Correspondence of I- and Q-balls as non-relativistic condensates
被引:12
|
作者:
Mukaida, Kyohei
论文数: 0引用数: 0
h-index: 0
机构:
Univ Tokyo, Dept Phys, Fac Sci, Bunkyo Ku, Tokyo 1330033, JapanUniv Tokyo, Dept Phys, Fac Sci, Bunkyo Ku, Tokyo 1330033, Japan
Mukaida, Kyohei
[1
]
Takimoto, Masahiro
论文数: 0引用数: 0
h-index: 0
机构:
Univ Tokyo, Dept Phys, Fac Sci, Bunkyo Ku, Tokyo 1330033, JapanUniv Tokyo, Dept Phys, Fac Sci, Bunkyo Ku, Tokyo 1330033, Japan
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.