中子星并合的多信使分析
高能天体物理现象
2018-02-07 v1
摘要
两颗中子星的并合是一个极其复杂的过程。为了厘清其发生的各个阶段，必须考察我们能够探测到的所有信号：引力波与电磁波，其频谱范围极广，从X射线和射线一直延伸到红外与射电波段。这些信号各自传递着一则讯息，而信息的整体不仅将使我们理解并合过程，还能揭示物质在极端条件下的行为。
引用
@article{arxiv.1802.01696,
title = {A multi-messenger analysis of neutron star mergers},
author = {Alessandro Drago and Giuseppe Pagliara and Silvia Traversi},
journal= {arXiv preprint arXiv:1802.01696},
year = {2018}
}
备注
To be published in the Proceedings of the THESEUS Workshop 2017 (http://www.isdc.unige.ch/theseus/workshop2017.html), Journal of the Italian Astronomical Society (Mem.SAIt), Editors L. Amati, E. Bozzo, M. Della Valle, D. Gotz, P. O'Brien. Details on the THESEUS mission concept can be found in the white paper Amati et al. 2017 (arXiv:171004638) and Stratta et al. 2017 (arXiv:1712.08153)