Curvature and Anisotropy Near a Nonsingular Bounce

          @misc{ pirsa_PIRSA:11070022,
            doi = {10.48660/11070022},
            url = {https://pirsa.org/11070022},
            author = {Xue, BingKan},
            keywords = {Cosmology},
            language = {en},
            title = {Curvature and Anisotropy Near a Nonsingular Bounce},
            publisher = {Perimeter Institute},
            year = {2011},
            month = {jul},
            note = {PIRSA:11070022 see, \url{https://pirsa.org}}
          }
          

Abstract

Problematic growths of curvature and anisotropy are found in nonsingular bouncing cosmologies that include both an ekpyrotic phase and a bouncing phase. Classically, initial curvature and anisotropy that are suppressed during the ekpyrotic phase will grow back exponentially during the nonsingular bouncing phase. Besides, curvature perturbations and anisotropy are generated by quantum fluctuations during the ekpyrotic phase. In the bouncing phase, an adiabatic curvature perturbation grows to dominate and gives rise to a blue spectrum that spoils the scale-invariance. Meanwhile, a scalar shear perturbation grows nonlinear and creates an overwhelming anisotropy that disrupts the nonsingular bounce altogether.