English

Inflation with an antisymmetric tensor field

General Relativity and Quantum Cosmology 2018-11-02 v3 Cosmology and Nongalactic Astrophysics High Energy Physics - Phenomenology High Energy Physics - Theory

Abstract

We investigate the possibility of inflation with models of antisymmetric tensor field having minimal and nonminimal couplings to gravity. Although the minimal model does not support inflation, the nonminimal models, through the introduction of a nonminimal coupling to gravity, can give rise to stable de-Sitter solutions with a bound on the coupling parameters. The values of field and coupling parameters are sub-planckian. Slow roll analysis is performed and slow-roll parameters are defined which can give the required number of e-folds for sufficient inflation. Stability analysis has been performed for perturbations to antisymmetric field while keeping the metric unperturbed, and it is found that only the sub-horizon modes are free of ghost instability for de-Sitter space.

Keywords

Cite

@article{arxiv.1808.04315,
  title  = {Inflation with an antisymmetric tensor field},
  author = {Sandeep Aashish and Abhilash Padhy and Sukanta Panda and Arun Rana},
  journal= {arXiv preprint arXiv:1808.04315},
  year   = {2018}
}

Comments

10 pages; minor correction to the claim of Sec. IV; to appear in EPJ C

R2 v1 2026-06-23T03:32:20.875Z