FINE TUNING PROBLEM IN FIVE-DIMENSIONAL BRANE WORLD MODELS
Fine tuning can be called a main disadvantage of the Randall-Sundrum model, representing the most popular brane world model, constructed quite artificially in the five-dimensional space-time. It needs a bare multidimensional cosmological constant, which is related strictly to four-dimensional tensio...
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Odessa I. I. Mechnykov National University
2012-11-01
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doaj-2094a043f819490b8e283b2302dadd172020-11-25T03:28:35ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152012-11-0125210.18524/1810-4215.2012.25.8333283332FINE TUNING PROBLEM IN FIVE-DIMENSIONAL BRANE WORLD MODELSS. H. Fakhr0M. EingornA. ZhukAstronomical Observatory, Odessa National University, Odessa, Ukraine;Fine tuning can be called a main disadvantage of the Randall-Sundrum model, representing the most popular brane world model, constructed quite artificially in the five-dimensional space-time. It needs a bare multidimensional cosmological constant, which is related strictly to four-dimensional tension (the brane physical property). Here we try to avoid this problem of naturalness, introducing a perfect fluid with arbitrary equations of state in both three-dimensional external and onedimensional internal spaces parallel with the cosmological constant. It enables to preserve randomness of parameters of the considered model, which represents the direct generalization of the Randall-Sundrum one. We derive equations for background metric coefficients, determining a wide class of new exact solutions, and discuss uselessness of subsequent development of brane world models in view of their unjustified plurality.http://oap.onu.edu.ua/article/view/83332 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
S. H. Fakhr M. Eingorn A. Zhuk |
spellingShingle |
S. H. Fakhr M. Eingorn A. Zhuk FINE TUNING PROBLEM IN FIVE-DIMENSIONAL BRANE WORLD MODELS Odessa Astronomical Publications |
author_facet |
S. H. Fakhr M. Eingorn A. Zhuk |
author_sort |
S. H. Fakhr |
title |
FINE TUNING PROBLEM IN FIVE-DIMENSIONAL BRANE WORLD MODELS |
title_short |
FINE TUNING PROBLEM IN FIVE-DIMENSIONAL BRANE WORLD MODELS |
title_full |
FINE TUNING PROBLEM IN FIVE-DIMENSIONAL BRANE WORLD MODELS |
title_fullStr |
FINE TUNING PROBLEM IN FIVE-DIMENSIONAL BRANE WORLD MODELS |
title_full_unstemmed |
FINE TUNING PROBLEM IN FIVE-DIMENSIONAL BRANE WORLD MODELS |
title_sort |
fine tuning problem in five-dimensional brane world models |
publisher |
Odessa I. I. Mechnykov National University |
series |
Odessa Astronomical Publications |
issn |
1810-4215 |
publishDate |
2012-11-01 |
description |
Fine tuning can be called a main disadvantage of the Randall-Sundrum model, representing the most popular brane world model, constructed quite artificially in the five-dimensional space-time. It needs a bare multidimensional cosmological constant, which is related strictly to four-dimensional tension (the brane physical property). Here we try to avoid this problem of naturalness, introducing a perfect fluid with arbitrary equations of state in both three-dimensional external and onedimensional internal spaces parallel with the cosmological constant. It enables to preserve randomness of parameters of the considered model, which represents the direct generalization of the Randall-Sundrum one. We derive equations for background metric coefficients, determining a wide class of new exact solutions, and discuss uselessness of subsequent development of brane world models in view of their unjustified plurality. |
url |
http://oap.onu.edu.ua/article/view/83332 |
work_keys_str_mv |
AT shfakhr finetuningprobleminfivedimensionalbraneworldmodels AT meingorn finetuningprobleminfivedimensionalbraneworldmodels AT azhuk finetuningprobleminfivedimensionalbraneworldmodels |
_version_ |
1724583207909720064 |