Effect of an Accretion Disk on the Gravitational Wave Signal from an Inspiralling Binary

Details Effect of an Accretion Disk on the Gravitational Wave Signal from an Inspiralling Binary Effect of an Accretion Disk on the Gravitational Wave Signal from an Inspiralling Binary

2000-12-29

arxiv.org/abs/astro-ph/0012529v1

Astronomy and Astrophysics

Astrophysics

World Scientific Style (Two pages)

Scientific paper

Since black holes can only accrete sub-Keplerian matter, a companion black hole orbiting on a circular and instantaneously Keplerian orbit around a central, massive black hole in a galactic Centre will loss angular momentum and energy to the accreting matter. This loss could be a significant fraction of the loss due to gravitational wave (GW) emission. The corresponding GW signal would be modified. We discuss this effects in the light of the modern accretion disk theory.

Affiliated with

Also associated with

No associations

Rating

Effect of an Accretion Disk on the Gravitational Wave Signal from an Inspiralling Binary 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 Effect of an Accretion Disk on the Gravitational Wave Signal from an Inspiralling Binary, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Effect of an Accretion Disk on the Gravitational Wave Signal from an Inspiralling Binary will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-233219