论马赫宇宙中的磁场与熵增
综合物理
2007-05-23 v2
摘要
通过背景微波辐射能量与星际磁场能量之间当前均分的实验结果，并推进一个马赫关系的磁场，该关系与其他作者的论文不同，适用于宇宙的整个寿命，意味着磁场依赖于宇宙半径的倒数，我们得到了一个通用公式，使得B依赖于R的倒数。我们对普朗克磁场的估计是Sabbata和Sivaram估计的千分之一。结果表明，上述问题中涉及的能量密度依赖于R的平方倒数。对于辐射，这暗示着，正如我们所展示的，宇宙的总熵随膨胀而增加。特别地，我们表明R依赖于T的平方倒数，其中T是绝对温度，熵与R的3/2次方成正比。
引用
@article{arxiv.physics/0611007,
title = {On the Magnetic Field, and Entropy Increase, in a Machian Universe},
author = {Marcelo Samuel Berman},
journal= {arXiv preprint arXiv:physics/0611007},
year = {2007}
}
备注
6 pages including front cover. Submitted. In v.2, minor corrections have been made, while pointing that, in the adopted formalism, each form of energy, which contributes to the total energy of the Universe, when taken as fractions of the energy M, (c=1) remain constant in time, for the whole history of the Universe; this is of course also true for the lambda-driven Universe as found experimentaly by A.Riess and colaborators