Cosmology of the proxy theory to massive gravity

Lavinia Heisenberg, Rampei Kimura, Kazuhiro Yamamoto

Research output: Contribution to journalArticle

67 Citations (Scopus)

Abstract

In this paper, we scrutinize very closely the cosmology in the proxy theory to massive gravity obtained in de Rham and Heisenberg [Phys. Rev. D 84, 043503 (2011)]. This proxy theory was constructed by covariantizing the decoupling limit Lagrangian of massive gravity, and it represents a subclass of Horndeski scalar-tensor theory. Thus, this covariantization unifies two important classes of modified gravity theories, namely, massive gravity and Horndeski theories. We go beyond the regime which was studied in de Rham and Heisenberg [Phys. Rev. D 84, 043503 (2011)] and show that the theory does not admit any homogeneous and isotropic self-accelerated solutions. We illustrate that the only attractor solution is the flat Minkowski solution; hence, this theory is less appealing as a dark energy model. We also show that the absence of de Sitter solutions is tightly related to the presence of shift symmetry breaking interactions.

Original languageEnglish
Article number103008
JournalPhysical Review D - Particles, Fields, Gravitation and Cosmology
Volume89
Issue number10
DOIs
Publication statusPublished - 2014 May 13
Externally publishedYes

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cosmology
gravitation
dark energy
decoupling
broken symmetry
tensors
scalars
shift
interactions

ASJC Scopus subject areas

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

Cite this

Cosmology of the proxy theory to massive gravity. / Heisenberg, Lavinia; Kimura, Rampei; Yamamoto, Kazuhiro.

In: Physical Review D - Particles, Fields, Gravitation and Cosmology, Vol. 89, No. 10, 103008, 13.05.2014.

Research output: Contribution to journalArticle

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