Reconstruction of Five-Dimensional Bounce Cosmological Models from Deceleration Factor
Abstract In this paper, we consider a class of five-dimensional Ricci-flat vacuum solutions, which contain two arbitrary functions μ(t) and ν(t). It is shown that μ(t) can be rewritten as a new arbitrary function f(z) in terms of redshift z and the f(z) can be determined by choosing particular decel...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Xu, Lixin [verfasserIn] |
|---|
| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2006 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer Science + Business Media, Inc. 2006 |
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| Übergeordnetes Werk: |
Enthalten in: International journal of theoretical physics - Springer US, 1968, 45(2006), 4 vom: Apr., Seite 843-850 |
|---|---|
| Übergeordnetes Werk: |
volume:45 ; year:2006 ; number:4 ; month:04 ; pages:843-850 |
| Links: |
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| DOI / URN: |
10.1007/s10773-006-9073-8 |
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OLC2052360743 |
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| 520 | |a Abstract In this paper, we consider a class of five-dimensional Ricci-flat vacuum solutions, which contain two arbitrary functions μ(t) and ν(t). It is shown that μ(t) can be rewritten as a new arbitrary function f(z) in terms of redshift z and the f(z) can be determined by choosing particular deceleration parameters q(z) which gives early deceleration and late time acceleration. In this way, the 5D cosmological model can be reconstructed and the evolution of the universe can be determined. | ||
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10.1007/s10773-006-9073-8 doi (DE-627)OLC2052360743 (DE-He213)s10773-006-9073-8-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Xu, Lixin verfasserin aut Reconstruction of Five-Dimensional Bounce Cosmological Models from Deceleration Factor 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science + Business Media, Inc. 2006 Abstract In this paper, we consider a class of five-dimensional Ricci-flat vacuum solutions, which contain two arbitrary functions μ(t) and ν(t). It is shown that μ(t) can be rewritten as a new arbitrary function f(z) in terms of redshift z and the f(z) can be determined by choosing particular deceleration parameters q(z) which gives early deceleration and late time acceleration. In this way, the 5D cosmological model can be reconstructed and the evolution of the universe can be determined. Kaluza–Klein theory cosmology Liu, Hongya aut Ping, Yongli aut Enthalten in International journal of theoretical physics Springer US, 1968 45(2006), 4 vom: Apr., Seite 843-850 (DE-627)129546097 (DE-600)218277-4 (DE-576)014996413 0020-7748 nnns volume:45 year:2006 number:4 month:04 pages:843-850 https://doi.org/10.1007/s10773-006-9073-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_24 GBV_ILN_40 GBV_ILN_70 GBV_ILN_2005 GBV_ILN_4116 33.00 VZ AR 45 2006 4 04 843-850 |
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10.1007/s10773-006-9073-8 doi (DE-627)OLC2052360743 (DE-He213)s10773-006-9073-8-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Xu, Lixin verfasserin aut Reconstruction of Five-Dimensional Bounce Cosmological Models from Deceleration Factor 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science + Business Media, Inc. 2006 Abstract In this paper, we consider a class of five-dimensional Ricci-flat vacuum solutions, which contain two arbitrary functions μ(t) and ν(t). It is shown that μ(t) can be rewritten as a new arbitrary function f(z) in terms of redshift z and the f(z) can be determined by choosing particular deceleration parameters q(z) which gives early deceleration and late time acceleration. In this way, the 5D cosmological model can be reconstructed and the evolution of the universe can be determined. Kaluza–Klein theory cosmology Liu, Hongya aut Ping, Yongli aut Enthalten in International journal of theoretical physics Springer US, 1968 45(2006), 4 vom: Apr., Seite 843-850 (DE-627)129546097 (DE-600)218277-4 (DE-576)014996413 0020-7748 nnns volume:45 year:2006 number:4 month:04 pages:843-850 https://doi.org/10.1007/s10773-006-9073-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_24 GBV_ILN_40 GBV_ILN_70 GBV_ILN_2005 GBV_ILN_4116 33.00 VZ AR 45 2006 4 04 843-850 |
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10.1007/s10773-006-9073-8 doi (DE-627)OLC2052360743 (DE-He213)s10773-006-9073-8-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Xu, Lixin verfasserin aut Reconstruction of Five-Dimensional Bounce Cosmological Models from Deceleration Factor 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science + Business Media, Inc. 2006 Abstract In this paper, we consider a class of five-dimensional Ricci-flat vacuum solutions, which contain two arbitrary functions μ(t) and ν(t). It is shown that μ(t) can be rewritten as a new arbitrary function f(z) in terms of redshift z and the f(z) can be determined by choosing particular deceleration parameters q(z) which gives early deceleration and late time acceleration. In this way, the 5D cosmological model can be reconstructed and the evolution of the universe can be determined. Kaluza–Klein theory cosmology Liu, Hongya aut Ping, Yongli aut Enthalten in International journal of theoretical physics Springer US, 1968 45(2006), 4 vom: Apr., Seite 843-850 (DE-627)129546097 (DE-600)218277-4 (DE-576)014996413 0020-7748 nnns volume:45 year:2006 number:4 month:04 pages:843-850 https://doi.org/10.1007/s10773-006-9073-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_24 GBV_ILN_40 GBV_ILN_70 GBV_ILN_2005 GBV_ILN_4116 33.00 VZ AR 45 2006 4 04 843-850 |
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10.1007/s10773-006-9073-8 doi (DE-627)OLC2052360743 (DE-He213)s10773-006-9073-8-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Xu, Lixin verfasserin aut Reconstruction of Five-Dimensional Bounce Cosmological Models from Deceleration Factor 2006 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer Science + Business Media, Inc. 2006 Abstract In this paper, we consider a class of five-dimensional Ricci-flat vacuum solutions, which contain two arbitrary functions μ(t) and ν(t). It is shown that μ(t) can be rewritten as a new arbitrary function f(z) in terms of redshift z and the f(z) can be determined by choosing particular deceleration parameters q(z) which gives early deceleration and late time acceleration. In this way, the 5D cosmological model can be reconstructed and the evolution of the universe can be determined. Kaluza–Klein theory cosmology Liu, Hongya aut Ping, Yongli aut Enthalten in International journal of theoretical physics Springer US, 1968 45(2006), 4 vom: Apr., Seite 843-850 (DE-627)129546097 (DE-600)218277-4 (DE-576)014996413 0020-7748 nnns volume:45 year:2006 number:4 month:04 pages:843-850 https://doi.org/10.1007/s10773-006-9073-8 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_11 GBV_ILN_24 GBV_ILN_40 GBV_ILN_70 GBV_ILN_2005 GBV_ILN_4116 33.00 VZ AR 45 2006 4 04 843-850 |
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Abstract In this paper, we consider a class of five-dimensional Ricci-flat vacuum solutions, which contain two arbitrary functions μ(t) and ν(t). It is shown that μ(t) can be rewritten as a new arbitrary function f(z) in terms of redshift z and the f(z) can be determined by choosing particular deceleration parameters q(z) which gives early deceleration and late time acceleration. In this way, the 5D cosmological model can be reconstructed and the evolution of the universe can be determined. © Springer Science + Business Media, Inc. 2006 |
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Abstract In this paper, we consider a class of five-dimensional Ricci-flat vacuum solutions, which contain two arbitrary functions μ(t) and ν(t). It is shown that μ(t) can be rewritten as a new arbitrary function f(z) in terms of redshift z and the f(z) can be determined by choosing particular deceleration parameters q(z) which gives early deceleration and late time acceleration. In this way, the 5D cosmological model can be reconstructed and the evolution of the universe can be determined. © Springer Science + Business Media, Inc. 2006 |
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Abstract In this paper, we consider a class of five-dimensional Ricci-flat vacuum solutions, which contain two arbitrary functions μ(t) and ν(t). It is shown that μ(t) can be rewritten as a new arbitrary function f(z) in terms of redshift z and the f(z) can be determined by choosing particular deceleration parameters q(z) which gives early deceleration and late time acceleration. In this way, the 5D cosmological model can be reconstructed and the evolution of the universe can be determined. © Springer Science + Business Media, Inc. 2006 |
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