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Thesis (M.S.)--University of Wisconsin--Madison, 1964. / eContent provider-neutral record in process. Description based on print version record.

A He³ cryostat was designed for steady state nuclear magnetic resonance measurements. The cryostat required about one liter of He³ at NTP. This amount of He³ was liquified at 1.2°K, which was the temperature of the surrounding liquid He⁴ bath, and then pumped on by means of a four-stage mercury diffusion pump. By this procedure, a liquid He³ temperature of 0.35 K was achieved and maintained for four hours. The r-f coil and sample were in direct contact with the liquid He³ to ensure sufficient heat transfer between the two. The temperature of the liquid He³ was measured by means of vapour pressure measurements of the evaporating He³ and by means of resistance measurements of a carbon resistance in contact with the liquid He³. The system was non-recirculating, since a total, uninterrupted run of four hours was considered long enough for most experiments. The He³ could also be retransferred within 20 minutes after such a run, and this process could be continued until in-sufficient quantities of liquid He⁴remained to cool the surroundings. / Science, Faculty of / Physics and Astronomy, Department of / Graduate

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A test cryostat was constructed to investigate the potential of a locally made thermal battery. A thermal battery is proposed to be a useful component in the construction of future superconducting fault current limiter (SFCL) systems. The heat generated from a SFCL under quench conditions can be conducted into a solid nitrogen thermal battery. This is an alternative to using a liquid cryogen which on evaporation would form a highly nonconductive vapour layer around the SFCL and could be potentially explosive. The relevant heat transfer mechanisms for cryostat design were analyzed to ensure that the cryostat was capable of solidifying nitrogen and thus be used as a thermal battery. The experimental stage was ultimately capable of reaching a temperature of 40 K. Using a resistor to mimic the normal state of a superconductor, the performance of the thermal battery was determined by subjecting it to transient thermal events. The effect of solid nitrogen crystal size was investigated by performing pulse tests on solid nitrogen formed at different rates. It was found that slowly formed solid nitrogen performed better and stabilised the resistor’s temperature more quickly. The phenomenon of ‘dry-out’ was also investigated for different formation rates by subjecting the solid nitrogen to multiple heating pulses. It was found to become very significant after the first pulse when using quickly formed solid nitrogen, but did not manifest in slowly formed solid nitrogen. / Thesis (M.Sc.Eng.)-University of KwaZulu-Natal, Durban, 2011.

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Thesis (Ph. D.)--Ohio State University, 2008. / Title from first page of PDF file. Includes bibliographical references (p. 115-116).

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The evidence supporting the presence of Dark Matter in the universe ranges over many length scales: from the rotational curves within galaxies that cannot be explained only by the dust and other visible component to the anisotropies in the cosmological microwave background that sets the most precise quantification for the DM content in the universe at 26.8% of the energy density. One of the candidates for DM with the most theoretical support is a family of particles that appear in extensions of the Standard Model of Particles. These new particles, known as Weakly Interacting Massive Particles (WIMPs), provide a natural solution to the missing mass in the universe that interact only via weak interaction and whose origin dates back from the very early universe. The XENON Dark Matter search experiments aim to the direct detection of WIMPs via scattering off xenon nuclei. Following the success of the first prototype, XENON10, the XENON100 detector has been, up to late 2013, the most sensitive DM detector setting an upper bound limit on the spin-independent WIMP-nucleon cross-section of 2. × 10 −45 cm 2 and the spin-dependent equivalent of 3.5 × 10 −44 cm 2 . The detector consists of a dual-phase xenon Time Projection Chamber (TPC) with an inner target of 62 kg, located at the un- derground facility at Laboratori Nazionali del Gran Sasso (LNGS) in Italy. XENON100 is still in operation, currently testing new calibration sources of potential use for the next generation XENON1T experiment, under commissioning in Hall B of LNGS, aims to im- prove the XENON100 sensitivity by two orders of magnitude by increasing the xenon target mass in the detector to the tonne scale and by reducing the intrinsic background rate and consequently, increase the expected number of WIMP events per year. The scale-up of a liquid xenon TPC imposes many technical challenges that needed to be addressed prior to the realization of the XENON1T phase of the project. The focus of my thesis work has been the research and development of Dark Matter detectors operated with a xenon mass at the tonne scale. In particular, the topic of purification of a large amount of Xe gas to reduce the concentration of electronegative impurities to levels below afew parts per billion in a reasonable amount of time has been a driver in my work with the XENON1T Demonstrator facility at the Columbia Nevis laboratories. Two complementary approaches were followed in order to address this problem: i) a study of the performance of XENON100 concerning the electron lifetime (eLT) among other parameters that depend on the purity and ii) the construction of a full-size Xe TPC prototype to test multiple technologies with the goal of an optimized XENON1T TPC, with several tonnes of Xe. In addition to my work on the XENON1T Demonstrator, I have also contributed to the operation and analysis of data from XENON100. In particular, I developed a cut based on the information theory concept of entropy to reduce the electronic noise in the data. A detailed description of the motivation and implementation of the entropy cut is presented in Chapter 3. The experience gained from the successful performance of XENON100 and the information from variety of measurements with the XENON1T Demonstrator have influenced the design of XENON1T and will impact other next-generation Dark Matter detectors using LXe in a TPC. More specifically, the design of the XENON1T cryogenic system which is at the heart of the experiment, has been guided by this experience. The testing of the system was performed at Nevis where the various components were assembled and leak checked before being shipped to LNGS. The XENON1T detector’s cryostat and its cryogenics system, designed by the Columbia University XENON group were installed underground in the Hall B of the LNGS laboratory in Summer/Fall 2014. Their commissioning represent a major milestone in the realization of XENON1T. The last chapter of the thesis summarizes the status of XENON1T, with particular focus on the design of the cryogenic, purification and cryostat system influenced by the R & D with the Demonstrator.

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