伽马射线与引力波
高能天体物理现象
2019-03-12 v1
摘要
首次中子星并合的多信使观测由 Fermi-GBM 与 INTEGRAL SPI-ACS 在伽马射线波段、以及 Advanced LIGO 与 Advanced Virgo 在引力波波段独立探测到。引力波由具有加速四极矩的系统发射，可探测源预期为致密天体。几乎所有遥远的 astrophysical 伽马射线源都是致密天体。因此，这两种信使的偶发观测将持续揭示引力波与伽马射线的源，并促成跨越 Astro2020 主题领域的多信使科学。这需要对地基引力波网络进行升级，以及需要约 keV–MeV 伽马射线覆盖以观测中子星并合，并需要引力波与伽马射线的宽带覆盖以监测其他预期的联合源。
引用
@article{arxiv.1903.04472,
title = {Gamma Rays and Gravitational Waves},
author = {E. Burns and S. Zhu and C. M. Hui and S. Ansoldi and S. Barthelmy and S. Boggs and S. B. Cenko and N. Christensen and C. Fryer and A. Goldstein and A. Harding and D. Hartmann and A. Joens and G. Kanbach and M. Kerr and C. Kierans and J. McEnery and B. Patricelli and J. Perkins and J. Racusin and P. Ray and J. Schlieder and H. Schoorlemmer and F. Schussler and A. Stamerra and J. Tomsick and Z. Wadiasingh and C. Wilson-Hodge and G. Younes and B. Zhang and A. Zoglauer},
journal= {arXiv preprint arXiv:1903.04472},
year = {2019}
}
备注
Astro2020 White Paper for the Thematic Area Multimessenger Astronomy and Astrophysics