Cosmological bounds on the "millicharges" of mirror particles

被引:50
作者
Berezhiani, Zurab [2 ,3 ]
Lepidi, Angela [1 ,4 ]
机构
[1] Ist Nazl Fis Nucl, Sez Ferrara, I-44100 Ferrara, Italy
[2] Univ Aquila, I-67010 Laquila, Italy
[3] Ist Nazl Fis Nucl, Lab Nazl Gran Sasso, I-67010 Laquila, Italy
[4] Univ Ferrara, I-44100 Ferrara, Italy
关键词
DARK-MATTER; UNIFIED PICTURE; WORLD; PHYSICS; NUCLEOSYNTHESIS; DAMA/LIBRA; UNIVERSE;
D O I
10.1016/j.physletb.2009.10.023
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Mirror world. a parallel hidden sector with microphysics identical to ordinary particle physics, can have several interesting phenomenological and astrophysical implications and mirror matter can be a natural candidate for dark matter in the universe. If the ordinary and the mirror photons have a kinetic mixing due to the Lagrangian term (epsilon/2)F mu nu F'(mu nu) then mirror particles effectively acquire the electric charges similar to epsilon with respect to the ordinary photon, so that they become a sort of particles historically coined as millicharged" though nowadays they must be called more appropriately as "nanocharged". In this Letter we revise the cosmological bounds on the kinetic mixing parameter and in the case of exact mirror parity set an upper limit epsilon < 3 x 10(-10). Much weaker limit can be obtained in the case of asymmetric mirror sector, with an electroweak symmetry breaking scale larger than the ordinary electroweak scale. (C) 2009 Elsevier B.V. All rights reserved.
引用
收藏
页码:276 / 281
页数:6
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