Coalescing binary systems of compact objects to(post)5/2-Newtonian order: Late-time evolution and gravitational-radiation emission

1990 ◽  
Vol 42 (4) ◽  
pp. 1123-1143 ◽  
Author(s):  
Craig W. Lincoln ◽  
Clifford M. Will
Keyword(s):  
Time Evolution ◽  
Gravitational Radiation ◽  
Binary Systems ◽  
Compact Objects ◽  
Late Time ◽  
Radiation Emission ◽  
Coalescing Binary Systems

Innermost stable orbits for coalescing binary systems of compact objects

1992 ◽  
Vol 9 (9) ◽  
pp. L125-L131 ◽  
Author(s):  
L E Kidder ◽  
C M Will ◽  
A G Wiseman
Keyword(s):  
Binary Systems ◽  
Compact Objects ◽  
Coalescing Binary Systems

Coalescing Binary Systems of Compact Objects to (Post)5/2-Newtonian Order

1991 ◽  
Vol 631 (1 Nonlinear Pro) ◽  
pp. 126-136 ◽  
Author(s):  
CLIFFORD M. WILL ◽  
CRAIG W. LINCOLN ◽  
ALAN G. WISEMAN
Keyword(s):  
Binary Systems ◽  
Compact Objects ◽  
Coalescing Binary Systems

scholarly journals GRAVITATIONAL WAVES FROM COALESCING BINARY SOURCES

2010 ◽  
Vol 19 (14) ◽  
pp. 2295-2298 ◽  
Author(s):  
M. D. MAIA
Keyword(s):  
Gravitational Waves ◽  
Gravitational Radiation ◽  
Theoretical Basis ◽  
Binary Systems ◽  
Translational Symmetry ◽  
Axially Symmetric ◽  
Poincaré Symmetry ◽  
Group Of Isometries ◽  
Coalescing Binary Systems ◽  
Binary Sources

Coalescing binary systems (e.g. pulsars, neutron stars and black holes) are currently considered to be the most likely sources of gravitational radiation, yet to be detected on or near Earth, where the local gravitational field is negligible and the Poincaré symmetry rules. On the other hand, the general theory of gravitational waves emitted by axially symmetric rotating sources predicts the existence of a nonvanishing news function. The existence of such function implies that, for a distant observer, the asymptotic group of isometries, the BMS group, has a translational symmetry that depends on the orbit periodicity of the source, thus breaking the isotropy of the Poincaré translations. These results suggest that the asymptotic BMS-covariant wave equation should be applied to obtain a proper theoretical basis for the gravitational waves observations from those binary sources.

scholarly journals Coalescing Binary Systems of Compact Objects: Dynamics of Angular Momenta

1998 ◽  
Vol 507 (1) ◽  
pp. 287-299 ◽  
Author(s):  
Carlo Del Noce ◽  
Giovanni Preti ◽  
Fernando de Felice
Keyword(s):  
Binary Systems ◽  
Compact Objects ◽  
Angular Momenta ◽  
Coalescing Binary Systems

Coalescing binary systems of compact objects to(post)52-Newtonian order. III. Transition from inspiral to plunge

1993 ◽  
Vol 47 (8) ◽  
pp. 3281-3291 ◽  
Author(s):  
Lawrence E. Kidder ◽  
Clifford M. Will ◽  
Alan G. Wiseman
Keyword(s):  
Binary Systems ◽  
Compact Objects ◽  
Coalescing Binary Systems
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