327
doumalofMolecultzrS~ture,12O(1986)327-336 THEOCHEM E&e&r
Science Publishers’ B_V., Amsterdam
SIKPLE
ATOMIC
M.
-
Printed in The Netherlands
MODELS
BERRONDO
lnstituto
de
Ffsica,
Cuernavaca,
Her.,
U.N.A.M..
Aptdo
Postal
139-B,
H&xico
62190,
ABSTRACT We present a comparison between different models of atomic structure, based on functionals of the density and simple model potentials, as well as en improvement of the minimal ST0 basis.
INTRODUCTION
1.
The vels
simplest
for
view,
the
this
atomic
model
is
non-relativistic
is
far
from
Bohr
model,
hydrogen
atom.
trivial1
The
one
which From
gives the
dimensional
the
correct
semiclassical
energy point
quantization
leof
condition
(1.1) becomes
exact
points
can
comes
exact
when
where
is
the
equation.
original
to
of
contour,
For
variable2
radial The
in the
r=ex
quantum
only so
integration
infinity
asymptotically.
change
nr
original
be deformed
Langer’s
dial
the
the
result
the
the
number,
(1.2)
complex
Coulomb
gives
singularities
contour
case,
surrounding plane,
radial
counting in
this
is
exact,
since
we have
the
turning
WKB theory
a radial
be-
equation,
and
condition:
the
number
integrand and
of
are
gives
nodes
of
contained
the
the
ra-
inside
quantization
the con-
dition:
(1.3)
Taking If
Bohr’s
angular
we now turn
one-electron
our
quantum attention
number to
k as the
k= x+1,
radial
it
Schradinger
atom:
016S1280/86/$03.30 01985
starts
ElsevierSciencePublishers B.V.
at
k=l.
equation
for
the
323
(1.4) we see The
that
It
has
behaviour
at
two
regular
these
two
singular
points
at
the
origin
and
at
infinity.
points:
(1.5)
gives
the
exact
nodeless
Matching
solutions.
the
asymptotic
conditions:
(1.6)
determines
their
states
be understood
can
tion.
This
example
ferential re
the
namely,
the having
are
Fock
model 4y5.
due
Its
the
and
lent
starting
serts
that
also
valid
as well
for as
of
more
the
singularities
general
cusp-like
of
is
oroital
conditions
field
of
net
attraction,
in
the
atomic
and a-@ for
dealing
virial
into
account.
in
an of
excited condiof
the
difwhe-
equations3, at
the
origin,be-
effects
This Thus
becomes the
6
case,
spin
also
The
exchange the
potential case:
with
theory term
in
antiparallel
important acting
on
the
in
orbital
number 9
in
asstate,
variational
Hartree-Fock
the
ground
imbalance
between
accounts
correlation
when
an exceltheorem
the
as is
porepul-
variational
constitute
perturbation-like
Hartree-Fock
while
the
per
resulting
an average
Brillouin’s
interact
Hartree-
spin-orbital
The
fulfills
principle.
the
one
and
orbitals
do not in
exclusion
function.
calculations5.
particularly
exchange
antiparallel
.
It
ingredients,
excellence:
attraction
Hartree-Fock
both in
wave
nuclear
configurations
drawback
Pauli’s
par
We associate
N-particle
sophisticated
two essential
and
known.
the
The
simplification
spin
well
are
model
interaction.
excitation
parallel
the
with
more
correlation
large.
are
theorem.
for
a great
the
virtues
interelectronic
the
there
contained
The main
well
atoms,
a superposition
single
this
many-electron
main
point
calculations.
very
both
hence
to
principle
is
of
instead is
vanishes
the
is
a central
indeed
electron,
d-a
importance
shows
condition,
case
They
tential
in
important.
For
and
This
The nodal behaviour for the n =O). r terms of the (weighed) orthogonality
(with
simply
clearly
equation. asymptotic
come very
sion
eigenvalues
is of
not
very taken
electrons
Hartree-Fock
N
Shell bitals
models and
such
assumes
and the X, model 7 starts
Hartree-Fock
as
each
that
electron
moves in an average
An alternative
approach
is
to view
varying
density,
as
in the Thomas-Fermi
to
charge
include
the charge This
exchange
consists
density,
taking
expression
the place
of
tential
( and modifications
in the orbitals’
In any event, of
dealing
inclusion
of
garding
Orbital
density
results Slater
exclusively,
for
of
view,
the
orbitals
as a functional
theory, to give
of
point.
used7 since
in
this
a non-local
po-
in which for
wave functions
too awkward,
restrictive,
inclusion
of
self-consistent,
while
(with
particularly
constraints
the
the use of re-
imposed by
this
without
depends
potential
3 contains of
such as Hartree-Fock
potential
the orbital?.
improvement (STO)
are
way
particles. into
section
to be the most satisfactory
to be too
effective
equations while
regarding
out
N-particle
instance)
and the proper
number of
and models
has proven
proves
the one-particle
linear
turns
10
modification
as the starting
in Hartree-Fock
in practice.
can be devided
to
type
energy
finite
models
matrix,
rise
mer point
is a prescribed In section
the
;tlinimal
latter.
basis
increasing
on the density
which
the number of
or
function,
2 we present
Section
sets,
and
gi-
the
4 includes modifies
the
forsome
the
parameters.
DENSITY FUNCTlONALS The total
matrix. matrix higher
energy
of
the atom can be calculated
In the Hartree-Fock is enough
y (1,2)
to the fact order
that
the
density
approximation, to calculate
density
matrices
matrix
are
all is
knowledge the physical
assumed
expressed
from the second
as
to
be
of
the first quantities.
idempotent.
(antisymmetrized)
variation of the total energy with respect one. In fact, 11,12 matrix to the two constraints of idempotency: , subject
the first sity
factors
in which
ving
2.
correlation
and
gas
field. a slowly
) have been extensively
and thus
orbitals
structure
the kinetic
energy
or-
equations.
atomic
density
antisymmetry
matrix
the use of
with
the charge
X &,
term appearing
on the density
electron
thereof
gas with
model 8.9 . Dirac’s
the exchange
the homogeneous
the exchange
term depends
electrostatic
the atom as an electron
in writing
from electron
order
density
order
density
This
is due
Hence all products
of
to the den-
(2.1) and
330
(2.2) gives
the correct Since
equations.
the kinetic
energy
charge
density
does
bitals
is very
important
formation
for
sity. for
even
the ground
This the
if
problem
does
term here
part
of
sity. of
is
it
is
The remaining
field
approximated density
In the atomic
thesis
the orin-
to be monotonically term
in the Thomas-
is very
picture,
attraction
which,
where
far
from satisof
the den-
the expression
contribution
as functionals the kinetic
is
repulsion,
The dominant given
in terms
a substantial
by an average
account
in the Coulomb part, numerical
different. indeed,
interelectronic
pieces
well
of
and this
on the gradient
is entirely
and correlation
Their
the
one.
the
included
form for
for
charge
den-
the correction
and the deviation
from an
is small
can be
of
the density.
energy
in the case
of
and they
a slowly
varying
by:
case
function in this
nuclear
out energy
terms depending in the orbital
structure energy,
the density
exchange
‘T-
creasing
turns
produced
reasonably
is given
The nodal
by the Coulomb repulsion
behaviour.
The functional
of
operator,
the kinetic
The kinetic
the situation
Regarding
the self-interaction
average
of
which
atoms.
the correct
energy,
given
of
correction
is
density.
purpose.
is a functional
the attractive
the charge
this
density,
not appear
energy
For the potential
of
state
which
we include
kinetic
for
by a differential
in the computation
in the charge
Fermi epproximation, factory
represented
not suffice
is erased
decreasing
is
CrcW
however, whose
case
is
=
the
(2.3) radial
logarithm to evaluate
y c,, 2)
c
density
is almost T hW+
behaves as a monotonically 13,14 . A more realistic
linear
assusIng
a density
matrix
of
dehypo-
the form
‘I[%) (2.4)
where %(rl is almost
1 inear.
The kinetic
energy
then
turns
out
to be ‘5:
(2.5)
331
written
in terms of
The expression
the density
(2.5)
is
ken as a correction
precisely
to the
the one found
free
electron
gas
16
by Weis&icker
Eq.(2.3)
choosing
.
It can be ta-
a different
coeffi-
cient:
(2.7) as suggested for
by Ki rzhnits
al 1 the atoms,
trends
17
the main value
and the asymptotic
Let
us next
expression
look
obtained
. Since
at
these of
behaviour’ the exchange
from the electron
approximations
these for
expressions
large
energy gas
are
N,
is
rather
not very
to obtain
accurate global
than specific
as a functional 10 is :
of
cases.
the density.
The
(2.8) with&
=l.
This
The proper and Kohn
term overestimates
value E
the variation
of
a
turns
the exchange
out
effects for neutral atoms 18 to be intermediate between the original
18-20
.
&=I,
Sham’s value 19 &=2/3, and decreases with N. A justification for 18,21 22,23 of d with N can be given by modelling the Fermi hole .
The correlation
function
can be approximated
as:
(2.9) ,yielding
a value
of atwhich
depends
on the number of&
electrons
N,
as:
(2.10) A different use Eq.(2.4)
starting for
point
the atomic
in the calculation
density
matrix,
of
the exchange
energy
is
to
with (2.11)
where
‘I(r)
sults
in:
is almost
constant
14
. The crudest
approximation
in this
case
re-
(2.12) while
the correction
depends
on the density
gradient,
since
(2.13)
(2.14) yielding
a fairly
accurate
expression
for
the exchange
energy
14
.
ATOMIC POTENTIALS.
3.
The original tion It
of
average
the non-local
is given
exchange
potential
appearing
as a multiplicative
24,25
potential
was
introduced
in the Hartree-Fock
as a simplificaorbital
equations.
operator:
(3.1) with 64,
and is
determined
The modification fulfill
proposed
the virial
orbitals.
in Ref.18
chooses
in the calculation 7 method , the potential
procedure,
yielding
in the Hartree-Fock-Slater
the value
theorem
In the X,
self-consistent
20
self-consistently
of
of
ti in such a way as to
the energy
(3.1)
is
spin-orbitals
model.
from the
resulting
used as a spin-unrestricted,
which
are
quite
close
to the
UHF orbitals. In this is
picture
incorrect.
nentially,
of
behaving
as can be readily
the case
of
negative
mogeneous
electron
t ree-Fock
does.
A local Eqs.(2.4) as well
the asymptotic
however,
Instead
ions,
where
13
potential
(2.11).
It depends
as on the density
p(G)
-t/r
behaviour for
local
which
This
exchange
does
explicitly
and its
of
large
in Eq.(3.1). do not give
gas expression
exchange and
seen
as
the exchange
distances, is
particularly
potentials
26
gradient
through
in
from the ho-
malady
uses
to the nucleus
y(q),
expo-
, even when Har-
from this
on the distance
potential
decays
dramatic
computed
a bound state
not suffer
it
r,
Eq.(2.13):
(3.2) where ;)(?\
= 2+1 (3.3)
This it
potential
should.
is
finite
at
the origin,
and decays
as
-Vr
asymptotically,
as
833 A further for
simplification
Coulomb repulsion
ming an exponential tial
turns
out
results
and for
by taking
the exchange
form for
a -bona fide potentia1*7’*3 in the orbital equations.
part
the density,
the Coulomb repulsion
both Assu-
effective
poten-
to be28:
(3.4) where
% is a parameter from Eqs.(3.2)
lows
determined
and (3.3)
29 . The exchange
variationally
taking
7 also
as a variational
potential
fol-
parameter:
(3.51 Orbitals
calculated
the unoccupied
scheme, case,
but
form of ions
with
refer
this
orbitals
to excited
are
potential states 29 .
The effective
very
not virtual
orbitals
the exchange
and excited
29 give
potential
created
(3.5)
good total
orbitais,
by the presence
is also
energies.
as
of
the approximate
In this
in Hartree-Fock’s N-l
electrons.
one for
ihe
negative
potential:
(3.6) behaves
as -Z/r
at
the origin,
stood
as a Coulomb-like
tween
the nuclear
at
large
4.
potential
charge
with
asymptotically.
a screened
2 and the asymptotic
charge
charge
It can be under-
which
Z-N+1
felt
interpolates by the
be-
electron
distances.
MINIMAL BASIS I:artree-Fock
theory
can be compared. Nevertheless, tion,
both
orbitals
in this
for
bottleneck zeta
basis
sets
sets
the correct
no longer
of
distances, of
of
Slater
atomic
zeta while
Hartree-Fock results,
potential
is
type
basis
the use of
approach
no longer
atomic
models
a tumbling
(algebraic)
these
atomic
to Hartree-Fock, stone.
equations.
The The most
are the minimal basis and the double 30 . orbitals Indeed the exponential behaviour as shown in Eq.(l.5).
the
the smaller
a minimal
as for
the
other
calculation
Hartree-Fock
basis,
of
which
results become a standard. basis 30 gives much informa-
In the algebraic
one asymptotically, for
with
in a fixed
the non-linearity
in atomic
an integer
In the case
numerical
the solutions
the exchange
using
In the double small
the yardstick
calculations.
then becomes
basis
sense, of
interpretation
in molecular
popular
constitutes
expansion
the non-locality
is
and (-Z+N-1)/r
larger one
The power
s however,
orbitals. exponent is
the exponent
closer turns
gives to out
the dominant
J-xc
term at
3 as in Eq.(1.6).
to be some average
value
is
between
the two zeta
We can
values
introduce
of
the double
an optimized symptotically,
Eq.fl.6).
origin
wer expansion cusp
to
the
gives
condition.
for
the
logarithmic
basis. by Jetting
so that
we modify
the correct
Thus,
basis
minmal
have as an exponential Close
zeta
its
exponent
behaviour
in
derivative
a Is wave function
the basis tends such
at
function
be-
to behave
a way that
the origin,
as
the
as
in po-
in the
we can write
&5 its> which
behaves
=
\
(4.1)
as:
(4.2) Hence the parameter
a can be taken
z-g
Q”
while
f
is determined
The rest at
of
the origin
(4.3)
variationally
the s functions
is given
as
as are
by Eq.(h.l),
in the minimal
taken once
as normal
basis
STO’s,
the orbital
is
with since
built
STO’s. the
behaviour
as a linear
combi-
nation. For higher
values
of
4,
we use a similar
procedure,
so that
(4.4)
with
(4.5) 0 As a result the minimal larly
for
we have a minimal
STO. The total
the
otherwise
lighter
basis
energies
atoms.
This
are is
with
the same number of
almost
illustrated
of
double for
zeta
parameters
quality,
a few cases
as
particu-
in Table
I_
in
335
TABLE Atom
ST0
He
fulfills near
oz
ours
2.847
Be
With
1
2.8615
14.557
2.8617
14.568
14.5723
Ne
127.81
128.396
128.535
Mg
198.86
199.468
199.607
Ar
525.76
526.370
526.815
the basis
defined
the proper combination.
ved by asking
cusp
above,
because
condition,
The resultsare
the orbital
we do not guarantee
itself
nevertheless to fulfill
of
that
the mixture
the orbital resulting
very
encouraging 31 the condition
itself from the
li-
and can be impro-
(4.6) CONCLUSIONS
5.
As a conclusion viour
of
gross
features
the orbitals
In the bly
we would
both of
at
simply
the origin
the effective
like
to
recall
the
and asymptotically, potential
intermediate region, all we need 29 showing some shell rtructure.
as of
is a smooth
importance since
it
the orbitals interpolation
of
the beha-
determines
the
themselves. scheme,
possi-
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M. Berrondo & J. Rbcamier, Kinam 5, 329 (1983) R.E. Langer, Phys. Rev. 5l, 669 (i937) C.L. Davis, H.J.A. Jensen 6 H.J. Honkhorst. J. Chem. Phys. 80,840 (1984) “Quantum Theory of Atomic Structure” J.C. Slater, (McGraw Hill, New York,1960) vol.2 “The Hartree-Fock Method for Atoms” C . Froese-Fi scher, (Wiley, New York 1977) P-0. LLSwdin, Adv. Chem. Phys. 2, 207 (1959) “The Self Consistent Field for Molecules and Solids” J.C. Slater, (McGraw Hi 11, New York, 1974) P. GombaL, “The Statistical Theory of Atoms” (Springer Verlag, Wien, 1949) N.H. March, Adv. Phys. 5, 1 (1957) P.A.M. Dirac, Proc. Camb. Philos. Sot. 26, 376 (1930) R. McWeeny, Rev. Mod. Phys. 32, 335 (19m M. Berrondo & 0. Goscinski, Int. J. Quantum Chem. Sg, 67 (1975) M. Berrondo 6 0. Goscinski, Chem. Phys. Lett. 62, 31 (1979) M. Berrondo 6 A. Flores-Riveros, J. Chem.Phys. 72, 6299 (1980) J.L. Gdzquez, to be published C.F. Weiszlcker, Z. Phys. 96, 431 (1935) D.A. Kirzhnits, Sov. Phys. JETP 2, 64 (1957) M. Berrondo & 0. Goscinski, Phys. Rev. 184, 10 (1969) W. Kohn 6 L.J. Sham, Phys. Rev. m, Al(1965)
336 20. 21. 22. 23. 24. 25. 26. 27. 28.
;:: 31.
F. Herman 6 S. Skillman, “Atomic Structure Calculations” (Prentice-Hal?, EngI:ewood Cliffs, N.J.. 1963) K. Schwars, Phys. Rev. 85, 2466 (1972) M.S. Gopinathan, M.A. W%tehead f R. Bogdanovi&, Phys. Rev. e. 1 (1976) J.L. Gdzquez k J. Keller, Phys. Rev. A16, 1358 (1977) J.C. Slater, Phys. Rev. 81. 385 (1951) P.O. Ltiwdin, Phys. Rev. 97, 1474 (1955) K. Schwarz, Chem. Phys. Lett. 57, 605 (1978) A.E.S. Green, Adv. Quantum Chem. 1, 221 (1973) M. Berrondo, J.P. Daudey 6 0. Goshinski, Chem. Phys. Lett. 62, 34 (1939) J.P. Daudey 6 M. Berrondo, Int. Quantum Chem. 19, 907 (198l.T E. Clementi & C. Roetti. At. Data Nuci. Data Tables l4, 177 (1974) M. Berrondo, to be published.