scholarly journals Search for TeV transients from Coalescing Binary systems discovered in Gravity Waves by LIGO/Virgo.

2018 ◽  
Author(s):  
Andrew Smith
1998 ◽  
Vol 11 (1) ◽  
pp. 398-398
Author(s):  
Kenji Tanabe

Propagation of the surface waves of the lobe-filing components of close binary systems is investigated theoretically. Such waves are considered to be analogous to the gravity waves of water on the earth. As a result, the equations of the surface wave in the rotating frame of reference are reduced to the so-called Kortewegde Vries (KdV) equation and non-linear Schroedinger (NLS) equation according to its ”depth”. Each of these equations is known to have the solution of soliton. When this soliton is sent to the other component of the binary system through the Lagrangian point, it can give rise to the flare activity observed in some kinds of close binary systems.


1992 ◽  
Vol 9 (9) ◽  
pp. L125-L131 ◽  
Author(s):  
L E Kidder ◽  
C M Will ◽  
A G Wiseman

2011 ◽  
Vol 333 (1) ◽  
pp. 29-35 ◽  
Author(s):  
S. Capozziello ◽  
M. De Laurentis ◽  
I. De Martino ◽  
M. Formisano ◽  
D. Vernieri

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

2010 ◽  
Vol 332 (1) ◽  
pp. 31-35 ◽  
Author(s):  
S. Capozziello ◽  
M. De Laurentis ◽  
I. De Martino ◽  
M. Formisano

2010 ◽  
Vol 19 (14) ◽  
pp. 2295-2298 ◽  
Author(s):  
M. D. MAIA

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.


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