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Dissertations / Theses on the topic 'Comic modes'

Author: Grafiati

Published: 24 April 2022

Last updated: 30 July 2025

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1

Johnson, Clive. "'Something strangely mixed' : a study of the comic modes of Charles Dickens." Thesis, University of Kent, 2012. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.580358.

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This thesis asserts the importance of Dickensian comic modes. It engages with academic discourse and popular culture which between them have formulated a serious, socially engaged and psychologically dramatic Dickens in which comedy is muted. It examines the nature of Dickens's comedy and his debt to traditions of comic writing. It attempts to construct an understanding of Dickens in which comic modes are as vital as the dramatic to our understanding of Dickens's methods, themes and purposes. It adopts an inclusive approach to methodology in recognition of the wide-ranging nature of Dickensian

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2

Nizaruddin, Fathima. "Nuclear hallucinations : creating the vantage point of tamasha through the use of comic modes and irony in order to destabilise the authoritarian knowledge claims of Indian pro-nuclear documentaries." Thesis, University of Westminster, 2017. https://westminsterresearch.westminster.ac.uk/item/q3q54/nuclear-hallucinations-creating-the-vantage-point-of-tamasha-through-the-use-of-comic-modes-and-irony-in-order-to-destabilise-the-authoritarian-knowledge-claims-of-indian-pro-nuclear-documentaries.

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This practice-based research uses the context of the documentary assertions around the Indian nuclear project to examine how comic modes and irony can be employed to undermine authoritarian knowledge claims that make use of the epistephilic dimensions of the documentary form. An analysis of the pro-nuclear assertions in the documentary narratives of two state institutions in India, Films Division and Vigyan Prasar, was done as part of this enquiry. The diverse ways in which Indian anti-nuclear films engage with these narratives in humorous and ironic ways was also studied. The insights gained

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3

Harper, Graeme. "'Moon Dance' and the comic mode of displacement." Thesis, University of East Anglia, 1996. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.317978.

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4

Da, Silva Caroline Dos Santos. "Cosmic strings and scalar tensor gravity." Thesis, Durham University, 1999. http://etheses.dur.ac.uk/4577/.

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This thesis is concerned with the study of cosmic strings. We studied the values for the Higgs mass and string coupling for which the gravitational effect of an infinite cosmic string in the context of the Einstein theory is not only locally but also globally weak. We conclude this happens for strings formed at scales less or equal to the Planck one with Higgs mass being less or equal to the boson vectorial mass. Then we examined the metric of an isolated self-gravitating abelian-Higgs vortex in dilatonic gravity for arbitrary coupling of the vortex fields to the dilaton. We looked for solutio

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5

Teodoro, Matheus do Carmo. "Perturbations of black holes pierced by cosmic strings." Universidade de São Paulo, 2018. http://www.teses.usp.br/teses/disponiveis/76/76131/tde-05062018-104405/.

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The present-day interest in gravitational waves, justified by the recent direct detections made by LIGO, is opening the exciting possibility to answer many questions regarding General Relativity in extreme situations. One of these questions is whether black hole are – indeed – described totally by their mass, charge and angular momentum or whether they can have additional long-range hair. This project is concerned with this question. We aim at studying the influence of additional structure on the black hole horizon in the form of long-range hair by studying linearized Einstein equa

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6

Vanchurin, Vitaly. "Evolution of cosmic strings /." Thesis, Connect to Dissertations & Theses @ Tufts University, 2005.

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Thesis (Ph.D.)--Tufts University, 2005.<br>Adviser: Alexander Vilenkin. Submitted to the Dept. of Physics and Astronomy. Includes bibliographical references (leaf 99). Access restricted to members of the Tufts University community. Also available via the World Wide Web;

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7

Mather, Nigel Derek. "'Tears of laughter' : 1990s British cinema in the comic mode." Thesis, University of Kent, 2004. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.410597.

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8

KO, CHUNG-MING. "COSMIC-RAY MODIFIED STELLAR WINDS (ACCELERATION, MODULATION, DIFFUSION, TRANSONIC SOLUTION)." Diss., The University of Arizona, 1986. http://hdl.handle.net/10150/183980.

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A two fluid hydrodynamical model describing the modification of a stellar wind flow due to its interaction with galactic cosmic-rays is investigated. The two fluids consist of the thermal stellar wind gas and the galactic cosmic-rays. A polytropic one fluid model is used to describe the stellar wind gas, and the cosmic-rays modify the wind via their pressure gradient. The cosmic-rays are considered to be a hot low density gas of negligible mass flux, but with a significant pressure and energy flux compared to the thermal gas. The equations used are essentially those employed in two fluid hydro

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9

Siemens, Xavier. "Gravitational waves and cosmic strings /." Thesis, Connect to Dissertations & Theses @ Tufts University, 2002.

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Thesis (Ph.D.)--Tufts University, 2002.<br>Adviser: Alexander Vilenkin. Submitted to the Dept. of Physics. Includes bibliographical references (leaves 95-98). Access restricted to members of the Tufts University community. Also available via the World Wide Web;

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10

Wagner, Alexander. "Two-fluid models of cosmic-ray modified radiative shocks." Thesis, University of Leeds, 2007. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.485190.

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Two-fluid models of cosmic-ray modified radiative shocks were constructed for the purpose of interpreting optical emission from astrophysical shocks, including shocks in supernova remnants. The structure and stability of cosmic-ray modified radiative shocks without additional source terms were investigated first. Such a shock differs from a radiative shock that does not co~tain cosmic rays in that a cold dense layer does not fo\-m and the radiative overstability is always suppressed. If the diffusion length is comparable to or greater than the cooling length, the shock is nearly isothermal. St

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11

Gregory, Richard. "COSMIC : a model of cellular genetic interaction and evolution." Thesis, University of Liverpool, 2004. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.408565.

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12

Marquardt, Johannes Verfasser], Bernd [Akademischer Betreuer] [Heber, and Wolfgang [Gutachter] Dröge. "Galactic and Anomalous Cosmic Rays in the inner heliosphere : HELIOS E6 results / Johannes Marquardt ; Gutachter: Wolfgang Dröge ; Betreuer: Bernd Heber." Kiel : Universitätsbibliothek Kiel, 2019. http://nbn-resolving.de/urn:nbn:de:gbv:8-mods-2019-00084-7.

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13

Legg, Stephen. "Multi-mode receiver systems for cosmic microwave background B-mode polarisation experiments." Thesis, University of Manchester, 2018. https://www.research.manchester.ac.uk/portal/en/theses/multimode-receiver-systems-for-cosmic-microwave-background-bmode-polarisation-experiments(11399beb-9f3d-455b-b236-7d612ab1a00b).html.

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A measurement of the primordial B-mode polarisation of the Cosmic Microwave Background would provide direct evidence of inflation in the early universe. The extremely weak nature of the B-mode signal necessitates an instrument with a high sensitivity and precise control over systematic effects. Multi-mode antenna feed horns offer higher sensitivity than their single-mode counterparts, however their behaviour is much more complex. The Short Wavelength Instrument for the Polarisation Explorer (SWIPE) onboard the Large Scale Polarisation Explorer (LSPE) is one instrument planning to implement mul

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14

Horlacher, Stefan. "Slightly Quixotic: Comic Strategies, Sexual Role Stereotyping and the Functionalization of Femininity in David Lodge's Trilogy of Campus Novels under Special Consideration of 'Nice Work' (1988)." De Gruyter, 2007. https://tud.qucosa.de/id/qucosa%3A36417.

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In view of the fact that David Lodge’s campus novels are renowned for their ability to make light of traditional gender stereotypes as well as for their purportedly liberal, pro-feminist, intertexual, dialogical and metatextual dimensions, this article seeks to explore more precisely the strategic and unavowedly political functions humour and the comic fulfil in Changing Places, Small World and Nice Work. What will be demonstrated is that Lodge’s light-hearted, tolerant and at times even progressive liberalism is little more than an effect produced by the textual surface structure. In the case

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15

Salmanoglu, Murat. "An Error Prevention Model For Cosmic Functional Size Measurement Method." Master's thesis, METU, 2012. http://etd.lib.metu.edu.tr/upload/12614632/index.pdf.

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Estimation and measurement of the size of software is crucial for project management activities. Functional size measurement is one of the most frequently used methods to measure size of software and COSMIC is one of the popular methods for functional size measurement. Although precise size measurement is critical, the results may differ because of the errors made in the measurement process. The erroneous measurement results cause lack of confidence for the methods as well as reliability problems for effort and cost estimations. This research proposes an error prevention model for COSMIC Funct

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16

Majerotto, Elisabetta. "The cosmic late-time acceleration : theoretical models and observational constraints." Thesis, University of Portsmouth, 2008. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.494017.

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In this thesis we place constraints on models of the late-time acceleration of the universe. We put constraints on DGP braneworld models using supernovae, the cosmic microwave background shift parameter, and the baryon oscillation peak in the SDSS luminous red galaxy sample. The flat self-accelerating DGP model is marginally allowed by the combined likelihood, but the standard Lambda COM model fits the data better. The best fit of the flat non-selfaccelerating DGP model corresponds to the LCDM limit, which therefore gives a slightly better fit to the data, having oi less parameter. However, th

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17

Longden, C. "Building and testing models of cosmic inflation with modified gravity." Thesis, University of Sheffield, 2018. http://etheses.whiterose.ac.uk/21311/.

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Cosmic inflation, the idea that the very early universe underwent a dramatic accelerating expansion of space, has found great success in explaining aspects of the universe that were previously poorly understood. As a result, it has gained popularity and traction in the scientific mainstream in recent decades. However, it is still unclear exactly how inflation could have occurred; nothing in the established laws of physics can explain it. Now, in the modern era of precision cosmology, experimental data capable of probing and testing the details of this epoch has become available. With this, a d

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18

Castro, De Knibbs Dina. "Models of the cosmic Christ a critical analysis and perspectives /." Theological Research Exchange Network (TREN), 1991. http://www.tren.com.

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19

Errard, Josquin. "A hunt for cosmic microwave background B-modes in the sytematic contaminants jungle." Paris 7, 2012. http://www.theses.fr/2012PA077260.

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Cette thèse présente une étude de certains effets systématiques instrumentaux et astrophysiques, pouvant affecter les performances des nouvelles et futures générations d'observations de la polarisation du fond diffus cosmologique (CMB). Nous étudions l'impact de ces effets sur les objectifs scientifiques de ces observations, ainsi que les techniques pour leur élimination. Ce travail se concentre sur les problèmes généraux que rencontrent les expériences de manière générale, mais se penche également sur les questions plus spécifiques soulevées dans le cadre de l'expérience d'observation des mod

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20

Ata, Metin [Verfasser], and Volker [Akademischer Betreuer] Müller. "Phase-space reconstructions of cosmic velocities and the cosmic web : structure formation models - galaxy bias models - galaxy redshift surveys - inference analysis / Metin Ata ; Betreuer: Volker Müller." Potsdam : Universität Potsdam, 2016. http://d-nb.info/1218402849/34.

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21

Birch, Robert A. C. "Myth in the heroic comic-book : a reading of archetypes from The number one game and its models." Thesis, Stellenbosch : Stellenbosch University, 2008. http://hdl.handle.net/10019.1/1781.

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Thesis (MPhil (Visual Arts))--Stellenbosch University, 2008.<br>This thesis considers the author's project submission, a comic-book entitled The Number One Game, as production of a local heroic myth. The author will show how this project attempts to engage with mythic and archetypal material to produce an entertaining narrative that has relevance to contemporary Cape Town. The narrative adapts previous incarnations of the hero, with reference to theories of archetypes and mythic patterning devices that are derived from the concept of the “mono-myth”. Joseph Campbell's conception of myth a

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22

Marín, Campusano Beatriz Mariela. "Functional Size Measurement and Model Verification for Software Model-Driven Developments: A COSMIC-based Approach." Doctoral thesis, Universitat Politècnica de València, 2011. http://hdl.handle.net/10251/11237.

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Historically, software production methods and tools have a unique goal: to produce high quality software. Since the goal of Model-Driven Development (MDD) methods is no different, MDD methods have emerged to take advantage of the benefits of using conceptual models to produce high quality software. In such MDD contexts, conceptual models are used as input to automatically generate final applications. Thus, we advocate that there is a relation between the quality of the final software product and the quality of the models used to generate it. The quality of conceptual models can be influ

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23

Sollom, Ian Fraser. "Bayesian analysis of the CMB beyond the concordance model." Thesis, University of Cambridge, 2011. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.609814.

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24

Kaya, Mahir. "E-cosmic: A Business Process Model Based Functional Size Estimation Approach." Master's thesis, METU, 2010. http://etd.lib.metu.edu.tr/upload/3/12611538/index.pdf.

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The cost and effort estimation of projects depend on software size. A software product size is needed at as early a phase of the project as possible. Conventional Early Functional Size Estimation methods generate size at the early phase but result in subjectivity and unrepeatability due to manual calculation. On the other hand, automated Functional Size Measurement calculation approaches require constructs which are available in considerably late software development phases. In this study we developed an approach called e-Cosmic to calculate and automate the functional size measurement based

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25

Celik, Gul. "Parameter Estimation In Generalized Partial Linear Models With Conic Quadratic Programming." Master's thesis, METU, 2010. http://etd.lib.metu.edu.tr/upload/12612531/index.pdf.

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In statistics, regression analysis is a technique, used to understand and model the relationship between a dependent variable and one or more independent variables. Multiple Adaptive Regression Spline (MARS) is a form of regression analysis. It is a non-parametric regression technique and can be seen as an extension of linear models that automatically models non-linearities and interactions. MARS is very important in both classification and regression, with an increasing number of applications in many areas of science, economy and technology. In our study, we analyzed Generalized Partial Linea

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26

Soberanis, Policarpio Antonio. "Risk optimization with p-order conic constraints." Diss., University of Iowa, 2009. https://ir.uiowa.edu/etd/437.

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My dissertation considers solving of linear programming problems with p-order conic constraints that are related to a class of stochastic optimization models with risk objective or constraints that involve higher moments of loss distributions. The general proposed approach is based on construction of polyhedral approximations for p-order cones, thereby approximating the non-linear convex p-order conic programming problems using linear programming models. It is shown that the resulting LP problems possess a special structure that makes them amenable to efficient decomposition techniques. The de

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27

Regan, Donough Michael. "Measuring CMB non-Gaussianity as a probe of inflation and cosmic strings." Thesis, University of Cambridge, 2011. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.609806.

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28

Pieroni, Mauro. "Classification of inflationary models and constraints on fundamental physics." Thesis, Sorbonne Paris Cité, 2016. http://www.theses.fr/2016USPCC258/document.

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Ce travail est concentré sur l'étude de la cosmologie primordiale et en particulier sur l'étude de l'inflation. Après une introduction sur la théorie standard du Big Bang, nous discutons de la physique du CMB et nous expliquons comment ses observations peuvent être utilisées pour définir des contraintes sur les modèles cosmologiques. Nous introduisons l'inflation et nous expliquons sa réalisation la plus simple. Nous présentons les observables et les contraintes expérimentales qui peuvent être utilisées pour mettre des contraintes sur les modèles d'inflation. La possibilité d'observer des onde

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29

Shojaei, Hamed. "Interacting dark energy models as an approach for solving Cosmic Coincidence Problem." [Bloomington, Ind.] : Indiana University, 2009. http://gateway.proquest.com/openurl?url_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:dissertation&res_dat=xri:pqdiss&rft_dat=xri:pqdiss:3378380.

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Thesis (Ph.D.)--Indiana University, Dept. of Physics, 2009.<br>Title from PDF t.p. (viewed on Jul 12, 2010). Source: Dissertation Abstracts International, Volume: 70-10, Section: B, page: 6316. Adviser: Mike Berger.

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30

Wu, Juan. "Measurements of cosmic ray antiprotons with PAMELA and studies of propagation models." Doctoral thesis, KTH, Partikel- och astropartikelfysik, 2012. http://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-95331.

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Studying the acceleration and propagation mechanisms of Galactic cosmic rays can provide information regarding astrophysical sources, the properties of our Galaxy, and possible exotic sources such as dark matter. To understand cosmic ray acceleration and propagation mechanisms, accurate measurements of different cosmic ray elements over a wide energy range are needed. The PAMELA experiment is a satellite-borne apparatus which allows different cosmic ray species to be identified over background. Measurements of the cosmic ray antiproton flux and the antiproton-to-proton flux ratio from 1.5 GeV

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31

Giannantonio, Tommaso. "Constraining cosmological models with cosmic microwave background fluctuations from the late universe." Thesis, University of Portsmouth, 2008. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.516237.

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32

Valkenburg, Wessel. "Confronting models with cosmic perturbations : cosmological perturbations in earliest and largest stages." Chambéry, 2009. https://tel.archives-ouvertes.fr/tel-00419187.

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Cette thèse illustre les nombreuses possibilités permettant de relier les perturbations cosmologiques aux modèles théoriques décrivant I'univers. Aujourd'hui, nous observons ces perturbations cosmologiques sous des formes diverses. Les observations considérées dans cette thèse sont les anisotropies du rayonnement de fond cosmologique (CMB) et la distribution de matière dans I'univers (galaxies et amas de galaxies). Si à un temps initial, I'univers consistait en un plasma homogène et isotrope de matière et de rayonnement, il serait toujours homogène et isotrope aujourd'hui. Les perturbations co

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33

Sayre, James. "Measuring Polarization of the Cosmic Microwave Background with the South Pole Telescope Polarization Experiment." Case Western Reserve University School of Graduate Studies / OhioLINK, 2014. http://rave.ohiolink.edu/etdc/view?acc_num=case1407351244.

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34

Su, Shi Chun. "Post-inflationary non-Gaussianities on the cosmic microwave background." Thesis, University of Cambridge, 2015. https://www.repository.cam.ac.uk/handle/1810/249054.

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The cosmic microwave background (CMB) provides unprecedented details about the history of our universe and helps to establish the standard model in modern cosmology. With the ongoing and future CMB observations, higher precision can be achieved and novel windows will be opened for studying different phenomena. Non-Gaussianity is one of the most exciting effects which fascinate many cosmologists. While numerous alternative inflationary models predict detectable primordial non-Gaussianities generated during inflation, the single-field slow-roll inflation of the standard model is known to produce

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35

Walsh, Susan F. "Modifing risk perceptions of Japanese university students using a culturally compatible mode of instruction." Morgantown, W. Va. : [West Virginia University Libraries], 1999. http://etd.wvu.edu/templates/showETD.cfm?recnum=427.

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Thesis (Ed. D.)--West Virginia University, 1999.<br>Title from document title page. Written by Susan F. Walsh. Document formatted into pages; contains viii, 67 p. : ill. Vita. Includes abstract. Includes bibliographical references (p. 40-45).

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36

Green, Anne M. "Constraining models of the early universe : inflation, primordial black holes and cosmic strings." Thesis, University of Sussex, 1998. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.263155.

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37

Barello, Gregory. "Models and Constraints for New Physics at the Energy, Intensity, and Cosmic Frontiers." Thesis, University of Oregon, 2016. http://hdl.handle.net/1794/20454.

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The modern era of particle physics is driven by experimental anomalies. Experimental efforts have become increasingly diverse and are producing enormous volumes of data. In such a highly data-driven scientific environment theoretical models are necessary to understand this data and to help inform the development of new experimental approaches. In this dissertation I present two significant contributions to this effort relevant to the energy, intensity, and cosmic frontiers of modern particle physics research. Part 1 of this dissertation discusses methods to understand modern dark matter dir

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38

Minnie, Jaco. "An ab initio approach to the heliospheric modulation of galactic cosmic rays / Jaco Minnie." Thesis, North-West University, 2006. http://hdl.handle.net/10394/1258.

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In the present study we aim to further our understanding of charged particle transport in a magnetized medium. To this end, we perform direct numerical simulations of particle transport in a turbulent magnetic field. From the particle trajectories we calculate diffusion and drift coefficients. In contrast to previous numerical simulations of this nature, we also consider a background magnetic field that contains a gradient perpendicular to the magnetic field direction. By using a non-uniform background magnetic field, we can investigate the simultaneous large scale drift due to the gradient in

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39

Hanna-Korpi, Chloe. "Show and Tell: Improving the transfer of knowledge through narrative, image, and built form." University of Cincinnati / OhioLINK, 2011. http://rave.ohiolink.edu/etdc/view?acc_num=ucin1305892676.

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40

Imara, Nia, Abraham Loeb, Benjamin D. Johnson, Charlie Conroy, and Peter Behroozi. "A Model Connecting Galaxy Masses, Star Formation Rates, and Dust Temperatures across Cosmic Time." IOP PUBLISHING LTD, 2018. http://hdl.handle.net/10150/627101.

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We investigate the evolution of dust content in galaxies from redshifts z = 0 to z = 9.5. Using empirically motivated prescriptions, we model galactic-scale properties-including halo mass, stellar mass, star formation rate, gas mass, and metallicity-to make predictions for the galactic evolution of dust mass and dust temperature in main-sequence galaxies. Our simple analytic model, which predicts that galaxies in the early universe had greater quantities of dust than their low-redshift counterparts, does a good job of reproducing observed trends between galaxy dust and stellar mass out to z ap

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41

Morejon, Leonel. "New Interaction Models of Ultra-high-energy Cosmic Rays from a Nuclear Physics Approach." Doctoral thesis, Humboldt-Universität zu Berlin, 2021. http://dx.doi.org/10.18452/22585.

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Der Ursprung der ultrahochenergetischen kosmischen Strahlung (UHECRs) benötigt Modelle der photonuklearen kosmischen Strahlungsinteraktionen. In dieser Arbeit stelle ich Modelle vor, die drei Aspekte der Modellierung der Hochenergie-Astronuklearphysik verbessern: die Photomesonenproduktion durch Kerne der kosmischen Strahlung, die schwerer als Protonen sind, die Gammastrahlenemission von instabilen Kernen, die durch den Photodisintegrationsprozess der kosmischen Strahlung erzeugt werden, und die Simulation der extragalaktischen Ausbreitung von Kernen, die schwerer als Eisen sind (sogenannte su

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42

Wong, Chin Lin. "Beam Characterization and Systematics of the Bicep2 and Keck Array Cosmic Microwave Background Polarization Experiments." Thesis, Harvard University, 2014. http://nrs.harvard.edu/urn-3:HUL.InstRepos:13065012.

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Inflation, which posits an exponential expansion in the early universe, is well motivated since it resolves questions that are left unexplained by standard LCDM cosmology, such as the flatness and homogeneity of the universe. The exponential expansion of universe during inflation explains the structure in the universe by freezing out the quantum fluctuations of space. These quantum fluctuations are also expected to generate a background of gravitational waves which would then imprint a B-mode polarization signal on the Cosmic Microwave Background. The Bicep2 and Keck Array experiments search f

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43

Sanyal, Subrata. "A Study of sensitivity of different high energy interaction models by the cosmic ray extensive air shower technique at the energy levels of 10^14 eV." Thesis, University of North Bengal, 1995. http://hdl.handle.net/123456789/678.

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44

Shi, Xun [Verfasser]. "Third-order Cosmic Shear Statistics: Covariance, Nulling, and E/B-mode decomposition / Xun Shi." Bonn : Universitäts- und Landesbibliothek Bonn, 2012. http://d-nb.info/1043910859/34.

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Ndiitwani, Dzivhuluwani Christopher. "A study of the time-dependent modulation of galactic cosmic rays in the heliosphere / Dzivhuluwani C. Ndiitwani." Thesis, North-West University, 2005. http://hdl.handle.net/10394/843.

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Time-dependent cosmic ray modulation in the heliosphere is studied by using a two-dimensional time dependent modulation model. To compute realistic cosmic ray modulation a compound approach is used, which combines the effect of the global changes in the heliospheric magnetic field magnitude and the current sheet tilt angle to establish realistic time dependent diffusion and drift coefficients. This approach is refined by scaling down drifts additionally (compared to diffusion) towards solar maximum. The amount of drifts needed in the model to realistically compute 2.5 GV proton and electron an

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46

O'Sullivan, Mark George. "Warping, dust settling and dynamics of protoplanetary disks." Thesis, St Andrews, 2008. http://hdl.handle.net/10023/782.

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47

Fraschetti, F., and M. Pohl. "Particle acceleration model for the broad-band baseline spectrum of the Crab nebula." OXFORD UNIV PRESS, 2017. http://hdl.handle.net/10150/625798.

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We develop a simple one-zone model of the steady-state Crab nebula spectrum encompassing both the radio/soft X-ray and the GeV/multi-TeV observations. By solving the transport equation for GeV-TeV electrons injected at the wind termination shock as a log-parabola momentum distribution and evolved via energy losses, we determine analytically the resulting differential energy spectrum of photons. We find an impressive agreement with the observed spectrum of synchrotron emission, and the synchrotron self-Compton component reproduces the previously unexplained broad 200-GeV peak that matches the F

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48

Itow, Y. "Verification of hadron interaction models of cosmic rays at 10**17 eV by the LHCf experiment." American Institite of Physics, 2008. http://hdl.handle.net/2237/12228.

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Morejon, Leonel [Verfasser]. "New Interaction Models of Ultra-high-energy Cosmic Rays from a Nuclear Physics Approach / Leonel Morejon." Berlin : Humboldt-Universität zu Berlin, 2021. http://d-nb.info/1230406751/34.

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Florinski, Vladimir A. "A two-dimensional, self-consistent model of galactic and anomalous cosmic rays in the solar wind." Diss., The University of Arizona, 2001. http://hdl.handle.net/10150/289934.

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Abstract:

We have developed a two-dimensional heliospheric model that includes galactic and anomalous cosmic rays as well as pickup ions. Cosmic rays are described via their number density in phase space, rather than pressure, as every preceding 2-D model has done. Cosmic-ray pressure is included in the total energy budget, allowing us to compute dynamical effects of the energetic particles on the solar wind. We include the magnetic field as well in order to consistently compute cosmic-ray diffusion coefficients. To accommodate' lower-energy cosmic rays with their short diffusion length, we implemented

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