HOW DISORIENTED CHIRAL CONDENSATES FORM - QUENCHING VERSUS ANNEALING

被引:100
作者
ASAKAWA, M [1 ]
HUANG, Z [1 ]
WANG, XN [1 ]
机构
[1] UNIV CALIF BERKELEY, LAWRENCE BERKELEY LAB, THEORET PHYS GRP, BERKELEY, CA 94720 USA
关键词
D O I
10.1103/PhysRevLett.74.3126
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We demonstrate that fluctuations, their relaxation, and the chiral phase transition are automatically incorporated in the numerical simulations of the classical equations of motion in the linear model when longitudinal and transverse expansions are included. We find that domains of disoriented chiral condensate with 45 fm in size can form through a quench while an annealing leads to domains of smaller sizes. We also demonstrate that quenching cannot be achieved by relaxing a chirally symmetric system through expansion. © 1995 The American Physical Society.
引用
收藏
页码:3126 / 3129
页数:4
相关论文
共 13 条
[1]  
Lattes C.M.G., Fujimoto Y., Hasegawa S., Hadronic interactions of high energy cosmic-ray observed by emulsion chambers, Physics Reports, 65, (1980)
[2]  
Anselm A.A., Ryskin M.G., Phys. Lett. B, 266, (1991)
[3]  
Blaizot J.-P., Krzywcki A., Phys. Rev. D, 46, (1992)
[4]  
Bjorken J.D., Kowalski K.L., Taylor C.C.
[5]  
Rajagopal K., Wilczek F., Nucl. Phys., 399 B, (1992)
[6]  
Rajagopal K., Wilczek F., Nucl. Phys., 404 B, (1993)
[7]  
Gavin S., Gocksch A., Pisarski R.D., Phys. Rev. Lett., 72, (1994)
[8]  
Huang Z., Wang X.-N., Phys. Rev. D, 49, (1994)
[9]  
Gavin S., Muller B., Phys. Lett., 329 B, (1994)
[10]  
Boyanovsky D., de Vega H.J., Holman R., Phys. Rev. D, 51, (1995)