Gauged Q-stars

CHENG Hong-Bo

Chinese Physics C> 1991, Vol. 15> Issue(11) : 991-996

Gauged Q-stars

CHENG Hong-Bo ^,

Department of Physics,Shanghai Jiao Tong University,Shanghai 200030

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Abstract：
We derive the theory about gauged non-topological soliton stars and their black holes,and find that the gauged Q-stars with maximum particle number Q_max in a definite range of mass are cold, stable and in coherent states of very large mass.Their characteristics are similar to those of general soliton stars.When Q>Q_max,the gauged Q-stars are not stable.

References

[1]

倪致祥, 李新洲, 高能物理与核物理, 15(1991), 92,[2] X. Shi, X. Li, Phys. Rev., D42(1990), 2035.[3] X. Shi, X. Li, Phys. Rev., D42(1990), 2144.[4] X. Shi, X. Li, Class. Quantan Gravity, 8(1991), 280.[5] S. Colemann, Nucl. Phys., B262(85), 263.[6] Kimyeong Lee, Jaime A. Stein-Schabes, Richard Watkins, Lawrence M. Widrow, Phys. Rev., D39(1989), 1665.[7] T. D. Lee, Ph ys, Rev.,D35(1987),3637.[8] R. Friedberg, T. D. Lee, Y. Pang,Phys. Rev., D35(1987), 3640[9] R. Friedberg, T. D. Lee, Y. Pang,Phys. Rev., D35(1987), 3658.[10] Moshe Carmeli, Classical Fields; General Relativity and Gauge Theory, A Wiley-Interscience Publication John WileySans, 1982.

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CHENG Hong-Bo. Gauged Q-stars[J]. Chinese Physics C, 1991, 15(11): 991-996.

CHENG Hong-Bo. Gauged Q-stars[J]. Chinese Physics C, 1991, 15(11): 991-996. shu

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Received: 1900-01-01
Revised: 1900-01-01

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沈阳化工大学材料科学与工程学院沈阳 110142

Gauged Q-stars

CHENG Hong-Bo ^,

Corresponding author: CHENG Hong-Bo,

Department of Physics,Shanghai Jiao Tong University,Shanghai 200030

Received Date: 1900-01-01
Accepted Date: 1900-01-01
Available Online: 1991-11-05

Abstract: We derive the theory about gauged non-topological soliton stars and their black holes,and find that the gauged Q-stars with maximum particle number Q_max in a definite range of mass are cold, stable and in coherent states of very large mass.Their characteristics are similar to those of general soliton stars.When Q>Q_max,the gauged Q-stars are not stable.