Gravitational Waveforms from Multiple-Orbit Simulations of Binary Neutron Stars

Nguyen Quynh Lan, In-Saeng Suh, Grant J Mathews, Reese Haywood
Author affiliations

Authors

  • Nguyen Quynh Lan Hanoi National University of Education, 136 Xuan Thuy, Cau Giay <br /> and<br /> Joint Institute for Nuclear Astrophysics (JINA), University of Notre Dame, Notre Dame, Indiana 46556, USA
  • In-Saeng Suh Center for Astrophysics, Department of Physics and Center for Research Computing,<br /> University of Notre Dame, Notre Dame, Indiana 46556, USA
  • Grant J Mathews Center for Astrophysics, Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA
  • Reese Haywood Center for Astrophysics, Department of Physics, University of Notre Dame, Notre Dame, Indiana 46556, USA

DOI:

https://doi.org/10.15625/0868-3166/25/4/7676

Abstract

We study the gravitational wave emission of equal-mass neutron stars in binary orbits as the stars approach the inner most last stable circular orbit.

We illustrate the extraction of gravitational wave forms in a sequence of quasi-circular orbit simulations including the general relativistic hydrodynamic response of the stars.

We compare the computed results with the Newtonian and post Newtonian results and show that substantial differences can arise as the orbits approach the final inspiral.

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Published

12-01-2016

How to Cite

[1]
N. Q. Lan, I.-S. Suh, G. J. Mathews, and R. Haywood, “Gravitational Waveforms from Multiple-Orbit Simulations of Binary Neutron Stars”, Comm. Phys., vol. 25, no. 4, p. 299, Jan. 2016.

Issue

Vol. 25 No. 4 (2015)

Section

Papers

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