English

Scattering of Straight Cosmic Strings by Black Holes: Weak Field Approximation

General Relativity and Quantum Cosmology 2009-10-31 v1

Abstract

The scattering of a straight, infinitely long string moving with velocity vv by a black hole is considered. We analyze the weak-field case, where the impact parameter (bimpb_{imp}) is large, and obtain exact solutions to the equations of motion. As a result of scattering, the string is displaced in the direction perpendicular to the velocity by an amount Δb2πGMvγ/c3π(GM)2/(4c3vbimp)\Delta b\sim -2\pi GMv\gamma/c^3 -\pi (GM)^2/ (4c^3 v b_{imp}), where γ=(1(v/c)2)1/2\gamma=(1-(v/c)^2)^{-1/2}. The second term dominates at low velocities v/c<(GM/bimp)1/2v/c<(GM/b_{imp})^{1/2} . The late-time solution is represented by a kink and anti-kink, propagating in opposite directions at the speed of light, and leaving behind them the string in a new ``phase''. The solutions are applied to the problem of string capture, and are compared to numerical results.

Keywords

Cite

@article{arxiv.gr-qc/9804087,
  title  = {Scattering of Straight Cosmic Strings by Black Holes: Weak Field Approximation},
  author = {Jean-Pierre De Villiers and Valeri Frolov},
  journal= {arXiv preprint arXiv:gr-qc/9804087},
  year   = {2009}
}

Comments

19 pages, 5 figures