1/r potential in higher dimensions

Abstract In Einstein gravity, gravitational potential goes as $$1/r^{d-3}$$ 1/rd-3 in d non-compactified spacetime dimensions, which assumes the familiar 1 / r form in four dimensions. On the other hand, it goes as $$1/r^{\alpha }$$ 1/rα , with $$\alpha =(d-2m-1)/m$$ α=(d-2m-1)/m , in pure Lovelock...

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Main Authors: Sumanta Chakraborty, Naresh Dadhich
Format: Article
Language:English
Published: SpringerOpen 2018-01-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-018-5546-1
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author Sumanta Chakraborty
Naresh Dadhich
author_facet Sumanta Chakraborty
Naresh Dadhich
author_sort Sumanta Chakraborty
collection DOAJ
description Abstract In Einstein gravity, gravitational potential goes as $$1/r^{d-3}$$ 1/rd-3 in d non-compactified spacetime dimensions, which assumes the familiar 1 / r form in four dimensions. On the other hand, it goes as $$1/r^{\alpha }$$ 1/rα , with $$\alpha =(d-2m-1)/m$$ α=(d-2m-1)/m , in pure Lovelock gravity involving only one mth order term of the Lovelock polynomial in the gravitational action. The latter offers a novel possibility of having 1 / r potential for the non-compactified dimension spectrum given by $$d=3m+1$$ d=3m+1 . Thus it turns out that in the two prototype gravitational settings of isolated objects, like black holes and the universe as a whole – cosmological models, the Einstein gravity in four and mth order pure Lovelock gravity in $$3m+1$$ 3m+1 dimensions behave in a similar fashion as far as gravitational interactions are considered. However propagation of gravitational waves (or the number of degrees of freedom) does indeed serve as a discriminator because it has two polarizations only in four dimensions.
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spelling doaj.art-c3ca666571804c2a82af6969d1a23b532022-12-22T00:24:36ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522018-01-017811710.1140/epjc/s10052-018-5546-11/r potential in higher dimensionsSumanta Chakraborty0Naresh Dadhich1Department of Theoretical Physics, Indian Association for the Cultivation of ScienceIUCAAAbstract In Einstein gravity, gravitational potential goes as $$1/r^{d-3}$$ 1/rd-3 in d non-compactified spacetime dimensions, which assumes the familiar 1 / r form in four dimensions. On the other hand, it goes as $$1/r^{\alpha }$$ 1/rα , with $$\alpha =(d-2m-1)/m$$ α=(d-2m-1)/m , in pure Lovelock gravity involving only one mth order term of the Lovelock polynomial in the gravitational action. The latter offers a novel possibility of having 1 / r potential for the non-compactified dimension spectrum given by $$d=3m+1$$ d=3m+1 . Thus it turns out that in the two prototype gravitational settings of isolated objects, like black holes and the universe as a whole – cosmological models, the Einstein gravity in four and mth order pure Lovelock gravity in $$3m+1$$ 3m+1 dimensions behave in a similar fashion as far as gravitational interactions are considered. However propagation of gravitational waves (or the number of degrees of freedom) does indeed serve as a discriminator because it has two polarizations only in four dimensions.http://link.springer.com/article/10.1140/epjc/s10052-018-5546-1
spellingShingle Sumanta Chakraborty
Naresh Dadhich
1/r potential in higher dimensions
European Physical Journal C: Particles and Fields
title 1/r potential in higher dimensions
title_full 1/r potential in higher dimensions
title_fullStr 1/r potential in higher dimensions
title_full_unstemmed 1/r potential in higher dimensions
title_short 1/r potential in higher dimensions
title_sort 1 r potential in higher dimensions
url http://link.springer.com/article/10.1140/epjc/s10052-018-5546-1
work_keys_str_mv AT sumantachakraborty 1rpotentialinhigherdimensions
AT nareshdadhich 1rpotentialinhigherdimensions