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Gravitational Waves from Merging Binary Neutron-Star Systems

  • Tanja Hinderer
  • Luciano RezzollaEmail author
  • Luca Baiotti
Chapter
Part of the Astrophysics and Space Science Library book series (ASSL, volume 457)

Abstract

The merger of binary neutron-star systems is among the scientifically richest events in the universe: it involves extremes of matter and gravity, copious emission of gravitational waves, complex microphysics, and electromagnetic processes that can lead to astrophysical signatures observable at the largest redshifts. We review here the recent progress in understanding the gravitational-wave signal emitted in this process, focussing in particular on its properties during the inspiral and then after the merger.

Notes

Acknowledgements

It is a pleasure to thank Kentaro Takami and the relativistic-astrophysics group in Frankfurt for their help and input in preparing this Chapter.

Partial support has come from “NewCompStar”, COST Action MP1304, from the LOEWE-Program in HIC for FAIR, the European Union’s Horizon 2020 Research and Innovation Programme under grant agreement No. 671698 (call FETHPC-1–2014, project ExaHyPE), from the ERC Synergy Grant “BlackHoleCam - Imaging the Event Horizon of Black Holes” (Grant 610058), from JSPS Grant-in-Aid for Scientific Research(C) No. 18K036220, from the International Centre for Theoretical Sciences Code: ICTS/Prog-GWS/2017/07, and from the Excellence Initiative at Radboud University Nijmegen.

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Copyright information

© Springer Nature Switzerland AG 2018

Authors and Affiliations

  • Tanja Hinderer
    • 1
  • Luciano Rezzolla
    • 2
    • 3
    Email author
  • Luca Baiotti
    • 4
  1. 1.Department of Astrophysics/IMAPPRadboud UniversityNijmegenThe Netherlands
  2. 2.Institute for Theoretical PhysicsFrankfurtGermany
  3. 3.Frankfurt Institute for Advanced StudiesFrankfurtGermany
  4. 4.Graduate School of ScienceOsaka UniversityToyonakaJapan

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