2p5 4d
10 1Ne I 2p5 6d 2p5 6d
10 1Ne I 2p5 8d 2p5 8d
10 1Ne I 2p5 .1d 2p5 99d 0.1
10 1Ne I 2p5 .2d 2p5 99d 0.2
10 1Ne I 2p5 1.d 2p5 99d 1.0
10 1Ne I 2p5 2.d 2p5 99d 2.0
-1
The above control card is for long output print (for debugging
purposes, for example); for nornal output, use
2 9 2 10 0.2 5.e-08 1.e-11-2 190 1.0 0.65 0.0 0.0 -6
Sample RCN2 input file, in2
g5inp 000 0.0000 01 9099909090 0.00 07229
-1
(The "1" on the control card deletes printing in RCG of
eigenvectors in the JJ-coupling representation, and the scale
factors of "90" are appropriate for 5- to 10-fold ionized atoms.)
C. Command-file methods
As an alternative to launching each program one at a time,
one can use a command file to run each program in turn, with the
input files contained within the command file.
C1. UNIX command file for running RCN/RCN2/RCG
A sample command file for running a three-configuration
problem in 5-fold ionized potassium on UNIX machines, including
execution of RCG as well as of RCN and RCN2, is the following:
#!/bin/csh -f
rm in36 in2 inputg ing11
cat << eod36 > in36
2 -9 2 10 0.2 5.e-08 1.e-11-2 090 1.0 0.65 0.0 0.0 -6
19 6K VI 3s2 3p2 3s2 3p2
19 6K VI 3p4 3p4
19 6K VI 3p 3d 3s2 3p 3d
-1
1 1H I 1s 1s
29 1Cu I 1s2 4s 1s2 3d10 4s
29 1Cu I 1s 4s .1p 1s 3d10 4s 99p 0.1
29 1Cu I 1s 4s 1.p 1s 3d10 4s 99p 1.0
-1
eod36
rcn36.out
cat << eod2 > in2
g5inp 000 0.0000 00 9099909090 0.00 07229
-1
eod2
rcn2.out
cat << eodg > inputg
3 10e-350e05 000005 10. 0 5.0 2.0 1.0 0.5 0.2
0 0000000000 1000.0000
eodg
cat inputg out2ing >> ing11
rcg11.out
cat in36 out36 in2 out2 ing11 outg11 >> out$1
Let us suppose that this command file is named "cosmos",
for example. Any desired input changes can be edited by hand into
this file, and then the command
chmod 777 cosmos
will probably have to be given before it can be executed. If it
is launched by the command
cosmos .KVI
then the final combined output file will be named
out.KVI
C2. UNIX command file for a dielectronic-recombination run, using
the DIEL feature:
#!/bin/csh -f
rm indiel in36 in2 inputg ing11
cat << eoddiel > indiel
2 -9 2 10 0.2 5.e-08 1.e-11-2 090 1.0 0.65 0.0 0.0 -6
34 26Se+25 s2 p5 2s2 2p5
34 25se+24 s2 p5 9i 2s2 2p5 9i
34 25se+24 sp6 9i 2s 2p6 9i
-1
eoddiel
cat << eod36 > in36
-1
eod36
rcn36.out
cat << eod2 > in2
g5inp 000 0.0000 00 9099909090 0.00 07229
-1
eod2
rcn2.out
cat << eodg > inputg
3 10e-350e05 000005 10. 0 5.0 2.0 1.0 0.5 0.2
0 0000000000 1000.0000
eodg
cat inputg out2ing >> ing11
rcg11.out
cat in36 out36 in2 out2 ing11 outg11 >> out$1
C3. Command file for VMS operating systems analogous to C1:
$create in36.dat
2 -9 2 10 0.2 5.e-08 1.e-11-2 090 1.0 0.65 0.0 0.0 -6
19 6K VI 3s2 3p2 3s2 3p2
19 6K VI 3p4 3p4
19 6K VI 3p 3d 3s2 3p 3d
-1
1 1H I 1s 1s
29 1Cu I 1s2 4s 1s2 3d10 4s
29 1Cu I 1s 4s .1p 1s 3d10 4s 99p 0.1
29 1Cu I 1s 4s 1.p 1s 3d10 4s 99p 1.0
-1
$run rcn36.exe
$create in2.dat
g5inp 000 0.0000 00 9099909090 0.00 07229
-1
$run rcn2.exe
$create inputg.dat
3 10e-350e05 000005 10. 0 5.0 2.0 1.0 0.5 0.2
0 0000000000 1000.0000
$copy inputg.dat,out2ing.dat ing11.dat
$run rcg11.exe
$copy in36.dat,out36.dat,in2.dat,out2.dat,ing11.dat,outg11.dat 'P1'.dat
If this file is named "cosmos.com"
and launched via
@cosmos KVI
then the combined output file will be named KVI.dat
D. Sample monitor screen output
D1. Output from RCN run for K VI
SCF iteration information written in subroutine rcn, formats 37 and 55;
Eav (in rydbergs) and Coulomb and spin-orbit radial integrals (in units of
1000/cm) written in subroutine rcn3s, format 58; times printed in subroutine
rcn, format 85 (for a Macintosh Centris 650).
it time delta idel kut itp 1s 2s 2p 3s 3p
2. 2. 6. 2. 2.
1 1.57 4.744663 141 0 1 0.40 0.00 0.00 0.00 0.00
2 2.70 2.327262 144 0 1 0.40 0.00 0.00 0.00 0.00
3 3.85 0.790523 146 0 1 0.50 0.00 0.00 0.00 0.00
4 4.95 0.188284 147 0 2 0.62 0.62 0.62 0.62 0.62
5 6.80 -0.031513 117 -1 2 0.62 0.62 0.62 0.62 0.62
6 8.12 0.008342 252 -1 3 0.62 0.94 0.94 0.94 0.94
7 9.37 0.002091 127 -1 4 0.42 0.94 0.94 0.94 0.94
8 10.58 -0.000486 128 -1 5 0.63 0.94 0.94 0.94 0.94
9 11.75 0.000110 64 -1 6 0.94 1.00 0.63 1.00 1.00
10 12.93 -0.000012 168 -1 7 0.94 1.00 0.63 0.67 0.67
11 14.05 -0.000003 202 -1 8 0.94 1.00 0.94 1.00 0.67
12 15.12 0.000000 164 -1 9 0.94 1.00 0.94 1.00 0.67
13 16.17 0.000000 196 -1 10 0.94 1.00 1.00 1.00 1.00
14 17.20 0.000000 199 -1 11 0.94 1.00 1.00 1.00 1.00
Eav & pars 3 -1187.7217 0 84.5526 1 1.7868 2
finished K VI 3p2 at t(run)= 26.57, t(job)= 26.57 seconds
it time delta idel kut itp 1s 2s 2p 3p
2. 2. 6. 4.
1 0.93 -0.187125 172 0 1 0.40 0.00 0.00 0.00
2 1.57 -0.088873 173 0 1 0.40 0.00 0.00 0.00
3 3.07 0.012388 112 -1 2 0.50 0.50 0.50 0.50
4 4.07 0.030905 172 -1 3 0.75 0.75 0.75 0.75
5 5.10 0.003080 248 -1 4 0.80 0.80 0.80 0.80
6 6.05 0.000440 251 -1 5 0.80 0.80 0.80 0.80
7 6.97 0.000077 251 -1 6 0.80 0.80 0.80 0.80
8 7.87 0.000014 252 -1 7 0.80 0.80 0.80 0.80
9 8.70 0.000003 252 -1 8 0.80 0.80 0.80 0.80
10 9.53 0.000000 253 -1 9 0.80 0.80 0.80 0.80
11 10.37 0.000000 253 -1 10 0.80 0.80 0.80 0.80
12 11.20 0.000000 253 -1 11 0.80 0.80 0.80 0.80
Eav & pars 3 -1184.5862 0 84.1596 1 1.7842 2
finished K VI 3p4 at t(run)= 14.50, t(job)= 41.07 seconds
it time delta idel kut itp 1s 2s 2p 3s 3p 3d
2. 2. 6. 2. 1. 1.
1 1.52 -0.089080 261 0 1 0.40 0.00 0.00 0.00 0.00 0.00
2 2.42 -0.050812 262 0 1 0.40 0.00 0.00 0.00 0.00 0.00
3 4.78 0.045897 170 -1 2 0.50 0.50 0.50 0.50 0.50 0.50
4 6.45 0.032785 171 -1 3 0.75 0.75 0.75 0.75 0.75 0.75
5 8.12 0.004219 254 -1 4 0.75 1.00 0.75 1.00 1.00 1.00
6 9.65 -0.000521 116 -1 5 1.00 1.00 1.00 1.00 1.00 1.00
7 11.13 0.000177 127 -1 6 1.00 1.00 1.00 1.00 1.00 1.00
8 12.63 -0.000039 129 -1 7 1.00 0.67 0.67 0.67 0.67 0.67
9 14.12 -0.000005 129 -1 8 0.67 0.67 0.67 0.67 0.67 0.67
10 15.47 -0.000001 128 -1 9 1.00 0.67 0.67 0.67 0.67 0.67
11 16.83 0.000000 122 -1 10 1.00 1.00 0.67 0.67 0.67 0.67
12 18.18 0.000000 197 -1 11 1.00 1.00 0.44 0.67 0.67 0.44
Eav & pars 6 -1185.6150 0 1.8036 2 0.0893 2 79.7522 3 98.1593 4
61.2455 4
finished K VI 3p 3d at t(run)= 29.77, t(job)= 70.83 seconds
STOP (normal exit)
D2. Output from RCN diel run for Se+24
it time delta idel kut itp 1s 2s 2p
2. 2. 5.
1 0.75 7.676686 112 0 1 0.40 0.00 0.00
2 1.25 4.506158 113 0 1 0.40 0.00 0.00
3 1.68 2.125476 118 0 1 0.50 0.00 0.00
4 2.08 0.726287 124 0 1 0.62 0.00 0.00
5 2.63 0.151054 127 -1 2 0.78 0.78 0.78
6 3.15 -0.008178 89 -1 3 0.52 0.78 0.52
7 3.63 -0.003905 89 -1 4 0.78 0.78 0.78
8 4.08 -0.000538 88 -1 5 0.78 1.00 0.78
9 4.52 -0.000080 88 -1 6 1.00 1.00 0.78
10 4.95 -0.000013 87 -1 7 1.00 1.00 0.78
11 5.37 -0.000002 86 -1 8 1.00 1.00 0.78
12 5.75 0.000000 85 -1 9 1.00 1.00 1.00
13 6.15 0.000000 88 -1 10 1.00 1.00 1.00
14 6.53 0.000000 92 -1 11 1.00 1.00 1.00
Eav & pars 2 -3925.0252 0232.7731 2
finished Se+25 s2 p5 at t(run)= 8.25, t(job)= 8.25 seconds
it time delta idel kut itp 1s 2s 2p 9i
2. 1. 6. 1.
1 0.58 2.000002 372 0 1 0.40 0.00 0.00 0.00
2 1.32 1.200001 372 0 1 0.40 0.00 0.00 0.00
3 1.75 0.600001 372 0 1 0.50 0.00 0.00 0.00
4 2.73 0.225000 372 -1 2 0.62 0.62 0.62 0.62
5 3.68 -0.001733 82 -1 3 0.62 0.94 0.94 0.42
6 4.37 -0.001180 279 -1 4 0.94 0.94 0.94 0.63
7 5.02 -0.000660 279 -1 5 0.94 0.94 0.94 0.94
8 5.60 -0.000041 279 -1 6 0.94 0.94 0.94 0.94
9 6.20 -0.000003 279 -1 7 0.94 0.94 0.94 0.94
10 6.78 0.000000 279 -1 8 0.94 0.94 0.94 0.94
11 7.37 0.000000 279 -1 9 0.94 0.94 0.94 0.94
Eav & pars 3 -3918.1048 0 0.0120 2 0.0001 4
finished Se+24 sp6 9i at t(run)= 10.00, t(job)= 18.25 seconds
**********************************************************
* The above two calculations are made to obtain the *
* kinetic energy of the captured electron, then the *
* following new file in36 is constructed for an *
* automatic second RCN calculation, using 99 for the *
* principal quantum number of a free electron, and *
* the kinetic energy 6.9204 Ry determined above. *
**********************************************************
2 -5 2 10 1.0 5.e-08 1.e-11-2 190 1.0 0.65 0.0 0.00 -6
34 25Se+24 s2 p5 9i 2s2 2p5 9i
34 25Se+24 sp6 9i 2s 2p6 9i
34 25Se+24a6.9204h 2s2 2p5 99h 6.9204
34 25Se+24a6.9204k 2s2 2p5 99k 6.9204
-1
*****************************************
* Monitor-screen output (continued) *
*****************************************
it time delta idel kut itp 1s 2s 2p 9i
2. 2. 5. 1.
1 1.20 6.956860 108 0 1 0.40 0.00 0.00 0.00
2 2.32 4.073497 109 0 1 0.40 0.00 0.00 0.00
3 3.45 1.904221 114 0 1 0.50 0.00 0.00 0.00
4 4.48 0.646166 121 0 1 0.62 0.00 0.00 0.00
5 6.02 0.128668 125 -1 2 0.78 0.78 0.78 0.78
6 7.47 -0.007808 89 -1 3 0.52 0.52 0.52 0.52
7 8.55 -0.004585 91 -1 4 0.78 0.78 0.78 0.78
8 9.57 -0.000778 85 -1 5 0.78 0.78 0.78 1.00
9 10.58 -0.000106 78 -1 6 0.78 0.78 0.78 1.00
10 11.57 -0.000017 61 -1 7 0.52 1.00 0.78 1.00
11 12.52 0.000000 90 -1 8 0.78 1.00 0.78 0.67
12 13.43 0.000000 87 -1 9 0.78 1.00 1.00 1.00
13 14.35 0.000000 75 -1 10 0.78 1.00 1.00 1.00
Eav & pars 6 -3932.7436 0232.7731 2 0.0120 2 0.5703 3 0.0001 4
0.0001 4
finished Se+24 s2 p5 9i at t(run)= 17.63, t(job)= 17.63 seconds
it time delta idel kut itp 1s 2s 2p 9i
2. 1. 6. 1.
1 0.82 0.067759 91 0 1 0.40 0.00 0.00 0.00
2 1.83 0.116740 87 0 1 0.40 0.00 0.00 0.00
3 3.07 0.056327 88 -1 2 0.50 0.50 0.50 0.50
4 4.18 -0.007341 78 -1 3 0.75 0.75 0.75 0.75
5 5.23 -0.001129 83 -1 4 0.75 1.00 1.00 1.00
6 6.23 0.000142 91 -1 5 1.00 1.00 1.00 1.00
7 7.22 -0.000020 96 -1 6 1.00 1.00 1.00 1.00
8 8.17 0.000002 98 -1 7 0.67 1.00 1.00 0.67
9 9.10 0.000000 56 -1 8 1.00 1.00 1.00 1.00
10 10.03 0.000000 88 -1 9 0.67 1.00 1.00 0.67
11 10.95 0.000000 99 -1 10 0.67 1.00 1.00 0.67
Eav & pars 3 -3918.1048 0 0.0120 2 0.0001 4
finished Se+24 sp6 9i at t(run)= 14.23, t(job)= 31.87 seconds
it time delta idel kut itp 1s 2s 2p 99h
2. 2. 5. 1.
1 0.67 1.573332 218 0 1 0.40 0.00 0.00 0.00
2 1.30 0.943982 218 0 1 0.40 0.00 0.00 0.00
3 2.47 0.472029 218 -1 2 0.50 0.50 0.50 1.00
4 3.63 -0.010638 86 -1 3 0.75 0.33 0.33 1.00
5 4.73 -0.009338 90 -1 4 0.75 0.50 0.50 1.00
6 5.83 -0.006180 90 -1 5 0.50 0.75 0.75 1.00
7 6.87 -0.000895 92 -1 6 0.75 0.75 0.75 1.00
8 7.90 -0.000172 90 -1 7 1.00 1.00 0.75 1.00
9 8.93 -0.000027 84 -1 8 1.00 1.00 0.75 1.00
10 9.95 -0.000007 88 -1 9 1.00 1.00 1.00 1.00
11 10.93 0.000001 93 -1 10 1.00 1.00 1.00 1.00
12 11.90 0.000000 99 -1 11 1.00 1.00 1.00 1.00
13 12.87 0.000000 106 -1 12 1.00 1.00 1.00 1.00
Eav & pars 6 -3918.1048 0232.7731 2 0.0000 2 0.0000 3 0.0000 4
0.0000 4
finished Se+24a6.9204h at t(run)= 15.63, t(job)= 47.50 seconds
it time delta idel kut itp 1s 2s 2p 99k
2. 2. 5. 1.
1 1.17********** 1 -1 2 0.40 0.40 0.40 1.00
2 2.37 0.016018 77 -1 2 0.40 0.40 0.40 1.00
3 3.47 0.011961 86 -1 3 0.40 0.60 0.60 1.00
4 4.57 0.005186 85 -1 4 0.27 0.90 0.90 1.00
5 5.65 0.000943 36 -1 5 0.40 0.90 0.90 1.00
6 6.70 0.000392 31 -1 6 0.60 0.90 0.90 1.00
7 7.77 0.000189 33 -1 7 0.90 1.00 0.90 1.00
8 8.77 -0.000051 43 -1 8 1.00 1.00 1.00 1.00
9 9.75 0.000007 44 -1 9 1.00 0.67 1.00 1.00
10 10.75 -0.000001 43 -1 10 1.00 0.67 0.67 1.00
11 11.73 0.000000 35 -1 11 1.00 1.00 1.00 1.00
12 12.70 0.000000 52 -1 12 0.67 1.00 1.00 1.00
Eav & pars 6 -3918.1048 0232.7731 2 0.0000 2 0.0000 3 0.0000 4
0.0000 4
finished Se+24a6.9204k at t(run)= 15.43, t(job)= 62.93 seconds
STOP (normal exit)