Abstract

We study the time evolution of early universe which is developed by a cosmological constant $\Lambda_4$ and supersymmetric Yang-Mills (SYM) fields in the Friedmann-Robertson-Walker (FRW) space-time. The renormalized vacuum expectation value of energy-momentum tensor of the SYM theory is obtained in a holographic way. It includes a radiation of the SYM field, parametrized as $C$. The evolution is controlled by this radiation $C$ and the cosmological constant $\Lambda_4$. For positive $\Lambda_4$, an inflationary solution is obtained at late time. When $C$ is added, the quantum mechanical situation at early time is fairly changed. Here we perform the early time analysis in terms of two different approaches, (i) the Wheeler-DeWitt equation and (ii) Lorentzian path-integral with the Picard-Lefschetz method by introducing an effective action. The results of two methods are compared.

Highlights

  • The holographic approach has been extended to supersymmetric Yang-Mills (SYM) theory in Friedmann-Robertson-Walker (FRW) space-time in Refs. [1,2,3]

  • We study the time evolution of the early Universe, which is developed by a cosmological constant Λ4 and supersymmetric Yang-Mills (SYM) fields in the Friedmann-Robertson-Walker space-time

  • Cosmology driven by SYM theory is studied in the FRW space-time

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Summary

INTRODUCTION

The holographic approach has been extended to supersymmetric Yang-Mills (SYM) theory in Friedmann-. A relevant path in the complex plane of the lapse field could provide a correct propagator of the Universe This propagator implies an appropriate boundary condition in solving the tunneling amplitude via the WDW equation. We find the validity of the Lorentzian path-integral method It could give the tunneling amplitude, which is obtained by solving the WDW equation with an appropriate boundary condition. A gravitational model with SYM theory is given and the Einstein equations in the FRW space-time are given They are solved at large a0ðtÞ, and why quantum cosmology is necessary at small a0ðtÞ is explained for small C. III, a tractable effective action corrected by SYM theory is proposed

COSMOLOGY DRIVEN BY CFT
QUANTUM COSMOLOGY AND EFFECTIVE ACTION
Change of variables
VeffðqÞ and tunneling
WDW EQUATION AND TUNNELING
QUANTUM COSMOLOGY WITH LORENTZIAN PATH INTEGRAL
Saddles for periodic Euclidean solution
SUMMARY AND DISCUSSIONS
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