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Browsing by department "Fysiikan osasto"

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  • Odiyo, Alex Nyakumba (2019)
    Physical Vapour Deposition (PVD) is a method of thin film deposition that involves transport of materials in the gas phase through physical means. The greatest advantage of using PVD is its ability to deposit hard coatings that are almost impossible to deposit by other liquid or chemical deposition methods. The applications of PVD include semiconductor devices, cutting and drilling tools, optical coating for displays, and decorative coatings for jewellery. When PVD process is accompanied by a separate (noble) gas ion bombardment, it is termed as Ion Beam Assisted Deposition (IBAD). These two processes can be subjected to atomistic simulation as opposed to conventional experimental methods. The idea behind such a simulation is the level of control in terms of material purity, dimensionality and simulation parameters. In this simulation work, the growth and overall morphology of epitaxial growth of copper film under both PVD and IBAD is considered. The film roughness and intrinsic stress are subjected to testing under various deposition energies in PVD. The same properties are also tested under variation of bombardment energies, and bombarding rates or ion fluence in IBAD. The results show that the nature of the film growth is primarily dependent on the deposition energy. In PVD, low deposition energies lead to growth dominated by island growth, while high deposition energies are mainly layer-by-layer growth dominated. In IBAD done at a constant low atom deposition energy, a similar trend is seen with an increasing argon ion bombardment energy at 0.5 ions/nm2 fluence. Since the deposition energy of 1 eV is geared towards island growth, the conversion rate of island like structures to relatively layer-by-layer structure depends on the ion bombardment energy (IBAD case). By comparison of IBAD and PVD outcomes, it has been established that the best layered PVD film occurs at a deposition energy of 30 eV. The overall film quality (in PVD) with respect to layer-by-layer growth is much better than that deposited using IBAD at similar bombardment energy at an ion fluence 0.5 ions/nm2. However, to attain a comparable or superior layer-by-layer growth as PVD, IBAD process has to be conducted at a much higher bombardment energy (50 eV) at fluence of 0.5 ions/nm2. The other alternative is to undertake IBAD process at bombardment energy of 30 eV, and at a much higher ion fluence. At a fluence of 0.8 ions/nm2 and equivalent ion bombardment energy (30 eV) produces a far much superior structure to PVD growth. The tradeoff between which ion fluence to use in IBAD is the deposition rate. Higher ion fluence translates to slow deposition but much improved layer-by-layer structure. The stress profile shows a decreasing stress profile as a function of thickness as predicted by Stoney's equation. At non-equilibrium deposition conditions, the film is generally stressed. However, under optimal conditions for layer-by-layer growth, IBAD grown films are generally less stressed in comparison to PVD.
  • Turkki, Mikael (2023)
    Near-Earth asteroids (NEAs) are celestial objects whose perihelion is distinctively in the inner Solar System. As these objects orbit the Sun mainly outside of the main belt, they are a separate category of asteroids. A fraction of these asteroids is especially interesting due to their small albeit existing impact probability with Earth. As acts of constant attention and interest toward NEAs, several probes have been sent to study the objects. Since the 1990s, astronomers have discovered moons orbiting asteroids. These asteroid moons also exist in the NEA population. A fraction of the primary components of binary asteroids rotates especially fast. A cause for the fast spin rates is the Yarkovsky–O’Keefe–Radzievskii–Paddack (YORP) effect that affects the rotational period of irregularly shaped asteroids. Moreover, some asteroid moons may form due to the solar radiation phenomena of the YORP effect. Additionally, the Yarkovsky effect caused by thermal re-emission influences the orbits of NEAs over long time periods. A third potentially influencing solar radiation effect is the binary YORP (BYORP) effect, an explanatory theory for the relatively short life spans of asteroid moons. The thesis discusses NEAs, emphasizing binary asteroids, their formation, and observations. Ground-based equipment is used for a significant number of asteroid observations, making the fields interconnected. Optical telescopes and planetary radars offer diverse information on NEAs, whose discovery rates and orbital analysis have progressed prominently since the 1990s. As a case study of the observation methods, I discuss the ternary system (3122) Florence and its close encounter in September 2017 in the thesis.