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A Model of Nonsingular Universe
AbstractIn the background of Friedmann–Robertson–Walker Universe, there exists Hawking radiation which comes from the cosmic apparent horizon due to quantum effect. Although the Hawking radiation on the late time evolution of the universe could be safely neglected, it plays an important role in the very early stage of the universe. In view of this point, we identify the temperature in the scalar field potential with the Hawking temperature of cosmic apparent horizon. Then we find a nonsingular universe sourced by the temperature-dependent scalar field. We find that the universe could be created from a de Sitter phase which has the Planck energy density. Thus the Big-Bang singularity is avoided.
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Gao, C. A Model of Nonsingular Universe. Entropy 2012, 14, 1296-1305.View more citation formats
Gao C. A Model of Nonsingular Universe. Entropy. 2012; 14(7):1296-1305.Chicago/Turabian Style
Gao, Changjun. 2012. "A Model of Nonsingular Universe." Entropy 14, no. 7: 1296-1305.
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