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Ab initio prediction of the rovibrational levels of the He-CO+ ionic complex
M. Mladenovic, Marius Lewerenz
To cite this version:
M. Mladenovic, Marius Lewerenz. Ab initio prediction of the rovibrational levels of the He-CO+
ionic complex. Molecular Physics, Taylor & Francis, 2013, pp.1. �10.1080/00268976.2013.783722�.
�hal-00823746�
Vol.00,No.00,Month2013,128
RESEARCH ARTICLE
Ab initio predition of the rovibrational levels of the He-CO
+
ioni omplex
MirjanaMladenovi¢
a∗
andMariusLewerenz
a a
UniversitéParis-Est,LaboratoireModélisation etSimulation MultiEhelle, MSME
UMR8208 CNRS,5bdDesartes, 77454Marne la Vallée, Frane
(January2013)
Theintermoleularpotentialforthe vanderWaalsomplexofthearbon monoxideation
with heliumisstudied bymeansof the partiallyspinadapted oupled lusterRCCSD(T)
method and the aug--pVXZ family of basis sets. In the ground eletroni state, or-
related with the lowest eletroni asymptote X2Σ+ of the monomer CO+, the omplex
He(
1S)-CO+(2Σ+)hasa nonlinearequilibrium struturewithaJaobi angleofabout46
◦
andabindingenergyofabout275m
−1
.FortheomplexHe(
1S)-CO+(A2Π)wendequi-
libriumJaobianglesof78
◦
and90
◦
andeletronibindingenergiesofabout160m
−1
and
303m
−1
fortheA′′andA′omponents,respetively,oalesingintotheΠstateatlinearity.
Two-dimensionalintermoleularpotentialenergysurfaesareonstrutedforthegroundele-
tronistateandusedtoomputerotation-vibrationstatesuptoJ= 10withthenumerially
exat disrete variable representation (DVR)tehnique.TheHe-CO
+
omplexisfound to
have19boundeven-parityJ= 0statesand16boundodd-parityJ= 1statesandtoexhibit
strongangular-radialouplingandquasilinearbehaviour.
Keywords:moleularions;vanderWaalsomplex;arbonmonoxideation;helium;
rovibrationalstruture;abinitioalulation;eletriproperties;quadrupolemoment
1. Introdution
Carbon monoxide isa relatively abundant moleule ininterstellar spae, where its
positive ion CO
+
has also been identied [1, 2℄. Even before its laboratory ob-
servation the
A
2Π − X
2Σ
+ system in CO+ was observed in the tail of a omet[3 , 4℄ and is still known as 'omet-tail bands'. CO
+
was the rst moleular ion
for whih a mirowave spetrum was reorded [5℄. Low energy ollisions of CO
+
with its seond most abundant ollision partner in spae, helium atoms, are gov-
ernedbytheweakintermoleularinterationleading tothevanderWaalsomplex
He-CO
+
. Evidenefor the formation ofthis omplex has been observed inseveral
ion drift tube experiments: onventional measurements at room temperature [6℄,
laser-indued uoresene measurements from various initial rotational states at
305K [7 ℄, and ion drift tube measurements at very low temperatures [8℄. No high
resolution spetraldatahave everbeen reported forthis omplex.
The relatively strong binding between CO
+
and heliumatoms should allowthe
reation ofmixedlustersof theompositionHen-CO+
indrifttubesormixedgas
expansionsoupledtoeletridisharges.Thelattertehniquehasbeensuessfully
applied in a series of elegant spetrosopi experiments on the energetially very
∗
Correspondingauthor.Email:mladenovuniv-mlv.fr
ISSN:00268976print/ISSN13623028online
2013Taylor&Franis
DOI:10.1080/0026897YYxxxxxxxx
2 Mladenovi¢andLewerenz
similar Hen-N+
2 omplexes[912℄,where size seletedhighresolution spetraould
be reorded. High resolution infrared spetrosopy of Ar-N
+2 reated in a plasma
slit jet experiment has been reently reported [13℄ indiating the possibility of an
infrared experiment on He-CO
+
.
Hen-CO+
lusters appearto be an ideal target for luster size spei high res-
olution depletion spetrosopy. Both mirowave and infrared experiments would
prot from the large permanenent dipole moment and large vibrational transition
moments ofthis system.Experiments onthis type oflusterwouldhelpus to bet-
ter understand mirosopi superuidity [14 ℄ byexpliit ontrol ofthe systemsize
and measurement ofthelustersizedependent evolution oftheeetiverotational
onstant of the CO
+
dopant. Neutral CO moleules embedded into large helium
lusters have been studied theoretially [15 18℄ and experimentally by high reso-
lution spetrosopy [17,19 23℄. Reent ionization experimentson CO doped large
heliumlustersdidnotyieldanyindiationfortheformationofHen-CO+
fragments
whereas speiesof the type Hen-(CO)+
m werereadily observed [24℄. TheCO/CO+
pair inside heliumis ofpartiular interestfor high resolution experimentsbeause
the rotationalonstantsofbothspeiesareverysimilarwhiletheirinterationwith
helium atoms isofvery dierent strength.Theoretial and experimental studiesof
Hen-CO+
an make amajor ontribution to this eld.
The He-CO
+
omplexhasbeen onlypartiallyharaterized inearliertheoretial
studies[24 28℄.Hamiltonetal.[25 ℄employedunrestritedHartree-FokandMøller-
Plesset perturbation theory to fourth order (MP4) to study linear and T-shaped
arrangements for the groundand rst exited eletroni states. For linearand T-
shaped He-CO
+
in the ground eletroni state, Lotrih and van der Avoird [27℄
tested a newmethodfor thedeterminationof interationenergies ofationi om-
plexesfrominterationenergiesandvertialionizationpotentialsofneutralspeies.
Salazar etal.[28℄usedspinunrestritedopen-shell oupledlustertheoriesinom-
binationwiththe-pVTZbasissetplusbondfuntionsandidentiedbentequilib-
rium geometries witha Jaobiangle of
θ
e= 45
◦,a Jaobidistane ofR
e= 2.85
Aand a binding energy of
D
e= 275
m−1 for the ground eletroni state, whereastheyfound
θ
e= 90
◦,R
e= 2.70
A andD
e= 218
m−1 fortherstexitedeletronistate. A MP4potential energy surfae developed byMalagan et al. [26 ℄ wasused
in lassial trajetory alulations for thetransport ross setions of CO
+
ions in
helium gas.
The main purpose of the present study of He-CO
+
is the onstrution of an
aurate potential energy surfae and the predition and interpretation of au-
rate vibration-rotation levels whihould be heked against futuredetailed spe-
trosopi experiments. This potential surfae will serve as a building blok in
many-bodymodels for CO
+
ionsinside larger heliumlusters [29 ℄.
Ab initio alulations have been arried out with supermoleule oupled luster
tehniques inombination withthe aug--pVXZfamily ofbasis funtionsfor the
ground andrstexited eletronistates.The ounterpoise proedureofBoys and
Bernardi and extrapolations to innite basis size have been used to orret for
nite basissizeeetsonthe shapeofthesurfaeandinpartiular onthedissoia-
tionenergy andtheequilibriumgeometry (Setion2).Inadditiontothestrutural
parameters, we have also studied the spetrosopi and eletri properties of the
monomers (Setion3) and the omplex (Setion4) inthe ground and rst exited
eletronistates.TheomplexHe-CO
+
isboundbyindutionanddispersionfores,
responsiblefor long-rangeattration between thetwo monomers.Two-dimensional
(2D)intermoleularpotentialenergysurfaeshavebeenonstrutedforHe-CO
+
in
the ground eletronistate (Setion5) and are usedto alulate the rovibrational
energy spetra bya numerially exat method based on a disrete variablerepre-
R
r
µµµµ
O z
He
C
θθθθ
x
Figure1. Jaobioordinatesr, R, θand theaxissystemusedforthe vander WaalsomplexHe-CO+.
Thedipolemomentvetorµorrespondingtotheequilibriumstrutureoftheomplexisalsoshown.
sentation (Setion6). The omplex is found to belong to the lass of quasi-linear
moleules. Indiations for lowenergy resonanes arealso observed.
2. Eletroni struturealulations
The ab initio omputations have been arried out by means of the partially spin
adapted oupled-luster RCCSD(T) methodwith fulliterative treatment of single
and double exitations and perturbative orretion for triple substitutions [30?
, 31℄, as implemented in the MOLPRO quantum hemistry program pakage [32 ℄.
Thesinglyaugmentedorrelationonsistentpolarizedvalenebasissets,ommonly
labelledaug--pVXZ,havebeenused[33,34 ℄.Fullyrelaxedgeometryoptimizations
and harmoni frequeny determinations were performed by means of numerial
derivatives.
The three Jaobi oordinates
r
,R
, andθ
, shown in Figure 1, are employed todesribe the internal geometry of the omplex. Here,
r
is the bond length of thediatomi fragmentCO
+
,
R
isavetoroflengthR
runningfromtheenter-of-mass of the diatom to the He atom, andθ
is the angle enlosed byR
and the CO+
axis. The Jaobi angle
θ
is measured from the C side of CO+, suh thatθ = 0
◦orrespondsto alinearomplex withHe loserto arbon.
The interation energies of the omplex were alulated in the supermoleular
approah as
E
int= E
ab(AB) − E
a(A) − E
b(B),
(1)where AB, A, and B stand respetively for He-CO
+
, He, and CO
+
. The lower
index
p
inE
p(Q)
referstothebasissetofthespeiesP
usedtoomputetheenergyE(Q)
forthespeiesQ
.TheinterationenergiesE
intwereorretedforthebasissetsuperpositionerror (BSSE) bymeans of the ounterpoise orretion (CP) method
of Boys andBernardi [35℄,givingthe CPorretedinteration energy
E
intCP asE
intCP= E
ab(AB) − E
ab(A) − E
ab(B ),
(2)where themonomerandomplexwavefuntionsareallomputedinthebasissetof
the omplex.The geometry optimizations were arriedout at theCP unorreted
level.
Theinteration energiesattheompletebasisset(CBS)limitwereestimatedby
4 Mladenovi¢andLewerenz
extrapolationfor the Hartree-Fok Self-Consistent Field(SCF) ontribution
E
SCF(X) = E
∞SCF+ ae
−bX (3)and a
1/X
3 extrapolation for the orrelationpartE
corr(X) = E
∞corr+ c/X
3,
(4)where
X
denotesthebasissetardinalnumber.Inthisfashion,theestimatedtotalCBS energy for speiesQbeomes
E
∞(Q) = E
∞SCF(Q) + E
∞corr(Q)
(5)and theinteration energy isomputed from thebest total energy estimatesas
E
int= E
∞(He − CO
+) − E
∞(He) − E
∞(CO
+).
(6)The eletridipolemoments
µ
q andeletriquadrupolemomentsΘ
ij withi, j = x, y, z
were obtained numerially at the RCCSD(T) level of theory by means ofnite-eld alulations, using eld strengths of 0.001-0.00005 a.u. It is noted that
Θ
xx+ Θ
yy= −Θ
zz holdsforthequadrupolemomentΘ
,whihisatraelessseondmomenttensor.Theeletripropertiesreportedinthepresentworkwereevaluated
withrespetto theaxissystem
x, y, z
shown inFigure1,where thez
-axis isalongthe diatombond vetor
r
,thez ∧ x
planeoinides withthemoleular plane, andthe originofthe frame isat the enterof massofthe
12
C
16
O
+
unit.
The quality of our RCCSD(T) alulations was investigated by means of sev-
eralothereletroni-struture approahes,inludingtheompleteative spaeself-
onsistent eld method (CASSCF), multi-referene Rayleigh-Shrödinger seond-
order perturbationtheory(RS2)inonnetionwiththemulti-statemulti-referene
omplete ative spae perturbation theory(CASPT2), and themulti-referene in-
ternally ontrated onguration interation (MRCI) method [3739 ℄. The latter
approahes were partiularly useful for the alulation of geometri and eletri
properties of the eletronistate
2
2A
′ ofthe omplex He-CO+.3. Monomerproperties
3.1. Carbon monoxide ation
ThegroundstateeletroniongurationofCOis
(1σ)
2(2σ)
2(3σ)
2(4σ)
2(1π)
4(5σ)
2.Removal of an eletron from the highest energy
σ
orbital leads to the groundeletroni state
(1σ)
2(2σ)
2(3σ)
2(4σ)
2(1π)
4(5σ)
1 ofCO+ whih isX
2Σ
+.Removalof an eletron from the
1π
orbital leads toA
2Π
i as the rst exited state,(1σ)
2(2σ)
2(3σ)
2(4σ)
2(1π)
3(5σ)
2, whih is split by a spin-orbit interation on-stant
A
SO of -117.5 m−1(Ref. [40℄). The singly oupied
5σ
moleular orbitalof CO
+
(
X
2Σ
+) isprimarily omposed ofthe2s, 2p
z atomi orbitals ofC, whereasthe singly oupied
1π
moleular orbital of CO+(A
2Π
) is primarily omposed ofthe out-of-bond-line
2p
x,y atomiorbital ofoxygen.Atomi oxygen has a
3
P
g ground state whih is split by spin-orbit interationinto
3
P
2 atE = 0
,3P
1 atE = 158.265
m−1,3P
0 atE = 226.977
m−1,and hasan ionizationlimit of150305.6m
−1
leading toO
+
(
4S
u)
.Thearbonatomgroundstate
3
P
g asymptote is split into 3P
0 atE = 0
, 3P
1 atE = 16.40
m−1, 3P
2 atE = 43.40
m−1. The arbon atom ionization limit is 90820.42 m−1 leading to0 5000 10000 15000 20000 25000 30000 35000 40000
1 1.2 1.4 1.6 1.8
E / cm-1
r(CO) / angs X 2
Σ
+A 2
Π
MRCI MRCI CASPT2 RCCSD(T) RCCSD(T)
Figure2. PotentialenergyurvesfortheX2Σ+andA2ΠstatesofCO+fromtheRCCSD(T),three-state CASPT2,andMRCIalulationswiththeaug--pVQZbasisset.
C
+
(
2P
1/2)
and to C+(
2P
3/2)
at90883.84 m−1.Thelowest dissoiationasymptote for CO+
isthereforeC
+
(
2P
u)
+O(
3P
g)
whihorrelateswiththemoleular states(2,4)
(Σ
+, Σ
−, Σ
−, Π, Π, ∆)
.The
2
Σ
+ and 2Π
urves of CO+ rossat aboutr = 1.5
A at an energy approx-imately 30000m
−1
above the potential energy minimum ofthe ground eletroni
state, as found in our CASPT2 and MRCI alulations with the basis set aug-
-pVQZ (see Figure 2). This nding is in agreement with Rydberg-Klein-Rees
urves derived by Coxon and Foster [41℄ in their deperturbation analysis of the
A
2Π ↔ X
2Σ
+ spetrosopidata.TheΩ = 1/2
omponentsofthesetwostatesaremixed by spin-orbitoupling whihaets aidentally near-degenerate zero-order
vibration-rotation levelsin thetwo eletroni statesat energiesfar belowtheele-
troni intersetionenergy. Thisis theorigin of theperturbations observed [4143 ℄
inthe
A
2Π(v = 0)
statebyrotational levelsof theX
2Σ
+(v = 10)
state,bothlyingabout 22000m
−1
abovethe minimum(Figure 1 ofRef.[41 ℄).
In the present work, we onsider the eletroni states
X
2Σ
+ andA
2Π
of CO+within the Born-Oppenheimer approximation, aiming only at a good zero-order
(adiabati)desription.Spin-orbitinterationanditseetonrovibrationalspetra
of CO
+
willbean important partof afuture study.
3.1.1. Results for CO
+
Strutural, spetrosopi, and eletri propertiesof the arbon monoxide ation
alulated bymeans oftheRCCSD(T) methodare reportedinTable 1alongwith
availableexperimentaldataprovided byRef.[40℄.All strutural andeletri prop-
ertieslearly exhibitsmooth andverysatisfatoryonvergene uponinreasingthe
size of thebasisset.
The theoretial values for
r
e obtained using the aug--pV5Z and aug--pV6Zbasis sets agree within 0.0003
A for both CO
+
(
X
2Σ
+) and CO+(A
2Π
). The ex-ponential extrapolation for
r
e from theX = 3 − 6
data givesr
∞e of 1.1166A and1.2459
Afor
X
2Σ
+andA
2Π
,respetively.Theseresultsareoverestimatedbyabouty17,201318:21MoleularPhysisartile-provera
6Mladenovi¢andLewerenz
Table1. Geometri,spetrosopi,andeletripropertiesofCO
+
(X2Σ+)andCO+(A2Π)obtainedbytheRCCSD(T)method.TheexperimentaldataintheolumndenotedbyExparetaken fromRefs.[40℄and[42℄.ThetheoretialBv valuesareomputedasexpetationvalueshBiv oftherotationalonstantBinthevibrationalstatev.TheabbreviationaVXZstandsforthebasis setsaug--pVXZ.Foradditionalinformation,seethemaintext.
CO
+
(
X
2Σ
+) CO+(A
2Π
)Property aVTZ aVQZ aV5Z aV6Z Exp aVTZ aVQZ aV5Z aV6Z Exp
re/A 1.1225 1.1181 1.1170 1.1167 1.11514 1.2523 1.2473 1.2462 1.2459 1.24377
T
e/m−1 19801 20254 20374 20417 20733.3˜
ν
1←0/m−1 2164.7 2183.0 2186.2 2187.7 1531.0 1539.3 1540.6 1541.4˜
ν
2←0/m−14300.2 4336.5 4342.8 4345.8 3036.7 3053.1 3055.9 3057.5
B
0/m−11.941 1.958 1.962 1.963 1.967465 1.560 1.572 1.574 1.575 1.5786