3.8 Proceedings Paper

How to interpret observations of neutron-star mergers?

期刊

出版社

IOP PUBLISHING LTD
DOI: 10.1088/1742-6596/1667/1/012018

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资金

  1. Special Postdoctoral Researchers (SPDR) program
  2. JSPS KAKENHI [JP16K21630, JP16KK0109, JP19K03878, JP19H00693]
  3. KAKENHI [19H00693]
  4. Interdisciplinary Theoretical and Mathematical Sciences Program of RIKEN (iTHEMS)
  5. Pioneering Program of RIKEN for Evolution of Matter in the Universe (r-EMU)
  6. European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme [759253]
  7. German Research Foundation (DFG) [Sonderforschungsbereich SFB 881]
  8. European Research Council [341157-COCO2CASA]
  9. Deutsche Forschungsgemeinschaft [SFB-1258, EXC 2094]

向作者/读者索取更多资源

The recent first multi-messenger observation of a neutron-star merger, GW170817 and its electromagnetic counterparts, has sparked tremendous excitement particularly because long-standing questions related to heavy-element nucleosynthesis and the nuclear equation of state could finally be tested with unprecedented capabilities. This proceedings article briefly reviews the main observation channels of neutron-star mergers and how those can be used to obtain insight about questions related to nucleosynthesis and the nuclear equation of state.

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