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- W1505253265 abstract "As two neutron stars n a coalescing binary approach one another general relativistic and hydrodynamic effects become significant and dominate the evolution of the system. The gravitational wave forms become quite complex as the stars merge, however this complexity carries information about various aspects of the coalescing system such as the neutron star equation of state. This talk discusses the development of a fully general relativistic (3+1) dimensional hydrodynamics code to describe the evolution of a neutron-star binary system. The relativistic field equations are exactly solved at each time slice with a constraint that spatial 3-metric remains conformally flat. Against this exact solution to the general relativistic field equations, the hydrodynamic variables and gravitational radiation are allowed to respond. The effect of gravitational radiation is recovered by introducing an acceleration term in the matter evolution based upon a radiation reaction derived via a multipole expansion. We discuss the sensitivity of the emergent gravity wave signal to the underlying neutron star equation of state." @default.
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- W1505253265 date "1995-10-01" @default.
- W1505253265 modified "2023-09-24" @default.
- W1505253265 title "Neutron star equation of state and binary neutron star coalescence" @default.
- W1505253265 hasPublicationYear "1995" @default.
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