Star spectroscopy in the constant B-field background

被引:10
作者
Chen, B
Lin, FL
机构
[1] Abdus Salam Int Ctr Theoret Phys, High Energy Sect, I-34014 Trieste, Italy
[2] Tamkang Univ, Dept Phys, Taipei 25137, Taiwan
关键词
D O I
10.1016/S0550-3213(02)00467-4
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
In this paper we calculate the spectrum of Neumann matrix with zero modes in the presence of the constant B-field in Witten's cubic string field theory. We find both the continuous spectrum inside [-1/3, 0) and the constraint on the existence of the discrete spectrum. For generic theta, -1/3 is not in the discrete spectrum but in the continuous spectrum. For each eigenvalue in the continuous spectrum there are four twist-definite degenerate eigenvectors except for -1/3 at which the degeneracy is two. However, for each twist-definite eigenvector the twist parity is opposite among the two spacetime components. Based upon the result at -1/3 we prove that the ratio of brane tension to be one as expected. Furthermore, we discuss the factorization of star algebra in the presence of B-field under the zero-slope limit and comment on the implications of our results to the recent proposed map of Witten's star to Moyal's star. (C) 2002 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:199 / 218
页数:20
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