Evolution of Weyl's Gauge Invariant Geometry under Ricci Flow
There is a classical fact conjectured by Albert Einstein, that the presence of matter causes the curvature of space-time. However, even a vacant space-time can have a non-zero Weyl's curvature. For instance, such a condition can be found near black holes and in the zones where gravitation waves...
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Universidad Católica del Norte, Departamento de Matemáticas
2011
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oai:scielo:S0716-091720110003000052012-06-18Evolution of Weyl's Gauge Invariant Geometry under Ricci FlowBahuguna,Sandeep KPetwal,Kailash C Diffusion Ricci flow (R.F.) Gauge Cosmos Weyl Tensor density Conformal rescaling pseudo vector There is a classical fact conjectured by Albert Einstein, that the presence of matter causes the curvature of space-time. However, even a vacant space-time can have a non-zero Weyl's curvature. For instance, such a condition can be found near black holes and in the zones where gravitation waves radiate. Getting inspirations from such a fabulous classical fact, authors have attempted to describe the purely differential geometric behaviour of Weyl's-Gauge invariant conceptions concerning to 4-dimensional structured cosmos. Under the well known Ricci flow (R.F.) techniques, various Weylian configurations have been evolved as heat diffusion equations, which can pave the way for new consequences in relativity theory and cosmology.info:eu-repo/semantics/openAccessUniversidad Católica del Norte, Departamento de MatemáticasProyecciones (Antofagasta) v.30 n.3 20112011-12-01text/htmlhttp://www.scielo.cl/scielo.php?script=sci_arttext&pid=S0716-09172011000300005en10.4067/S0716-09172011000300005 |
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Scielo Chile |
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Scielo Chile |
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English |
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Diffusion Ricci flow (R.F.) Gauge Cosmos Weyl Tensor density Conformal rescaling pseudo vector |
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Diffusion Ricci flow (R.F.) Gauge Cosmos Weyl Tensor density Conformal rescaling pseudo vector Bahuguna,Sandeep K Petwal,Kailash C Evolution of Weyl's Gauge Invariant Geometry under Ricci Flow |
description |
There is a classical fact conjectured by Albert Einstein, that the presence of matter causes the curvature of space-time. However, even a vacant space-time can have a non-zero Weyl's curvature. For instance, such a condition can be found near black holes and in the zones where gravitation waves radiate. Getting inspirations from such a fabulous classical fact, authors have attempted to describe the purely differential geometric behaviour of Weyl's-Gauge invariant conceptions concerning to 4-dimensional structured cosmos. Under the well known Ricci flow (R.F.) techniques, various Weylian configurations have been evolved as heat diffusion equations, which can pave the way for new consequences in relativity theory and cosmology. |
author |
Bahuguna,Sandeep K Petwal,Kailash C |
author_facet |
Bahuguna,Sandeep K Petwal,Kailash C |
author_sort |
Bahuguna,Sandeep K |
title |
Evolution of Weyl's Gauge Invariant Geometry under Ricci Flow |
title_short |
Evolution of Weyl's Gauge Invariant Geometry under Ricci Flow |
title_full |
Evolution of Weyl's Gauge Invariant Geometry under Ricci Flow |
title_fullStr |
Evolution of Weyl's Gauge Invariant Geometry under Ricci Flow |
title_full_unstemmed |
Evolution of Weyl's Gauge Invariant Geometry under Ricci Flow |
title_sort |
evolution of weyl's gauge invariant geometry under ricci flow |
publisher |
Universidad Católica del Norte, Departamento de Matemáticas |
publishDate |
2011 |
url |
http://www.scielo.cl/scielo.php?script=sci_arttext&pid=S0716-09172011000300005 |
work_keys_str_mv |
AT bahugunasandeepk evolutionofweylsgaugeinvariantgeometryunderricciflow AT petwalkailashc evolutionofweylsgaugeinvariantgeometryunderricciflow |
_version_ |
1718439778947432448 |