985 resultados para Quest


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Includes bibliography

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Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

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Context. The Sun shows abundance anomalies relative to most solar twins. If the abundance peculiarities are due to the formation of inner rocky planets, that would mean that only a small fraction of solar type stars may host terrestrial planets. Aims. In this work we study HIP 56948, the best solar twin known to date, to determine with an unparalleled precision how similar it is to the Sun in its physical properties, chemical composition and planet architecture. We explore whether the abundances anomalies may be due to pollution from stellar ejecta or to terrestrial planet formation. Methods. We perform a differential abundance analysis (both in LTE and NLTE) using high resolution (R similar to 100 000) high S/N (600-650) Keck HIRES spectra of the Sun (as reflected from the asteroid Ceres) and HIP 56948. We use precise radial velocity data from the McDonald and Keck observatories to search for planets around this star. Results. We achieve a precision of sigma less than or similar to 0.003 dex for several elements. Including errors in stellar parameters the total uncertainty is as low as sigma similar or equal to 0.005 dex (1%), which is unprecedented in elemental abundance studies. The similarities between HIP 56948 and the Sun are astonishing. HIP 56948 is only 17 +/- 7 K hotter than the Sun, and log g, [Fe/H] and microturbulence velocity are only +0.02 +/- 0.02 dex, +0.02 +/- 0.01 dex and +0.01 +/- 0.01 km s(-1) higher than solar, respectively. Our precise stellar parameters and a differential isochrone analysis shows that HIP 56948 has a mass of 1.02 +/- 0.02 M-circle dot and that it is similar to 1 Gyr younger than the Sun, as constrained by isochrones, chromospheric activity, Li and rotation. Both stars show a chemical abundance pattern that differs from most solar twins, but the refractory elements (those with condensation temperature T-cond greater than or similar to 1000 K) are slightly (similar to 0.01 dex) more depleted in the Sun than in HIP 56948. The trend with T-cond in differential abundances (twins -HIP 56948) can be reproduced very well by adding similar to 3 M-circle plus of a mix of Earth and meteoritic material, to the convection zone of HIP 56948. The element-to-element scatter of the Earth/meteoritic mix for the case of hypothetical rocky planets around HIP 56948 is only 0.0047 dex. From our radial velocity monitoring we find no indications of giant planets interior to or within the habitable zone of HIP 56948. Conclusions. We conclude that HIP 56948 is an excellent candidate to host a planetary system like our own, including the possible presence of inner terrestrial planets. Its striking similarity to the Sun and its mature age makes HIP 56948 a prime target in the quest for other Earths and SETI endeavors.

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Die letzten Jahrzehnte brachten eine Vielzahl neuer organischen Halbleiter hervor, welche erfolgreich als aktive Materialien in Bauteilen eingesetzt wurden, wie zum Beispiel Feldeffekttransistoren (FET), organische Leuchtdioden (OLED), organischen Photovoltaikzellen (OPV) und Sensoren. Einige dieser Materialien haben, obwohl sich die Technolgie noch in der „Pubertät“ befindet, die minimalen Anforderungen für eine kommerzielle Anwendung erreicht, wobei jedoch vieles noch zu entdecken, erklären und verstehen bleibt. Diese Arbeit beschreibt das Design, die Synthese und Charakterisierung neuartiger halbleitender Polymere mit speziell eingestellten optoelektronischen Eigenschaften, welche effiziente ambipolare oder n-Leitung in OFET’s und OPV’s zeigen. Das Hauptziel wurde dadurch erreicht, dass sowohl die vorteilhaften Eigenschaften des planaren, elektronenarmen heterozyklischen Bausteines Thiadiazolo[3,4-g]quinoxalin als auch von Ethinbrücken, welche den Donor (D) und den Akzeptor (A) in einem D-A-Copolymer verbinden, durch systematische Optimierung ausgenutzt wurden. Neben synthetischen Herausforderungen werden in dieser Arbeit auch detailiiete Untersuchungen der optoelektronischen Eigenschaften der hergestellten konjugierten Polymere und Modellverbindungen dargelegt. Darüber hinaus beschreibt diese Arbeit erstmals ein Beispiel für ein Polymer, welches Dreifachbindungen im Polymerrückgrat enthält, und nahezu eine ausgeglichene ambipolare Ladungsträgerleitung in OFET’s zeigt. Zusätzlich werden gemischt-valente Phenothiazine, verbrückt mittels elektronenarmen pi-Brücken wie etwa Benzo[c][2,1,3]thiadiazol, und deren Elektronentransferprozesse, im Rahmen der Marcus-Hush-Theorie, untersucht.

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Lo scopo della presente ricerca è sottolineare la tendenza alla ossessiva e spesso superflua ricerca del simbolismo nell’analisi di opere, specificatamente testi letterari e film, e proporre una possibile soluzione per porre fine o almeno diminuire gli effetti del fenomeno. A partire da una definizione esaustiva della parola simbolo, l’analisi verterà sull’evoluzione del concetto di simbolismo attraverso i media, e il cambiamento intrinseco causato da tale evoluzione. In seguito, analizzerò un semisconosciuto ma emblematico sondaggio, condotto nel 1973 da Bruce McAllister, all’epoca studente, che interrogò acutamente numerosi autori riguardo al loro rapporto con il simbolismo, ponendo l’accento su alcune delle risposte da lui ricevute, che gettano una luce rivelatrice sul symbol hunting e symbol planting. Dopodiché scenderò ancor più nel dettaglio, esemplificando con due storie brevi: Signs and Symbols (Segni e Simboli), di Vladimir Nabokov e Big Two-hearted River (Grande fiume a due cuori) di Hernest Hemingway. Dopodiché, analizzerò il falso simbolismo come luogo cinematografico, ponendo l’accento sugli aspetti di planting e hunting, e mi avvarrò dell’aiuto di due film significativi sul tema realizzati in tempi recenti, ovvero Inception (2010) e Memento (2000), di Christopher Nolan, che possono essere interpretati come una meta-critica dell’abuso di simboli, e rappresentano una pietra miliare nell’analisi di symbol planting e symbol hunting. In conclusione, proporrò la mia personale possibile soluzione, ovvero il prendere le opere d’arte in qualunque forma, specialmente di fiction, “così come sono”, separandole e scindendole dalle proprie aspettative. È necessario prendere in considerazione un ritorno alla letteralità, per poter avvicinarsi maggiormente alla vera anima di una storia, di un libro, di un film, altrimenti esiste la possibilità che tutto ciò che guardiamo o vediamo sia per sempre irrimediabilmente contaminato dalla nostra dimensione privata.

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This paper provides an analysis of the key term aidagara (“betweenness”) in the philosophical ethics of Watsuji Tetsurō (1889-1960), in response to and in light of the recent movement in Japanese Buddhist studies known as “Critical Buddhism.” The Critical Buddhist call for a turn away from “topical” or intuitionist thinking and towards (properly Buddhist) “critical” thinking, while problematic in its bipolarity, raises the important issue of the place of “reason” versus “intuition” in Japanese Buddhist ethics. In this paper, a comparison of Watsuji’s “ontological quest” with that of Martin Heidegger (1889-1976), Watsuji’s primary Western source and foil, is followed by an evaluation of a corresponding search for an “ontology of social existence” undertaken by Tanabe Hajime (1885-1962). Ultimately, the philosophico-religious writings of Watsuji Tetsurō allow for the “return” of aesthesis as a modality of social being that is truly dimensionalized, and thus falls prey neither to the verticality of topicalism nor the limiting objectivity of criticalism.