三萘基膦在Ag(110)面上沉积的紫外光电子能谱研究

利用紫外光电子能谱（UPS）对新型有机半导体三萘基膦（TNP）在金属Ag(110)表面上沉积生长及其电子性质等进行了研究.三萘基膦的价带谱峰分别位于费米能级以下38，63，93和110 eV处，其中，价带顶 (HOS)位于费米能级以下约25 eV处.清洁Ag(110)表面的功函数为43 eV.随着三萘基膦在Ag(110)表面的沉积，功函数减小到38 eV，并达到饱和.根据UPS的测量结果，给出了三萘基膦/Ag(110)界面的能带结构，且三萘基膦与衬底Ag之间呈弱相互作用行为. 关键词： 紫外光电子谱 价电子结构 功函数     

tetracene 分子在Ru(1010)表面的吸附结构及其电子态研究

利用紫外光电子能谱(UPS)、角分辨紫外光电子能谱(ARUPS)和扫描隧道显微镜(STM)等方法研究了tetracene分子在Ru(1010)表面上吸附的电子态，吸附位置和吸附取向.UPS实验显示，与tetracene分子有关的光电子谱峰在费米能级以下2.1, 3.5, 4.8, 6.0, 7.1和9.2 eV处；ARUPS 结果表明，tetracene分子的分子平面基本平行于衬底表面；从STM图像中可以看到tetracene分子的长轴沿［0001］和［1210］两个晶向.基于密度泛函理论的从头算计算证实了上述结论.当分子长轴沿［0001］晶向时，分子中心位置在衬底表面的“短桥位”上，当分子长轴沿［1210］晶向时，分子中心位置在衬底表面的“四原子中心空位”上. 关键词： tetracene分子 Ru(1010)表面 吸附结构 吸附电子态     

tetracene分子在Ru(100)表面的吸附结构及其电子态研究

利用紫外光电子能谱(UPS)、角分辨紫外光电子能谱(ARUPS)和扫描隧道显微镜(STM)等方法研究了tetracene分子在Ru(100)表面上吸附的电子态,吸附位置和吸附取向.UPS实验显示,与tetracene分子有关的光电子谱峰在费米能级以下2.1,3.5,4.8,6.0,7.1和9.2eV处;ARUPS结果表明,tetracene分子的分子平面基本平行于衬底表面;从STM图像中可以看到tetracene分子的长轴沿[0001]和[1■10]两个晶向.基于密度泛函理论的从头算计算证实了上述结论.当分子长轴沿[0001]晶向时,分子中心位置在衬底表面的“短桥位”上,当分子长轴沿[1210]晶向时,分子中心位置在衬底表面的“四原子中心空位”上.     

Ag(110)表面吸附酞菁铜分子的紫外光电子谱研究

用紫外光电子能谱(UPS)研究了酞菁铜分子在Ag(110)单晶表面上的吸附，随着酞菁铜分子覆盖度增加，衬底Ag的3d电子信号逐渐减弱，在此能带区域出现两个新的谱峰，这两个与吸附有机分子轨道有关的谱峰的束缚能分别为4.45 和6.36 eV.随着覆盖度的增加，在结合能为1.51和9.20 eV处又出现了两个谱峰，它们同样来自吸附有机分子的轨道.随着覆盖度的继续增加，上述四个谱峰的强度逐渐增加，其能量位置均发生了明显的偏移.根据角分辨光电子能谱的实验结果，酞菁铜分子的分子平面基本与衬底表面平行.密度泛函理论计     

Ag(110)表面吸附酞菁铜分子的紫外光电子谱研究

用紫外光电子能谱(UPS)研究了酞菁铜分子在Ag(110)单晶表面上的吸附,随着酞菁铜分子覆盖度增加,衬底Ag的3d电子信号逐渐减弱,在此能带区域出现两个新的谱峰,这两个与吸附有机分子轨道有关的谱峰的束缚能分别为4.45 和6.36 eV.随着覆盖度的增加,在结合能为1.51和9.20 eV处又出现了两个谱峰,它们同样来自吸附有机分子的轨道.随着覆盖度的继续增加,上述四个谱峰的强度逐渐增加,其能量位置均发生了明显的偏移.根据角分辨光电子能谱的实验结果,酞菁铜分子的分子平面基本与衬底表面平行.密度泛函理论计 关键词： 酞菁铜 紫外光电子谱 吸附电子态 密度泛函理论     

CO分子与碱金属原子在Fe(110)表面上的相互作用

本文介绍了CO分子分别与K原子或Na原子在Fe(110)表面上共吸附的研究。角分辨率紫外光电子能谱(ARUPS)的结果表明,碱金属原子在Fe(110)表面上的存在,紫外光电子能谱中出现了结合能低于通常CO分子1π能级的新峰。该峰位于费密能级以下6.3eV处,是C0在碱金属影响下电子结构改变的结果。该峰的出现对应着CO分子处于C—O键明显减弱的状态。偏振紫外光电子能谱的研究表明:6.3eV处的谱峰联系的电子轨道有一个对称平面和一个反对称平面,分别平行于<001>晶向和<110>晶向。CO分子轨道的对称性不因 关键词：     

O在预覆盖K的Ag(110)表面的共吸附及其性质

本文用X射线光电子能谱(XPS),紫外光电子能谱(UPS),电子能量损失谱(EELS)和低能电子衍射(LEED)研究了O与预覆盖K的Ag(110)表面相互作用及其性质。在低覆盖度K下,发现有两种O的吸附态,经鉴别为溶解到表面下的O^2-和表面上吸附的O^x-增加K的覆盖度,出现分子状态的吸附物O₂^δ-,它与表面下存在的K相联系。XPS和UPS均清楚地显示出对应于三种不同吸附态的光电子发射峰。Ag(110)表面预覆盖K后的粘滞系数大大增加。K和O的共吸附引起它们彼此向Ag(110)表面下的溶解。LEED实验结果表明,清洁Ag(110)表面覆盖单层K原子后衍射图形从(1×1)变到(1×2),再吸附O后表面吸附层结构变为(2×1)。另外,结合UPS和EELS测量初步考察了O/K/Ag(110)共吸附系统的电子结构。本文还提出了一个共吸附模型来解释这些现象。 关键词：     

用ARUPS研究在Cs/Ru(1010)面上的CO分子轨道对称性

用同步辐射角分辨紫外光电子能谱对CO与Cs在Ru(1010)面上共吸附的研究结果表明,由于Cs的强烈影响,CO的分子轨道重新排列.对应清洁表面上CO分子的(5σ+1π)轨道的7.5eV谱峰分裂成两个,分别处于6.3和7.8eV,6.3eV谱峰关于一个垂直于Ru(1010)面而平行于〈0001〉晶向的镜象面反对称性. 关键词：     

有机半导体外延生长的扫描隧道显微镜研究

有机半导体薄膜的光、电等性质取决于有机分子的取向以及长程有序性.研究有机半导体的生长机理以及内在驱动力是一个重要环节.文章通过两个典型生长体系,perylene在Ru(0001)表面上的生长和tetracene在Ag(110)表面上生长过程的介绍,给出了形成有机半导体晶化薄膜的可能性以及决定其有序生长的内在驱动力.对于perylene在Ru(0001)表面上的生长,决定其过程的主要驱动力是分子间的相互排斥作用,在单分子层时,由于这种相互作用导致形成Ru(0001)-12×12-8 perylene有序超结构.而对于tetracene/Ag(110)体系,决定生长的驱动力主要表现为相互吸引作用,因此,在小于单分子层时,tetracene呈有序的岛状生长;而当tetracene膜的厚度大于单分子层时,呈逐层生长模式,并形成具有正交晶系结构的晶化薄膜.     

OPCOT在Ru(0001)表面上的紫外光电子能谱研究

采用紫外光电子能谱,研究了新型有机发光材料八芳基环辛四烯(OPCOT)在金属Ru(0001)表面上的电子结构,以及它们之间的相互作用.位于费米能级以下43,69,93和114eV处的4个谱峰分别来自于OPCOT材料中苯环的πCC,σCC,σCH和σHH轨道,位于30eV处的谱峰反映了8个苯环聚合后具有π轨道特性的C—C键.OPCOT材料的价带顶位于费米能级以下25eV处,OPCOT材料在Ru(0001)表面上的功函数为395eV.150℃以下,OPCOT材料可以在Ru(0001)表面稳定存在.随温度的升高,OPCOT材料主要以脱附的形式减少 关键词： 八芳基环辛四烯 光电子能谱 价电子结构 脱附     

Low energy electron diffraction and electron spectroscopy studies of the clean (110) and (100) titanium dioxide (rutile) crystal surfaces

Low-energy electron diffraction (LEED), Auger electron spectroscopy (AES), electron energy loss (ELS) and ultraviolet photoemission spectroscopies (UPS) were used to study the structures, compositions and electron state distributions of clean single crystal faces of titanium dioxide (rutile). LEED showed that both the (110) and (100) surfaces are stable, the latter giving rise to three distinct surface structures, viz. (1 × 3), (1 × 5) and (1 × 7) that were obtained by annealing an argon ion-bombarded (100) surface at ~600,800 and 1200° C respectively. AES showed the decrease of the $\text{O(510 eV)}\text{Ti(380 eV)}$ peak ratio from ~1.7 to ~1.3 in going from the (1 × 3) to the (1 × 7) surface structure. Electron energy loss spectra obtained from the (110) and (100)?(1 × 3) surfaces are similar, with surface-sensitive transitions at 8.2, 5.2 and 2.4 eV. The energy loss spectrum from an argon or oxygen ion bombarded surface is dominated by the transition at 1.6 eV. UPS indicated that the initial state for this ELS transition is peaked at ?0.6 eV (referred to the Fermi level E_F in the photoemission spectrum, and that the 2.4 eV surface-sensitive ELS transition probably arises from the band of occupied states between the bulk valence band maximum to the Fermi level. High energy electron beams (1.6 keV 20 μA) used in AES were found to disorder clean and initially well-ordered TiO₂ surfaces. Argon ion bombardment of clean ordered TiO₂ (110) and (100)?(1 × 3) surfaces caused the work function and surface band bending to decrease by almost 1 eV and such decrease is explained as due to the loss of oxygen from the surface.     

Chemisorption and reaction of NH3 on Ni(111)

The chemisorption of ammonia on Ni(111) has been investigated using LEED, thermal desorption, and angle-resolved photoemission. For exposures at 200 K, thermal desorption shows a coverage-dependent binding energy associated with dipole-dipole interactions. A (2 × 2) LEED pattern occurs at 2–4 L exposure. Time dependence of the LEED pattern and changes in the thermal desorption induced by the LEED beam indicate that the (2 × 2) pattern is due to a stable intermediate decomposition species. Using synchrotron radiation photoemission all three valence orbitals of ammonia have been observed for the first time. The energies of the ammonia-induced features in the photoemission (?22.0, ?11.0 and ?6.7 eV below the Fermi energy) and the observed symmatries positively identify the absorbed species as molecular ammonia. Additional structure observed in the photoemission spectra after electron bombardment is associated with the stable adsorbed intermediate.     

Investigation of the Shockley surface state on clean and air-exposed Au (1 1 1)

Scanning tunneling microscopy (STM) and spectroscopy (STS) carried out in vacuum and air were used to study the electronic structure of the Au (1 1 1) surface in the range of 0.0-0.7 eV below the Fermi level. The STS experiment carried out in UHV showed the existence of the Shockley surface state (SS) located 0.48 eV below the Fermi level. STS carried out in air showed strong local maximum located 0.35 eV below the Fermi level. This maximum was ascribed to the SS shifted toward lower energy due to carbon and oxygen overlayer. To confirm that the SS could exist on the sample exposed to air we did ultraviolet photoemission spectroscopy (UPS) experiment on air-treated and clean Au (1 1 1). Our results suggest that the SS position initially measured at 0.38 eV below the Fermi level was shifted to 0.27 eV after air treatment. Additionally, the level of contamination was measured using X-ray photoelectron spectroscopy (XPS).     

Interaction of NO and O2 with Pd(111) surfaces. I.

The adsorption of NO on Pd(111) was studied by means of LEED, UPS and thermal desorption measurements. Non-dissociative adsorption is characterized by additional maxima in the photomission spectra at 2.6, 9.2 and 14.6 eV below the Fermi level originating from chemisorption levels which are derived from the highest occupied molecular orbitais of NO. Thermal desorption takes place from three distinct states (α, β and γ) corresponding to binding energies of about 15, 17 and 31 kcal/mole, respectively, with about equal populations. The α-state is associated with a 2 × 2 LEED pattern and the β-state with a c4 × 2 structure, whereas the γ-state corresponds to disordered adsorption at low coverages. Plausible structure models are proposed for the ordered structures with θ = 0.75 for the α-state and θ = 0.5 for the β-state. The strong decrease of the adsorption energy is explained in terms of pronounced short-range repulsive interactions between neighbouring adsorbate molecules.     

A study of surface reproducibility and impurity segregation using ion neutralization and photoemission spectroscopies

We have studied the reproducibility of electron spectra obtained from a series of Si(111) surfaces on lightly doped crystals that were subjected to a common sputtering procedure but different subsequent heat treatments. Each of the surfaces displayed a sharp 7 × 7 LEED pattern and showed no impurities above the minimum detection limit of our Auger electron spectrograph. Ion neutralization spectroscopy (INS) and photoemission (UPS) at ?ω = 16.8 and 21.2 eV were used to obtain the electron spectra. From the observed differences in the electron spectra, the known characteristics of these spectroscopies, and a comparison with theory we conclude that these surfaces had small and differing amounts of impurity located principally in the selvedge or near-surface bulk rather than directly on or in the surface monolayer. The surface was cleaner than the near surface bulk. Longer heating of one sample to higher temperatures brought to the surface detectable amounts of Mo impurity that had diffused into the crystal from the Mo mounting clamps, changing the LEED pattern to √3 × √3(R 30°) and producing large modifications of both the INS and UPS spectra.     

Adsorption of 1,3,5-Triphenylbenzene Molecules and Growth of Graphene Nanoflakes on Cu(100) Surface

Adsorption of 1,3,5-triphenylbenzene(TPB) molecules on Cu( 100) surface is studied using ultraviolet photoelectron spectroscopy(UPS) and density functional theory(DFT) calculations. Researches on the bottom-up fabrication of graphene nanoflakes(GNFs) with TPB as a precursor on the Cu(100) surface are carried out based on UPS and DFT calculations. Three emission features d, e and f originating from the TPB molecules are located at 3.095, 7.326 and 9.349 eV below the Fermi level, respectively. With the increase of TPB coverage on the Cu(100) substrate, the work function decreases due to the formation of inter facial dipoles and charge(electron)rearrangement at the TPB/Cu(100) interface. Upon the formation of GNFs, five emission characteristic peaks of g, h, i, j and k originating from the GNFs are located at 1.100, 3.529, 6.984, 8.465 and 9.606 eV below the Fermi level, respectively. Angle resolved ultraviolet photoelectron spectroscopy(ARUPS) and DFT calculations indicate that TPB molecules adopt a lying-down configuration with their molecular plane nearly parallel to the Cu(100) substrate at the monolayer stage. At the same time, the lying-down configuration for the GNFs on the Cu(100) surface is also unveiled by ARUPS and DFT calculations.     

Study of chemisorption on copper low-index and stepped surfaces

Adsorption of CHCl₃, O₂, and hydrocarbons has been studied on Cu(111) and stepped surfaces using LEED, AES, and UPS at room temperature. We find that ordered Cl overlayers form upon Cu(111), Cu[3(111) × (100)], and Cu[5(111) × (100)] surfaces upon exposure to CHCl₃. Exposure to O₂ results in rearrangement of the Cu[5(111) × (100)] surface to hill-and-valley regions with large (111) areas, whereas Cu[2(111) × (100)] is stable for the same exposure. The photoemission spectra show new energy levels due to C1 above and below the Cu d band region and a small splitting of the halogen p orbitals. Effects consistent with interaction with the Cu d band are observed. Similar effects are observed with oxygen adsorption. The initial rate of Cl or O₂ chemisorption as measured by photoemission is proportional to the density of steps on these surfaces. Apparently, structural effects play an important role in chemisorption on metals (such as copper) with low density of states at the Fermi energy.