# The final phase of inspiral of neutron stars: Realistic equations of state

@article{GondekRosiska2007TheFP, title={The final phase of inspiral of neutron stars: Realistic equations of state}, author={Dorota Gondek-Rosińska and Michał Bejger and Tomasz Bulik and E. Gourgoulhon and Paweł Haensel and François Limousin and Keisuke Taniguchi and Leszek Zdunik}, journal={Advances in Space Research}, year={2007}, volume={39}, pages={271-274} }

## 9 Citations

Neutron star equation of state via gravitational wave observations

- Physics, Geology
- 2011

Gravitational wave observations can potentially measure properties of neutron star equations of state by measuring departures from the point-particle limit of the gravitational waveform produced in…

Gravitational-wave astrophysics from neutron star inspiral and coalescence

- PhysicsInternational Journal of Modern Physics D
- 2018

Prior to the observation of a double neutron star inspiral and merger, its possible implications were striking. Events whose light and gravitational waves are simultaneously detected could resolve…

Population synthesis of double neutron stars

- Physics
- 2009

Using the StarTrack binary population synthesis code we model the population of double neutron stars in the Galaxy. We include a detailed treatment of the spin evolution of each pulsar due to…

Motion deviation of test body induced by spin and cosmological constant in extreme mass ratio inspiral binary system

- PhysicsThe European Physical Journal C
- 2019

The future space-borne detectors will provide the possibility to detect gravitational waves emitted from extreme mass ratio inspirals of stellar-mass compact objects into supermassive black holes.…

Systematic errors in measuring parameters of non-spinning compact binary coalescences with post-Newtonian templates

- Physics
- 2010

We study the astrophysical impact of inaccurate and incomplete modeling of the gravitational waveforms from compact binary coalescences (CBCs). We do so by the matched filtering of phenomenological…

Status of neutron star–black hole and binary neutron star simulations

- Physics
- 2009

We review the current status of black hole–neutron star and neutron star–neutron star binary merger calculations, focusing on recent results about gravitational wave signals and the characteristics…

Properties of double neutron stars

- Physics
- 2008

We summarize our studies on properties of double neutron stars observable in gravitational waves and in the radio. Binary population synthesis is used to calculate expected masses of neutron stars in…

Spectral Methods for Numerical Relativity

- PhysicsLiving reviews in relativity
- 2009

This paper focuses on a class called spectral methods in which, typically, the various functions are expanded in sets of orthogonal polynomials or functions, and presents results obtained by various groups in the field of general relativity by means of spectral methods.

Innermost stable circular orbit of spinning particle in charged spinning black hole background

- Physics
- 2017

In this paper we investigate the innermost stable circular orbit (ISCO) (spin-aligned or anti-aligned orbit) for a classical spinning test particle with the pole-dipole approximation in the…

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