ABSTRACT
The adsorption of Ca on the MgO(100) surface at 300 K has been studied using microcalorimetry, in combination with LEED, AES, ISS, work function, sticking probability measurements, and density functional theory (DFT) calculations. The MgO(100) thin films (approximately 4 nm thick) were grown epitaxially on a 1 microm thick Mo(100) single-crystal. The sticking probability of Ca on MgO(100) at 300 K is unity. On the basis of AES and ISS measurements, it was determined that Ca grows mainly as 3D particles on the MgO(100) surface with a density of approximately 1 x 10(12) islands/cm2. Ca adsorbs initially at defect sites with a very high heat of adsorption (approximately 410 kJ/mol). DFT calculations attribute this high initial heat to Ca binding to kink sites (376 kJ/mol), step sites (205 kJ/mol), and lower concentrations of stronger binding sites. The heat of adsorption decreases rapidly with coverage, reaching a minimum of 162 kJ/mol at approximately 0.3 ML, where Ca is mainly adding to small 3D Ca clusters. Afterward, it increases to the value of bulk Ca heat of sublimation (178 kJ/mol) at approximately 1.2 ML, attributed to the increase in stability with increasing Ca particle size. A 1.0 eV decrease of the work function with Ca coverage from 0 to 0.3 ML indicates that Ca adsorbed at defects is cationic, in agreement with calculations showing that Ca donates electron density to the MgO. Light ion sputtering of the MgO(100) surface generates point defects, but these do not change the heat of adsorption versus coverage, implying that they do not nucleate Ca particles. Oxygen vacancies are a likely candidate; DFT calculations show that F and F+ center vacancies bind Ca more weakly than terrace sites. More extensive sputtering creates extended defects (such as steps and kinks) that adsorb Ca with heats of adsorption up to approximately 400 kJ/mol, similar to that at the intrinsic defect sites.
ABSTRACT
The adsorption of Ca atoms on pristine and electron-irradiated poly(methyl methacrylate) (PMMA) surfaces at 300 K has been studied by adsorption microcalorimetry, atomic beam/surface scattering, and low-energy He+ ion scattering spectroscopy (ISS). On pristine PMMA, the initial sticking probability of Ca is 0.5, increasing quickly with Ca coverage. Below 0.5 ML, the heat of adsorption is 730-780 kJ/mol, much higher than Ca's sublimation energy (178 kJ/mol). The Ca here is invisible to ISS, which is attributed to Ca binding to ester groups below the CH3/CH2-terminated PMMA surface. The adsorption energy increases with coverage, suggesting attractions between neighboring Ca-ester complexes. Above 0.5 ML, Ca starts to grow as three-dimensional (3D) Ca clusters on top of the surface, which dominate growth after 2 ML. It is proposed that each Ca reacts with two esters to form the Ca carboxylate of PMMA, because this reaction's heat would be close to that observed. The total amount of Ca that binds to subsurface sites is estimated from the integral heat of adsorption to involve 4-6 layers of ester groups. Exposing the PMMA surface to electrons increases Ca's initial sticking probability but lowers its adsorption energy. This is attributed to electron-induced defects acting as nucleation sites for 3D Ca islands, whose growth now competes kinetically with Ca diffusing to subsurface esters. Consequently, only two layers of subsurface esters get populated at saturation. The heat eventually reaches Ca's bulk heat of sublimation on all PMMA surfaces, where pure, bulk-like Ca thin films form.
