Akademik Veri Yönetim Sistemi
Turkish Journal of Physics, cilt.48, sa.1, ss.28-39, 2024 (ESCI, Scopus)
In this work, we examine the reheating constraints to symmetry-breaking mechanism, which is associated with Coleman-Weinberg inflation in the early universe. We consider the Coleman-Weinberg inflation potential, where the inflaton has a v ≠ 0 after inflation. Setting Treh = 105 GeV, we first show wreh dependency on ns , r, and N∗ for AV case. Then, we demonstrate the results of ns , r, N∗ , α = dns/d ln k for different reheating temperatures and compare the results with the latest BICEP/Keck data. We also present that ns - r and ns - N∗ planes and the effect of reheating temperature which is in a wide range, on inflationary predictions for both AV and BV cases. Finally, we indicate how N∗ and α change according to the reheating temperature values.