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Winding Number in String Field Theory

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arxiv 1111.2389 v2 pith:5KPC7UXI submitted 2011-11-10 hep-th

classification hep-th
keywords regularizationcsfttheoryfieldnumberstringvaluewinding
verification ladder T0 review T1 audit T2 compute T3 formal

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Motivated by the similarity between cubic string field theory (CSFT) and the Chern-Simons theory in three dimensions, we study the possibility of interpreting N=(\pi^2/3)\int(U Q_B U^{-1})^3 as a kind of winding number in CSFT taking quantized values. In particular, we focus on the expression of N as the integration of a BRST-exact quantity, N=\int Q_B A, which vanishes identically in naive treatments. For realizing non-trivial N, we need a regularization for divergences from the zero eigenvalue of the operator K in the KBc algebra. This regularization must at same time violate the BRST-exactness of the integrand of N. By adopting the regularization of shifting K by a positive infinitesimal, we obtain the desired value N[(U_tv)^{\pm 1}]=\mp 1 for U_tv corresponding to the tachyon vacuum. However, we find that N[(U_tv)^{\pm 2}] differs from \mp 2, the value expected from the additive law of N. This result may be understood from the fact that \Psi=U Q_B U^{-1} with U=(U_tv)^{\pm 2} does not satisfy the CSFT EOM in the strong sense and hence is not truly a pure-gauge in our regularization.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Deriving on-shell open string field amplitudes without using Feynman rules

    hep-th 2019-08 conditional novelty 7.0 of 10

    New gauge-invariant functionals of the open string field are shown to reproduce on-shell tree-level amplitudes around known D-brane backgrounds without using Feynman rules.

  2. Bernoulli Numbers and Multi-brane Solutions in Cubic String Field Theory

    hep-th 2019-08 conditional novelty 6.0 of 10

    The parameters alpha_k of the proposed (N+1)-brane solutions in cubic string field theory are expressed in closed form using Bernoulli numbers for a generic N.

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