arXiv Analytics

Sign in

arXiv:gr-qc/0209070AbstractReferencesReviewsResources

Thick domain walls around a black hole

Yoshiyuki Morisawa, Daisuke Ida, Akihiro Ishibashi, Ken-ichi Nakao

Published 2002-09-20, updated 2002-11-13Version 2

We discuss the gravitationally interacting system of a thick domain wall and a black hole. We numerically solve the scalar field equation in the Schwarzschild spacetime and obtain a sequence of static axi-symmetric solutions representing thick domain walls. We find that, for the walls near the horizon, the Nambu--Goto approximation is no longer valid.

Related articles: Most relevant | Search more
arXiv:0906.1442 [gr-qc] (Published 2009-06-08)
Is it possible to see the infinite future of the Universe when falling into a black hole?
arXiv:1306.5976 [gr-qc] (Published 2013-06-25, updated 2014-08-26)
An excision scheme for black holes in constrained evolution formulations: spherically symmetric case
arXiv:gr-qc/9404058 (Published 1994-04-28, updated 1994-06-21)
Aspects of the Thermo-Dynamics of a Black Hole with a Topological Defect