The relative sensitivity factor is practically useful for semi-quantitative analysis by X-ray photoelectron spectroscopy (XPS). The accurate values relative to C 1s peak, however, are not simply determined, since the carbonaceous contamination level on the standard samples is not always estimated correctly.We are dealing with the carbonization and graphitization of organic polymer films such as polyimide films which are known to be good precursors of highly oriented graphite films. It is known that upon the carbonization of nitrogen-containing polymers such as polyimides, the nitrogen atoms remain in the carbonized films 1-3 and affect the graphitization subsequently carried out. 4 Therefore, information on the chemical state and amount of nitrogen remaining in the carbonized films is essentially important. We have been studying the carbonization of different types of nitrogen-containing polymer films up to 1200˚C by XPS, and have reported on the transitions of the states of nitrogen with the carbonization time and temperature.3,5 So far, it has not been possible to estimate the surface composition of nitrogen accurately, because with some samples the relative intensity of N 1s peak to C 1s peak was proportional to the matrix composition determined by elemental analysis, but not with others. By accumulating a number of XPS data on various polymer films with different thicknesses, however, the difficulty was found to be due to the uniformity of carbonization, which depends on the thickness of the precursor films. In the present work, the relative sensitivity factor of N 1s/C 1s was determined by a statistical treatment of the experimental data.
ExperimentalThree types of polyimide films (Kapton, NOVAX and Upilex) and poly-p-phenylene-1,3,4-oxadiazole (POD) film on hand were used: the structure and thickness of the films are shown in Fig. 1. The N/C mole ratios in the film are all different. Carbonization was carried out at temperatures between 500 and 1200˚C for 1 h in a flow of high-purity argon. The heating rate was 400 K h -1 . After carbonization, the specimens were kept in a silica gel desiccator of non-grease type.The XPS measurements were carried out at the normal position by irradiating Mg K α X-rays (15 kV, 20 mA) with a VG Scientific ESCALAB MkII. The analyzer energy was fixed at 20 eV. The X-ray satellites were subtracted by the VG Eclipse data system. The binding energy, E B , was corrected by referring to the E B of Au 4f 7/2 electrons (84.0 eV) for gold particles sputtered on sample films. The integral intensities were calculated by subtracting background by the Shirley method:6 although this procedure is only an approximation 7 , it is useful and valid for uncomplicated spectra having similar background levels at both sides of the peak. 7,8 The energy ranges for background subtraction were selected to include shake-up satellites and plasmon peak.The elemental analysis of carbonized film was carried out by a conventional combustion method: about 3 mg of sample was heated up to 900˚C in a flow of oxy...