Since the development of interactive music software in the 1980s, a new genre of works for clarinet and computer has emerged. The rapid proliferation of interactive music resulted in a great deal of experimentation, creating a lack of standardization in both the composition and performance of this repertoire. In addition, many performers are reluctant to approach these works due to unfamiliarity with the genre and its technical and musical considerations. Performance practice commonly refers to interpretation of a written score, but the technology involved in interactive music requires a broader definition of performance practice; one that also addresses computer software, coordination between the performer and computer system, and technology such as microphones and pedals. The problems and potential solutions of interactive music performance practice are explored in this paper through review of the relevant published literature, interviews with experts in the field, and examination of musical examples from works for clarinet and computer by Lippe, May, Pinkston, Rowe, and Welch. Performance practice considerations of interactive music fall into the categories of notation, technology, collaboration, interpretation, and rehearsal. From the interviews and the literature, it is clear that the performance of interactive music requires specific knowledge and skills that performers may not encounter in other genres of contemporary music, including microphone technique, spatialization, sound processing, and improvisation. Performance practice issues are often mediated by close collaboration between performers and composers, but they can inhibit the accessibility of these works to new performers, and may be detrimental to the long-term viability of interactive music. Recommendations for resolving these issues are directed at both composers and performers of interactive music. A listing of over one hundred interactive works for clarinet and computer is also included.

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The cantata A World Without War (2009), by Armenian-born composer Edward Manukyan (b. 1981), was written, in part, to support increased awareness of human rights issues. Based on a quote from linguist and philosopher Noam Chomsky (b. 1928), the narrative of the cantata states: "We can, for example, be fairly confident that either there will be a world without war or there won't be a world." In addition to Chomsky's words, the cantata excerpts quotes of two additional literary giants advocating human rights, Bertrand Russell (1872-1970), and Andrei Sakharov (1921-1989). The purpose of this dissertation is to focus attention on human rights activism; using Manukyan's A World Without War, I highlight moral and ethical questions at the center of this work and explain how this cantata embraces the ideal of moral cosmopolitanism. I strongly believe in the importance of human rights for all citizens of the world, and the role music plays in advancing its cause through performance arts.

Globular clusters are tracers of the formation and evolution of their host galaxies. Kinematics, chemical abundances, age and position of the clusters allows tracing interactions between Milky Way and surrounding galaxies and outlines their chemical enrichment history. In this thesis we analyse mid-resolution spectra of about 800 red giant stars in 51 Galactic globular clusters. It is the first time that [Fe/H] and [Mg/Fe] derived in a consistent way are published for such a huge sample of globular clusters, almost 1/3 of the total number of catalogued clusters. Our metallicities are showed to be more precise than previous works based on mid-resolution spectroscopy. A turnover at [Fe/H] ~ -1.0 is found in the plot [Fe/H] vs. [Mg/Fe] for bulge and halo, although bulge seems to have a more metal-rich turnover, i.e, bulge has more efficient formation than the halo. Comparing the abundances with age the timescale for SNIa to start to become important is 1Gyr. [Fe/H] vs. age corroborates the different star formation efficiency of bulge and halo while [Mg/Fe] does not follow that. Halo was formed in mini halos or dwarf galaxies, and two multiple population clusters had their origin analysed to check it. M 22 seems to have been formed in the Milky Way while NGC 5824 possibly was originated in a dwarf galaxy, although our results are inconclusive for NGC 5824. The Galactic bulge seems to have been formed fast i.e., probably the oldest globular cluster is there. In fact HP 1 has a bluer horizontal branch than expected for its metallicity and we interpret that as an age effect. We determine its distance using light curves of variable stars in order to constrain future age determinations via colour-magnitude diagram. Finally, we investigate interaction between Milky Way and its neighbour galaxy SMC. We find that some star clusters are being stripped out of the SMC main body, which is consistent with tidal stripping scenario for the interaction between the galaxies, instead of ram pressure that would only affect gas. / Aglomerados globulares são traçadores da formação e evolução de suas galáxias. Cinemática, abundâncias químicas, idades e posições dos aglomerados permitem traçar interações entre Via Láctea e galáxias vizinhas e suas histórias de enriquecimento químico. Nesta tese analisamos espectros de média resolução de mais de 800 estrelas gigantes vermelhas em 51 aglomerados globulares Galácticos. É a primeira vez que [Fe/H] and [Mg/Fe] determinados de modo consistente são publicados para uma amostra desse porte, ~1/3 dos objetos catalogados. Nossas metalicidades são mais precisas que trabalhos anteriores similares. Uma quebra em [Fe/H] ~ -1.0 é encontrada no gráfico [Fe/H] vs. [Mg/Fe] para o bojo e halo, embora bojo parece ter uma quebra em [Fe/H] maior, i.e, bojo tem formaçãao mais eficiente que o halo. Comparando abundâncias com idade, a escala de tempo para SNIa ficar importante é 1Gano. [Fe/H] vs. idade corrobora diferentes eficiências de formação do bojo e halo, mas [Mg/Fe] vs. idade não mostra isso. O halo foi formado em mini halos ou galáxias anãs, e dois aglomerados com dispersão em [Fe/H] tiveram suas origens analisadas. M 22 parece ter sido formado na Via Láctea e NGC 5824 possivelmente foi originado em uma galáxia anã, embora os resultados são inconclusivos para NGC 5824. O bojo parece ter sido formado rapidamente e deve possuir o aglomerado mais velho. De fato, HP 1 tem um ramo horizontal mais azul que o esperado para sua metalicidade e vemos isso como um efeito da idade. Determinamos sua distância usando curvas de luz de RR Lyrae de maneira a restringir futuras determinações de idade via diagrama cor-magnitude. Finalmente, investigamos a interação entre Via Láctea e sua galáxia vizinha SMC. Encontramos aglomerados sendo removidos do corpo central da SMC, consistente com cenário de remoção por força de maré para a interação entre as galáxias, em vez de ``ram pressure\'\' que afeta só gás.

Globular clusters are tracers of the formation and evolution of their host galaxies. Kinematics, chemical abundances, age and position of the clusters allows tracing interactions between Milky Way and surrounding galaxies and outlines their chemical enrichment history. In this thesis we analyse mid-resolution spectra of about 800 red giant stars in 51 Galactic globular clusters. It is the first time that [Fe/H] and [Mg/Fe] derived in a consistent way are published for such a huge sample of globular clusters, almost 1/3 of the total number of catalogued clusters. Our metallicities are showed to be more precise than previous works based on mid-resolution spectroscopy. A turnover at [Fe/H] ~ -1.0 is found in the plot [Fe/H] vs. [Mg/Fe] for bulge and halo, although bulge seems to have a more metal-rich turnover, i.e, bulge has more efficient formation than the halo. Comparing the abundances with age the timescale for SNIa to start to become important is 1Gyr. [Fe/H] vs. age corroborates the different star formation efficiency of bulge and halo while [Mg/Fe] does not follow that. Halo was formed in mini halos or dwarf galaxies, and two multiple population clusters had their origin analysed to check it. M 22 seems to have been formed in the Milky Way while NGC 5824 possibly was originated in a dwarf galaxy, although our results are inconclusive for NGC 5824. The Galactic bulge seems to have been formed fast i.e., probably the oldest globular cluster is there. In fact HP 1 has a bluer horizontal branch than expected for its metallicity and we interpret that as an age effect. We determine its distance using light curves of variable stars in order to constrain future age determinations via colour-magnitude diagram. Finally, we investigate interaction between Milky Way and its neighbour galaxy SMC. We find that some star clusters are being stripped out of the SMC main body, which is consistent with tidal stripping scenario for the interaction between the galaxies, instead of ram pressure that would only affect gas. / Aglomerados globulares são traçadores da formação e evolução de suas galáxias. Cinemática, abundâncias químicas, idades e posições dos aglomerados permitem traçar interações entre Via Láctea e galáxias vizinhas e suas histórias de enriquecimento químico. Nesta tese analisamos espectros de média resolução de mais de 800 estrelas gigantes vermelhas em 51 aglomerados globulares Galácticos. É a primeira vez que [Fe/H] and [Mg/Fe] determinados de modo consistente são publicados para uma amostra desse porte, ~1/3 dos objetos catalogados. Nossas metalicidades são mais precisas que trabalhos anteriores similares. Uma quebra em [Fe/H] ~ -1.0 é encontrada no gráfico [Fe/H] vs. [Mg/Fe] para o bojo e halo, embora bojo parece ter uma quebra em [Fe/H] maior, i.e, bojo tem formaçãao mais eficiente que o halo. Comparando abundâncias com idade, a escala de tempo para SNIa ficar importante é 1Gano. [Fe/H] vs. idade corrobora diferentes eficiências de formação do bojo e halo, mas [Mg/Fe] vs. idade não mostra isso. O halo foi formado em mini halos ou galáxias anãs, e dois aglomerados com dispersão em [Fe/H] tiveram suas origens analisadas. M 22 parece ter sido formado na Via Láctea e NGC 5824 possivelmente foi originado em uma galáxia anã, embora os resultados são inconclusivos para NGC 5824. O bojo parece ter sido formado rapidamente e deve possuir o aglomerado mais velho. De fato, HP 1 tem um ramo horizontal mais azul que o esperado para sua metalicidade e vemos isso como um efeito da idade. Determinamos sua distância usando curvas de luz de RR Lyrae de maneira a restringir futuras determinações de idade via diagrama cor-magnitude. Finalmente, investigamos a interação entre Via Láctea e sua galáxia vizinha SMC. Encontramos aglomerados sendo removidos do corpo central da SMC, consistente com cenário de remoção por força de maré para a interação entre as galáxias, em vez de ``ram pressure\'\' que afeta só gás.

從亞里斯多德問題，團體就成為學者研究的焦點之一。歷來有關利益團體的研究即備 受爭議，特別是在利益團體的源起部分，學說層出不窮，至今仍未有定論。公益性團 體的興起，更使得團體理論愈加複雜。 近年來，我國政治情勢及社會環境的變遷，人們參與團體活動的趨勢有增無減，特別 是一些新興的公益性團體，除了消費者文教基金會，另外最惹人注目的該是一些以環 境保護為訴求反公害團體了。我們所感興趣的是，用什麼理論來解釋這些團體的發展 呢？ 本文企圖由複雜的團體理論分析中，歸納出一個適合解釋反污染團體源起及維持的分 析架構，並以彰化縣公害妨治協會為個案分析對象，希望獲得一個初步的了解。 全文共分五章，計六萬餘言。 第一章緒論部分，將就本文的研究目的、研究方法、名詞界定分別闡述。 第二章理論探討，抱括杜魯門（David Truman），奧爾森（Mancur Olscn），哈定（ Russell hardin），薩利伯瑞（Rcbert H．Salisbury ）等人的理論要點闡述，並就 各項之優劣點予以評估而提出本文之研究架構。 第三章源起分析，就整體社會變遷、政治企業家，約定俗成及道德理性等因素探討彰 化縣公害防治協會的源起。 第四章維持分析，就組織目標、向心力、資源等方面探討彰化縣公害防治協會的維持 狀況。 第五章結論。檢討及建議。

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This paper seeks to explore the dialogue between postmodern thought and Christian theology. The dialogue will be grounded in four postmodern novels: Toni Morrison's Beloved, Ian McEwan's Atonement, Jill Paton Walsh's Knowledge of Angels, and Jeanette Winterson's Oranges Are Not the Only Fruit. In many Church circles, it has often been said that postmodernism, as it manifests itself in popular culture, is a threat to the Christian faith. However, I will be arguing that the opposite is the case, and that postmodernism has allowed for new ways of thinking about the self that has great resonance with certain theological conceptions of the self. It will be argued that the postmodern subject is one that seeks to make sense of 'the other' without risking the exploitation of the other, and that this lies very close to the theological concept of relationship, based on the idea of covenant. The self as responsible to an other and as a participant in community will be explored, from both the postmodern and theological perspectives. Before exploring issues of the self, this thesis will contextualize the dialogue by exploring postmodern conceptions of space and time. It will examine how ideas around space and time have been imagined throughout human history, thereby contextualizing the emergence of postmodern thinking. It will then show how this emergence of a postmodern space and time in fact creates new possibilities for the Christian faith to reexpress itself in ways that are more relevant to the 21st century. The concluding chapter of this thesis brings to light the longing within our postmodern reality for a place we can call home, a place where we can belong, and find healing. Such a place, such a homecoming, is offered to us in the spaces opened up to us by the dialogue between the Christian faith and postmodernity, and is found within a community of people who are learning that, as, postmodern philosopher Emmanuel Levinas states, "there is something more important than my life, and that is the life of the other" (in Beavers, 1996,16). / Thesis (M.A.)-University of KwaZulu-Natal, Pietermaritzburg, 2004.

Teaching is, and always has been, important in the work of The Church of Jesus Christ of Latter-day Saints. As one of the auxiliaries of the Church, the Sunday School has made an ongoing effort to provide effective teaching aids for its teachers in order to improve instruction in the Church. This work documents and examines change in principles of gospel teaching over the course of a century. By comparing teaching aids provided for Gospel Doctrine teachers in different time periods with guidelines found in the scriptures and words of modern prophets this work seeks to increase understanding of themes and fundamentals of inspired teaching in the Church.

Fundação de Amparo à Pesquisa do Estado do Rio de Janeiro / No romance A defesa Lujin, de Vladimir Nabokov, publicado em russo em 1930, o texto procura levar o leitor a adotar processos mentais similares ao de um jogador de xadrez e de um esquizofrênico, características do personagem-título do romance. Delineiam-se as expectativas e circunstâncias de um ser de papel que se vê jogando um xadrez em que também é peça e traçam-se paralelos com as expectativas e circunstâncias do leitor perante esse texto literário. O prefácio de Nabokov à edição em inglês de 1964 é tomado como indício de um leitor e um autor implícitos que ele procura moldar. Para análise dos elementos textuais e níveis de abstração mental envolvidos, recorre-se à estética da recepção de Wolfgang Iser e a diversas ideias do psiquiatra e etnólogo Gregory Bateson, entre elas o conceito de duplo vínculo, com atenção às distinções entre mapa/território e play/game. Um duplo duplo vínculo é perpetrado na interação leitor-texto: 1) o leitor é convidado a sentir empatia pela situação do personagem Lujin e a considerá-lo lúcido e louco ao mesmo tempo; e 2) o leitor é colocado como uma instância pseudo-transcendental incapaz de comunicação com a instância inferior (Lujin), gerando uma angústia diretamente relacionável ao seu envolvimento com a ficção, replicando de certa forma a loucura de Lujin. A sinestesia do personagem Lujin é identificada como um dos elementos do texto capaz de recriar a experiência de jogar xadrez até para quem não aprecia o jogo. Analisa-se a conexão entre a esquizofrenia ficcional do personagem Lujin e a visão batesoniana do alcoolismo / In Vladimir Nabokovs novel, The Luzhin Defense, published in Russian in 1930, the text beckons the reader on to adopt mental processes similar to a chess players and a schizophrenic persons both traits of the novels title character. This character sees himself both as player and piece of an ongoing game of chess; his expectations and predicaments are traced in parallel to the readers own as he or she navigates the text. Nabokovs preface to the 1964 English edition is taken as an indication that he tries to shape both an implicit reader and an implicit author. In order to analyze the elements of the text and degrees of mental abstraction involved in this, we refer to Wolfgang Isers reader-response theory and also many of psychiatrist and ethnologist Gregory Batesons ideas, such as the double bind, with special regard to map vs. territory and play vs. game distinctions. A double double bind is built within the reader-text interplay as follows: 1) the reader is invited to feel empathy for Luzhins predicament and to regard him at once as sane and insane; and 2) the reader is posited as a pseudo-transcendental instance unable to communicate with his nether instance (Luzhin) in such a way that it brews a feeling of anxiety directly relatable to his or her engagement in the work of fiction, reproducing, in a way, Luzhins madness. Luzhins synesthesia is identified as one of the text elements with the ability to recreate the chess-playing experience even to readers who are not fond of the game. The connection between Luzhins fictional schizophrenia and Batesons views on alcoholism is analyzed