Light propagation in a background field for time-space non-commutativity and axionic non-commutative QED

被引:12
|
作者
Chatillon, N. [1 ]
Pinzul, A. [1 ]
机构
[1] Syracuse Univ, Dept Phys, Syracuse, NY 13244 USA
基金
美国国家科学基金会;
关键词
D O I
10.1016/j.nuclphysb.2006.12.003
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We study the low-energy effects of space-time non-commutativity on light propagation in a background electromagnetic field. Contrary to some of the previous claims, we find no polarization rotation for vanishing time-space commutator [(x) over cap (i), (x) over cap (0)] = 0, although dispersion relation is modified, allowing for propagation faster than the vacuum speed of light. For non-zero [(x) over cap (i), (x) over cap (0)], as allowed with a proper quantization, a naive rotation effect is found to be actually absent when physical fields are defined through Seiberg-Witten map. We also consider non-commutative QED weakly coupled to small mass particles such as axions. Non-commutativity is found to dominate the inverse oscillation length, compared to axion mass and QED effects, for mixing particle masses smaller than 10(-12) eV. Conventional constraints on axion coupling based on photon-axion transition rates are unmodified, however induced ellipticity is proportional to the non-commutativity squared length scale. This last effect is found to be too small to account for the ellipticity reported by the PVLAS experiment, yet unexplained by conventional QED or axion physics. (c) 2007 Elsevier B.V. All rights reserved.
引用
收藏
页码:95 / 108
页数:14
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