旋转中子星外场的精确解
广义相对论与量子宇宙学
2009-12-30 v1 天体物理学
摘要
给出一类四参数、仅含有理函数的 Einstein-Maxwell 方程的精确渐近平直解。它能够描述具有极向磁场的慢速或快速旋转中子星的外场。
引用
@article{arxiv.gr-qc/0001081,
title = {Exact Solution for the Exterior Field of a Rotating Neutron Star},
author = {Vladimir S. Manko and Eckehard W. Mielke and José D. Sanabria-Gómez},
journal= {arXiv preprint arXiv:gr-qc/0001081},
year = {2009}
}
备注
Accepted for publication in Phys. Rev. D as Rapid Communication. 8 pages, 2 eps figures