Gravitational Waves From Inspiralling Compact Binaries : 3PN Polarisations, Angular Momentum Flux And Applications To Astrophysics And Cosmology
Binary systems comprising of compact objects like neutron stars (NS) and/or black holes (BH) lose their energy and angular momentum via gravitational waves (GW). Radiation reaction due to the emission of GW results in a gradual shrinking of the binary orbit and an accompanying gradual increase in th...
Main Author: | Sinha, Siddhartha |
---|---|
Other Authors: | Iyer, Bala R |
Language: | en_US |
Published: |
2010
|
Subjects: | |
Online Access: | http://hdl.handle.net/2005/853 |
Similar Items
-
On the Time Scales of Optical Variability of AGN and the Shape of Their Optical Emission Line Profiles
by: Edi Bon, et al.
Published: (2019-02-01) -
Gravitational Waves From Binary Black Hole Mergers: Modeling and Observations
by: Patricia Schmidt
Published: (2020-06-01) -
Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries
by: Blanchet Luc
Published: (2006-06-01) -
Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries
by: Luc Blanchet
Published: (2014-02-01) -
Observational Studies of Accretion Disks in Black Hole X-ray Binaries
by: Shidatsu, Megumi
Published: (2015)