Stability and attractor in a higher-dimensional cosmology. I

K. Maeda*

*この研究の対応する著者

研究成果: Article査読

84 被引用数 (Scopus)

抄録

The stability condition of (the four-dimensional Friedmann universe)*(a compact internal space) (F4*KD) is presented for a class of higher-dimensional theories, in which the effective potential depends only on a scale length of the internal space. The Candelas-Weinberg model (i.e. one-loop quantum correction+a cosmological constant Lambda ), eleven-dimensional supergravity+ Lambda , Einstein-Yang-Mills theory and six-dimensional Einstein-Maxwell theory are classified into this class. It is shown that the F4*KD solution is stable against small perturbations in the above models. The stability against non-linear perturbation is also investigated. The author finds that the stable F4*KD solution is an attractor for a finite range of initial conditions if the proper volume of the universe is increasing with time.

本文言語English
論文番号017
ページ(範囲)233-247
ページ数15
ジャーナルClassical and Quantum Gravity
3
2
DOI
出版ステータスPublished - 1986 12月 1
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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