Skewon field and cosmic wave propagation

被引:18
作者
Ni, Wei-Tou [1 ]
机构
[1] Natl Tsing Hua Univ, Dept Phys, Ctr Gravitat & Cosmol, Hsinchu 30013, Taiwan
关键词
Classical electrodynamics; Skewon field; General relativity; Equivalence principle; Dilaton field; Axion field; EQUIVALENCE PRINCIPLES;
D O I
10.1016/j.physleta.2014.02.039
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We study the propagation of the Hehl-Obukhov-Rubilar skewon field in weak gravity field/dilute matter or with weak violation of the Einstein Equivalence Principle (EEP), and further classify it into Type I and Type II skewons. From the dispersion relation we show that no dissipation/no amplification condition implies that the additional skewon field must be of Type II. For Type I skewon field, the dissipation/amplification is proportional to the frequency and the CMB spectrum would deviate from Planck spectrum. From the high precision agreement of the CMB spectrum with 2.755 K Planck spectrum, we constrain the Type I cosmic skewon field vertical bar(Skl)vertical bar chi(ijkl)vertical bar to <= a few x10(-35). The skewon part of constitutive tensor constructed from asymmetric metric is of Type II, hence it is allowed. This study may also be applied to macroscopic electrodynamics in the case of laser pumped medium or dissipative medium. (C) 2014 Elsevier B.V. All rights reserved.
引用
收藏
页码:1217 / 1223
页数:7
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