249 citations · 724 across the 7 of their papers we have counts for
7 papers
Influence of the black hole spin on the chaotic particle dynamics within a dipolar halo
Sankhasubhra Nag, Siddhartha Sinha, Deepika B. Ananda +1
We investigate the role of the spin angular momentum of astrophysical black holes in controlling the special relativistic chaotic dynamics of test particles moving under the influe…
Third post-Newtonian angular momentum flux and the secular evolution of orbital elements for inspiralling compact binaries in quasi-elliptical orbits
K. G. Arun, Luc Blanchet, Bala R. Iyer +1
The angular momentum flux from an inspiralling binary system of compact objects moving in quasi-elliptical orbits is computed at the third post-Newtonian (3PN) order using the mult…
Massive Black Hole Binary Inspirals: Results from the LISA Parameter Estimation Taskforce
K. G. Arun, Stas Babak, Emanuele Berti +14
The LISA Parameter Estimation (LISAPE) Taskforce was formed in September 2007 to provide the LISA Project with vetted codes, source distribution models, and results related to para…
LISA as a dark energy probe
K G Arun, Chandra Kant Mishra, Chris Van Den Broeck +3
Recently it was shown that the inclusion of higher signal harmonics in the inspiral signals of binary supermassive black holes (SMBH) leads to dramatic improvements in parameter es…
The third post-Newtonian gravitational wave polarisations and associated spherical harmonic modes for inspiralling compact binaries in quasi-circular orbits
Luc Blanchet, Guillaume Faye, Bala R. Iyer +1
The gravitational waveform (GWF) generated by inspiralling compact binaries moving in quasi-circular orbits is computed at the third post-Newtonian (3PN) approximation to general r…
Higher signal harmonics, LISA's angular resolution, and dark energy
K. G. Arun, Bala R. Iyer, B. S. Sathyaprakash +2
It is generally believed that the angular resolution of the Laser Interferometer Space Antenna (LISA) for binary supermassive black holes (SMBH) will not be good enough to identify…
Higher harmonics increase LISA's mass reach for supermassive black holes
K. G. Arun, Bala R. Iyer, B. S. Sathyaprakash +1
Current expectations on the signal to noise ratios and masses of supermassive black holes which the Laser Interferometer Space Antenna (LISA) can observe are based on using in matc…