Elsevier

Nuclear Physics B

Volume 293, 1987, Pages 189-214
Nuclear Physics B

Three-reggeon light-cone vertex of the Neveu-Schwarz string

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Abstract

We construct in the superfield formalism the vertex operator corresponding to the most general physical state of the Neveu-Schwarz model. These vertex operators are then used to compute the on-shell three-reggeon vertex.

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Cited by (27)

  • String coherent vertex operators of Neveu-Schwarz and Ramond states

    2020, Nuclear Physics B
    Citation Excerpt :

    Some work regarding the study of the physical spectrum has been done also in the case of non critical strings, both bosonic and fermionic, and also for the massive string [18–21]. The power of the DDF operators emerges also in the computation of string scattering amplitudes such as in the work [22] for the representation of multistates scattering amplitudes in bosonic string, [23,24] for the explicit computation of three-point amplitude of arbitrarily massive states still in bosonic string and [25] for the generalization of the three-point amplitude in the Neveu-Schwartz model. Finally recent progress, using different contextualizations of the DDF operators, has been done in [26] for the decay of macroscopic strings and in [27] for the computation of three and four-point scattering amplitudes involving the open bosonic coherent states constructed in [16,17] finding a new saddle point in the Veneziano-like amplitudes.

  • DDF operators, open string coherent states and their scattering amplitudes

    2020, Nuclear Physics B
    Citation Excerpt :

    A possible way out is to rely on the time-honoured Del Giudice, Di Vecchia and Fubini (DDF) operators [71,72], that produce BRST invariant states by construction. Three-point amplitudes have been studied and the three-Reggeon Vertex has been derived for bosonic strings [73,74] as well as for the Neveu-Schwarz sector of the superstring [75]. In the past ten years or so, the DDF approach and the construction of macroscopic ‘coherent’ states of strings has been revived in connection with cosmic strings,1 [77–79], including applications to the decay of macroscopic strings [80] and to the generating function for highly excited strings [81].

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