Avoiding instabilities in antisymmetric tensor field driven inflation
General Relativity and Quantum Cosmology
2019-09-25 v3 Cosmology and Nongalactic Astrophysics
High Energy Physics - Theory
Abstract
Models of inflation with antisymmetric tensor studied in the past are plagued with ghost instability even in an unperturbed FRW background. We show that it is possible to avoid ghosts in an unperturbed FRW background by considering the most general kinetic term for antisymmetric tensor field. The kinetic part acquires a new gauge symmetry violating term whose effect on perturbed modes is to prevent the appearance of nondynamical modes, and thus avoid ghosts. For completeness, we perform a check for gradient instability and derive the conditions for perturbations to be free of gradient instability.
Keywords
Cite
@article{arxiv.1901.10959,
title = {Avoiding instabilities in antisymmetric tensor field driven inflation},
author = {Sandeep Aashish and Abhilash Padhy and Sukanta Panda},
journal= {arXiv preprint arXiv:1901.10959},
year = {2019}
}
Comments
14 pages; Sec. III rewritten, with new and improved calculations for gradient stability analysis; matches published version