### Abstract

For pt.I see ibid., vol.3, p.233 (1986). In most higher-dimensional theories, the effective matter Lagrangian after compactification is described not only by the radius of the internal space but also by a set of scalar fields (e.g. a dilaton). The author presents stability conditions for (the four-dimensional Friedmann universe (F^{4}))*(a constant internal space (K)) in the above class. The stability against non-linear (large) perturbations and the attractor property of the F^{4}*K solution are also investigated in order to explain why our universe is the present one. If the local zero minimum of the effective four-dimensional potential U is isolated, the stable F^{4}*K solution is always one of the attractors when the 3-space is expanding. In the case that U has a degenerate zero minimum, which appears in theories involving some scale invariance, sufficient conditions for the F^{4}*K solution to be the attractor are presented. Both the S^{2} monopole compactification in the six-dimensional, N=2 supergravity theory and the Calabi-Yau compactification in the ten-dimensional, N=1 supergravity theory with or without the gluino condensation SUSY breaking potential are the cases in question. As an example of an isolated zero minimum, the model by Chapline and Gibbons (1984) (a coset compactification in the ten-dimensional, N=1 supergravity theory plus the SUSY breaking mass term) with a cosmological constant is also discussed.

Original language | English |
---|---|

Article number | 019 |

Pages (from-to) | 651-663 |

Number of pages | 13 |

Journal | Classical and Quantum Gravity |

Volume | 3 |

Issue number | 4 |

DOIs | |

Publication status | Published - 1986 |

Externally published | Yes |

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### ASJC Scopus subject areas

- Physics and Astronomy(all)

### Cite this

*Classical and Quantum Gravity*,

*3*(4), 651-663. [019]. https://doi.org/10.1088/0264-9381/3/4/019

**Stability and attractor in a higher-dimensional cosmology. II.** / Maeda, Keiichi.

Research output: Contribution to journal › Article

*Classical and Quantum Gravity*, vol. 3, no. 4, 019, pp. 651-663. https://doi.org/10.1088/0264-9381/3/4/019

}

TY - JOUR

T1 - Stability and attractor in a higher-dimensional cosmology. II

AU - Maeda, Keiichi

PY - 1986

Y1 - 1986

N2 - For pt.I see ibid., vol.3, p.233 (1986). In most higher-dimensional theories, the effective matter Lagrangian after compactification is described not only by the radius of the internal space but also by a set of scalar fields (e.g. a dilaton). The author presents stability conditions for (the four-dimensional Friedmann universe (F4))*(a constant internal space (K)) in the above class. The stability against non-linear (large) perturbations and the attractor property of the F4*K solution are also investigated in order to explain why our universe is the present one. If the local zero minimum of the effective four-dimensional potential U is isolated, the stable F4*K solution is always one of the attractors when the 3-space is expanding. In the case that U has a degenerate zero minimum, which appears in theories involving some scale invariance, sufficient conditions for the F4*K solution to be the attractor are presented. Both the S2 monopole compactification in the six-dimensional, N=2 supergravity theory and the Calabi-Yau compactification in the ten-dimensional, N=1 supergravity theory with or without the gluino condensation SUSY breaking potential are the cases in question. As an example of an isolated zero minimum, the model by Chapline and Gibbons (1984) (a coset compactification in the ten-dimensional, N=1 supergravity theory plus the SUSY breaking mass term) with a cosmological constant is also discussed.

AB - For pt.I see ibid., vol.3, p.233 (1986). In most higher-dimensional theories, the effective matter Lagrangian after compactification is described not only by the radius of the internal space but also by a set of scalar fields (e.g. a dilaton). The author presents stability conditions for (the four-dimensional Friedmann universe (F4))*(a constant internal space (K)) in the above class. The stability against non-linear (large) perturbations and the attractor property of the F4*K solution are also investigated in order to explain why our universe is the present one. If the local zero minimum of the effective four-dimensional potential U is isolated, the stable F4*K solution is always one of the attractors when the 3-space is expanding. In the case that U has a degenerate zero minimum, which appears in theories involving some scale invariance, sufficient conditions for the F4*K solution to be the attractor are presented. Both the S2 monopole compactification in the six-dimensional, N=2 supergravity theory and the Calabi-Yau compactification in the ten-dimensional, N=1 supergravity theory with or without the gluino condensation SUSY breaking potential are the cases in question. As an example of an isolated zero minimum, the model by Chapline and Gibbons (1984) (a coset compactification in the ten-dimensional, N=1 supergravity theory plus the SUSY breaking mass term) with a cosmological constant is also discussed.

UR - http://www.scopus.com/inward/record.url?scp=0000977206&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0000977206&partnerID=8YFLogxK

U2 - 10.1088/0264-9381/3/4/019

DO - 10.1088/0264-9381/3/4/019

M3 - Article

AN - SCOPUS:0000977206

VL - 3

SP - 651

EP - 663

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

SN - 0264-9381

IS - 4

M1 - 019

ER -