Probing the Lambda-DGP Braneworld model

We study cosmic dynamics in the context of the normal branch of the DGP braneworld model. Using current Planck data, we find the best fitting model and associated cosmological parameters in non-fiat ADGP. With the transition redshift as a basic variable and statefinder parameters, our result shows t...

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Published inResearch in astronomy and astrophysics Vol. 16; no. 9; pp. 31 - 38
Main Authors Ravanpak, Arvin, Farajollahi, Hossein, Fadakar, Golnaz
Format Journal Article
LanguageEnglish
Published National Astronomical Observatories of Chinese Academy of Sciences and IOP Publishing 01.09.2016
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ISSN1674-4527
2397-6209
2397-6209
DOI10.1088/1674-4527/16/9/137

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Abstract We study cosmic dynamics in the context of the normal branch of the DGP braneworld model. Using current Planck data, we find the best fitting model and associated cosmological parameters in non-fiat ADGP. With the transition redshift as a basic variable and statefinder parameters, our result shows that the Universe starts its accelerated expansion phase slightly earlier than expected in ACDM cosmology. The result also alleviates the coincidence problem of the ACDM model.
AbstractList We study cosmic dynamics in the context of the normal branch of the DGP braneworld model. Using current Planck data, we find the best fitting model and associated cosmological parameters in non-flat [Lambda]DGP. With the transition redshift as a basic variable and statefinder parameters, our result shows that the Universe starts its accelerated expansion phase slightly earlier than expected in [Lambda]CDM cosmology. The result also alleviates the coincidence problem of the [Lambda]CDM model.
We study cosmic dynamics in the context of the normal branch of the DGP braneworld model. Using current Planck data, we find the best fitting model and associated cosmological parameters in non-flat ΛDGP. With the transition redshift as a basic variable and statefinder parameters, our result shows that the Universe starts its accelerated expansion phase slightly earlier than expected in ΛCDM cosmology. The result also alleviates the coincidence problem of the ΛCDM model.
We study cosmic dynamics in the context of the normal branch of the DGP braneworld model. Using current Planck data, we find the best fitting model and associated cosmological parameters in non-fiat ADGP. With the transition redshift as a basic variable and statefinder parameters, our result shows that the Universe starts its accelerated expansion phase slightly earlier than expected in ACDM cosmology. The result also alleviates the coincidence problem of the ACDM model.
Author Arvin Ravanpak Hossein Faraiollahi Golnaz Fadakar
AuthorAffiliation Department of Physics, Vali-e-Asr University, Rafsanjan, Iran Department of Physics, University of Guilan, Rasht, Iran School of Physics, University of New South Wales, Sydney, NSW, 2052, Australia
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We study cosmic dynamics in the context of the normal branch of the DGP braneworld model. Using current Planck data, we find the best fitting model and associated cosmological parameters in non-fiat ADGP. With the transition redshift as a basic variable and statefinder parameters, our result shows that the Universe starts its accelerated expansion phase slightly earlier than expected in ACDM cosmology. The result also alleviates the coincidence problem of the ACDM model.
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SubjectTerms (cosmology:) cosmological parameters
Astronomy
Cosmology
dark energy
DM模型
Dynamic tests
Dynamics
Mathematical models
methods: numerical
observations
Parameters
Red shift
theory
Universe
一致性问题
世界
加速膨胀
动力学
宇宙学参数
拟合模型

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