Astronomy and Astrophysics – Astronomy
Scientific paper
Aug 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989nascp3046...14w&link_type=abstract
In NASA, Relativistic Gravitational Experiments in Space p 14-17 (SEE N90-19940 12-90)
Astronomy and Astrophysics
Astronomy
1
Black Holes (Astronomy), Gravitational Waves, Radiation Measurement, Radiation Sources, X Ray Binaries, Galactic Nuclei, Gravity Waves, Neutron Stars, Polarization (Waves), Signal To Noise Ratios, White Dwarf Stars
Scientific paper
One of the most attractive possible sources of strong gravitational waves would be a binary system comprising massive black holes (BH). The gravitational radiation from a binary is an elliptically polarized, periodic wave which could be observed continuously - or at intervals whenever a detector was available. This continuity of the signal is certainly appealing compared to waiting for individual pulses from infrequent random events. It also has the advantage over pulses that continued observation can increase the signal-to-noise ratio almost indefinitely. Furthermore, this system is dynamically simple; the theory of the generation of the radiation is unambiguous; all characteristics of the signal can be precisely related to the dynamical parameters of the source. The current situation is that while there is no observational evidence as yet for the existence of massive binary BH, their formation is theoretically plausible, and within certain coupled constraints of mass and location, their existence cannot be observationally excluded. Detecting gravitational waves from these objects might be the first observational proof of their existence.
No associations
LandOfFree
Detecting gravity waves from binary black holes does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Detecting gravity waves from binary black holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detecting gravity waves from binary black holes will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1519642