A Scenario for Strong Gravity without Extra Dimensions
高能物理 - 理论
2007-05-23 v1 广义相对论与量子宇宙学
摘要
A different reason for the apparent weakness of the gravitational interaction is advanced, and its consequences for Hawking evaporation of a Schwarzschild black hole are investigated. A simple analytical formulation predicts that evaporating black holes will undergo a type of phase transition resulting in variously long-lived objects of reasonable sizes, with normal thermodynamic properties and inherent duality characteristics. Speculations on the implications for particle physics and for some recently-advanced new paradigms are explored.
引用
@article{arxiv.hep-th/0602183,
title = {A Scenario for Strong Gravity without Extra Dimensions},
author = {D. G. Coyne},
journal= {arXiv preprint arXiv:hep-th/0602183},
year = {2007}
}
备注
49 pages, 13 figures, pdf. For a high resolution file contact me at [email protected]