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The Taming of Closed Time-like Curves
We formulate QFT on a $R^{1,d}/Z_2$ orbifold, in a manner which is invariant under the $Z_2$ time and space reversal. This is a background with closed time-like curves. It is also relevant for the elliptic interpretation of de Sitter space. We calculate the one-loop vacuum expectation value of the s...
Autores principales: | , , , , |
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Lenguaje: | eng |
Publicado: |
2003
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/1126-6708/2004/01/064 http://cds.cern.ch/record/614446 |
_version_ | 1780900280766824448 |
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author | Biswas, Rahul Keski-Vakkuri, Esko Leigh, Robert G. Nowling, Sean Sharpe, Eric |
author_facet | Biswas, Rahul Keski-Vakkuri, Esko Leigh, Robert G. Nowling, Sean Sharpe, Eric |
author_sort | Biswas, Rahul |
collection | CERN |
description | We formulate QFT on a $R^{1,d}/Z_2$ orbifold, in a manner which is invariant under the $Z_2$ time and space reversal. This is a background with closed time-like curves. It is also relevant for the elliptic interpretation of de Sitter space. We calculate the one-loop vacuum expectation value of the stress tensor in the invariant QFT, and show that it does not diverge at the boundary of the region of closed time-like curves. Rather, the only divergence is at the initial time slice of the orbifold, analogous to a spacelike Big-Bang singularity. We then calculate the one-loop graviton tadpole in bosonic string theory, and show that the answer is the same as if the target space would be just the Minkowski space $R^{1,d}$, suggesting that the tadpole vanishes for the superstring. Finally, we argue that it is possible to define local S-matrices, even if the spacetime is globally time-nonorientable. |
id | cern-614446 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2003 |
record_format | invenio |
spelling | cern-6144462023-03-14T18:43:08Zdoi:10.1088/1126-6708/2004/01/064http://cds.cern.ch/record/614446engBiswas, RahulKeski-Vakkuri, EskoLeigh, Robert G.Nowling, SeanSharpe, EricThe Taming of Closed Time-like CurvesParticle Physics - TheoryWe formulate QFT on a $R^{1,d}/Z_2$ orbifold, in a manner which is invariant under the $Z_2$ time and space reversal. This is a background with closed time-like curves. It is also relevant for the elliptic interpretation of de Sitter space. We calculate the one-loop vacuum expectation value of the stress tensor in the invariant QFT, and show that it does not diverge at the boundary of the region of closed time-like curves. Rather, the only divergence is at the initial time slice of the orbifold, analogous to a spacelike Big-Bang singularity. We then calculate the one-loop graviton tadpole in bosonic string theory, and show that the answer is the same as if the target space would be just the Minkowski space $R^{1,d}$, suggesting that the tadpole vanishes for the superstring. Finally, we argue that it is possible to define local S-matrices, even if the spacetime is globally time-nonorientable.We consider a $R^{1,d}/Z_2$ orbifold, where $Z_2$ acts by time and space reversal, also known as the embedding space of the elliptic de Sitter space. The background has two potentially dangerous problems: time-nonorientability and the existence of closed time-like curves. We first show that closed causal curves disappear after a proper definition of the time function. We then consider the one-loop vacuum expectation value of the stress tensor. A naive QFT analysis yields a divergent result. We then analyze the stress tensor in bosonic string theory, and find the same result as if the target space would be just the Minkowski space $R^{1,d}$, suggesting a zero result for the superstring. This leads us to propose a proper reformulation of QFT, and recalculate the stress tensor. We find almost the same result as in Minkowski space, except for a potential divergence at the initial time slice of the orbifold, analogous to a spacelike Big Bang singularity. Finally, we argue that it is possible to define local S-matrices, even if the spacetime is globally time-nonorientable.hep-th/0304241HIP-2003-28-THCERN-TH-2003-097CERN-TH-2003-097HIP-2003-28-THoai:cds.cern.ch:6144462003-04-28 |
spellingShingle | Particle Physics - Theory Biswas, Rahul Keski-Vakkuri, Esko Leigh, Robert G. Nowling, Sean Sharpe, Eric The Taming of Closed Time-like Curves |
title | The Taming of Closed Time-like Curves |
title_full | The Taming of Closed Time-like Curves |
title_fullStr | The Taming of Closed Time-like Curves |
title_full_unstemmed | The Taming of Closed Time-like Curves |
title_short | The Taming of Closed Time-like Curves |
title_sort | taming of closed time-like curves |
topic | Particle Physics - Theory |
url | https://dx.doi.org/10.1088/1126-6708/2004/01/064 http://cds.cern.ch/record/614446 |
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