Quadrupolar power radiation by a binary system in de Sitter Background
  Cosmological observations over past couple of decades favor our universe with
a tiny positive cosmological constant. Presence of cosmological constant not
only imposes theoretical challenges in gravitational wave physics, it has also
observational relevance. Inclusion of cosmological constant in linearized
theory of gravitational waves modifies the power radiated quadrupole formula.
There are two types of observations which can be impacted by the modified
quadrupole formula. One is the orbital decay of an inspiraling binary and other
is the modification of the waveform at the detector. Modelling a compact binary
system in an elliptic orbit on de Sitter background we obtain energy and
angular momentum radiation due to emission of gravitational waves. We also
investigate evolution of orbital parameters under back reaction and its impact
on orbital decay rate. In the limit to circular orbit our result matches to
that obtained in ref. [26].
