Light-front quantized Chiral Schwinger model and its vacuum structure

被引:14
|
作者
Srivastava, PP [1 ]
机构
[1] Stanford Univ, Stanford Linear Accelerator Ctr, Stanford, CA 94309 USA
关键词
D O I
10.1016/S0370-2693(99)00036-2
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The bosonized Chiral Schwinger model (CSM) is quantized on the Light-front (LF). The physical Hilbert space of CSM is obtained directly once the constraints on the LF phase space are eliminated. The discussion of the degenerate vacua and the absence in the CSM of the theta-vacua, as found in the Schwinger model (SM), becomes straightforward. The differences in the structures of the the mass excitations and the vacua in these gauge theories are displayed transparently. The procedure followed is the one used successfully in the previous works for describing the spontaneous symmetry breaking (SSB) and the SM on the LF. The physical contents following from the LF quantized theory agree with those known in the conventional treatment. The LF hyperplane is argued to be equally appropriate as the conventional equal-time one for the canonical quantization. Some comments on the irrelevance, in quantized field theory, of the fact that the hyperplanes x (+/-)= 0 constitute characteristic surfaces of hyperbolic partial differential equation are also made. (C) 1999 Published by Elsevier Science B.V. All rights reserved.
引用
收藏
页码:68 / 75
页数:8
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