Can higher curvature corrections cure the singularity problem in f(R) gravity?

Tsutomu Kobayashi*, Kei Ichi Maeda

*この研究の対応する著者

研究成果: Article査読

75 被引用数 (Scopus)

抄録

Although f(R) modified gravity models can be made to satisfy solar system and cosmological constraints, it has been shown that they have the serious drawback of the nonexistence of stars with strong gravitational fields. In this paper, we discuss whether or not higher curvature corrections can remedy the nonexistence consistently. The following problems are shown to arise as the costs one must pay for the f(R) models that allow for neutrons stars: (i) the leading correction must be fine-tuned to have the typical energy scale μ 10-19GeV, which essentially comes from the free fall time of a relativistic star; (ii) the leading correction must be further fine-tuned so that it is not given by the quadratic curvature term. The second problem is caused because there appears an intermediate curvature scale, and laboratory experiments of gravity will be under the influence of higher curvature corrections. Our analysis thus implies that it is a challenge to construct viable f(R) models without very careful and unnatural fine-tuning.

本文言語English
論文番号024009
ジャーナルPhysical Review D - Particles, Fields, Gravitation and Cosmology
79
2
DOI
出版ステータスPublished - 2009 1 5

ASJC Scopus subject areas

  • 核物理学および高エネルギー物理学
  • 物理学および天文学(その他)

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