A Scalar Field Dark Matter Model and Its Role in the Large-Scale Structure Formation in the Universe
We present a model of dark matter based on scalar-tensor theory of gravity. With this scalar field dark matter model we study the non-linear evolution of the large-scale structures in the universe. The equations that govern the evolution of the scale factor of the universe are derived together with...
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Language: | English |
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Wiley
2012-01-01
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Series: | Advances in Astronomy |
Online Access: | http://dx.doi.org/10.1155/2012/509682 |
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author | Mario A. Rodríguez-Meza |
author_facet | Mario A. Rodríguez-Meza |
author_sort | Mario A. Rodríguez-Meza |
collection | DOAJ |
description | We present a model of dark matter based on scalar-tensor theory of gravity. With this scalar field dark matter model we study the non-linear evolution of the large-scale structures in the universe. The equations that govern the evolution of the scale factor of the universe are derived together with the appropriate Newtonian equations to follow the nonlinear evolution of the structures. Results are given in terms of the power spectrum that gives quantitative information on the large-scale structure formation. The initial conditions we have used are consistent with the so-called concordance ΛCDM model. |
format | Article |
id | doaj-art-de99edae97da4d57aa3ee2375cc96a18 |
institution | Kabale University |
issn | 1687-7969 1687-7977 |
language | English |
publishDate | 2012-01-01 |
publisher | Wiley |
record_format | Article |
series | Advances in Astronomy |
spelling | doaj-art-de99edae97da4d57aa3ee2375cc96a182025-02-03T05:51:31ZengWileyAdvances in Astronomy1687-79691687-79772012-01-01201210.1155/2012/509682509682A Scalar Field Dark Matter Model and Its Role in the Large-Scale Structure Formation in the UniverseMario A. Rodríguez-Meza0Departamento de Física, Instituto Nacional de Investigaciones Nucleares, Apdo. Postal 18-1027, 11801 México, DF, MexicoWe present a model of dark matter based on scalar-tensor theory of gravity. With this scalar field dark matter model we study the non-linear evolution of the large-scale structures in the universe. The equations that govern the evolution of the scale factor of the universe are derived together with the appropriate Newtonian equations to follow the nonlinear evolution of the structures. Results are given in terms of the power spectrum that gives quantitative information on the large-scale structure formation. The initial conditions we have used are consistent with the so-called concordance ΛCDM model.http://dx.doi.org/10.1155/2012/509682 |
spellingShingle | Mario A. Rodríguez-Meza A Scalar Field Dark Matter Model and Its Role in the Large-Scale Structure Formation in the Universe Advances in Astronomy |
title | A Scalar Field Dark Matter Model and Its Role in the Large-Scale Structure Formation in the Universe |
title_full | A Scalar Field Dark Matter Model and Its Role in the Large-Scale Structure Formation in the Universe |
title_fullStr | A Scalar Field Dark Matter Model and Its Role in the Large-Scale Structure Formation in the Universe |
title_full_unstemmed | A Scalar Field Dark Matter Model and Its Role in the Large-Scale Structure Formation in the Universe |
title_short | A Scalar Field Dark Matter Model and Its Role in the Large-Scale Structure Formation in the Universe |
title_sort | scalar field dark matter model and its role in the large scale structure formation in the universe |
url | http://dx.doi.org/10.1155/2012/509682 |
work_keys_str_mv | AT marioarodriguezmeza ascalarfielddarkmattermodelanditsroleinthelargescalestructureformationintheuniverse AT marioarodriguezmeza scalarfielddarkmattermodelanditsroleinthelargescalestructureformationintheuniverse |