Constraining the neutron star equation of state with gravitational wave signals from coalescing binary neutron stars

Constraining the neutron star equation of state with gravitational wave signals from coalescing binary neutron stars

Recently exploratory studies were performed on the possibility of constraining the neutron star equation of state (EOS) using signals from coalescing binary neutron stars, or neutron star–black hole systems, as they will be seen in upcoming advanced gravitational wave detectors such as Advanced LIGO...

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Bibliographic Details
Main Authors: Agathos, M., Meidam, J., Del Pozzo, W., Li, T. G. F., Tompitak, M., Veitch, J., Van Den Broeck, C., Vitale, Salvatore
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:English
Published: American Physical Society 2015
Online Access:http://hdl.handle.net/1721.1/97910
https://orcid.org/0000-0003-2700-0767

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http://hdl.handle.net/1721.1/97910
https://orcid.org/0000-0003-2700-0767

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