2010

Unstable growth of curvature perturbation in non-singular bouncing cosmologies

Xue, BingKan, Steinhardt, Paul J.

Understand

We consider non-singular bouncing cosmologies, such as the new ekpyrotic model, in which the universe undergoes a slow contraction phase with equation of state $w \gg 1$, followed by a bounce that occurs at a finite scale factor when quantum gravity corrections are still negligible.

  • Such a non-singular bounce requires a violation of the null energy condition in which $w$ falls below -1 at some time before the bounce.
  • In this paper, we show that a component of the adiabatic curvature perturbations, though decaying and negligible during the ekpyrotic phase, is exponentially amplified just before $w$ approaches -1, enough to spoil the scale-invariant perturbation spectrum.
  • We discuss how the problem may be avoided, for example, in singular bounces.

Built on

  • J. Khoury, B. A. Ovrut, P. J. Steinhardt and N. Turok, Phys. Rev. D 64

    2001

    Earlier work this paper cites.

  • J. Khoury, B. A. Ovrut, N. Seiberg, P. J. Steinhardt and N. Turok, Phys. Rev. D 65

    2002

    Earlier work this paper cites.

  • J. K. Erickson, D. H. Wesley, P. J. Steinhardt and N. Turok, Phys. Rev. D 69

    2004

    Earlier work this paper cites.

  • N. Arkani-Hamed, H. C. Cheng, M. A. Luty and S. Mukohyama, JHEP 0405

    2004

    Earlier work this paper cites.

Similar

Then

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…