Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
1996-10-15
Prog.Theor.Phys. 96 (1996) 901-916
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
13 pages, LaTeX, 15 figures, to appear in Prog. Theor. Phys. vol.96
Scientific paper
10.1143/PTP.96.901
We have calculated evolution of neutron star binaries towards the coalescence driven by gravitational radiation. The hydrodynamical effects as well as the general relativistic effects are important in the final phase. All corrections up to post$^{2.5}$-Newtonian order and the tidal effect are included in the orbital motion. The star is approximated by a simple Newtonian stellar model called affine star model. Stellar spins and angular momentum are assumed to be aligned. We have showed how the internal stellar structure affects the stellar deformation, variations of the spins, and the orbital motion of the binary just before the contact. The gravitational wave forms from the last a few revolutions significantly depend on the stellar structure.
Kojima Yasufumi
Ogawaguchi W.
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