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CGWAS 2013: The compact binary inspiral Alan Weinstein, July 22, 2013 Consider a binary neutron star (BNS) system, composed of two neutron stars, each of mass 1.4 M , in a tight circular orbit around their common center
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Document Date: 2014-06-20 12:53:42


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potential and total energy / equal-mass systems / gravitational wave energy flux / kinetic energy / energy loss / gravitational potential energy / energy / /

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Alan Weinstein / /

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