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• W2035561637 endingPage "041" @default.
• W2035561637 startingPage "041" @default.
• W2035561637 abstract "In this work we investigate the utility of using SNe Ia observations in constraining the cosmological parameters in BSBM theory where a scalar field is responsible for both fine structure constant variation and late time universe acceleration. The model is discussed in the presence of an exponential self potential for the scalar field. Stability and phase space analysis of the solutions are studied. The model is tested against observational data for Hubble parameter and quasar absorption spectra. With the best fitted model parameters, the theory predicts a good match with the experimental results and exhibits fine structure constant variation. The analysis also shows that for the equation of state parameter, recent universe acceleration and possible phantom crossing in future is forecasted." @default.
• W2035561637 created "2016-06-24" @default.
• W2035561637 creator A5016382401 @default.
• W2035561637 creator A5090856826 @default.
• W2035561637 date "2012-02-28" @default.
• W2035561637 modified "2023-09-26" @default.
• W2035561637 title "Universe acceleration and fine structure constant variation in BSBM theory" @default.
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• W2035561637 doi "https://doi.org/10.1088/1475-7516/2012/02/041" @default.
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