dc.contributor.advisor |
Visser, Matt |
|
dc.contributor.author |
Jozef Skakala |
|
dc.date.accessioned |
2011-07-14T20:35:58Z |
|
dc.date.available |
2011-07-14T20:35:58Z |
|
dc.date.copyright |
2011 |
|
dc.date.issued |
2011 |
|
dc.identifier.uri |
http://researcharchive.vuw.ac.nz/handle/10063/1697 |
|
dc.description.abstract |
This thesis is based on three different projects, all of them are directly linked to
the classical general theory of relativity, but they might have consequences for
quantum gravity as well.
The first chapter deals with pseudo-Finsler geometric extensions of the classical
theory, these being ways of naturally representing high-energy Lorentz
symmetry violations. In this chapter we prove a certain type of “no-go” result
for significant number of theories. This seems to have important consequences
for the question of whether some weaker formulation of Einstein’s equivalence
principle is sustainable, if (at least) certain types of Lorentz violations occur.
The second chapter deals with the problem of highly damped quasi-normal
modes related to different types of black hole spacetimes. First, we apply to
this problem the technique of approximation by analytically solvable potentials.
We use the Schwarzschild black hole as a consistency check for our method
and derive many new and interesting results for the Schwarzschild-de Sitter (SdS)
black hole. One of the most important results is the equivalence between
having a rational ratio of horizon surface gravities and periodicity of quasinormal
modes. By analysing the complementary set of analytic results derived
by the use of monodromy techniques we prove that all our theorems almost
completely generalize to all the known analytic results. This relates to all the
types of black holes for which quasi-normal mode results are currently known.
The third chapter is related to the topic of multiplication of tensorial distributions.
We focus on an alternative approach to the ones presently known.
The new approach is fully based on the Colombeau equivalence relation, but
technically avoids the Colombeau algebra construction. The advantage of this
approach is that it naturally generalizes the covariant derivative operator into
the generalized tensor algebra. It also operates with much more general concept
of piecewise smooth manifold, which is in our opinion natural to the language
of distributions. |
en_NZ |
dc.language.iso |
en_NZ |
|
dc.publisher |
Victoria University of Wellington |
en_NZ |
dc.subject |
Quantum gravity |
en_NZ |
dc.subject |
Gravitation |
en_NZ |
dc.subject |
General relativity |
en_NZ |
dc.title |
Aspects of General Relativity:
Pseudo-Finsler Extensions,
Quasi-Normal Frequencies and
Multiplication of Tensorial
Distributions |
en_NZ |
dc.type |
Text |
en_NZ |
vuwschema.contributor.unit |
School of Mathematics, Statistics and Operations Research |
en_NZ |
vuwschema.subject.marsden |
230120 Mathematics not Elsewhere Classified |
en_NZ |
vuwschema.type.vuw |
Awarded Doctoral Thesis |
en_NZ |
thesis.degree.discipline |
Mathematics |
en_NZ |
thesis.degree.grantor |
Victoria University of Wellington |
en_NZ |
thesis.degree.level |
Doctoral |
en_NZ |
thesis.degree.name |
Doctor of Philosophy |
en_NZ |
vuwschema.subject.anzsrcfor |
019999 Mathematical Sciences not elsewhere classified |
en_NZ |