Spinning Up Asymptotically Flat Spacetimes

E. N. Glass; J. P. Krisch

doi:10.1088/0264-9381/21/23/015

Spinning Up Asymptotically Flat Spacetimes

广义相对论与量子宇宙学 2010-11-19 v1

作者: E. N. Glass , J. P. Krisch

在 arXiv 上查看 ↗ PDF ↗ DOI ↗

摘要

We present a method for constructing stationary, asymptotically flat, rotating solutions of Einstein's field equations. One of the spun-up solutions has quasilocal mass but no global mass. It has an ergosphere but no event horizon. The angular momentum is constant everywhere beyond the ergosphere. The energy-momentum content of this solution can be interpreted as a rotating string-fluid.

关键词

static spherically symmetric solutions in general relativity general relativity perfect fluids in general relativity

引用

@article{arxiv.gr-qc/0410089,
  title  = {Spinning Up Asymptotically Flat Spacetimes},
  author = {E. N. Glass and J. P. Krisch},
  journal= {arXiv preprint arXiv:gr-qc/0410089},
  year   = {2010}
}

备注

Class. Quantum Grav. (to appear)

相关论文

查看更多相关论文 →