This collection includes most of the ASU Theses and Dissertations from 2011 to present. ASU Theses and Dissertations are available in downloadable PDF format; however, a small percentage of items are under embargo. Information about the dissertations/theses includes degree information, committee members, an abstract, supporting data or media.

In addition to the electronic theses found in the ASU Digital Repository, ASU Theses and Dissertations can be found in the ASU Library Catalog.

Dissertations and Theses granted by Arizona State University are archived and made available through a joint effort of the ASU Graduate College and the ASU Libraries. For more information or questions about this collection contact or visit the Digital Repository ETD Library Guide or contact the ASU Graduate College at gradformat@asu.edu.

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Description
Islamist groups in Somalia define themselves by their opposition. From the pre-Islamist movement of Mohammed Hassan in the nineteenth century to al-Itihaad al-Islaami in the twentieth to al-Shabaab in the twenty-first, Islamism exists as a form of resistance against the dominant power of the era. Furthermore these Islamist groups have

Islamist groups in Somalia define themselves by their opposition. From the pre-Islamist movement of Mohammed Hassan in the nineteenth century to al-Itihaad al-Islaami in the twentieth to al-Shabaab in the twenty-first, Islamism exists as a form of resistance against the dominant power of the era. Furthermore these Islamist groups have all been influenced by the type of state in which they exist, be it colonial, independent, or failed. This work seeks to examine the relationship between the uniquely Somali form of Islamism and the state. Through use of historical records, modern media, and existing scholarship this dissertation will chart the development of Islamism in Somalia from the colonial period to the present and explore the relationship Somali Islamism has with various forms of state.
ContributorsFurlow, Richard Bennett (Author) / Gallab, Abdullahi (Thesis advisor) / Talebi, Shahla (Committee member) / Ali, Souad (Committee member) / Arizona State University (Publisher)
Created2013
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Description
In this thesis, we present the study of several physical properties of relativistic mat- ters under extreme conditions. We start by deriving the rate of the nonleptonic weak processes and the bulk viscosity in several spin-one color superconducting phases of quark matter. We also calculate the bulk viscosity in the

In this thesis, we present the study of several physical properties of relativistic mat- ters under extreme conditions. We start by deriving the rate of the nonleptonic weak processes and the bulk viscosity in several spin-one color superconducting phases of quark matter. We also calculate the bulk viscosity in the nonlinear and anharmonic regime in the normal phase of strange quark matter. We point out several qualitative effects due to the anharmonicity, although quantitatively they appear to be relatively small. In the corresponding study, we take into account the interplay between the non- leptonic and semileptonic weak processes. The results can be important in order to relate accessible observables of compact stars to their internal composition. We also use quantum field theoretical methods to study the transport properties in monolayer graphene in a strong magnetic field. The corresponding quasi-relativistic system re- veals an anomalous quantum Hall effect, whose features are directly connected with the spontaneous flavor symmetry breaking. We study the microscopic origin of Fara- day rotation and magneto-optical transmission in graphene and show that their main features are in agreement with the experimental data.
ContributorsWang, Xinyang, Ph.D (Author) / Shovkovy, Igor (Thesis advisor) / Belitsky, Andrei (Committee member) / Easson, Damien (Committee member) / Peng, Xihong (Committee member) / Vachaspati, Tanmay (Committee member) / Arizona State University (Publisher)
Created2013
Description
ABSTRACT In this thesis, I probe into the ways in which the much-debated word Jihad lends itself to multifarious meanings within the Mourid Sufi Order and examine the foundations of the principles of peace and non-violence that informed the relationships between Cheikh Ahmadou Bamba, the founder of Mouridism (1853 ca

ABSTRACT In this thesis, I probe into the ways in which the much-debated word Jihad lends itself to multifarious meanings within the Mourid Sufi Order and examine the foundations of the principles of peace and non-violence that informed the relationships between Cheikh Ahmadou Bamba, the founder of Mouridism (1853 ca - 1927) and the French colonial state from 1883 to 1927. As a matter of fact, unlike some Senegalese Muslim leaders who had waged a violent Jihad during the colonial conquest and expansion, Cheikh Ahmadou Bamba promoted peaceful forms of Jihad which partook of his reform and revival movement in the Senegalese society. Yet, it is worth pointing out that the Mourid leader's ethics of peace and philosophy of non-violence as methods of struggle (the etymological sense of the word Jihad) during colonial times have been largely unexplored within academia. The contours of these new forms of resistance were grounded on a peaceful and non-violent approach which, according to Cheikh Ahmadou Bamba, was the only way to reach his spiritual, educational and social goals. This thesis proffers a counter-example to religious violence often associated with and perpetrated in the name of Islam. I argue in this thesis that a close investigation into Cheikh Ahmadou Bamba's epistemology of Jihad evidences that the term Jihad has spiritual, educational, social, cultural and economic functions which naturally contrast with its one-sided and violent connotation spotlighted over the last two decades. In conducting research for this work, I used a transdisciplinary approach that can allow me to address the complex issues of Jihad, peace and non-violence in a more comprehensive way. Accordingly, I have used a methodology that crosses the boundaries of several disciplines (historical, anthropological, sociological and literary).
ContributorsSeye, Cheikh (Author) / Haines, Charles (Thesis advisor) / Gallab, Abdullahi (Committee member) / Talebi, Shahla (Committee member) / Saikia, Yasmin (Committee member) / Arizona State University (Publisher)
Created2013
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Description
In this thesis I model the thermal and structural evolution of Kuiper Belt Objects (KBOs) and explore their ability to retain undifferentiated crusts of rock and ice over geologic timescales. Previous calculations by Desch et al. (2009) predicted that initially homogenous KBOs comparable in size to Charon (R ~ 600

In this thesis I model the thermal and structural evolution of Kuiper Belt Objects (KBOs) and explore their ability to retain undifferentiated crusts of rock and ice over geologic timescales. Previous calculations by Desch et al. (2009) predicted that initially homogenous KBOs comparable in size to Charon (R ~ 600 km) have surfaces too cold to permit the separation of rock and ice, and should always retain thick (~ 85 km) crusts, despite the partial differentiation of rock and ice inside the body. The retention of a thermally insulating, undifferentiated crust is favorable to the maintenance of subsurface liquid and potentially cryovolcanism on the KBO surface. A potential objection to these models is that the dense crust of rock and ice overlying an ice mantle represents a gravitationally unstable configuration that should overturn by Rayleigh-Taylor (RT) instabilities. I have calculated the growth rate of RT instabilities at the ice-crust interface, including the effect of rock on the viscosity. I have identified a critical ice viscosity for the instability to grow significantly over the age of the solar system. I have calculated the viscosity as a function of temperature for conditions relevant to marginal instability. I find that RT instabilities on a Charon-sized KBO require temperatures T > 143 K. Including this effect in thermal evolution models of KBOs, I find that the undifferentiated crust on KBOs is thinner than previously calculated, only ~ 50 km. While thinner, this crustal thickness is still significant, representing ~ 25% of the KBO mass, and helps to maintain subsurface liquid throughout most of the KBO's history.
ContributorsRubin, Mark (Author) / Desch, Steven J (Thesis advisor) / Sharp, Thomas (Committee member) / Christensen, Philip R. (Philip Russel) (Committee member) / Arizona State University (Publisher)
Created2013
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Description
A significant portion of stars occur as binary systems, in which two stellar components orbit a common center of mass. As the number of known exoplanet systems continues to grow, some binary systems are now known to harbor planets around one or both stellar components. As a first look into

A significant portion of stars occur as binary systems, in which two stellar components orbit a common center of mass. As the number of known exoplanet systems continues to grow, some binary systems are now known to harbor planets around one or both stellar components. As a first look into composition of these planetary systems, I investigate the chemical compositions of 4 binary star systems, each of which is known to contain at least one planet. Stars are known to vary significantly in their composition, and their overall metallicity (represented by iron abundance, [Fe/H]) has been shown to correlate with the likelihood of hosting a planetary system. Furthermore, the detailed chemical composition of a system can give insight into the possible properties of the system's known exoplanets. Using high-resolution spectra, I quantify the abundances of up to 28 elements in each stellar component of the binary systems 16 Cyg, 83 Leo, HD 109749, and HD 195019. A direct comparison is made between each star and its binary companion to give a differential composition for each system. For each star, a comparison of elemental abundance vs. condensation temperature is made, which may be a good diagnostic of refractory-rich terrestrial planets in a system. The elemental ratios C/O and Mg/Si, crucial in determining the atmospheric composition and mineralogy of planets, are calculated and discussed for each star. Finally, the compositions and diagnostics of each binary system are discussed in terms of the known planetary and stellar parameters for each system.
ContributorsCarande, Bryce (Author) / Young, Patrick (Thesis advisor) / Patience, Jennifer L (Thesis advisor) / Anbar, Ariel D (Committee member) / Arizona State University (Publisher)
Created2013
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Description
Recent research has identified affirmation of transcendence and exposure to violent Bible verses as being related to greater prejudice toward value-violating out-groups (Blogowska & Saroglou, 2012; Shen et al., 2013). Effects of exposure to specific Bible verses on attitudes toward out-groups have not been measured in combination with the Post-Critical

Recent research has identified affirmation of transcendence and exposure to violent Bible verses as being related to greater prejudice toward value-violating out-groups (Blogowska & Saroglou, 2012; Shen et al., 2013). Effects of exposure to specific Bible verses on attitudes toward out-groups have not been measured in combination with the Post-Critical Belief Scale developed by Hutsebaut (1996). The relationships between exposure to scriptural endorsements of prejudice, affirmation vs. disaffirmation of transcendence, literal vs. symbolic processing of religious content, and prejudice toward value-violating out-groups were examined using an online survey administered to a sample of U.S. adults (N=283). Greater affirmation of transcendence scores were linked to greater prejudice toward atheists and homosexuals and more favorable ratings of Christians and highly religious people. Lower affirmation of transcendence scores were linked to less favorable ratings of Christians and highly religious people and more favorable ratings of atheists. Exposure to scriptural endorsements of prejudice did not have a significant effect on levels of prejudice in this study.
ContributorsGrove, Richard (Author) / Robles, Elías (Thesis advisor) / Hall, Deborah (Committee member) / Schweitzer, Nicholas (Committee member) / Arizona State University (Publisher)
Created2013
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Description
This study aimed to fill the gap in research with regards to how individuals who define themselves as LGBT (lesbian, gay, bisexual, and transgendered) and devoutly religious (either currently or in the past) manage the interaction between these two conflicting identities. The researchers conducted 8 semi-structured qualitative interviews to examine

This study aimed to fill the gap in research with regards to how individuals who define themselves as LGBT (lesbian, gay, bisexual, and transgendered) and devoutly religious (either currently or in the past) manage the interaction between these two conflicting identities. The researchers conducted 8 semi-structured qualitative interviews to examine how these individuals manage this conflict and what affects these individuals experience internally and externally. To analyze the interviews, researchers used an open coding method to determine the common themes amongst the participants. Results indicated that these participants traveled a similar path when attempting to manage the conflict between their religion and sexuality and similar internal and external affects were experienced amongst the participants.
ContributorsWheeler, Heather (Author) / Gerdes, Karen (Thesis advisor) / Klimek, Barbara (Committee member) / Segal, Elizabeth (Committee member) / Arizona State University (Publisher)
Created2013
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Description
A novel about an Orthodox priest who seeks solace in Greece after the death of his wife. While Father Christopolous struggles to find forgiveness and restoration in the Paschal celebration, he grows increasingly entangled with a young priest-activist and his striking, self-destructive wife. Amid the tumult of a country in

A novel about an Orthodox priest who seeks solace in Greece after the death of his wife. While Father Christopolous struggles to find forgiveness and restoration in the Paschal celebration, he grows increasingly entangled with a young priest-activist and his striking, self-destructive wife. Amid the tumult of a country in political upheaval, he unravels the secrets of his hosts and confronts truths about his own marriage that threaten his faith and his place in the world. Set over the course of Holy Week, the novel explores the tensions in the bodily experience of faith and in the dichotomy between the knowledge of the mind and that of the heart.
ContributorsHynes, Sarah (Author) / Mcnally, Thomas M (Thesis advisor) / Ison, Tara (Committee member) / Pritchard, Melissa (Committee member) / Arizona State University (Publisher)
Created2013
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Description
Solar system orbital dynamics can offer unique challenges. Impacts of interplanetary dust particles can significantly alter the surfaces of icy satellites and minor planets. Impact heating from these particles can anneal away radiation damage to the crystalline structure of surface water ice. This effect is enhanced by gravitational focusing for

Solar system orbital dynamics can offer unique challenges. Impacts of interplanetary dust particles can significantly alter the surfaces of icy satellites and minor planets. Impact heating from these particles can anneal away radiation damage to the crystalline structure of surface water ice. This effect is enhanced by gravitational focusing for giant planet satellites. In addition, impacts of interplanetary dust particles on the small satellites of the Pluto system can eject into the system significant amounts of secondary intra-satellite dust. This dust is primarily swept up by Pluto and Charon, and could explain the observed albedo features on Pluto's surface. In addition to Pluto, a large fraction of trans-neptunian objects (TNOs) are binary or multiple systems. The mutual orbits of these TNO binaries can range from very wide (periods of several years) to near-contact systems (less than a day period). No single formation mechanism can explain this distribution. However, if the systems generally formed wide, a combination of solar and body tides (commonly called Kozai Cycles-Tidal Friction, KCTF) can cause most systems to tighten sufficiently to explain the observed distributions. This KCTF process can also be used to describe the orbital evolution of a terrestrial-class exoplanet after being captured as a satellite of a habitable-zone giant exoplanet. The resulting exomoon would be both potentially habitable and potenially detectable in the full Kepler data set.
ContributorsPorter, Simon Bernard (Author) / Desch, Steven (Thesis advisor) / Zolotov, Mikhail (Committee member) / Timmes, Francis (Committee member) / Scannapieco, Evan (Committee member) / Robinson, Mark (Committee member) / Arizona State University (Publisher)
Created2013
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Description
Galaxies represent a fundamental catalyst in the ``lifecycle'' of matter in the Universe, and the study of galaxy assembly and evolution provides unique insight into the physical processes governing the transformation of matter from atoms to gas to stars. With the Hubble Space Telescope, the astrophysical community is able to

Galaxies represent a fundamental catalyst in the ``lifecycle'' of matter in the Universe, and the study of galaxy assembly and evolution provides unique insight into the physical processes governing the transformation of matter from atoms to gas to stars. With the Hubble Space Telescope, the astrophysical community is able to study the formation and evolution of galaxies, at an unrivaled spatial resolution, over more than 90% of cosmic time. Here, I present results from two complementary studies of galaxy evolution in the local and intermediate redshift Universe which used new and archival HST images. First, I use archival broad-band HST WFPC2 optical images of local (d<63 Mpc) Seyfert-type galaxies to test the observed correlation between visually-classified host galaxy dust morphology and AGN class. Using quantitative parameters for classifying galaxy morphology, I do not measure a strong correlation between the galaxy morphology and AGN class. This result could imply that the Unified Model of AGN provides a sufficient model for the observed diversity of AGN, but this result could also indicate the quantitative techniques are insufficient for characterizing the dust morphology of local galaxies. To address the latter, I develop a new automated method using an inverse unsharp masking technique coupled to Source Extractor to detect and measure dust morphology. I measure no strong trends with dust-morphology and AGN class using this method, and conclude that the Unified Model remains sufficient to explain the diversity of AGN. Second, I use new UV-optical-near IR broad-band images obtained with the HST WFC3 in the Early Release Science (ERS) program to study the evolution of massive, early-type galaxies. These galaxies were once considered to be ``red and dead'', as a class uniformly devoid of recent star formation, but observations of these galaxies in the local Universe at UV wavelengths have revealed a significant fraction (30%) of ETGs to have recently formed a small fraction (5-10%) of their stellar mass in young stars. I extend the study of recent star formation in ETGs to intermediate-redshift 0.35<1.5 with the ERS data. Comparing the mass fraction and age of young stellar populations identified in these ETGs from two-component SED analysis with the morphology of the ETG and the frequency of companions, I find that at this redshift many ETGs are likely to have experienced a minor burst of recent star formation. The mechanisms driving this recent star formation are varied, and evidence for both minor merger driven recent star formation as well as the evolution of transitioning ETGs is identified.
ContributorsRutkowski, Michael (Author) / Windhorst, Rogier A. (Thesis advisor) / Bowman, Judd (Committee member) / Butler, Nathaniel (Committee member) / Desch, Steven (Committee member) / Young, Patrick (Committee member) / Arizona State University (Publisher)
Created2013