In a preceding paper a one‐configuration wavefunction of strong orthogonal group functions was found to give a rather poor description of the orientation dependence of short‐range intermolecular forces in H2–H2. As an alternative to the necessity of relaxing the strong orthogonality condition, it is suggested that the introduction of a small amount of the charge‐transfer state H2–H2+ describing one‐electron transfer between the two molecules should improve the interaction energy and its change with the relative molecular orientation. Ab initio calculations in a region of intermolecular separations ranging from two to four times the internuclear equilibrium distance of an isolated H2 molecule show that less than 1% of such a charge‐transfer state gives interaction energies which are in substantial agreement with those obtained with a complete configurational interaction.

1.
V.
Magnasco
and
G. F.
Musso
,
J. Chem. Phys.
46
,
4015
(
1967
) (PartI).
2.
V.
Magnasco
and
G. F.
Musso
,
J. Chem. Phys.
47
,
1723
(
1967
) (Part II).
3.
V.
Magnasco
,
G. F.
Musso
, and
R.
McWeeny
,
J. Chem. Phys.
47
,
4617
(
1967
) (Part III).
4.
V.
Magnasco
and
G. F.
Musso
,
J. Chem. Phys.
47
,
4629
(
1967
) (Part IV).
5.
By restricted wavefunctions we mean here wavefunctions not allowing for the full configurational interaction proper to a given atomic basis.
6.
The “barrier” is here the difference in intermolecular energy between the two relative orientations of the two molecules defined by τ = 0° and τ = 180°.
7.
The strong orthogonality condition for the many‐electron group functions Φ(1,2,…NA) and ΦBb(NA+l,…N) is expressed by ∫Φ(1,xiBb(l,xi)dx1 = 0 for A≠B,a≠b or both [see
R.
McWeeny
,
Proc. Roy. Soc. (London)
A253
,
242
(
1959
)].The simplest way of ensuring strong orthogonality in a GF approach is to build Φ and ΦBb from mutually orthogonal sets of atomic orbitals.
8.
J. C.
Slater
,
J. Chem. Phys.
19
,
220
(
1951
);
J. C.
Slater
,
Rev. Mod. Phys.
25
,
199
(
1953
).
9.
R.
McWeeny
,
Proc. Roy. Soc. (London)
A223
,
63
(
1954
).
10.
The (singlet) Heitler‐London wavefunction can be considered as arising from the coupling to zero resultant spin of two degenerate product functions Φk = a (aαbβ),Φk = a(aβbα) constructed from the doublet (S = 12,Ms = ±12) group functions describing the single electron of each atom [see R. McWeeny, Uppsala Univ. Quantum Chem. Group, Tech. Note No. 59, January 15, 1959 (unpublished)]. Here and in the following sections is worth including the normalization factor in the antisymmetrizer a exchanging electrons between the two groups.
11.
The strong interconfigurational mixing between Φ0 and Fgr;1 occurs because the matrix element describing the interaction,
contains large one‐electron contributions (we use here the Diracnotation and denote by 𝒽 the one‐electron Hamiltonian). At R0 = 1.4166 a.u. (with ζH = 1.193) the numerical value in atomic units (see Ref. 23) resulting for the interaction is Ho1 = −0.7472, to be compared with H00 = −1.2603 and H11 = −0.9130.
12.
The one‐electron density is simply the sum of the electron densities of each group, namely P1(00|r1;r1) = P1A(00|r1;r1).
13.
When locally doubly excited configurations are admitted on each molecule the interaction is simply H01 = J(01,01)−(01,01), where J and K are the two‐electron Coulomb and exchange interactions between the pairs of transition densities P1(0l|r1;r2)P1(01|r2;r2) and p1(01|r2;r1)P1(01|r1;r2).
14.
J. N.
Murrell
,
M.
Randic
, and
D. R.
Williams
,
Proc. Roy. Soc. (London)
A284
,
566
(
1965
).
15.
The antisymmetrizer a is assumed to include the normalization factor. See Ref. 10.
16.
P.‐O.
Löwdin
,
J. Chem. Phys.
18
,
365
(
1950
).
17.
Doubly ionic states are expected to occur with extremely low weight. This view is supported by the results obtained in Part II.
18.
Each relative orientation of the two molecules possesses at least a twofold symmetry axis (see Sec. III).
19.
Both Φ0 and Φ1 describe an electronic state A1 when the overall symmetry is C2, and A10 for C2A.
20.
R.
McWeeny
,
Rev. Mod. Phys.
32
,
335
(
1960
).
21.
We thank the staff of the Computation Centre for its kind cooperation.
22.
Group functions Φ,ΦBb are written as a linear combination of many‐electron basis functions consisting of Slater determinants of order NA and NB (see Sec. II). It follows then
where ΦrA,ΦcB, denote many‐electron basis functions and 1̄ = NA+1,…NB = NA+NB, each term in the right‐hand member merely expressing the Laplace expansion of a determinant of order NA+NB according to minors from its first NA rows and their cofactors from the remaining NB rows. Hence, no matter how the N=NA+NB electrons are partitioned between the two groups, Slater’s rules for orthonormal determinants can be used to evaluate matrix elements between generalized product functions such as aAaΦBb].
23.
Energy atomic unit (a.u.) = 27.210 eV, length a.u. = 0.52917 Å, charge a.u. = 4.77×10−10esu.
24.
The iteraction energy ΔE is defined as the total molecular energy (incuding nuclear repulsion) of the composite system minus twice the ground‐state energy of an isolated hydrogen moculecul in the “Heitler‐LOndon+ionic” approximation (2EH = −2.29578 a.u)
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