Increased interactions at the graphene-metal interface are here demonstrated to yield an effective prevention of intercalation of foreign species below the graphene cover. Hereby, an engineering pathway for increasing the usability of graphene as a metal coating is demonstrated. Graphene on Ir(111) (Gr/Ir(111)) is used as a model system, as it has previously been well-established that an increased interaction and formation of chemical bonds at the graphene-Ir interface can be induced by hydrogen functionalization of the graphene from its top side. With X-ray photoelectron spectroscopy, it is shown that hydrogen-induced increased interactions at the Gr/Ir(111) interface effectively prevents intercalation of CO in the millibar range. The scheme leads to protection against at least 10 times higher pressure and 70 times higher fluences of CO, compared to the protection offered by pristine Gr/Ir(111).
Increased interactions at the graphene-metal interface are here demonstrated to yield an effective prevention of intercalation of foreign species below the graphene cover. Hereby, an engineering pathway for increasing the usability of graphene as a metal coating is demonstrated. Graphene on Ir(111) (Gr/Ir(111)) is used as a model system, as it has previously been well-established that an increased interaction and formation of chemical bonds at the graphene-Ir interface can be induced by hydrogen functionalization of the graphene from its top side. With X-ray photoelectron spectroscopy, it is shown that hydrogen-induced increased interactions at the Gr/Ir(111) interface effectively prevents intercalation of CO in the millibar range. The scheme leads to protection against at least 10 times higher pressure and 70 times higher fluences of CO, compared to the protection offered by pristine Gr/Ir(111).
Graphene is a two-dimensional
(2D) semimetal consisting of pure
sp2 hybridized C atoms in a hexagonal lattice conformation.[1] The graphene basal plane is inert and impenetrable
to most species.[2] For this reason, graphene
has been suggested to perform well as a physical barrier between metal
surfaces and oxidizing species, thus being suitable for corrosion
protection.[3−6] Graphene possesses additional properties that may be desirable for
coating applications, for example, high flexibility,[7] visual transparency,[8] and the
ultimate thinness of one atomic layer.Demonstrations of graphene
performing as an anticorrosion coating
for a range of metals, like Cu,[4,9−11] Pt,[12−14] Ni,[4,15,16] Ru,[17] Fe,[18] and stainless steel 304,[19] exposed to
various corrosive environments, such as air, seawater, O2, and CO, have been reported. Several studies, however, show that
wrinkles,[20−22] grain boundaries,[6,21] and atomic
and structural defects[22−24] lead to failure of the graphene coating. These imperfections
in the graphene layer can promote reactions with oxidizing species
and facilitate intercalation below the graphene cover. Once intercalation
occurs, intercalants are likely to diffuse also toward areas covered
by defect-free graphene sheets. The presence of graphene may, in such
cases, be antiprotective, since graphene here acts as a source of
electrons that stimulate galvanic corrosion processes on the metal
surface.[25] Therefore, attempts to eliminate
direct exposure of defective areas to reactive species have been explored.
For example, a few-layer graphene coating makes a direct horizontal
overlap between defects in the different layers unlikely, which in
turn increases the diffusion length for intercalating species toward
the metal surface. This makes few-layer graphene more efficient as
a coating.[3,5,26] Alternatively,
improvement of the coating by passivation of defects in graphene using
Cu adatoms has also been demonstrated.[24]It has previously been suggested that graphene–metal
systems
exhibiting a high interaction at their interface are less prone to
intercalation, when compared to weakly interacting systems.[27] Here we investigate the effect of increasing
the interaction in graphene–metal systems via chemical functionalization.
The test system is graphene on an Ir(111) substrate. This system represents
a weakly bound van der Waals system with an average binding energy
of 55 meV/C atom.[28] Upon CO intercalation
the binding energy drops to 22 meV/C atom. Hence, for intercalation
to proceed, the energy gain from the newly formed Ir–CO interaction
must exceed the energy cost associated with decoupling the graphene
sheet. The condition can be met when a sufficient amount of CO covers
the Ir(111) surface, which consequently determines a critical CO pressure
for intercalation to occur.[28−30] This behavior indicates that
by increasing the interaction between graphene and the Ir substrate
it may be possible to prevent the intercalation process if sufficiently
large interaction strength can be achieved.While the graphene
sheet interacts weakly with Ir(111),[31,32] the interaction
is modulated with a ∼25 Å periodicity
due to a mismatch of ∼10% between the lattice constants of
graphene and Ir(111).[33] See a sideview
sketch of graphene on Ir(111) in Figure a. The largest interaction is found in areas
of the moiré unit cell called the hexagonal close-packed (HCP)
and face-centered cubic (FCC) areas, and the graphene–Ir distance
is smallest here.[31] In earlier work we
demonstrated that when H atoms chemisorb on top of C atoms in HCP
and FCC areas, graphane-like structures[34,35] are formed.
These single-sided hydrogenation structures represent clusters of
fully sp3 hybridized C atoms with alternating C–H
and C–Ir bonds. See the sideview sketch of hydrogenated graphene
on Ir(111) in Figure c. The functionalization with hydrogen therefore leads to an increased
interaction strength in certain areas through covalent bond formation
to the substrate. We also note that the most stable graphane-like
clusters were found to be those comprising 7 to 12 C–H bonds,
as revealed by scanning tunneling microscopy (STM) and density functional
theory (DFT).[36]
Figure 1
Sketch of (a) graphene
on Ir(111), (b) CO intercalated graphene
on Ir(111), (c) hydrogenated graphene on Ir(111), and (d) hydrogenated
graphene on Ir(111) after CO exposure (not intercalated).
Sketch of (a) graphene
on Ir(111), (b) CO intercalated graphene
on Ir(111), (c) hydrogenated graphene on Ir(111), and (d) hydrogenated
graphene on Ir(111) after CO exposure (not intercalated).
Results and Discussion
CO Intercalation
In the following, we demonstrate how
H-functionalization of graphene and subsequent carbon–metal
bond formation can be used to prevent the intercalation of CO molecules
at the graphene–Ir interface, as sketched in Figure . We first measure the conditions
that lead to intercalation of CO at the metal interface for Gr/Ir(111)
and compare this to hydrogen-functionalized graphene (H-Gr/Ir(111))
at different stages of functionalization. We show that from a certain
degree of H-functionalization the H-graphene coating eliminates intercalation
under all tested conditions. X-ray photoelectron spectra (XPS) of
the C 1s, Ir 4f7/2, and O 1s core levels were obtained
on the Gr/Ir(111) sample before and after the CO test exposure and
are presented in Figure a,b,c, respectively. Throughout this article the CO test exposure
conditions, which lead to CO intercalation below a nonfunctionalized
graphene coating, were 1 mbar CO with the sample kept at 473 K for
10 min. The temperature of 473 K was chosen, as it is below the desorption
temperature of CO from Ir(111) (523 K, this work, not shown) but sufficiently
high to enhance the intercalation rate. All XPS measurements related
to CO exposure were performed after reduction of the CO pressure to
5 × 10–8 mbar, keeping the sample at 473 K.
The C 1s core-level spectrum for the clean Gr/Ir(111) (Figure a, bottom panel) is fit using
a single component, Cc, at 284.1 eV binding energy, representing sp2 hybridized C atoms on the Ir(111) surface.[36−38] Upon exposure
to CO, two new components, Ci and CCO, are observed in
the corresponding C 1s core-level spectrum, presented in Figure a, top panel. The
Ci component, positioned at a binding energy of −0.37 eV relative
to Cc, represents the intercalated graphene. An induced downshift
in binding energy of more than 0.3 eV and a slight peak narrowing
following CO intercalation are consistent with the findings by Grånäs
et al.[28] The CCO peak at 286.2
eV represents the CO adsorbed on the Ir(111) surface below the graphene.
In Figure b the Ir
4f7/2 spectra for the sample before (bottom) and after
(top) CO intercalation are shown. For the clean Gr/Ir(111) sample,
the spectrum is fit using two components representing Ir bulk atoms
(IrB) and Ir surface atoms (IrS), positioned
at binding energies 60.79 and 60.28 eV, respectively. After CO intercalation, Figure b top, the IrS component has transformed into a new component, IrCO, at +0.23 eV relative to IrB. The IrCO component
is assigned to CO adsorbed on Ir surface atoms, below the graphene,
consistent with previous observations.[28]
Figure 2
XPS
core-level spectra of clean Gr/Ir(111) (bottom) and CO intercalated
Gr/Ir(111), after exposure to 1 mbar CO, for 10 min, with the sample
at 473 K (top). XPS measurements of the CO exposed sample were performed
after reducing the CO pressure to 5 × 10–8 mbar,
keeping the sample at 473 K. (a) C 1s (hν =
490 eV). (bottom) Clean Gr/Ir(111), fit using the Cc component. (inset)
A sideview sketch of nonintercalated Gr/Ir(111). (top) CO intercalated
Gr/Ir(111), fit using the Cc, Ci, and CCO components. (inset)
A sideview sketch of CO intercalated Gr/Ir(111). (b) Ir 4f7/2 (hν = 275 eV). (bottom) Clean Gr/Ir(111),
fit using the IrB and IrS components. (top)
CO intercalated Gr/Ir(111), fit using the IrB, IrS, and IrCO components. (c) O 1s (hν
= 735 eV). (bottom) Clean Gr/Ir(111), no oxygen species is present
on the surface. (top) CO intercalated Gr/Ir(111), fit using the OCO component.
XPS
core-level spectra of clean Gr/Ir(111) (bottom) and CO intercalated
Gr/Ir(111), after exposure to 1 mbar CO, for 10 min, with the sample
at 473 K (top). XPS measurements of the CO exposed sample were performed
after reducing the CO pressure to 5 × 10–8 mbar,
keeping the sample at 473 K. (a) C 1s (hν =
490 eV). (bottom) Clean Gr/Ir(111), fit using the Cc component. (inset)
A sideview sketch of nonintercalated Gr/Ir(111). (top) CO intercalated
Gr/Ir(111), fit using the Cc, Ci, and CCO components. (inset)
A sideview sketch of CO intercalated Gr/Ir(111). (b) Ir 4f7/2 (hν = 275 eV). (bottom) Clean Gr/Ir(111),
fit using the IrB and IrS components. (top)
CO intercalated Gr/Ir(111), fit using the IrB, IrS, and IrCO components. (c) O 1s (hν
= 735 eV). (bottom) Clean Gr/Ir(111), no oxygen species is present
on the surface. (top) CO intercalated Gr/Ir(111), fit using the OCO component.In the O 1s spectra in Figure c, clearly oxygen is only present on the surface after the CO intercalation (top). The component denoted
OCO thus stems from oxygen in the CO molecules.
Prevention
of CO Intercalation by H Functionalization
In Figure a–c,
bottom panels, we show the C 1s, Ir 4f7/2, and O 1s core-level
spectra of H-functionalized graphene (H-Gr/Ir(111)) prepared by exposure
of a 473 K Gr/Ir(111) sample to hot H atoms. The C 1s core-level spectrum
of H-Gr/Ir(111) in Figure a, bottom, is fit using the Cc component, representing clean
graphene, and three additional hydrogenation-related components: Ca,
Cb, and Cd, positioned with binding energies of +0.81, + 0.44, and
−0.27 eV relative to Cc, respectively.[37] The Ca component is assigned to H adsorption on Gr/Ir(111) away
from HCP and FCC regions of the moiré pattern, where C–Ir
bonds cannot be formed.[37] Such structures
are most likely hydrogen dimers, similar to those observed on hydrogenated
quasi-freestanding graphene, exemplified by graphite.[39] The Cb component is related to hydrogenation structures
in HCP and FCC areas of the Gr/Ir(111) moiré, where the formation
of graphane-like clusters is possible. The Cb component is thus directly
linked to the formation of C–Ir bonds.[35,37,38] The Cd component is related to hydrogen
vacancies in the graphane-like clusters and in general to sp2carbon atoms that are neighbors to sp3carbon.[37]
Figure 3
XPS core-level spectra of Gr/Ir(111) hydrogenated at 473
K (bottom)
and the same sample after a subsequent exposure to 1 mbar CO for 10
min with the sample at 473 K (top). XPS measurements of the CO exposed
sample were performed after reducing the CO pressure to 5 × 10–8 mbar, keeping the sample at 473 K. (a) C 1s (hν = 490 eV), (bottom) H-Gr/Ir(111) fit using the
Cc, Ca, Cb, and Cd components. (insets) Top- and side-view sketches
of Gr/Ir(111) hydrogenated at 473 K. Hydrogen clusters form on FCC
and HCP areas of the moiré unit cell, and dimer structures
form outside these areas. (top) H-Gr/Ir(111) after CO exposure, fit
using the Cc, Cb, and Cd components. No CO-related components are
present. (insets) Top- and side-view sketches of the hydrogenated
Gr/Ir(111) after the CO exposure, where only the most stable structures
are present. (b) Ir 4f7/2 (hν =
275 eV), (bottom) H-Gr/Ir(111) fit using the IrB, IrS, and IrG components. (top) H-Gr/Ir(111) after
CO exposure, fit using IrB, IrS, and IrG components. No CO-related components are present. (c) O 1s
(hν = 735 eV), (bottom) H-Gr/Ir(111), no oxygen
species are present. (top) H-Gr/Ir(111) after CO exposure, no CO or
other oxygen-related species are present.
XPS core-level spectra of Gr/Ir(111) hydrogenated at 473
K (bottom)
and the same sample after a subsequent exposure to 1 mbar CO for 10
min with the sample at 473 K (top). XPS measurements of the CO exposed
sample were performed after reducing the CO pressure to 5 × 10–8 mbar, keeping the sample at 473 K. (a) C 1s (hν = 490 eV), (bottom) H-Gr/Ir(111) fit using the
Cc, Ca, Cb, and Cd components. (insets) Top- and side-view sketches
of Gr/Ir(111) hydrogenated at 473 K. Hydrogen clusters form on FCC
and HCP areas of the moiré unit cell, and dimer structures
form outside these areas. (top) H-Gr/Ir(111) after CO exposure, fit
using the Cc, Cb, and Cd components. No CO-related components are
present. (insets) Top- and side-view sketches of the hydrogenated
Gr/Ir(111) after the CO exposure, where only the most stable structures
are present. (b) Ir 4f7/2 (hν =
275 eV), (bottom) H-Gr/Ir(111) fit using the IrB, IrS, and IrG components. (top) H-Gr/Ir(111) after
CO exposure, fit using IrB, IrS, and IrG components. No CO-related components are present. (c) O 1s
(hν = 735 eV), (bottom) H-Gr/Ir(111), no oxygen
species are present. (top) H-Gr/Ir(111) after CO exposure, no CO or
other oxygen-related species are present.The Ir 4f7/2 core-level spectrum for the H-Gr/Ir(111)
is shown in Figure b, bottom, and is fit with three components: The IrB,
IrS, and a new component, IrG, positioned with
a binding energy of +0.31 eV relative to the position of IrS. The IrG component corresponds to Ir surface atoms that
make bonds with C atoms from the graphene, in the graphane-like clusters,[37] as sketched in the insets of Figure . No oxygen is present on the
surface after hydrogenation, as evidenced by the featureless O 1s
signal in Figure c
bottom.The H-functionalized graphene sample was further exposed
to 1 mbar
CO with a sample temperature of 473 K for 10 min. The corresponding
C 1s spectra are presented in the top panels of Figure a–c. No indication of CO intercalation
is observed in the spectra, as there are no intercalation-related
components: No signal corresponding to CCO or Ci is observed.
Also, no oxygen-related species are present on the surface, as evidenced
by the featureless O 1s signal in Figure c top.Although the graphene overlayer
protects the metal from exposure
to CO at given conditions, a small decrease in the hydrogen coverage
is observed as revealed by the absence of the Ca component but also
by a minor decrease in the intensities of the Cb and Cd components.
The decrease in intensity of the C–H-related components is
accompanied by an increase of the Cc component indicating simple removal
of hydrogen by the CO exposure without any etching of the graphene.
From the disappearance of the Ca component it appears that CO efficiently
reacts with adsorbed dimer structures. The small decrease in the Cb
component points toward the removal of H from the periphery of large
graphane-like structures.An observed decrease of the IrG component in Figure b top concurs with
the minor decrease in Cb, as both IrG and Cb are linked
to graphane-like structures. Importantly, the absence of the IrCO component ascertains that no CO is adsorbed onto the Ir(111)
surface after the exposure. The results, summarized in Figure , therefore show that hydrogenated
graphene prevents the intercalation of CO at the graphene–metal
interface under conditions that would normally lead to CO intercalation
in the clean Gr/Ir(111) system.To test the limits of the H-functionalized
graphene, the sample
was further exposed to a 10 times higher pressure of CO (10 mbar)
with no observable signs of intercalation. The corresponding C 1s,
Ir 4f7/2, and O 1s spectra are shown in Figure after an exposure of 10 min,
bottom panels, and after an additional 60 min exposure, top panels.
The C 1s and Ir 4f7/2 core-level spectra show no features
related to CO intercalation in either case. Importantly, after the
initial decrease of H coverage under CO exposure evidenced by the
data displayed in Figure , no further decrease in hydrogenation level was observed
even for extended CO exposures, signifying the high stability of smaller
graphane-like clusters and the hydrogenated graphene layer in general.
Figure 4
XPS core-level
spectra of Gr/Ir(111), hydrogenated at 473 K, after
a subsequent exposure to 10 mbar CO for 10 min (bottom) and for 70
min (top) while kept at 473 K. XPS measurements of the CO exposed
sample were performed after reducing the CO pressure to 5 × 10–8 mbar, keeping the sample at 473 K. (a) C 1s (hν = 490 eV), (bottom) H-Gr/Ir(111) after 10 min CO
exposure, fit using the Cc, Cb, and Cd components. No CO-related components
are present. (top) H-Gr/Ir(111) after 70 min of CO exposure, fit using
the Cc, Cb, and Cd components. No CO-related components are present.
(b) Ir 4f7/2 (hν = 275 eV). (bottom)
H-Gr/Ir(111) after 10 min of CO exposure, fit using the IrB, IrS, and IrG components. No CO-related components
are present. (top) H-Gr/Ir(111) after 70 min of CO exposure, fit using
the IrB, IrS, and IrG components.
No CO-related components are present. (c) O 1s (hν = 735 eV). (bottom) H-Gr/Ir(111) after 10 min of CO exposure,
no oxygen species are present on the surface. (top) H-Gr/Ir(111) after
70 min of CO exposure; negligible oxygen is present on the surface.
XPS core-level
spectra of Gr/Ir(111), hydrogenated at 473 K, after
a subsequent exposure to 10 mbar CO for 10 min (bottom) and for 70
min (top) while kept at 473 K. XPS measurements of the CO exposed
sample were performed after reducing the CO pressure to 5 × 10–8 mbar, keeping the sample at 473 K. (a) C 1s (hν = 490 eV), (bottom) H-Gr/Ir(111) after 10 min CO
exposure, fit using the Cc, Cb, and Cd components. No CO-related components
are present. (top) H-Gr/Ir(111) after 70 min of CO exposure, fit using
the Cc, Cb, and Cd components. No CO-related components are present.
(b) Ir 4f7/2 (hν = 275 eV). (bottom)
H-Gr/Ir(111) after 10 min of CO exposure, fit using the IrB, IrS, and IrG components. No CO-related components
are present. (top) H-Gr/Ir(111) after 70 min of CO exposure, fit using
the IrB, IrS, and IrG components.
No CO-related components are present. (c) O 1s (hν = 735 eV). (bottom) H-Gr/Ir(111) after 10 min of CO exposure,
no oxygen species are present on the surface. (top) H-Gr/Ir(111) after
70 min of CO exposure; negligible oxygen is present on the surface.In summary, we find that hydrogenation
of graphene/Ir(111) at 473
K prevents intercalation of CO at the graphene–Ir interface
at CO pressure up to at least 10 times higher and at fluences at least
70 times higher than those leading to intercalation in the clean Gr/Ir(111)
system.
Hydrogenation at Elevated Temperature
In the following
we test the number density and distribution of C–Ir bonds necessary
for the successful prevention of CO intercalation. Two different samples
were prepared by hydrogenation at elevated sample temperatures of
645 and 695 K, respectively. The 645 K exposure delivers the most
stable hydrogen clusters, namely, graphane-like structures in HCP
areas only, as sketched at topview in the inset of Figure a. All other hydrogen configurations
are not stable at this temperature, but the hydrogenation degree in
the HCP areas is still high as demonstrated by STM measurements,[36] meaning that there is almost always one graphane-like
cluster per moiré unit cell.[36] Thus,
the 645 K exposure yields a homogeneous hydrogen coverage with localized
clusters of graphane-like areas, each of which contains the required
C–Ir bonds.
Figure 5
XPS core-level spectra of Gr/Ir(111) hydrogenated at 645
K (bottom
left) and at 695 K (top left) and subsequently exposed to 10 mbar
CO for 10 min while kept at 473 K (bottom and top right, respectively).
XPS measurements of the CO-exposed samples were performed after reducing
the CO pressure to 5 × 10–8 mbar, keeping the
sample at 473 K. (a) C 1s (hν = 490 eV). (bottom
left) 645 K H-Gr/Ir(111) fit using the Cc, Cb, and Cd components.
(inset) Sketches the situation where hydrogenation structures are
only present on HCP areas of the moiré unit cell. (bottom right)
645 K H-Gr/Ir(111) after CO exposure, fit using the Cc, Cb, and Cd
components. (top left) 695 K H-Gr/Ir(111) fit using the Cc and Cb
components. (top right) 695 K H-Gr/Ir(111) after CO exposure, fit
using the Cc, Ci, and CCO components. (b) Ir 4f7/2 (hν = 275 eV). (bottom) 645 K H-Gr/Ir(111)
after CO exposure, fit using the IrB, IrS, and
IrG components. (top) 695 K H-Gr/Ir(111) after CO exposure,
fit using the IrB, IrS, and IrCO components.
(c) O 1s (hν = 735 eV). (bottom) 645 K H-Gr/Ir(111)
after CO exposure, no oxygen species on the surface. (top) 695 K H-Gr/Ir(111)
after CO exposure, fit using the OCO component.
XPS core-level spectra of Gr/Ir(111) hydrogenated at 645
K (bottom
left) and at 695 K (top left) and subsequently exposed to 10 mbar
CO for 10 min while kept at 473 K (bottom and top right, respectively).
XPS measurements of the CO-exposed samples were performed after reducing
the CO pressure to 5 × 10–8 mbar, keeping the
sample at 473 K. (a) C 1s (hν = 490 eV). (bottom
left) 645 K H-Gr/Ir(111) fit using the Cc, Cb, and Cd components.
(inset) Sketches the situation where hydrogenation structures are
only present on HCP areas of the moiré unit cell. (bottom right)
645 K H-Gr/Ir(111) after CO exposure, fit using the Cc, Cb, and Cd
components. (top left) 695 K H-Gr/Ir(111) fit using the Cc and Cb
components. (top right) 695 K H-Gr/Ir(111) after CO exposure, fit
using the Cc, Ci, and CCO components. (b) Ir 4f7/2 (hν = 275 eV). (bottom) 645 K H-Gr/Ir(111)
after CO exposure, fit using the IrB, IrS, and
IrG components. (top) 695 K H-Gr/Ir(111) after CO exposure,
fit using the IrB, IrS, and IrCO components.
(c) O 1s (hν = 735 eV). (bottom) 645 K H-Gr/Ir(111)
after CO exposure, no oxygen species on the surface. (top) 695 K H-Gr/Ir(111)
after CO exposure, fit using the OCO component.Exposing the Gr/Ir(111) to hot H atoms, with the
sample at 695
K, yields an even lower hydrogen coverage, as some HCP areas are left
without a hydrogen cluster, giving pure graphene in the entire moiré
supercell.[36] Hence this sample with a lower
hydrogen coverage also exhibits a substantially decreased number of
C–Ir bonds.In Figure a the
C 1s core-level spectra of Gr/Ir(111) samples hydrogenated at 645
K, bottom left, and at 695 K, top left, are shown. The C 1s core-level
spectra after the exposure of both samples to 10 mbar CO while kept
at 473 K are shown in Figure a, bottom right and top right, respectively, for the 645 and
695 K case.After the 10 mbar CO exposure, the 645 K H-Gr/Ir(111)
remains unchanged,
and no sign of any intercalation is observed as revealed by the absence
of CO-related components in the C 1s (Figure a, bottom right) and Ir 4f7/2 (Figure b, bottom) core-level
spectra but also by the absence of oxygen-related features in the
O 1s spectrum (Figure c, bottom).On the contrary, the C 1s core-level spectrum for
the 695 K H-Gr/Ir(111),
after exposure to 10 mbar CO, resembles the spectrum of the CO intercalated
graphene and consequently can be fit using the Cc, Ci, and CCO components. Additionally, all sp3-related carbon components
are now transformed back to sp2 type, meaning all hydrogen
has been removed during the exposure.The Ir 4f7/2 spectrum in Figure b, top, also reveals that CO has intercalated
and hydrogen has desorbed from the graphene. This is evidenced by
the presence of the IrCO component and the absence of the
IrG component in the fit. The CO adsorption on the Ir(111)
is additionally confirmed by the presence of the OCO component
in the O 1s spectra.From Figure it
is thus evident that the Gr/Ir(111) hydrogenated at 645 K, that is,
with a single graphane-like cluster in each moiré unit cell,
prevents CO intercalation. The 695 K H-Gr/Ir(111) sample, however,
does not protect, and the CO exposure leads to the removal of hydrogen
and intercalation of CO at the graphene–Ir interface.Previous experiments show that CO intercalates under graphene on
Ir(111) at millibar pressures forming a (3√3 × 3√3)R30°
structure.[28] STM measurements show a coverage
of 0.7 ML, while DFT calculations predict binding energies of 1.59
eV per CO molecule. The CO intercalation results in a displacement
of the graphene layer from a height of 3.51 to 6.42 Å and a decrease
in graphene binding energy from 55 to 22 meV per carbon atom.[28] This results in a total binding energy for the
system of CO-intercalated graphene on Ir(111) of 0.93 eV per graphene
unit cell. This value can be compared to the binding energy of hydrogenated
graphene on Ir(111). For surfaces hydrogenated at 645 K STM measurements
show hydrogen coverages of 9%, indicating that 18% of C atoms are
bound to either H or Ir atoms. The hydrogenated areas are placed in
a regular array with a periodicity of ∼25 Å determined
by the moiré structure. DFT calculations show that hydrogenated
areas are pinned to the Ir(111) substrate at a distance of 2.2–2.4
Å, making the regularly functionalized structure incompatible
with CO intercalation. Binding energies per H atom are of the order
of 2.5 eV, resulting in a binding energy of 2.5 eV per graphene unit
cell in the hydrogenated areas,[36] which
makes this structure energetically more stable than the CO intercalation
structure. In the case of hydrogenation at 695 K the hydrogen coverage
falls below ∼8%, and missing hydrogen clusters in the hydrogenation
array locally allow for CO intercalation. At such low hydrogen coverages
the binding energy of CO dominates, and the hydrogenation structures
are destabilized and desorb either thermally or via interaction with
CO. The stability of the lower-temperature hydrogenation structures
against reactions with CO is ascribed to the high binding energies
(several eV) of these structures[36] and
indicate that they may also be stable against more corrosive species.
Conclusions
Hydrogenation of graphene on an Ir substrate
has been demonstrated
to lead to the formation of strong bonds between the graphene and
the metal substrate, which facilitate efficient prevention of intercalation
of CO at the graphene–metal interface, thus increasing the
protection of the graphene-based coating. The homogeneous distribution
of interfacial bonding across a large area was observed to yield a
protection against CO gas, up to at least 10 times higher pressure
and 70 times higher fluence than that required to intercalate a pure
graphene coating on Ir. Hydrogenated graphene on Ir(111) was used
as a model system, but the results may well be transferable to other
graphene-on-metal systems where interfacial C-metal bonds can form.
The reported method may thus provide a means to enhance the properties
of graphene-based materials as anticorrosion coating for metals.
Experimental Section
Gr/Ir(111)
samples were prepared in a dedicated chamber with a
base pressure of 5 × 10–10 mbar. A single-layer
graphene was grown using ethylene gas by a combination of temperature-programmed
growth (TPD) and chemical vapor deposition (CVD) as described elsewhere.[40,41] The Ir(111) crystals were cleaned by sputtering with high-energy
Ar (5 × 10–6 mbar) ions at room temperature,
followed by flash annealing to 1473 K. Afterward, oxygen (1 ×
10–7 mbar, flash annealing to 1073 K, and cooling
to 673 K) and hydrogen treatments (1 × 10–6 mbar, flash annealing to 1073 K, and cooling to 473 K) were performed
to remove residual amorphous carbon and any remaining oxygen, respectively.The CVDgraphene growth parameters were 17 cycles of flash annealing
to 1500 K in 5 × 10–7 mbar ethylene gas.The pristine graphene samples were shipped to Berkeley, California,
to perform the experiments at beamline 11.0.2, at the Advanced Light
Source, Lawrence Berkeley National Laboratory. The experiments were
performed under ultrahigh vacuum (UHV) conditions, with a base pressure
of 1 × 10–9 mbar. The samples were annealed
to 1100 K to desorb any contaminants, when reintroduced to UHV, prior
to experiments. Cleanliness of the graphene samples was confirmed
using XPS, after the introduction to, and annealing at, beamline 11.0.2.CO intercalation experiments were performed at beamline 11.0.2
by backfilling the chamber to pressures in the millibar range, measured
using a baratron gauge. The pressure was static in all cases. A high
degree of beam damage on the graphene was observed when irradiating
the sample at high CO pressure. The CO intercalation experiments were
therefore performed using conventional XPS, when the pressure was
reduced to 5 × 10–8 mbar after the CO exposures
at higher pressures. The decrease of the CO pressure was not observed
to affect the CO intercalation coverage over time. It can, however,
not be excluded that an even higher coverage and/or other intercalation
structures had been present during the high-pressure CO exposure.The formation of C–Ir bonds at the graphene–Ir interface
was obtained by exposing the Gr/Ir(111) to hot H atoms. The hot atoms
were produced by running H2 gas through a ∼2000
K W capillary, at a 4 × 10–7 mbar H2 pressure for 10 min, keeping the sample in line of sight and ∼15
cm from the capillary outlet. Samples were kept at 473 K (Figures and 4), 645 K (Figure , bottom panels), and 695 K (Figure , top panels) during hydrogenation. All hydrogenation
was performed at beamline 11.0.2.XPS C 1s, O 1s, and Ir 4f7/2 core-level data were fit
using Doniach–Šunjić functions[42] convoluted with Gaussian functions. The backgrounds were
fit using linear backgrounds (C 1s and O 1s) and Shirley-type backgrounds
(Ir 4f7/2). The shapes and positions of the components
used to fit C 1s and Ir 4f7/2 core-level spectra, representing
H-Gr/Ir(111), were based on the work by Balog et al.[37] Shapes and positions of the components used to fit C 1s
and Ir 4f7/2 spectra representing CO-intercalated Gr/Ir(111)
were based on the work by Grånäs et al.[28]
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Authors: Richard Balog; Bjarke Jørgensen; Louis Nilsson; Mie Andersen; Emile Rienks; Marco Bianchi; Mattia Fanetti; Erik Laegsgaard; Alessandro Baraldi; Silvano Lizzit; Zeljko Sljivancanin; Flemming Besenbacher; Bjørk Hammer; Thomas G Pedersen; Philip Hofmann; Liv Hornekaer Journal: Nat Mater Date: 2010-03-14 Impact factor: 43.841
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Authors: Jennifer L Achtyl; Raymond R Unocic; Lijun Xu; Yu Cai; Muralikrishna Raju; Weiwei Zhang; Robert L Sacci; Ivan V Vlassiouk; Pasquale F Fulvio; Panchapakesan Ganesh; David J Wesolowski; Sheng Dai; Adri C T van Duin; Matthew Neurock; Franz M Geiger Journal: Nat Commun Date: 2015-03-17 Impact factor: 14.919
Authors: Claus F P Kastorp; David A Duncan; Anders L Jørgensen; Martha Scheffler; John D Thrower; Tien-Lin Lee; Liv Hornekær; Richard Balog Journal: Faraday Discuss Date: 2022-08-25 Impact factor: 4.394