English

Determinant-Gravity: Cosmological implications

General Relativity and Quantum Cosmology 2008-11-26 v2

Abstract

We analyze the action d4xdetBgμν+CRμν\int d^4x \sqrt{\det||{\cal B} g_{\mu\nu}+ {\cal C} R_{\mu\nu}}|| as a possible alternative or addition to the Einstein gravity. Choosing a particular form of B(R)=R{\cal B}(R)= \sqrt {R} we can restore the Einstein gravity and, if B=m2{\cal B}=m^2, we obtain the cosmological constant term. Taking B=m2+B1R{\cal B} = m^2 + {\cal B}_1 R and expanding the action in 1/m2 1/m^2, we obtain as a leading term the Einstein Lagrangian with a cosmological constant proportional to m4m^4 and a series of higher order operators. In general case of non-vanishing B{\cal B} and C{\cal C} new cosmological solutions for the Robertson-Walker metric are obtained.

Keywords

Cite

@article{arxiv.gr-qc/0404065,
  title  = {Determinant-Gravity: Cosmological implications},
  author = {D. Comelli and A. Dolgov},
  journal= {arXiv preprint arXiv:gr-qc/0404065},
  year   = {2008}
}

Comments

revtex format, 5 pages,8 figures,references added