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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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GM /
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IndustryTerm
potential and total energy /
equal-mass systems /
gravitational wave energy flux /
kinetic energy /
energy loss /
gravitational potential energy /
energy /
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Person
Alan Weinstein /
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Astrodynamics
Conservation laws
Physical quantities
Gravitational wave
Orbit
Circular orbit
Kinetic energy
Angular momentum
Momentum
Physics