Three dimensional strings. I. Classical theory

dc.creatorRamos, Eduardo
dc.date1997-03-17
dc.date1997-04-03
dc.date.accessioned2026-07-07T09:08:14Z
dc.date.available2026-07-07T09:08:14Z
dc.descriptionI consider a three-dimensional string theory whose action, besides the standard area term, contains one of the form $\int_Σ ε_{μνσ} X^μ d X^ν \wedge d X^σ$. In the case of closed strings this extra term has a simple geometrical interpretation as the volume enclosed by the surface. The associated variational problem yields as solutions constant mean curvature surfaces. One may then show the equivalence of this equation of motion to that of an SU(2) principal chiral model coupled to gravity. It is also possible by means of the Kemmotsu representation theorem, restricted to constant curvature surfaces, to map the solution space of the string model into the one of the $CP^1$ nonlinear sigma model. I also show how a description of the Gauss map of the surface in terms of SU(2) spinors allows for yet a different description of this result by means of a Gross-Neveu spinorial model coupled to 2-D gravity. The standard three-dimensional string equations can also be recovered by setting the current-current coupling to zero.
dc.description15 pages, LaTeX (elsart macros), I drop a conjecture about the quantization of the model that now seems unwarranted. This does not alter the results of the paper. A few misprints are also corrected
dc.identifierhttps://arxiv.org/abs/hep-th/9703117
dc.identifierhttp://arxiv.org/abs/hep-th/9703117
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/150650
dc.subjectHigh Energy Physics - Theory
dc.titleThree dimensional strings. I. Classical theory
dc.typetext

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