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Dissertations / Theses on the topic 'HiCi'

Author: Grafiati
Published: 3 June 2025
Last updated: 31 July 2025

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1

Daimon, Yasushi. "Activation of Toxin-Antitoxin System Toxins Suppresses Lethality Caused by the Loss of σE in Escherichia coli". Kyoto University, 2016. http://hdl.handle.net/2433/215457.

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2

Bürger, Thomas. "Kreatives Hick-Hack." Saechsische Landesbibliothek- Staats- und Universitaetsbibliothek Dresden, 2014. http://nbn-resolving.de/urn:nbn:de:bsz:14-qucosa-148802.

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Zwischen 1989 und 2009 zeichneten, malten, dichteten und druckten die beiden Künstler Andreas Dress (geb. 1943 in Sebnitz) und Claus Weidensdorfer (geb. 1931 in Coswig) einen „Deutschen Hausschatz“, ein Künstlerbuch mit 19 Radierungen in 16 Exemplaren. Mit ungebremster Phantasie und künstlerischer Leidenschaft verwandelten sie im kreativen Hick-Hack Märchenmotive der Gebrüder Grimm und Hans Christian Andersens in eigenständige Kunstwerke. Fast jedes der Blätter aus den 16 Exemplaren wurde übermalt, und wenn der Platz für neue Bilder und Texte nicht ausreichte, dann wurde er gesucht und gefunde
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3

Smith, Donald W. "The christology of John Hick." Theological Research Exchange Network (TREN), 1993. http://www.tren.com.

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4

Manetta, Emily Walker. "Peripheries in Kashmiri and Hini-Urdu /." Diss., Digital Dissertations Database. Restricted to UC campuses, 2006. http://uclibs.org/PID/11984.

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5

Doležal, Pavel. "HiFi DA převodník a sluchátkový zesilovač." Master's thesis, Vysoké učení technické v Brně. Fakulta informačních technologií, 2014. http://www.nusl.cz/ntk/nusl-236104.

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This thesis is dealing with a design and fabrication of D/A coverter and headphone amplifier for stereo reproduction in Hi-Fi class. In opening chapter, overall problematics of digital audio signal distribution is discussed. Following chapters are dedicated to converter design, communication protocols, component selection, converter production, circuitry design and firmware programming. The final chapter is dealing with expansion options such as HDMI inputs and surround sound.
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6

Steggles, Harrison. "Ultra-compact HII regions." Thesis, University of Leeds, 2016. http://etheses.whiterose.ac.uk/15813/.

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In this thesis I have studied hydrodynamical models of cometary HII regions and distributions of UCHII regions in simulated surveys, for comparison with CORNISH. I present the numerical method used to model the evolution of cometary HII regions produced by ZAMS stars of O and B spectral types, which are driving strong winds and are born off-centre from spherically symmetric cores with power-law (alpha = 2) density slopes. A model parameter grid was produced that spans stellar mass, age and core density. Exploring this parameter space I investigated limb-brightening, a feature commonly seen in
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7

Ravera, Laurent. "Spectromètre-autocorrélateur numérique spatialisable pour l'instrument FIRST-HIFI." Phd thesis, INSA de Toulouse, 1999. http://tel.archives-ouvertes.fr/tel-00332342.

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Cette thèse s'inscrit dans le cadre d'un programme de R&T dont l'objectif est de spatialiser les techniques de spectrométrie par autocorrélation numérique, notamment pour HIFI, l'instrument hétérodyne de la mission spatiale FIRST (Herschel) de l'ESA. Lancé en 2007, FIRST sera le premier observatoire submillimétrique dans l'espace. Les contraintes spatiales en terme de poids, d'encombrement, de consommation, imposaient des développements majeurs. Une architecture optimisée de spectromètre a été conçue à partir d'ASICs numériques à haut degré d'intégration. Elle inclut 3 principaux éléments. 1)
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8

Terzic, Aleksandra. "Analysis and characterisation of the mouse Hic2 gene." Diss., lmu, 2004. http://nbn-resolving.de/urn:nbn:de:bvb:19-20694.

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9

RAVERA, LAURENT. "Spectrometre - autocorrelateur numerique spatialisable pour l'instrument first-hifi." Toulouse, INSA, 1999. http://www.theses.fr/1999ISAT0041.

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Cette these s'inscrit dans le cadre d'un programme de r&t dont l'objectif est de spatialiser les techniques de spectrometrie par autocorrelation numerique, notamment pour hifi, l'instrument heterodyne de la mission spatiale first de l'esa. Lance en 2007, first sera le premier observatoire submillimetrique dans l'espace. Les contraintes spatiales en terme de poids, d'encombrement, de consommation, imposaient des developpements majeurs. Une architecture optimisee de spectrometre a ete concue a partir d'asics numeriques a haut degre d'integration. Elle inclut 3 principaux elements. 1) un sous-sys
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10

Krisak, Paul E. "The religious pluralism of John Hick a critique /." Lynchburg, Va. : Liberty University, 2000. http://digitalcommons.liberty.edu.

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11

Clayton, C. A. "Echelle observations of HII complexes." Thesis, University of Manchester, 1987. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.382745.

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12

Velusamy, Chandramohan Pavithra. "Intergration of CloudMe to Sonos wireless HiFi speaker system." Thesis, Linköpings universitet, Institutionen för datavetenskap, 2013. http://urn.kb.se/resolve?urn=urn:nbn:se:liu:diva-105177.

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CloudMe is a cloud computing service used for business and home users. CloudMe facilitates the user to store their personal files like music, video, documents and images. The primary focus of this thesis is on music. The personal music files can be uploaded to CloudMe manually or by using CloudMe sync in any order just like in personal computer. CloudMe offers different services to access the cloud from other devices like smart phones, web browser and the home computer.   Sonos wireless HiFi system is a set of Sonos component interconnected with the mesh network with the primary function to pl
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13

Corrias, Maria Elena. "Caratteristiche di emissione delle regioni HII." Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2016. http://amslaurea.unibo.it/10954/.

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Le regioni HII sono nubi di idrogeno ionizzato da stelle di recente formazione, massicce e calde. Tali stelle, spesso raggruppate in ammassi, emettono copiosamente fotoni di lunghezza d’onda λ ≤ 912 Å, capaci di ionizzare quasi totalmente il gas che le circonda, composto prevalentemente da idrogeno, ma in cui sono presenti anche elementi ionizzati più pesanti, come He, O, N, C e Ne. Le dimensioni tipiche di queste regioni vanno da 10 a 100 pc, con densità dell’ordine di 10 cm−3. Queste caratteristiche le collocano all’interno del WIM (Warm Ionized Medium), che, insieme con HIM (Hot Ionized Med
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14

Ceccia, Domenico. "Caratteristiche di emissione delle regioni HII." Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2018. http://amslaurea.unibo.it/15843/.

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Prendiamo in considerazione la nostra Galassia, e osserviamo una precisa regione che emette della radiazione tramite alcuni processi. La regione considerata è rilevata nei bracci della nostra Galassia, e soprattutto dove vi è presente dell’ idrogeno ionizzato, che è l’ elemento dominante in queste regioni che stiamo osservando. Stiamo parlando delle regioni HII. In questo elaborato andremo ad analizzare e capire cos’ è una regione HII e le sue principali caratteristiche, la sua formazione e collocazione, ma soprattutto capire quali sono i principali meccanismi che portano all’emissione di radi
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15

Borghi, Nicola. "Caratteristiche principali dell'emissione di regioni HII." Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2018. http://amslaurea.unibo.it/16213/.

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Le regioni HII sono, in prima approssimazione, nubi di idrogeno ionizzato dai fotoni di stelle OB. Tali stelle massicce hanno temperature superficiali T∗>10^4 K e una vita media relativamente breve. Se all'interno della regione di formazione si osservano stelle a diversi stage evolutivi, è possibile seguire e studiare in dettaglio l'evoluzione delle regioni HII ad esse associate. Il mezzo interstellare ionizzato (WIM) si trova immerso in un mezzo neutro (WNM e CNM) dal quale la formazione stellare ha avuto origine. Pertanto per avere una panoramica completa delle caratteristiche di emissione n
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16

Pignataro, Giada Venusta. "Caratteristiche principali dell'emissione di regioni HII." Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2018. http://amslaurea.unibo.it/16358/.

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In questo elaborato ci si ripropone di studiare l'emissione delle regioni HII. Si può definire una regione HII come una zona molto calda di idrogeno ionizzato, che si trova in un background di idrogeno neutro più freddo. Vengono analizzati i processi di emissione nel continuo e in riga, e analizzate in particolare le nebulose planetarie.
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17

Tedino, Simone. "Caratteristiche principali dell’emissione di regioni HII." Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2019. http://amslaurea.unibo.it/17875/.

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La formazione stellare ha inizio quando massicce nubi di gas freddo collassano a causa della gravità. Le stelle così formatesi, giovani, calde ed estremamente massive, vengono classificate come stelle di classe spettrale O-B, caratterizzate da una temperatura superficiale media dell’ordine di 10^4/5 K. A queste temperature esse sono in grado di generare intensi flussi di radiazione ultravioletta (UV) che si compongono di fotoni di lunghezza d’onda <= 912 A°, e conseguente energia maggiore a hv=13.6eV, corrispondente al valore specifico del potenziale di ionizzazione dell’idrogeno (H). Questa r
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18

Bianchera, Sergio. "Caratteristiche principali dell'emissione delle regioni HII." Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2020. http://amslaurea.unibo.it/19907/.

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Le regioni HII sono nubi di gas composte principalmente da idrogeno ionizzato. Si sviluppano attorno popolazioni di stelle giovani e molto massive di tipo O-B che riscaldano il materiale circostante. Queste regioni si possono trovare solo nelle galassie a spirale andando a comporre il Warm Ionized Medium, collocandosi principalmente nei bracci a spirale e circondate dal Cold Neutral Medium. In questo testo andremo a introdurre le principali caratteristiche astrofisiche di queste regioni, soffermandoci sui meccanismi di emissione nel continuo e in riga, approfondendo anche alcuni casi particola
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19

Pasquale, Lorenzo. "Caratteristiche principali dell'emissione di regioni HII." Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2020. http://amslaurea.unibo.it/21224/.

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Le Regioni HII sono plasmi astrofisici composti da idrogeno ionizzato che si formano a seguito della foto-ionizzazione, da parte di stelle giovani e massive, del mezzo neutro e freddo tipico delle regioni di formazione stellare. Lo studio del loro spettro e dei loro processi di emissione illustrati esaustivamente in questo elaborato è di cruciale importanza in quanto fornisce informazioni riguardo non solo la formazione e l’evoluzione stellare ma anche riguardo le abbondanze chimiche dell’ISM, la distanza delle galassie e la loro dinamica interna. In particolare il tipico spettro di una regio
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20

Zanetti, Francesca. "Caratteristiche principali dell'emissione di regioni HII." Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2021. http://amslaurea.unibo.it/24847/.

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Le regioni HII sono regioni del mezzo interstellare costituite da idrogeno ionizzato. Il processo di ionizzazione si deve alle stelle giovani e di grande massa che sono in grado di produrre un flusso continuo di fotoni ultravioletti. Nella trattazione che segue, si accennerà alla struttura e all'evoluzione di tali regioni. Si analizzeranno nel dettaglio i processi fisici che determinano l'emissione di radiazione, sia nel continuo che in riga. A partire dalle caratteristiche spettrali si deriveranno le caratteristiche osservabili di tali regioni. Inoltre, si evidenzierà il ruolo della riga H al
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21

von, Knorring Olof. "Comparison of Religions Based on John Hick´s Theory on Pluralism." Thesis, Uppsala universitet, Teologiska institutionen, 2016. http://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-295700.

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“Who am I / What is my identity?” This is one of the most important questions in a person’s life and also one of the most difficult to answer. The identity is developed and internalized mostly during the socialization process in childhood. Part of socialization is to learn what groups to identify with, ingroups, and distinguish them from outgroups that you do not belong to. This is a universal tendency of humans and it gives a bias in people´s thinking to see ingroups as “natural”, as opposed to outgroups with strange and different thinking and behaviour. At the same time we must realise that
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22

Heller, Christian. "John Hicks Projekt einer religiösen Interpretation der Religionen : Darstellung und Analyse, Diskussion, Rezeption /." Münster : Lit, 2001. http://catalogue.bnf.fr/ark:/12148/cb388813446.

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23

Van, Rechem Capucine. "Mécanismes différentiels de répression transcriptionnelle des gènes cibles de HIC1." Phd thesis, Université du Droit et de la Santé - Lille II, 2009. http://tel.archives-ouvertes.fr/tel-00420474.

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HIC1 (Hypermethylated in Cancer 1) est un répresseur transcriptionnel codé par un gène suppresseur de tumeurs localisé en 17p13.3. Cette région est perdue ou inactivée par hyperméthylation dans de nombreux cancers humains ; et les souris hétérozygotes Hic+/- développent des tumeurs spontanées avec une incidence beaucoup plus élevée que les souris contrôle.<br />Cette protéine est impliquée dans des boucles de régulation complexes impliquant p53, la désacétylase de classe III SIRT1 ainsi qu'une des protéines de contrôle du cycle cellulaire, E2F1.<br />En réponse aux dommages à l'ADN, HIC1 répri
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24

Sengo, Tigiti Shaaban Yusuf. "Hali ya kutatanisha ya Kiswahili hivi leo Afrika ya Mashariki." Universitätsbibliothek Leipzig, 2012. http://nbn-resolving.de/urn:nbn:de:bsz:15-qucosa-98041.

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The essay critically discusses the confusing state of the various Swahili language policies and studies brought forth in the colonial and post-colonial periods and examines the historical factors of the diversity within the Swahili language, which was once confined to the coastal area and later spread to the present area of distribution. The discussion focusses on the construction of Standard Swahili and the status of Swahili in regard to other East African languages. Special criticism is raised against recent East African and other authors, who wrote on the apparent unity of the Swahili langu
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25

Svensson, Phauline. "Hihi puss ;* : En studie av SMS-språket hos svenska högstadieungdomar." Thesis, Linnéuniversitetet, Institutionen för svenska språket (SV), 2013. http://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-28997.

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This study is about language use in text messaging. In this study there are 338 text messages: 206 of them written by girls and 132 written by boys. The informants in the study are 16 years old and they live in the countryside on the outskirts of a small town in southern Sweden. The purpose of this study was to investigate characteristic linguistic features in the messages, in order to determine what significant meaning an emoticon such as a smiley brings to a text and further, to explore what speech acts smileys occur in. The results show that the language in the messages is a mix of spoken a
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26

Washatka, John W. "A critical analysis of the religious epistemology of John Hick." Theological Research Exchange Network (TREN), 1988. http://www.tren.com.

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27

Fleuriel, Capucine. "Mécanismes différentiels de répression transcriptionnelle des gènes cibles de HIC1." Lille 2, 2009. http://tel.archives-ouvertes.fr/tel-00420474/fr/.

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HIC1 (Hypermethylated in Cancer 1) est un répresseur transcriptionnel codé par un gène suppresseur de tumeurs localisé en 17p13. 3. Cette région est perdue ou inactivée par hyperméthylation dans de nombreux cancers humains ; et les souris hétérozygotes Hic+/- développent des tumeurs spontanées avec une incidence beaucoup plus élevée que les souris contrôle. Cette protéine est impliquée dans des boucles de régulation complexes impliquant p53, la désacétylase de classe III SIRT1 ainsi qu'une des protéines de contrôle du cycle cellulaire, E2F1. En réponse aux dommages à l'ADN, HIC1 réprime SIRT1,
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28

Mafuta, Willy L. "Soteriology of the Bantu in the thought of John Hick." Online full text .pdf document, available to Fuller patrons only, 2002. http://www.tren.com.

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29

Tibaldo, Riccardo. "Caratteristiche principali di emissione di regioni HII." Bachelor's thesis, Alma Mater Studiorum - Università di Bologna, 2017. http://amslaurea.unibo.it/14089/.

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Si trattano le caratteristiche principali di regioni HII. Un particolare approfondimento viene condotto ai processi di generazione di fotoni, come emissione free-free, free-bound e bound-bound, e di interazione con la materia nei processi di estinzione. Dopodiché si impostano le equazioni di equilibrio: termico e di ionizzazione. Inoltre vengono forniti tre esempi di spettri in modo tale da verificare empiricamente i risultati teorici. Un capitolo finale è riservato allo studio delle abbondanze chimiche e del caso particolare delle Ultra-Compact HII.
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30

Giannakopoulou, Creighton Jean. "Molecular gas in HII regions of M101." Thesis, National Library of Canada = Bibliothèque nationale du Canada, 1998. http://www.collectionscanada.ca/obj/s4/f2/dsk2/tape15/PQDD_0014/NQ30597.pdf.

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31

Telles, Jose Eduardo. "The structure and environment of HII galaxies." Thesis, University of Cambridge, 1995. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.387723.

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32

Dubuissez, Marion. "Modifications post-traductionnelles de HIC1 et de BCL11 modulant le recrutement du complexe NuRD et mise en évidence de trois nouveaux gènes cibles directs de HIC1." Thesis, Lille 1, 2015. http://www.theses.fr/2015LIL10080/document.

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La famille des protéines MTA (Metastasis Tumor Antigen) compte trois membres MTA1, 2 et 3 qui diffèrent au niveau de leur extrémité C-terminale, une région désorganisée. La région N-terminale est impliquée dans l’interaction avec le complexe corépresseur NuRD. NuRD est recruté par des facteurs de transcription au niveau de leurs gènes cibles pour réprimer la transcription. Les protéines HIC1 et BCL11 recrutent le complexe NuRD via les protéines MTA afin de réprimer leurs gènes cibles.Au cours de ma thèse, je me suis intéressée aux modalités d’interactions entre les protéines HIC1 et BCL11 inte
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33

Jenal, Mathias. "HIC1 and BCL2A1 : novel factors involved in myeloid differentiation and survival /." Bern : [s.n.], 2009. http://www.zb.unibe.ch/download/eldiss/09jenal_m.pdf.

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34

Celander, Filip. "Rumsklang för hifi-lyssning : En undersökning av vanliga vardagsrums akustiska egenskaper." Thesis, University of Kalmar, Department of Technology, 2008. http://urn.kb.se/resolve?urn=urn:nbn:se:hik:diva-275.

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35

Arenas, Patricia Brekke. "Conservation genetics of an Island endemic bird, The Hihi (Notiomystis Cincta)." Thesis, Imperial College London, 2009. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.504901.

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36

Komatsu, Hiroko. "Prototypes and Metaphorical Extensions: The Japanese Numeral Classifiers hiki and hatsu." Thesis, The University of Sydney, 2018. http://hdl.handle.net/2123/19648.

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This study concerns the meaning of Japanese numeral classifiers (NCs) and, particularly, the elements which guide us to understand the metaphorical meanings they can convey. In the typological literature, as well as in studies of Japanese, the focus is almost entirely on NCs that refer to entities. NCs are generally characterised as being matched with a noun primarily based on semantic criteria such as the animacy, the physical characteristics, or the function of the referent concerned. However, in some languages, including Japanese, nouns allow a number of alternative NCs, so that it is consi
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37

Wall, William Frank. "Two HII/HI complexes in the outer galaxy." Thesis, University of British Columbia, 1986. http://hdl.handle.net/2429/26101.

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The HII regions S211 and S212 have been observed at 1420MHz, in both line and continuum, using the synthesis telescope at the Dominion Radio Astrophysical Observatory. S211 and S212 and their associated atomic hydrogen were studied as part of an ongoing investigation of HII/HI complexes within molecular clouds. S211 and S212 both require a flux of ionizing photons consistent with the ultraviolet emission from an 06V star. S211 was barely resolved (1.6 beam widths) and was thus modelled with a constant density model with density 85cm⁻³. S212 was modelled with linear density gradients and a cen
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Doherty, Ruth Mary. "Infrared spectroscopy of HII regions and starburst galaxies." Thesis, University of Edinburgh, 1994. http://hdl.handle.net/1842/27920.

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Observations of UCHII regions shown that HII region models with electron densities of n<I><SUB>e</SUB></I> = 10<SUP>4</SUP>cm<SUP>-3</SUP>, electron temperatures in the range T<I><SUB>e</SUB></I> = 5,000-10,000K and a Galactic helium abundance can reproduce the observed HeI 2.058<I>μ</I>m/Br<I>γ</I> ratios in these objects, subject to one condition. As the electron temperature is increased from T<I><SUB>e</SUB></I>=5,000K, microturbulence is incorporated into the model which counteracts the increase in the HeI 2.058<I>μ</I>m/Br<I>γ</I> ratio with electron temperature. Microturbulent velocities
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Bosch, G. "Giant extragalactic HII regions : 30 Doradus and beyond." Thesis, University of Cambridge, 1999. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.596793.

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This thesis aims to study both the stellar and the gaseous components of a sample of GEHRs and analyse the possible mechanisms that govern these forming regions. As there are no giant HII regions in our Galaxy, GEHRs from our Local Group of galaxies provide us with the data needed to understand these regions. Much has been done in this direction, and I review the latest efforts and our current knowledge in Chapter 1. Chapter 2 is focused on the analysis of the stellar population of the object that can better help us to understand GEHRs: 30 Doradus, our closest and largest neighbouring starburs
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Campbell, A. W. "The stellar populations and evolution of HII galaxies." Thesis, University of Cambridge, 1986. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.372865.

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41

Obonyo, Willice Odhiambo. "Open clusters and HII regions of our Galaxy." Master's thesis, University of Cape Town, 2015. http://hdl.handle.net/11427/19997.

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Open clusters are essential laboratories for understanding stellar evolution, as they allow constraints to be placed on stellar ages and luminosities. As distance indicators they are also important tracers of star formation in the Milky Way. One such cluster is Trumpler 27 that we identified for detailed study.The aim of the study is to estimate the distance, radial velocity, age, membership and reddening of the cluster using both spectroscopic and photometric techniques. We used new spectroscopic data collected from SAAO's 1.9m telescope together with existing photometric data from catalogues
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Mazou, Sébastien. ""Hic sunt leones" : défendre l'empire vénitien, 1453-1503." Thesis, Toulouse 2, 2018. http://www.theses.fr/2018TOU20023.

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Ce travail de recherche constitue une étude du dispositif militaire dans le Stato da Mar, les territoires maritimes de l’empire vénitien, pendant la seconde moitié du XVe siècle. Au cours de cette période, deux guerres opposent la république de Venise à l’Empire ottoman. Elles se concluent par des pertes territoriales pour Venise. Nous avons analysé l’articulation entre les trois outils de la défense du Stato da Mar, – les garnisons, la flotte de guerre et les stradiotes (cavaliers légers d’origine balkanique) – et les tentatives des dirigeants vénitiens de répondre au défi de la lutte contre
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Santos, Fabio Pereira. "Estudo fotométrico e polarimétrico de regiões HII galácticas." Universidade Federal de Minas Gerais, 2013. http://hdl.handle.net/1843/BUOS-97WFMS.

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Massive stars cause critical effects on the properties of the interstellar medium, ionizing, heating, evacuating the material, and consequently altering significantly the gas and dust spatial distribution. In such ionized environments, known as Hii regions, there is a strong relation between the characteristics of the interstellar medium and the young stellar population, with the properties of the magnetic field lines, which pervade the galactic disk. This relation may determine fundamental aspects of the influence of magnetic fields on the processes of star formation. In this research, our go
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44

Mendoza, Adalberto Rosales. "Relationship between microstructure, properties and HICC resistance of HSLA steel weld metals." Thesis, University of Leeds, 2008. http://etheses.whiterose.ac.uk/697/.

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The effects of microstructure, mechanical properties and hydrogen content on the hydrogen induced cold cracking (HICC) resistance of high strength low alloy (HSLA) steel weld metals were studied in this investigation. The weld metals were designed in a previous work. Their microstructures were characterised by optical and electron microscopy (FEG-SEM and TEM). Microphases, such as non metallic inclusions (NMI) and martensite-austenitecarbide constituent (MAC), were studied in some detail due to their hydrogen trapping capacity. Fractographic studies of hydrogen charged tensile samples were car
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45

Brady, Stephen William. "The intermediate state in the theology of Barth, Hick, Moltmann and Rahner." Thesis, London School of Theology, 1992. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.314780.

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46

Lienti, David A. "An analysis of the universalism contained in several works of John Hick." Theological Research Exchange Network (TREN), 1996. http://www.tren.com.

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47

Adams, Paul David. "The mystery of God incarnate an analysis and critique of John Hick's christology /." Theological Research Exchange Network (TREN) Access this title online, 1995. http://www.tren.com.

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48

Perry, T. S. "The Christian message in a postmodern world : a critical re-appropriation of Hendrik Kraemer's theology of religions." Thesis, Durham University, 1996. http://etheses.dur.ac.uk/5351/.

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This thesis is a critical re-appropriation of Hendrik Kraemer's theology of religions. Part I introduces theology of religions through the now familiar threefold typology: Kari Earth represents 'exclusivism,' Kari Rahner, 'inclusivism,' and John Hick, 'pluralism' (Chapter 1). It then argues that the typology implicitly represents non-pluralist approaches as theologically deficient and ethically insensitive while masking problems in pluralist positions (Chapter 2). It thus releases Kraemer from the typology and from the more emotive charges directed against 'exclusivism.' Part II chronologicall
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49

D'Costa, G. G. "A critical evaluation of John Hick's Copernican revolution in the Christain theology of religions." Thesis, University of Cambridge, 1986. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.382522.

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50

Loughlin, Gerard Patrick. "Mirroring God's world : a critique of John Hick's speculative theology." Thesis, University of Cambridge, 1987. https://www.repository.cam.ac.uk/handle/1810/284367.

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John Rick's work is important in its own right and as exemplary of a dominant empiricist tendency in academic religious thought. This dissertation seeks to display that tendency by exploring the possibility of reading Rick's work as Christian theology. To this end it examines Rick's reflections on six themes: religion, theology, theodicy, eschatology, Christology and theology of religions. It seeks to expose the faults and fissures, disruptions and distortions in Rick's texts. This explains the form of each chapter: a lengthy exposition and criticism of how Hick handles a particular theme, fol
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