Correspondence of I- and Q-balls as non-relativistic condensates

被引:12
|
作者
Mukaida, Kyohei [1 ]
Takimoto, Masahiro [1 ]
机构
[1] Univ Tokyo, Dept Phys, Fac Sci, Bunkyo Ku, Tokyo 1330033, Japan
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2014年 / 08期
关键词
physics of the early universe; cosmological phase transitions; inflation; INFLATIONARY UNIVERSE; CONFIGURATIONS; BARYOGENESIS; FLATNESS; HORIZON;
D O I
10.1088/1475-7516/2014/08/051
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
If a real scalar field is dominated by non-relativistic modes, then it approximately conserves its particle number and obeys an equation that governs a complex scalar field theory with a conserved global U(1) symmetry. From this fact, it is shown that the I-ball (oscillon) can be naturally understood as a projection (e.g., real part) of the non-relativistic Q-ball solution. In particular, we clarify that the stability of the I-ball is guaranteed by the U(1) symmetry in the corresponding complex scalar field theory as long as the non-relativistic condition holds. We also discuss the longevity of I-ball from the perspective of the complex scalar field in terms of U(1) charge violating processes.
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页数:16
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