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arXiv 1712.02489hep-thgr-qc
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Tunneling in Quantum Cosmology and Holographic SYM theory

Kazuo Ghoroku, Yoshimasa Nakano, Motoi Tachibana, Fumihiko Toyoda

英文摘要:

We study the time evolution of early universe which is developed by a cosmological constant $Λ_4$ 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 $Λ_4$. For positive $Λ_4$, 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.

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