标题： 核心坍缩超新星：爆炸动力学、中微子和引力波 显示英文标题

标题： Core-Collapse Supernovae: Explosion Dynamics, Neutrinos and Gravitational Waves

摘要： 寻找超新星爆炸机制一直是计算天体物理学几十年来的重要挑战。 模拟现在已经进展到一个阶段，使得解决方案似乎接近，来自自洽爆炸模型的中微子和引力波信号也开始可用。 在这里，我们关注超新星建模中的一个最新进展，即在多维中微子流体动力学模拟中包含广义相对论，并展示了对11.2和15太阳质量前身星的最新模拟结果。 我们还提到3D效应作为超新星物理中的另一个方面，有待进一步更深入的研究。 显示英文摘要

摘要： The quest for the supernova explosion mechanism has been one of the outstanding challenges in computational astrophysics for several decades. Simulations have now progressed to a stage at which the solution appears close and neutrino and gravitational wave signals from self-consistent explosion models are becoming available. Here we focus one of the recent advances in supernova modeling, the inclusion of general relativity in multi-dimensional neutrino hydrodynamics simulations, and present the latest simulation results for an 11.2 and a 15 solar mass progenitor. We also mention 3D effects as another aspect in supernova physics awaiting further, more thorough investigation.