Constraints from Type Ia supernovae on the Λ-CDM model in Randers-Finsler space
Gravitational field equations in Randers-Finsler space of approximate Berwald type are investigated. A modified Friedmann equation and a new luminosity distance-redshift relation is proposed. A best-fit to the Type Ia supernovae (SNe) observations yields that the Λ in the Λ-CDM model is suppressed t...
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Published in | Chinese physics C Vol. 36; no. 8; pp. 710 - 715 |
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Main Author | |
Format | Journal Article |
Language | English |
Published |
01.08.2012
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Subjects | |
Online Access | Get full text |
ISSN | 1674-1137 0254-3052 |
DOI | 10.1088/1674-1137/36/8/005 |
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Abstract | Gravitational field equations in Randers-Finsler space of approximate Berwald type are investigated. A modified Friedmann equation and a new luminosity distance-redshift relation is proposed. A best-fit to the Type Ia supernovae (SNe) observations yields that the Λ in the Λ-CDM model is suppressed to almost zero. This fact indicates that the astronomical observations on the Type Ia SNe can be described well without invoking any form of dark energy. The best-fit age of the universe is given. It is in agreement with the age of our galaxy. |
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AbstractList | Gravitational field equations in Randers-Finsler space of approximate Berwald type are investigated. A modified Friedmann equation and a new luminosity distance-redshift relation is proposed. A best-fit to the Type Ia supernovae (SNe) observations yields that the Λ in the Λ-CDM model is suppressed to almost zero. This fact indicates that the astronomical observations on the Type Ia SNe can be described well without invoking any form of dark energy. The best-fit age of the universe is given. It is in agreement with the age of our galaxy. |
Author | 常哲 李明华 李昕 |
AuthorAffiliation | Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China Theoretical Physics Center for Science Facilities, Chinese Academy of Sciences, Beijing 100049, China |
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Notes | 11-5641/O4 Gravitational field equations in Randers-Finsler space of approximate Berwald type are investigated. A modified Friedmann equation and a new luminosity distance-redshift relation is proposed. A best-fit to the Type Ia supernovae (SNe) observations yields that the Λ in the Λ-CDM model is suppressed to almost zero. This fact indicates that the astronomical observations on the Type Ia SNe can be described well without invoking any form of dark energy. The best-fit age of the universe is given. It is in agreement with the age of our galaxy. dark energy, Finsler geometry, Type Ia supernovae, luminosity distance-redshift relation |
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SubjectTerms | DM模型 Finsler空间 Ia型超新星 兰德斯 天文观测 宇宙年龄 引力场方程 弗里德曼 |
Title | Constraints from Type Ia supernovae on the Λ-CDM model in Randers-Finsler space |
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