Rb and Cs which is gained by the C
60
molecule as it has a higher
electron affinity. The calculations show that the encapsulation en-
ergies
of
Rb
and
Cs
are
highly
exothe
rmic
[see
Fig. 3b]
meaning
that
they are more stable in the inner cage of C
60
than as isolated atoms.
Bader analysis also shows that both Rb and Cs gain a charge close
to þ1 by donating their outer s-electron to the C
60
cage. Cs and Rb
are therefore ions, which exhibit smaller radii than their corre-
sponding atoms. The resultant complex can be considered as a
donor-acceptor endohedral complex (M
þ
-C
60
calculated the formation energies for the endohedral encapsulation
of Rb and Cs using Hartree-Fock calculations together with the
Born-Haber cycle. In their calculations, they assumed that both
metals lose one electron to form a þ1 charge and C
60
gains that lost
electron to form 1 charge. The calculated formation energies by
W
ang
et
al.
[
7]
for
Rb
and
Cs
are
1
.91
eV
and
1
.64
eV
respectively
,
in good agreement with our corresponding calculated values
of 1.82 eV and 1.86 eV though the trend is slightly reversed.
60
is zero
before and after the incorporation of Rb and Cs, indicating that
encapsulation does not affect the magnetism. Calculations indicate
that C
60
exhibits zero magnetic moment. As Rb
þ
and Cs
þ
exhibit
zero magnetic moment, overall complexes Rb
þ
-C
60
e
and Cs
þ
-C
60
e
are
thus also non-magnetic. The total DOS for the Rb and Cs encapsu-
lated in C
60
are
shown
in
Fig. 3f
and
(g)
respectively
.
The
encap-
sulation of Rb and Cs shift their DOS towards higher energies and
the lowest unoccupied band of C
60
becomes occupied by the s
1
electron transferred to C
60
.
Turning now to the inert gasses, the outer electronic configu-
rations of Xe and Kr are unaffected by encapsulation. This is a
consequence of their higher ionization potentials. This is further
supported by the very low encapsulation energies and the Bader
charge. The encapsulation energies are a balance between attrac-
tive van der Waals forces of the polarisable atoms and Pauli
repulsion of the electron clouds. Since Xe is large the Pauli repul-
sion is greater than exhibited by Kr and so Xe exhibits a slightly
positive (unfavourable) encapsulation energy whereas for Kr the
energy is slightly favourable.
The electron affinities of Br and I are reflected in the encapsu-
lation
energies
and
the
Bader
charges
shown
in
Fig. 3;
the
encap-
sulation energy of Br is much more favourable than that of I due to
the high electron affinity of Br but also because the smaller Br fits
better inside C
60
. The Bader charges on Br and I are 0.50 and 0.21
respectively. The outer electronic configuration of both Br and I are
s
2
p
5
with one unpaired electron. As C
60
and C
60
þ
are non-magnetic
and both Br and I gain electronic charge from C
60,
the overall
magnetic moment is reduced. The magnitude of the magnetic
moment is reflected in the degree of the Bader charge. The total
DOS
(see
Fig. 3e)
show
s
that
incorporation
of
Br
introduces
addi-
tional bands in the HOMO of C
60
but the band gap is not much
affected.
The positive encapsulation energy for Te reveals that it is un-
stable inside the cage due to its larger size and its inability to donate
charge to C-C 66 single bonds. A small Bader charge and magnetic
moment show that its outer electronic configuration is not altered.
Next, we consider how fission products can be trapped (or not)
by the outer surface of C
60
(i.e. the association energy). The
behaviour of fission products occupying positions on the inner and
outer faces of the C
60
cage are different as the faces are convex and
concave respectively. As explained earlier, we consider five possible
initial exohedral configurations. These have been relaxed to give
the final configurations and association energies. The relative as-
sociation
energies
of
each
atom,
report
ed
in
Table 1, are energiesrelative to the most stable site (which therefore has zero relative
energy
but
not
zero
absolute
association
energy
(see
Fig. 4)).
The most stable exohedral position for Xe and Kr is on top of the
hexagonal ring (H). However, differences in energy compared with
the other sites are very small, a consequence of how unreactive are
the noble fission product gas atoms. The shortest FP-C distance,
formation energies, Bader charge, magnetic moment of the super-
cell and the total DOS for the most stable configurations (identified
in
Table 1) are plotted in Fig. 4. While the (absolute) associationenergy is very small, it is negative due to the vdW interaction (see
Fig. 4 a). Both a zero Bader charge and magnetic moment validate this conclusion. This is why the two noble gas atoms are almost
4.00 Å away from the surface of C
60
. Interestingly the exohedral
association energy for Kr is smaller than the encapsulation energy
because Kr only interacts on the surface with six C atoms while
inside C
60
it interacts with the whole molecule. For Xe the situation
is reversed: larger Xe is stable on the surface while its encapsula-
tion energy is positive due to the large Pauli repulsion (compare
Br and I show a preference to be on top of the C-C bond, site (66),
and
gain
a
small
charg
e
(see
Fig. 4c).
That
their
magnetic
moments
are closer to 1 and Bader charge small means that their s
2
p
5
configuration with one spin up electron is unaltered. The formation
energy for Br is 0.93 eV, a more favourable value than that for I
(0.56 eV). The association energy calculated for I by Kobayashi
et
al.
[
35]is0.10 eV (without dispersion correction). This deviatesfrom our calculated value of 0.56 eV where a dispersion correc-
tion is included. The stronger absorption of Br is due to its higher
electron affinity compared to I and the shorter bond distance (C-Br
v’s C-I). Compared to Br and I inside C
60
, less charge is transferred.
This can be due to the halide atoms inside the cage being adjacent
to and thus able to gain electron density from all the C atoms of C
60
.
However, inside the cage the bonding process is in opposition to
Pauli repulsion; this is enough that I is more stable outside C
60
.
Conversely exohedral absorption of smaller Br is less favourable
than inside the cage. Furthermore, with Br the Fermi level is shifted
slightly to higher energies and the DOS spectrum of C
60
is now
dispersed with additional peaks. This is due to the chemical inter-
action of Br with the C atoms.
The (66) position is the preferred site for the Te, which loses ~1
electron
(see
Bader
charge
in
Fig. 4 c)
due
to
its
lower
electron
af-
finity than C
60
. Its formation energy is 1.39 eV showing strong
absorption by the C
60
surface, in contrast to endohedral adsorption.
There is a significant bonding interaction between Te and carbon in
the (66) position. This geometry of Te associated with (66) carbon
can be described as an icosahedral triangle with the C-Te bond
distance of 2.24 Å and C-C bond distance of 1.51 Å. The observed C-C
bond distance of 1.51 Å is 0.11 Å longer than the C-C distance pre-
dicted for the (66) positions in other parts of the relaxed C
60
configuration. It is further evidence of the significant interaction
with Te. The Bader charge approximation shows that Te has lost 1.11
|e| and the carbons in the (66) position have gained those electrons
with the ratio of 0.66:0.51. As the carbon in (66) position are now
four coordinated, the
p
-
p
interaction is reduced with the elonga-
tion in the C-C bond. However, Te is unstable inside the cage and
shows no interaction with C
60
as evidenced by the Bader change
and magnetic moment. This is due to the larger size of the Te and its
inability to donate charge to C-C 66 single bonds (in the relaxed
configuration, Te occupies the center of the C
60
and the distance
between the Te and C-C 66 bond is 3.55 Å).
Rb and Cs exhibit strong association energies, essentially to the
same extent as they did for encapsulation. This is because the alkali
atoms have low ionization potentials and electron affinities. Bader
analysis shows that both Rb and Cs form ~þ1 charge donating their
single s electrons to C
60
. The resultant supercells exhibit zero
magnetic
moment.
Fig. 4g
shows
there
is
a
substantial
Fermi
energy
shift to the higher energy levels upon absorption of Cs due to
electron transfer to the C
60
cage. The calculated association energy
N. Kuganathan et al. / Carbon 132 (2018) 477e485480