A Scale at 10 MeV, Gravitational Topological Vacuum, and Large Extra Dimensions

We discuss a possible scale of gravitational origin at around 10 MeV, or 10−12 cm, which arises in the MacDowell–Mansouri formalism of gravity due to the topological Gauss–Bonnet term in the action, as pointed out by Bjorken several years ago. A length scale of the same size emerges also in the Koda...

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Main Author: Ufuk Aydemir
Format: Article
Language:English
Published: MDPI AG 2018-07-01
Series:Universe
Subjects:
Online Access:http://www.mdpi.com/2218-1997/4/7/80
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spelling doaj-ef522d2ae4514198bb05efd10d7d72e22020-11-24T21:17:18ZengMDPI AGUniverse2218-19972018-07-01478010.3390/universe4070080universe4070080A Scale at 10 MeV, Gravitational Topological Vacuum, and Large Extra DimensionsUfuk Aydemir0School of Physics, Huazhong University of Science and Technology, Wuhan 430074, Hubei, ChinaWe discuss a possible scale of gravitational origin at around 10 MeV, or 10−12 cm, which arises in the MacDowell–Mansouri formalism of gravity due to the topological Gauss–Bonnet term in the action, as pointed out by Bjorken several years ago. A length scale of the same size emerges also in the Kodama solution in gravity, which is known to be closely related to the MacDowell–Mansouri formulation. We particularly draw attention to the intriguing incident that the existence of six compact extra dimensions originated from TeV-scale quantum gravity as well points to a length scale of 10−12 cm, as the compactification scale. The presence of six such extra dimensions is also in remarkable consistency with the MacDowell–Mansouri formalism; it provides a possible explanation for the factor of ∼10120 multiplying the Gauss–Bonnet term in the action. We also comment on the relevant implications of such a scale regarding the thermal history of the universe motivated by the fact that it is considerably close to 1–2 MeV below which the weak interactions freeze out, leading to Big Bang Nucleosynthesis.http://www.mdpi.com/2218-1997/4/7/80MacDowell–Mansouri formalismBjorken–Zeldovich scaleGauss–Bonnet termEinstein–Cartan formalismBig Bang nucleosynthesiscosmological constantKodama wavefunctions
collection DOAJ
language English
format Article
sources DOAJ
author Ufuk Aydemir
spellingShingle Ufuk Aydemir
A Scale at 10 MeV, Gravitational Topological Vacuum, and Large Extra Dimensions
Universe
MacDowell–Mansouri formalism
Bjorken–Zeldovich scale
Gauss–Bonnet term
Einstein–Cartan formalism
Big Bang nucleosynthesis
cosmological constant
Kodama wavefunctions
author_facet Ufuk Aydemir
author_sort Ufuk Aydemir
title A Scale at 10 MeV, Gravitational Topological Vacuum, and Large Extra Dimensions
title_short A Scale at 10 MeV, Gravitational Topological Vacuum, and Large Extra Dimensions
title_full A Scale at 10 MeV, Gravitational Topological Vacuum, and Large Extra Dimensions
title_fullStr A Scale at 10 MeV, Gravitational Topological Vacuum, and Large Extra Dimensions
title_full_unstemmed A Scale at 10 MeV, Gravitational Topological Vacuum, and Large Extra Dimensions
title_sort scale at 10 mev, gravitational topological vacuum, and large extra dimensions
publisher MDPI AG
series Universe
issn 2218-1997
publishDate 2018-07-01
description We discuss a possible scale of gravitational origin at around 10 MeV, or 10−12 cm, which arises in the MacDowell–Mansouri formalism of gravity due to the topological Gauss–Bonnet term in the action, as pointed out by Bjorken several years ago. A length scale of the same size emerges also in the Kodama solution in gravity, which is known to be closely related to the MacDowell–Mansouri formulation. We particularly draw attention to the intriguing incident that the existence of six compact extra dimensions originated from TeV-scale quantum gravity as well points to a length scale of 10−12 cm, as the compactification scale. The presence of six such extra dimensions is also in remarkable consistency with the MacDowell–Mansouri formalism; it provides a possible explanation for the factor of ∼10120 multiplying the Gauss–Bonnet term in the action. We also comment on the relevant implications of such a scale regarding the thermal history of the universe motivated by the fact that it is considerably close to 1–2 MeV below which the weak interactions freeze out, leading to Big Bang Nucleosynthesis.
topic MacDowell–Mansouri formalism
Bjorken–Zeldovich scale
Gauss–Bonnet term
Einstein–Cartan formalism
Big Bang nucleosynthesis
cosmological constant
Kodama wavefunctions
url http://www.mdpi.com/2218-1997/4/7/80
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