Interacting black holes on the brane: the seeding of binaries

Details Interacting black holes on the brane: the seeding of binaries Interacting black holes on the brane: the seeding of binaries

2003-11-06

arxiv.org/abs/astro-ph/0311148v3

Phys.Lett. B607 (2005) 219-224

Astronomy and Astrophysics

Astrophysics

5 pages, LaTex, discussion of binary parameters in terms of mass differences, references updated, accepted for publication in

Scientific paper

10.1016/j.physletb.2004.12.059

We consider the evolution of sub-horizon-sized black holes which are formed during the high energy phase of the braneworld scenario. These black holes are long-lived due to modified evaporation and accretion of radiation during the radiation dominated era. We argue that an initial mass difference between any two neighbouring black holes is always amplified because of their exchange of energy with the surrounding radiation. We present a scheme of binary formation based on mass differences suggesting that such a scenario could lead to binaries with observable signatures.

Affiliated with

Also associated with

No associations

Rating

Interacting black holes on the brane: the seeding of binaries 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 Interacting black holes on the brane: the seeding of binaries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Interacting black holes on the brane: the seeding of binaries will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-518986