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Gaussian Basis Sets for the Calulation of

Some States of the Lanthanides

P.R. Librelonand F.E. Jorge

Departamento deFsia

UniversidadeFederaldo EspiritoSanto

29060-900Vitoria, ES,Brasil

Reeivedon19Otober,2000

HighlyaurateadaptedGaussianbasissetsareusedtostudythegroundandsomeexitedstates

fortheneutralatomsandalsosomeorresponding6sand4fionizedstatesfromCsthroughLu. Our

totalenergiesareomparedwiththosealulatedwithanumerialHartree-Fokmethod.Themean

error ofourenergyresults isequalto0.74 mhartree. Ouralulations reproduetheexperimental

trendtoinreaseortodereasethe6sand4fionizationpotentialswithinreasingatominumber,

althoughtheyarerespetivelysmallerandlargerthantheexperimentalvalues.

I Introdution

In this last deade lanthanide hemistry and physis

have experiened tremendous growth, for example in

the eld of atalysts [1℄ and high temperature

super-ondutors [2℄. Thus, it would be highly desirable to

eluidate the eletroni struture of lanthanide atoms

at least in theHartree-Fok (HF) approximation. For

these atoms, numerial HF (NHF) alulations [3-5℄

were performedmainlyonthegroundstates.

Inthis work,theadapted Gaussianbasissets

[AG-BSs-onedierentsetofGaussian-typefuntion(GTF)

exponentsfor eah atomi speies for the atoms from

Cs (Z=55) through Lu (Z=71) [6℄ are initially

aug-mented until saturation is ahieved for eah

symme-tryof eahatomandthen, usingthegenerator

oordi-nateHF(GCHF) [7℄method, theyarereoptimizedfor

eah atomi speies. Next the energies for the atoms

Cs-Lu and theirpositiveions arealulated and

om-paredwiththoseobtainedwithaNHF[5℄method. The

ionizationpotentials(IPs)arealsoomputedand

om-paredwiththeorrespondingexperimentalvalues[8,9℄.

II The method

An approah to selet the basis sets arises from the

GCHF method [7℄. In the GCHF method the

one-eletronfuntionsareintegraltransforms,i.e.,

1 (1)= Z i (1;)f i

()d i=1;:::;n; (1)

where

i

are the generator funtions (GTFs in our

ase), f

i

are the unknown weight funtions, and is

the generatoroordinate. Theappliation ofthe

vari-ational priniple to alulate the energy expetation

value built with suh one-eletron funtions leads to

the Gritn-Hill-Wheeler-HF (GHWHF) equations [7℄.

The GHWHF equations are integrated using a

proe-dureknownasintegraldisretization(ID)[10℄.TheID

tehniqueis implemented througha relabelling of the

generatoroordinatespae,i.e.,

=ln

A

; A>1 (2)

where A is a numerially determined saling fator.

In the new generator oordinate spae , an equally

spaedN-pointmeshf

i

gisseleted,andthe

integra-tion range is haraterized by a starting point

min ,

an inrement , and N (number of disretization

points). The highest value (

max

) for the generator

oordinateisgivenby

max =

min

+(N 1): (2)

The hoie of thedisretization pointsdetermines the

exponentsoftheGTFs.

In the last four years, the GCHF [7℄ method was

suessfully tested in the generation of basis sets for

atomiandmoleularsystems[11-16℄.

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III III Results and disussion

By employing the GCHF method we have generated

AGBSs for the atomi speies presented in Table 1.

Throughout the alulations we have used the

sal-ing fator A (see Eq. (2)) equal to 6.0, and for all

atomi speies we have sought the best disretization

parameter(

min

and)valuesforeahs,p,dandf

symmetries. All alulations were arriedout using a

modiedversionof theATOMSCF program [17℄,and

for eah atomi speies theoptimization proessis

re-peateduntilthetotalenergyvalueisstabilizedwithin

ten signiant gures. The resulting wave funtions

are available by request through the e-mail address

jorgee.ufes.br.

Table I shows the ground and some exited state

HF total energies (in hartrees)for the neutral atoms

and someationsfrom Cs(Z=55)throughLu(Z=71)

omputedwithourAGBSsandwithaNHF[5℄method.

Ourbasissetsizesarepresentedintheseventholumn.

WereallthattheAGBSsaregeneratedfromthebasis

sets of Ref. [6℄. First, weaugmentedthese basissets

until saturate eah symmetry of eah atom, and

se-ond, usingtheGCHF [7℄method, wereoptimizedeah

AGBSofeahatomispeiesstudiedhere. FromTable

I,weanseethatourtotalenergies,forallatomispeie

ofinterest,areingoodagreementwiththe

orrespond-ing NHF [5℄ valuesand that ourenergy errorsdo not

exeed1.72mhartree. Hereitisimportanttosaythat

thevetorouplingoeÆientsusedinthealulations

of the open-shell ongurations havebeen taken from

the tabulation by Malli and Olive [18℄. These tables

show the vetor oupling oeÆients for the eletron

ongurationss,p n ,sp n ,d n ,sd n ,p m d n ,sp m d n andf n .

TheHFtotalenergiesofthegroundstatesoftheatoms

CeandGdandofsomestatesoftheationsPr + ,Nd + , Pm + , Sm + , Eu + , Tb + ,Dy + ,Ho + , Er + and Tm + are

notalulatedhere,beausetheeletronongurations

of these atomi speies have 5d and 4f and 6sand 4f

openshells,respetively. Theeletronongurationof

Lu +

( 3

H)has5dand4fopenshells,andthusthewave

funtion forthisationisnotgenerated here.

Table II ontainstheIPs(in eV)omputed by

us-ing the Koopmans theorem (" is our orbital energy),

thetotalenergydiereneE =E(X +

) E(X)[X is

the atomi symboland E(X +

)and E(X) are our

to-tal energiesrespetivelyfortheationandtheneutral

atompresentedinTableI℄,andtheexperimentalvalues

(E

expt: )[8,9℄.

From Table II we an see that the dierenes

be-tween our IP's alulated through " (see the fourth

olumn) and through E (see the fth olumn) are

oremworksforthe6sionization. Besidesthis,forthe6s

orbitals,ourIPsalulatedwith thesetwoapproahes

areverysimilartothoseomputedwithaNHFmethod

(seethe sixth olumn). For all lanthanide atoms

pre-sentedinTableII,andfromourresultsfor ",wean

see that the6sorbitals are morediuse thanthe

or-responding 4f orbitals, that is, the 6s IPs are smaller

thanthe4flPs. Fortheseatoms, itisknownthat the

meanvaluesofrforthe6sorbitalsarelargerthanthose

forthe4forbitals,that is,the6seletronsarefarfrom

the nuleus than the 4f eletrons. From La through

Eu,boththealulated " (4.4-4.6eV)and the

ex-perimental (5.4-5.8 eV) 6s IPs are almost onstant.

AfterTb, the "and experimental[8,9℄IPsgradually

inrease. Theexperimental IPsare alwayslargerthan

the " values. Toorretthis disrepany,itis

nees-saryto inlude in the alulationseletronorrelation

eets and relativisti orretions, but this is outside

the sope of this work. Here, it is important to say

that Jorge et al. have developed the generator

oor-dinateDira-Fok(GCDF) [19,20℄method for

losed-shellatoms andasegmentedontrationmethodology

forrelativistiGaussianbasissets[21,22℄. FromTable

II,onlyYb (Z=70)haslosed-shell,thus,fortheother

atomspresentedinthisTable,weannotusetheGCDF

methodtoalulate therelativistiIPs.

Besidesthis,TableIIshowsthatforthelanthanides,

the4fIPsalulatedbyusthrough "andthroughE

giveverydierent results. The ionization of the

ele-trons in theoutermost 6s shell auses small

reorgani-zationonthe wholeeletrondistribution, whereasthe

inner4feletronionizationauseslargerreorganization

eetsbeauseoftheappearaneofaholeintheinner

shell. Thus, for these atoms, itis notappropriated to

usetheKoopmanstheoremtoalulatethe4feletron

ionization. Forall lanthanide atoms, the4fIPs

alu-latedbyus(E)areingoodagreementwiththe

orre-spondingvaluesobtainedwithaNHF[5℄method, and

althoughthealulated4fIPsare1-3eVgreaterthan

theorresponding experimentalvalues [8,9℄,NHF and

our E alulations desribe the experimental trend

well.

IV Conlusions

In this work we have generated AGBSs for the 45

atomispeiespresentedinTableIwiththeGCHF[7℄

method. Thelargestdierenebetweenthetotal

ener-giesalulatedbyusandbyaNHF[5℄methodisequal

to 1.72 mhartree for Lu. Although our 6sand 4f IPs

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ulations reprodue theexperimental trendson the6s

and4feletronionizationswell. Forthe4fIPs,ourE

resultsarebetterthanthoseomputedwiththe

Koop-mans theorem, whereasfor 6sIPsthetwoapproahes

givesimilarresults.

Aknowledgements

WeaknowledgethenanialsupportofCNPqand

Dr. L.T. Peixotoforvaluabledisussions.

Referenes

[1℄ G.Jeske,H.Lauke,H.Mauermam,H.ShumamandT.

J.Marks,J.Am.ChemSo.107,8111 (1985).

[2℄ C.N.Rao andG.W.Raveau, A. Chem.Res.22,106

(1989).

[3℄ B.Mann,At.DataNul.Dat.Tables12,1(1973).

[4℄ C. Frose-Fisher, The Hartree-Fok method for Atoms

(Wiley,NewYork,1977).

[5℄ H.Tatewaki,O.MatsuokaandT.Koga, Phys.Rev.A

51,19791995).

[6℄ F.E. Jorge, P.R. Librelon, A. Canal Neto, J. Comp.

Chem.19,858(1998).

[7℄ J.R. Mohallem, R. M. Dreizler and M. Trsi, Int. J.

QuantumChem.20,45(1986).

[8℄ W.C.Martin,L.Hagan,J.KeaderandJ.Sugar,J.Phys.

Chem.Kel.Data3,771(1974).

[10℄ J.R.Mohallem,Z.Phys.D3,339(1986).

[11℄ F.E. Jorge and R.F. Martins, Chem. Phys. 233, 1

(1998).

[12℄ E.V.R.deCastroandF.E.Jorge,J.Chem.Phys.108,

5225 (1998).

[13℄ F.E. Jorge and M.L. Frano, Chem. Phys. 253, 21

(2000).

[14℄ F.E.JorgeandE.P.Muniz,Int.J.QuantumChem.71,

307(1999).

[15℄ J.C. Pinheiro, A.B.F. da Silva and M. Trsi, Int. J.

QuantumChem.63,927(1997).

[16℄ M.GiordanandR.Custodio,J.Comp.Chem.18,1918

(1997).

[17℄ S.J. Chakravorty, G. Corongiu, J.R. Flores, V.

Son-nad, E. Clementi, V. Carravetta and I.Caelli, in: E.

Clementi (Ed), Modern Tehniques in Computational

Chemistry: MOTECC-89,(ESCOM,Leiden,1989).

[18℄ G.L. Malli and J.F. Olive, Tehnial Report, Part 2,

Laboratory of Moleular Struture and Spetra,

Uni-versityofChiago,1962-1963.

[19℄ F.E.Jorge,A.B.F.daSilva,J.Chem.Phys.104,6278

(1996).

[20℄ F.E.Jorge,A.B.F.daSilva,J.Chem.Phys.105,5503

(1996).

[21℄ F.E. Jorge, A.B.F.da Silva, Chem. Phys.Lett. 289,

469(1998).

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