This repository presents the key files and final results of a binary neutron star (BNS) simulation project based on Einstein Toolkit and Lorene. The project was completed as part of a numerical relativity selection task, with emphasis on simulation setup, waveform extraction, visualization and result organization.
The repository includes:
- the main simulation parameter file
- extracted waveform data for the target gravitational-wave modes
- a Python post-processing script
- final waveform figures
- representative simulation logs
- an evolution video
The objective of this project is to:
- compile and use Einstein Toolkit and Lorene
- construct an equal-mass binary neutron star system
- set the component masses to 1.2 + 1.2 solar masses
- use an initial separation of 45 km
- adopt a polytropic equation of state
- evolve the system dynamically
- extract gravitational-wave signals in the following modes:
- ( l = 2, m = 0 )
- ( l = 2, m = 2 )
- produce waveform plots and an evolution video
.
├── README.md
├── data/
│ ├── processed/
│ │ ├── l2_m0_psi4.txt
│ │ └── l2_m2_psi4.txt
│ └── waveforms/
│ ├── psi4_l2_m0_r100.asc
│ └── psi4_l2_m2_r100.asc
├── figures/
│ ├── psi4_comparison.png
│ ├── psi4_l2_m0.png
│ └── psi4_l2_m2.png
├── logs/
│ ├── run_bns45_mpi16.err
│ └── run_bns45_mpi16.out
├── media/
│ └── bns_evolution.mp4
├── params/
│ └── bns_45km.par
└── scripts/
└── plot_psi4.py