On-brane data for braneworld stars
高能物理 - 理论
2009-11-07 v2 天体物理学
广义相对论与量子宇宙学
摘要
Stellar structure in braneworlds is markedly different from that in ordinary general relativity. As an indispensable first step towards a more general analysis, we completely solve the ``on brane'' 4-dimensional Gauss and Codazzi equations for an arbitrary static spherically symmetric star in a Randall--Sundrum type II braneworld. We then indicate how this on-brane boundary data should be propagated into the bulk in order to determine the full 5-dimensional spacetime geometry. Finally, we demonstrate how this procedure can be generalized to solid objects such as planets.
引用
@article{arxiv.hep-th/0212333,
title = {On-brane data for braneworld stars},
author = {Matt Visser and David L. Wiltshire},
journal= {arXiv preprint arXiv:hep-th/0212333},
year = {2009}
}
备注
5 pages, RevTeX4, v2: Main algorithm and results substantially simplified, further discussion and references added