polymathic-ai/post_neutron_star_merger

这是一个关于中子星合并后效应的模拟数据集，包含了多种物理量的时间序列数据，如流体密度、内部能量、电子分数、温度、熵、速度、磁场等。数据集是基于三维广义相对论性磁流体动力学与 neutrino 辐射传输的模拟结果，用于研究中子星合并后产生的吸积盘以及相关的核合成过程。

This dataset consists of simulations of the aftermath of a neutron star merger, containing time-series data of various physical quantities such as fluid density, internal energy, electron fraction, temperature, entropy, velocity, magnetic field, etc. The dataset is based on three-dimensional general relativistic magnetohydrodynamics with neutrino radiation transport simulations, used to study the accretion disks formed after neutron star mergers and the associated nucleosynthesis processes.