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  • About
  • The Global ETD Search service is a free service for researchers to find electronic theses and dissertations. This service is provided by the Networked Digital Library of Theses and Dissertations.
    Our metadata is collected from universities around the world. If you manage a university/consortium/country archive and want to be added, details can be found on the NDLTD website.
1

An investigation of student understanding of basic concepts in special relativity /

Scherr, Rachel Ellen, January 2001 (has links)
Thesis (Ph. D.)--University of Washington, 2001. / Vita. Includes bibliographical references (leaves 178-181).
2

Problems for presentism the inconsistency of presentism with the special theory of relativity /

Dixon, Thomas S. January 2008 (has links)
Thesis (M.A.)--University of Wyoming, 2008. / Title from PDF title page (viewed on July 13, 2009). Includes bibliographical references (p. 88-90).
3

On philosophical implications of the special theory of relativity

Forman, Barry January 1969 (has links)
No description available.
4

Geometry of deformed special relativity

Sixaba, Vuyile January 2018 (has links)
We undertake a study of the classical regime in which Planck's constant and Newton's gravitational constant are negligible, but not their ratio, the Planck mass, in hopes that this could possibly lead to testable quantum gravity (QG) effects in a classical regime. In this quest for QG phenomenology we consider modifications of the standard dispersion relation of a free particle known as deformed special relativity (DSR). We try to geometrize DSR to find the geometric origin of the spacetime and momentum space. In particular, we adopt the framework of Hamilton geometry which is set up on phase space, as the cotangent bundle of configuration space in order to derive a purely phase space formulation of DSR. This is necessary when one wants to understand potential links of DSR with modifications of quantum mechanics such as Generalised Uncertainty Principles. It is subsequently observed that space-time and momentum space emerge naturally as curved and intertwined spaces. In conclusion we mention examples and applications of this framework as well as potential future developments.
5

The relativistic foundations of synchrotron radiation

Margaritondo, Giorgio, Rafelski, Johann 20 June 2017 (has links)
Special relativity (SR) determines the properties of synchrotron radiation, but the corresponding mechanisms are frequently misunderstood. Time dilation is often invoked among the causes, whereas its role would violate the principles of SR. Here it is shown that the correct explanation of the synchrotron radiation properties is provided by a combination of the Doppler shift, not dependent on time dilation effects, contrary to a common belief, and of the Lorentz transformation into the particle reference frame of the electromagnetic field of the emission-inducing device, also with no contribution from time dilation. Concluding, the reader is reminded that much, if not all, of our argument has been available since the inception of SR, a research discipline of its own standing.
6

Numerical Hydrodynamics of Relativistic Extragalactic Jets

Choi, Eunwoo 04 May 2007 (has links)
This dissertation describes a multidimensional relativistic hydrodynamic code which solves the special relativistic hydrodynamic equations as a hyperbolic system of conservation laws based on the total variation diminishing (TVD) scheme. Several standard tests and test simulations are presented to demonstrate the accuracy, robustness and flexibility of the code. Using this code we have studied three-dimensional hydrodynamic interactions of relativistic extragalactic jets with two-phase ambient media. The deflection angle of the jet is influenced more by the density contrast of the cloud than by the beam Mach number of the jet, and a relativistic jet with low relativistic beam Mach number can eventually be slightly bent after it crosses the dense cloud. Relativistic jet impacts on dense clouds do not necessarily destroy the clouds completely, and much of the cloud body can survive as a coherent blob due to the combination of the geometric influence of off-axis collisions and the lower rate of cloud fragmentation through the Kelvin-Helmholtz instability for relativistic flows. We find that relativistic jets interacting with clouds can produce synchrotron emission knots similar to structures observed in many VLBI-scale radio sources and the synchrotron emission peaks right before the jet passes through the cloud.
7

A special Davidsonian theory of events

Douglas, Keith 11 1900 (has links)
What is an event? What sort of object are they? How is a given event distinguished from other events and other objects? This thesis on science oriented metaphysics will take Davidson's account of events as its starting point to answer the above questions. It will develop this conception of events into one that is consistent with the special theory of relativity by updating its notions of change, cause and property. The new concept of a proper property, a generalization of the notion of an invariant, is introduced to solve some of these metascientific problems. Other features of the work include an analysis of the Lorentz force equation as it applies to one family of cases of causation, showing that a use of cause and effect to help individuate events cannot be complete until relativistic features are built into it. I propose that the conception of a proper property will also solve this worry over the nature of causation as it affects the issues of events above. In particular, it will attempt to solve a charge of circularity which has been leveled at Davidson's account. This property analysis also has the feature that it makes the account of events which started with Davidsonian inspiration (i.e. causes and effects are intimately connected to events) more like Kim's. Kim's account of events is modified on the grounds it does not do justice to our intuitions about changes and events.
8

Photospheric emission from structured, relativistic jets : applications to gamma-ray burst spectra and polarization

Lundman, Christoffer January 2013 (has links)
The radiative mechanism responsible for the prompt gamma-ray burst (GRB) emission remains elusive. For the last decade, optically thin synchrotron emission from shocks internal to the GRB jet appeared to be the most plausible explanation. However, the synchrotron interpretation is incompatible with a significant fraction of GRB observations, highlighting the need for new ideas. In this thesis, it is shown that the narrow, dominating component of the prompt emission from the bright GRB090902B is initially consistent only with emission released at the optically thick jet photosphere. However, this emission component then broadens in time into a more typical GRB spectrum, which calls for an explanation. In this thesis, a previously unconsidered way of broadening the spectrum of photospheric emission, based on considerations of the lateral jet structure, is presented and explored. Expressions for the spectral features, as well as polarization properties, of the photospheric emission observed from structured, relativistic jets are derived analytically under simplifying assumptions on the radiative transfer close to the photosphere. The full, polarized radiative transfer is solved through Monte Carlo simulations, using a code which has been constructed for this unique purpose. It is shown that the typical observed GRB spectrum can be obtained from the photosphere, without the need for additional, commonly assumed, physical processes (e.g. energy dissipation, particle acceleration, or additional radiative processes). Furthermore, contrary to common expectations, it is found that the observed photospheric emission can be highly linearly polarized (up to $\sim 40 \, \%$). In particular, it is shown that a shift of $\pi/2$ of the angle of polarization is the only shift allowed by the proposed model, consistent with the only measurement preformed to date. A number of ways to test the theory is proposed, mainly involving simultaneous spectral and polarization measurements. The simplest measurement, which tests not only the proposed theory but also common assumptions on the jet structure, involves only two consecutive measurements of the angle of polarization during the prompt emission. / <p>QC 20131204</p>
9

A special Davidsonian theory of events

Douglas, Keith 11 1900 (has links)
What is an event? What sort of object are they? How is a given event distinguished from other events and other objects? This thesis on science oriented metaphysics will take Davidson's account of events as its starting point to answer the above questions. It will develop this conception of events into one that is consistent with the special theory of relativity by updating its notions of change, cause and property. The new concept of a proper property, a generalization of the notion of an invariant, is introduced to solve some of these metascientific problems. Other features of the work include an analysis of the Lorentz force equation as it applies to one family of cases of causation, showing that a use of cause and effect to help individuate events cannot be complete until relativistic features are built into it. I propose that the conception of a proper property will also solve this worry over the nature of causation as it affects the issues of events above. In particular, it will attempt to solve a charge of circularity which has been leveled at Davidson's account. This property analysis also has the feature that it makes the account of events which started with Davidsonian inspiration (i.e. causes and effects are intimately connected to events) more like Kim's. Kim's account of events is modified on the grounds it does not do justice to our intuitions about changes and events. / Arts, Faculty of / Philosophy, Department of / Graduate
10

Relativistic Visualizations / Relativistic Visualizations

Ringstam, Andreas January 2020 (has links)
Special relativity is an area of physics that is abstract and consists of concepts and effects that is hard to link to everyday experience. From a learning perspective, that is problematic as we form new knowledge by linking it to old experiences. One approach to experience a relativistic environment is through computer simulations. MIT game lab has developed the game “A Slower Speed of Light” where the user slows down the speed of light in discrete steps. That allows the user to experience what the surroundings would look like if we were traveling at a relativistic speed. As the user does that, he/she will experience that certain visual effects do not appear as the course literature describes it. In this project, we study how visual effects of special relativity are perceived by students by letting them play the game and solve an assignment. In the assignment, there was one problem where they were instructed to identify two relativistic effects and describe the physics behind them. The project aims to find an answer to what students while playing the game think they see and how they relate the visual effects to quantities arrived by applying the Lorentz transformation. The project also investigates whether the game can be used productively in teaching. The findings of project show that it is easier for students to describe visual effects where observation match with what the students actually see. We have also found that the students' perception of visual effects is that they are consistent with the predictions of the Lorentz transformation as they try to force their observations onto the theory. That despite the fact that the game clearly shows that it is not the case. The game can be used productively by a teacher when lecturing e.g. relativistic optics. / Speciell relativitetsteori är ett område inom fysiken som är abstrakt och består av begrepp och effekter som är svåra att länka till vardagslivet. Från ett lärandeperspektiv blir det problematiskt då vi bildar ny kunskap genom att länka det till gamla erfarenheter. Ett sätt att få uppleva en relativistisk miljö är genom datorsimuleringar. MIT game lab har utvecklat spelet “A Slower Speed of Light” där användaren stegvis saktar ner ljusets hastighet. Detta gör det möjligt för användaren att uppleva hur omgivningen skulle se ut om vi färdades i en relativistisk hastighet. När användaren färdas relativistiskt kommer han/hon uppleva att vissa visuella effekter inte stämmer överens med beskrivningar från kurslitteratur. I detta projekt studerar vi hur visuella effekter av den speciella relativitetsteorin uppfattas av studenter genom att låta dem spela spelet och lösa en inlämningsuppgift. I inlämningsuppgiften fanns ett problem där de skulle identifiera två relativistiska effekter och beskriva fysiken bakom dessa. Projektet försöker att besvara vilka effekter studenter tror att de ser när de spelar spelet men också hur de relaterar de visuella effekterna till värden som förutsägs genom Lorentz transformationen. Projektet undersöker också om spelet kan användas produktivt i undervisning. Projektets observationer visar att studenterna har lättare att beskriva visuella effekter där observation stämmer överens med vad studenterna faktiskt ser. Vi har ocksånoterat att studenternas föreställning om visuella effekter är att de stämmer överens med Lorentztransformationens förutsägelser då de försöker tvinga sina observationer att överensstämma med teorin trots att spelet tydligt visar att det inte är fallet. Spelet kan användas produktivt av en lärare vid föreläsning av t.ex. relativistisk optik.

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