Aspects of finite temperature corrections in string theory

In this thesis some aspects of temperature corrections in string theory are analyzed: in particular, we study the thermal contributions to the 4 dimensional effective potential arising from string theory compactifications. String theory predicts that the spacetime has more than 4 dimensions; in part...

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Main Author: Calo, Vincenzo
Published: Queen Mary, University of London 2011
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Online Access:https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.531452
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spelling ndltd-bl.uk-oai-ethos.bl.uk-5314522019-02-27T03:16:53ZAspects of finite temperature corrections in string theoryCalo, Vincenzo2011In this thesis some aspects of temperature corrections in string theory are analyzed: in particular, we study the thermal contributions to the 4 dimensional effective potential arising from string theory compactifications. String theory predicts that the spacetime has more than 4 dimensions; in particular, supersymmetric string theories are consistent only if the spacetime has 10 dimensions, 1 time plus 9 space directions. In order to describe the physics of our Universe with string theory we make 6 spatial directions very small, namely, we curl them into a 6-dimensional space. The resulting 4-dimensional theory depends on a large number of parameters which are massless scalar fields called moduli. The different values that the moduli can take represent both the possible deformations of the 6- dimensional compact space and the values of the coupling constants and masses in the 4-dimensional spacetime. Allowing them to have arbitrary values leads to a lack of predictability of various 4D physical quantities, to a huge vacuum degeneracy and to unobserved long range fifth forces. In the thesis we review some methods established in the literature in order to fix the moduli values and hence to fix a particular geometry and we investigate how the inclusion of temperature corrections alter their values and affect the geometry of the compact space. The analysis seems to suggest that at least in the specific compactification scenarios considered in this thesis, temperature corrections do not alter substantially the zero temperature results. In the final part of this work, we analyze instead an example in which the inclusion of temperature corrections alters dramatically the picture at zero temperature. In particular, we study an unstable system constituted by a pair of Dirichlet (D) and anti-D brane that, although being unstable at zero temperature, it can become stable once finite temperature corrections are switched on.530.1PhysicsQueen Mary, University of Londonhttps://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.531452http://qmro.qmul.ac.uk/xmlui/handle/123456789/701Electronic Thesis or Dissertation
collection NDLTD
sources NDLTD
topic 530.1
Physics
spellingShingle 530.1
Physics
Calo, Vincenzo
Aspects of finite temperature corrections in string theory
description In this thesis some aspects of temperature corrections in string theory are analyzed: in particular, we study the thermal contributions to the 4 dimensional effective potential arising from string theory compactifications. String theory predicts that the spacetime has more than 4 dimensions; in particular, supersymmetric string theories are consistent only if the spacetime has 10 dimensions, 1 time plus 9 space directions. In order to describe the physics of our Universe with string theory we make 6 spatial directions very small, namely, we curl them into a 6-dimensional space. The resulting 4-dimensional theory depends on a large number of parameters which are massless scalar fields called moduli. The different values that the moduli can take represent both the possible deformations of the 6- dimensional compact space and the values of the coupling constants and masses in the 4-dimensional spacetime. Allowing them to have arbitrary values leads to a lack of predictability of various 4D physical quantities, to a huge vacuum degeneracy and to unobserved long range fifth forces. In the thesis we review some methods established in the literature in order to fix the moduli values and hence to fix a particular geometry and we investigate how the inclusion of temperature corrections alter their values and affect the geometry of the compact space. The analysis seems to suggest that at least in the specific compactification scenarios considered in this thesis, temperature corrections do not alter substantially the zero temperature results. In the final part of this work, we analyze instead an example in which the inclusion of temperature corrections alters dramatically the picture at zero temperature. In particular, we study an unstable system constituted by a pair of Dirichlet (D) and anti-D brane that, although being unstable at zero temperature, it can become stable once finite temperature corrections are switched on.
author Calo, Vincenzo
author_facet Calo, Vincenzo
author_sort Calo, Vincenzo
title Aspects of finite temperature corrections in string theory
title_short Aspects of finite temperature corrections in string theory
title_full Aspects of finite temperature corrections in string theory
title_fullStr Aspects of finite temperature corrections in string theory
title_full_unstemmed Aspects of finite temperature corrections in string theory
title_sort aspects of finite temperature corrections in string theory
publisher Queen Mary, University of London
publishDate 2011
url https://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.531452
work_keys_str_mv AT calovincenzo aspectsoffinitetemperaturecorrectionsinstringtheory
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