English

Observational Viability of Anisotropic Inflation Revisited

Cosmology and Nongalactic Astrophysics 2025-03-12 v1 General Relativity and Quantum Cosmology High Energy Physics - Theory

Abstract

We investigate anisotropic inflation within the single-field model featuring an intermediate scale factor. Our analysis reveals that the anisotropic nature of the Friedmann equations in this framework affects the slow-roll parameters, which in turn influence key perturbation parameters. Using a numerical approach, we derive constraints on the intermediate parameter β\beta and the anisotropic parameter cc. Our results show that the model is consistent with Planck2018 TT, TE, EE +lowE+lensing+BK14+BAO data at 68%68\% CL, for 0.84<β<10.84<\beta<1 and 7.34<c<27.77.34<c<27.7. At 95%95\% CL the consistency holds for 0.77<β<10.77<\beta<1 and 7.17<c<28.97.17<c<28.9. The model is also consistent with Planck2018 TT, TE, EE +lowE+lensing+BK18+BAO data, for 0.91<β<10.91<\beta<1 and 8.00<c<27.48.00<c<27.4 (at 68%68\% CL), and 0.88<β<10.88<\beta<1 and 7.40<c<28.87.40<c<28.8 (at 95%95\% CL). Additionally, we examine the reheating phase using these constraints on constraints on β\beta and cc and determine the observationally consistent ranges for the number of e-folds and the temperature during the reheating phase.

Keywords

Cite

@article{arxiv.2503.08277,
  title  = {Observational Viability of Anisotropic Inflation Revisited},
  author = {Maryam Roushan and Narges Rashidi and Kourosh Nozari},
  journal= {arXiv preprint arXiv:2503.08277},
  year   = {2025}
}

Comments

12 pages, 5 figures, 3 tables