Tunneling wave function of the universe. II. the backreaction problem

Alexander Vilenkin, Masaki Yamada

研究成果: Article査読

23 被引用数 (Scopus)

抄録

The tunneling wave function of the Universe is calculated exactly for a de Sitter minisuperspace model with a massless conformally coupled scalar field, both by solving the Wheeler-DeWitt equation and by evaluating the Lorentzian path integral. The same wave function is found in both approaches. The backreaction of quantum field fluctuations on the scale factor amounts to a constant renormalization of the vacuum energy density. This is in contrast to the recent suggestion of Feldbrugge et al. that the backreaction should diverge when the scale factor gets small, a→0. Similar results are found for a massive scalar field in the limit of a large mass. We also verified that the tunneling wave function can be expressed as a transition amplitude from a universe of vanishing size with the scalar field in the state of Euclidean vacuum, as was suggested in our earlier work.

本文言語English
論文番号066010
ジャーナルPhysical Review D
99
6
DOI
出版ステータスPublished - 2019 3月 15
外部発表はい

ASJC Scopus subject areas

  • 物理学および天文学(その他)

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