Input Parameter
The following parameters are taken from Calabi-Yau type IIB compactification (KKLT) and Planck 2018 observations:
| Parameters| Description| Value/Random Value |
| \( q_i \) | Muatan flux | \( q_i \sim \mathcal{N}(0.1, 0.02) \, M_{\text{Pl}} \) (Gaussian) |
| \( A, B \) | Instanton coefficient | \( A = 10^{-5} M_{\text{Pl}}^4 \), \( B = 0.95A \) (Kachru et al., 2003) |
| \( a, b \) | Eksponen potensial | \( a = 0.1 M_{\text{Pl}}^{-1} \), \( b = 0.2 M_{\text{Pl}}^{-1} \) |
| \( \phi_0 \) | Initial value of inflaton | \( \phi_0 \sim \mathcal{U}(10, 20) M_{\text{Pl}} \) (Uniform) |
| \( N \) | Amount of flux | 100 |
Algorithm
The simulation steps are implemented in Python with the following scheme:
1. Generate Flux Integers:
