RF Sputtering Coating Techniques
RF Sputtering Coating Techniques
Radio frequency (RF) sputtering is a technique that is used to create thin films, such as those found in the computer and semiconductor industry. Like direct current (DC) sputtering, this technique involves running an energetic wave through an inert gas to create positive ions. The target material, which will ultimately become the thin film coating, is struck by these ions and broken up into a fine spray that covers the substrate, the inner base of the thin film. RF sputtering differs from DC sputtering in the voltage, system pressure, sputter deposition pattern, and ideal type of target material.
During the sputtering process, the target material, substrate, and RF electrodes begin in a vacuum chamber. Next, the inert gas, which is usually argon, neon, or krypton, depending on the size of the target material’s molecules, is directed into the chamber. The RF power source is then turned on, sending radio waves through the plasma to ionize the gas atoms. Once the ions begin to contact the target material, it is broken into small pieces that travel to the substrate and begin to form a coating.
Typical Application of DC & RF Sputtering Techniques
Since RF sputtering uses radio waves instead of a direct electron current, it has different requirements and effects on the sputtering system. For instance, DC systems require between 2,000 and 5,000 volts, while RF systems require upwards of 1012 volts to achieve the same rate of sputter deposition. This is largely because DC systems involve the direct bombardment of the gas plasma atoms by electrons, while RF systems use energy to remove the electrons from the gas atoms’ outer electron shells. The creation of the radio waves requires more power input to achieve the same effect as an electron current. While a common side effect of DC sputtering involves a charge build-up on the target material from the large number of ions in the chamber, overheating is the most common issue with RF systems.
As a result of the different powering method, the inert gas plasma in an RF system can be maintained at a much lower pressure of less than 15 mTorr, compared to the 100 mTorr necessary for optimizing DC sputtering. This allows for fewer collisions between the target material particles and the gas ions, creating a more direct pathway for the particles to travel to the substrate material. The combination of this decreased pressure, along with the method of using radio waves instead of a direct current for the power source, makes RF sputtering ideal for target materials that have insulating qualities.
High quality ITO thin films grown by dc and RF sputtering without oxygen
High quality indium tin oxide (ITO) thin films were grown without oxygen by both dc and RF magnetron sputtering techniques on glass substrates. The effects of substrate temperature, film thickness and sputtering method on the structural, electrical and optical properties of the as-grown films were investigated. The results showed that the substrate temperature had substantial effects on the film properties, in particular on the crystallization and resistivity. When the substrate temperature was increased to 150 °C, crystallization in the (2 2 2) plane started appearing for both dc and RF sputtered films. We additionally found that with further increments of substrate temperature, the preferred crystallization orientation changed differently for DC and RF sputtered films. Optical transmission in the visible region for a film thickness of 70 nm was found to be above 85%. The bandgap was calculated to be about 3.64 eV for the substrate temperature of 150 °C for a 70 nm thick film. The value of the bandgap increased with respect to the increment in film thickness as well as substrate temperature. We also measured the temperature dependence of the resistivity and Hall coefficient of the films, and calculated the carrier concentration and Hall mobility. Very low room temperature resistivities for dc and RF magnetron sputtered grown films of about 1.28 × 10−4 Ω cm and 1.29 × 10−4 Ω cm, respectively, were obtained.