Can the cosmological constant support a scalar field?

Takashi Torii, Kengo Maeda, Makoto Narita

Research output: Contribution to journalArticle

12 Citations (Scopus)

Abstract

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.

Original languageEnglish
Pages (from-to)1-7
Number of pages7
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume59
Issue number10
Publication statusPublished - 1999 May 15
Externally publishedYes

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scalars
horizon
perturbation
radii
interactions

ASJC Scopus subject areas

  • Mathematical Physics
  • Physics and Astronomy(all)
  • Nuclear and High Energy Physics
  • Physics and Astronomy (miscellaneous)

Cite this

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

In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 59, No. 10, 15.05.1999, p. 1-7.

Research output: Contribution to journalArticle

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