A Unified Model of Phantom Energy and Dark Matter
To explain the acceleration of the cosmological expansion researchers have considered an unusual form of mass-energy generically called dark energy. Dark energy has a ratio of pressure over mass density which obeys $w=p/ ho <-1/3$. This form of mass-energy leads to accelerated expansion. An extre...
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doaj-f8a27e14c67a43fcb03911c31ef3609e2020-11-24T22:59:11ZengNational Academy of Science of UkraineSymmetry, Integrability and Geometry: Methods and Applications1815-06592008-01-014009A Unified Model of Phantom Energy and Dark MatterDouglas SingletonMax ChavesTo explain the acceleration of the cosmological expansion researchers have considered an unusual form of mass-energy generically called dark energy. Dark energy has a ratio of pressure over mass density which obeys $w=p/ ho <-1/3$. This form of mass-energy leads to accelerated expansion. An extreme form of dark energy, called phantom energy, has been proposed which has $w=p/ ho <-1$. This possibility is favored by the observational data. The simplest model for phantom energy involves the introduction of a scalar field with a negative kinetic energy term. Here we show that theories based on graded Lie algebras naturally have such a negative kinetic energy and thus give a model for phantom energy in a less ad hoc manner. We find that the model also contains ordinary scalar fields and anti-commuting (Grassmann) vector fields which act as a form of two component dark matter. Thus from a gauge theory based on a graded algebra we naturally obtained both phantom energy and dark matter. http://dx.doi.org/10.3842/SIGMA.2008.009dark energyphantom energygraded algebras |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Douglas Singleton Max Chaves |
spellingShingle |
Douglas Singleton Max Chaves A Unified Model of Phantom Energy and Dark Matter Symmetry, Integrability and Geometry: Methods and Applications dark energy phantom energy graded algebras |
author_facet |
Douglas Singleton Max Chaves |
author_sort |
Douglas Singleton |
title |
A Unified Model of Phantom Energy and Dark Matter |
title_short |
A Unified Model of Phantom Energy and Dark Matter |
title_full |
A Unified Model of Phantom Energy and Dark Matter |
title_fullStr |
A Unified Model of Phantom Energy and Dark Matter |
title_full_unstemmed |
A Unified Model of Phantom Energy and Dark Matter |
title_sort |
unified model of phantom energy and dark matter |
publisher |
National Academy of Science of Ukraine |
series |
Symmetry, Integrability and Geometry: Methods and Applications |
issn |
1815-0659 |
publishDate |
2008-01-01 |
description |
To explain the acceleration of the cosmological expansion researchers have considered an unusual form of mass-energy generically called dark energy. Dark energy has a ratio of pressure over mass density which obeys $w=p/ ho <-1/3$. This form of mass-energy leads to accelerated expansion. An extreme form of dark energy, called phantom energy, has been proposed which has $w=p/ ho <-1$. This possibility is favored by the observational data. The simplest model for phantom energy involves the introduction of a scalar field with a negative kinetic energy term. Here we show that theories based on graded Lie algebras naturally have such a negative kinetic energy and thus give a model for phantom energy in a less ad hoc manner. We find that the model also contains ordinary scalar fields and anti-commuting (Grassmann) vector fields which act as a form of two component dark matter. Thus from a gauge theory based on a graded algebra we naturally obtained both phantom energy and dark matter. |
topic |
dark energy phantom energy graded algebras |
url |
http://dx.doi.org/10.3842/SIGMA.2008.009 |
work_keys_str_mv |
AT douglassingleton aunifiedmodelofphantomenergyanddarkmatter AT maxchaves aunifiedmodelofphantomenergyanddarkmatter AT douglassingleton unifiedmodelofphantomenergyanddarkmatter AT maxchaves unifiedmodelofphantomenergyanddarkmatter |
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