新型非临界宇宙弦构型的Wilson重整化群性质
高能物理 - 理论
2007-05-23 v3 广义相对论与量子宇宙学
高能物理 - 唯象学
摘要
我们证明了在文献[1]中发现的精确的非临界弦宇宙学膨胀子和引力子背景构型,构成了精确Wilson重整化群方程的红外稳定不动点。
引用
@article{arxiv.hep-th/0602232,
title = {Wilsonian renormalization group properties of a novel non-critical cosmological string configuration},
author = {J. Alexandre and N. E. Mavromatos},
journal= {arXiv preprint arXiv:hep-th/0602232},
year = {2007}
}
备注
Talk presented at the University of Southampton, Department of Physics and Astronomy, September 2005