Crystalline Sulfuric Acid in Ultrahigh Vacuum
J. Phys. Chem., Vol. 100, No. 50, 1996 19585
water is released from a film as it cools through ≈255 K,
approximately the temperature at which infrared spectra indicate
that crystallization occurs. All of these phenomena are associ-
ated with the cooling and/or crystallization of liquid H2SO4 +
H2O. The release of water is a consequence of the fact that
freezing, like melting, is incongruent, since the composition of
crystalline H2SO4 is different from that of liquid H2SO4 + H2O.
Water evolution below Tm indicates that the liquids pass through
a metastable, supercooled state as they cool. That the m/e 98,
80, and 18 cooling curves are not superimposable on their
corresponding heating curves is at least partly attributable to
the fact that the cooling films are metastable between 285 and
255 K: the vapor pressure of a metastable substances is always
greater than that of a stable substance. Because the vacuum
system is subjected to a gas load during heating, the higher mass
spectrometer signals upon cooling may also be associated with
pumping speed effects. However, it is unlikely that pumping
speed effects account for the different heating and cooling curves
in Figure 3. In our hands, the heating and cooling curves of an
80 ML crystalline ice film are nearly superimposable. If
pumping speed effects were responsible for all hysteresis in the
sulfuric acid cooling curves, they should be manifest as well in
the cooling curves of ice.
were studied some time ago by Kunzler19 and Giauque.16
They found that the mole fraction of H2SO4 in an equilibrium
H2SO4 + H2O solution at its boiling point smoothly increases
with decreasing externally applied pressure, from 0.920 at 1.33
× 105 Pa to 0.937 at 1.33 × 104 Pa. Extrapolation to UHV,
where the pressure is essentially zero, implies an H2SO4 mole
fraction of between 0.94 and 0.95 in an ultrathin liquid film at
its melting point. Since vapor pressure increases with temper-
ature, the composition of an H2SO4 + H2O mixture in
equilibrium with the gas phase changes with temperature.
Specifically, the solutions gradually become enriched in water.
This accounts, at least in part, for the different line shapes of
the m/e 98, 80, and 18 TPD spectra above the sulfuric acid
melting point.
Mass spectrometric and FTIRAS measurements of the cooling
H2SO4 + H2O films show that they do not freeze at Tm, but
supercool, eventually crystallizing at approximately 257 K, ≈30
K below Tm. Supercooling is a well-known phenomenon in
concentrated sulfuric acid solutions, which are viscous and reach
equilibrium slowly.20 However, it is surprising that recrystal-
lization is inhibited to such an extent in a film only several
tens of monolayers thick. Slow recrystallization may be due
in part to the fact that freezing requires the migration of excess
H2O from the film interior to the surface and its subsequent
expulsion into the gas phase. In any case, because supercooled
films of ultrathin sulfuric acid films are so stable, UHV
experiments on the surface of liquid sulfuric acid are now
possible. At 262 K, just above the transition temperature from
the supercooled liquid to the crystalline solid, the vapor pressure
of sulfuric acid is so low that the lifetime of an 80 ML thick
film is several minutes. Under such conditions, reactive and
nonreactive sticking of numerous gases can be investigated, as
can adsorbate and absorbate structure. These subjects are
currently under investigation in this laboratory.
Preliminary work suggests that the sulfuric acid freezing
kinetics are a function of film thickness and cooling rate. Thick
films freeze at lower temperatures than thin films, and the
freezing temperature decreases with increasing cooling rate. The
origin of these effects is currently under investigation, as is the
possibility that the freezing kinetics are influenced by the
underlying film substrate.
Discussion
The results presented herein establish that ultrathin films of
pure, crystalline sulfuric acid can be deposited on a Pt(111)
substrate in UHV and that the films melt incongruently at 285
K. The resulting liquids can be supercooled to ≈260 K (Tc),
at which temperature they crystallize. Also, the close cor-
respondence of the ultrathin film infrared spectra, as well as
Tm, Esub, and Evap, with those of macroscopic sulfuric acid
samples suggests that the properties of the ultrathin films are
essentially equal to those of bulk sulfuric acid. The significance
of these findings is twofold. First, they provide what is to our
knowledge the first observation of melting of a molecular solid
under ultrahigh vacuum. Detailed kinetic studies of the solid-
liquid and liquid-solid phase transitions in ultrathin sulfuric
acid films may now be carried out, as they were for the
amorphous-crystalline phase transition in ultrathin ice films.17,18
Second, by establishing a protocol for the preparation and
characterization of liquid and solid sulfuric acid in UHV, they
open the possibility of using UHV-based methods to probe
differences between the surface chemical properties of the solid
and liquid acids.
Note Added in Proof. Since this paper was submitted for
publication, a paper appeared concerning the surface composi-
tion of liquid H2SO4 + H2O solutions, as studied by Auger
electron spectroscopy and X-ray photoelectron spectroscopy.21
This work provides convincing evidence that molecular liquids
like sulfuric acid can be studied in ultrahigh vacuum.
Acknowledgment. This work was supported by the National
Science Foundation through Grant CHE-9527665.
References and Notes
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