Effect of the Inverse Volume Modification in Loop Quantum Cosmology
XIONG Hua-Hui1**, ZHU Jian-Yang2***
1Physics Teaching and Research Group, School of Biomedical Engineering, Capital Medical University, Beijing 100069 2Department of Physics, Beijing Normal University, Beijing 100875
Effect of the Inverse Volume Modification in Loop Quantum Cosmology
XIONG Hua-Hui1**, ZHU Jian-Yang2***
1Physics Teaching and Research Group, School of Biomedical Engineering, Capital Medical University, Beijing 100069 2Department of Physics, Beijing Normal University, Beijing 100875
摘要After incorporating the inverse volume modifications both in the gravitational and matter part in the improved framework of LQC, we find that the inverse volume modification can decrease the bouncing energy scale, and the presence of nonsingular bounce is generic. For the backward evolution in the expanding branch, in terms of different initial states, the evolution trajectories classify into two classes. One class with larger initial energy density leads to the occurrence of bounce in the region a>ach where ach marks the different inverse volume modification region. The other class with smaller initial energy density evolves back into the region ach. In this region, both the energy density for the scalar field and the bouncing energy scale decrease with the backward evolution. The bounce is present when the bouncing energy scale decreases to be equal to the energy density of the scalar field.
Abstract：After incorporating the inverse volume modifications both in the gravitational and matter part in the improved framework of LQC, we find that the inverse volume modification can decrease the bouncing energy scale, and the presence of nonsingular bounce is generic. For the backward evolution in the expanding branch, in terms of different initial states, the evolution trajectories classify into two classes. One class with larger initial energy density leads to the occurrence of bounce in the region a>ach where ach marks the different inverse volume modification region. The other class with smaller initial energy density evolves back into the region ach. In this region, both the energy density for the scalar field and the bouncing energy scale decrease with the backward evolution. The bounce is present when the bouncing energy scale decreases to be equal to the energy density of the scalar field.
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2011, Vol. 28 
