### 抄録

Static spherically symmetric gravitational equilibria of the real scalar field are discussed in the presence of the cosmological constant. We find nontrivial solutions if we take the self-interaction of the field into account while there is no such equilibria in the noninteracting case. The system has critical parameters beyond which new solutions disappear. They are determined by the ratio of the cosmological horizon to the “Compton radius” of the scalar field. We also discuss the stability of the solutions by means of a linear perturbation method and find that the number of unstable modes depends on the node number of the scalar field.

元の言語 | English |
---|---|

ジャーナル | Physical Review D - Particles, Fields, Gravitation and Cosmology |

巻 | 59 |

発行部数 | 10 |

DOI | |

出版物ステータス | Published - 1999 3 26 |

外部発表 | Yes |

### Fingerprint

### ASJC Scopus subject areas

- Nuclear and High Energy Physics
- Physics and Astronomy (miscellaneous)

### これを引用

**Can the cosmological constant support a scalar field?** / Torii, Takashi; Maeda, Kengo.

研究成果: Article

}

TY - JOUR

T1 - Can the cosmological constant support a scalar field?

AU - Torii, Takashi

AU - Maeda, Kengo

PY - 1999/3/26

Y1 - 1999/3/26

N2 - Static spherically symmetric gravitational equilibria of the real scalar field are discussed in the presence of the cosmological constant. We find nontrivial solutions if we take the self-interaction of the field into account while there is no such equilibria in the noninteracting case. The system has critical parameters beyond which new solutions disappear. They are determined by the ratio of the cosmological horizon to the “Compton radius” of the scalar field. We also discuss the stability of the solutions by means of a linear perturbation method and find that the number of unstable modes depends on the node number of the scalar field.

AB - Static spherically symmetric gravitational equilibria of the real scalar field are discussed in the presence of the cosmological constant. We find nontrivial solutions if we take the self-interaction of the field into account while there is no such equilibria in the noninteracting case. The system has critical parameters beyond which new solutions disappear. They are determined by the ratio of the cosmological horizon to the “Compton radius” of the scalar field. We also discuss the stability of the solutions by means of a linear perturbation method and find that the number of unstable modes depends on the node number of the scalar field.

UR - http://www.scopus.com/inward/record.url?scp=85037887054&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85037887054&partnerID=8YFLogxK

U2 - 10.1103/PhysRevD.59.104002

DO - 10.1103/PhysRevD.59.104002

M3 - Article

AN - SCOPUS:85037887054

VL - 59

JO - Physical review D: Particles and fields

JF - Physical review D: Particles and fields

SN - 1550-7998

IS - 10

ER -