Integrals of periodic motion and periodic solutions for classical equations of relativistic string with masses at ends. I. Integrals of periodic motion

dc.creatorBarbashov, B. M.
dc.date1996-09-20
dc.date.accessioned2026-07-07T10:58:47Z
dc.date.available2026-07-07T10:58:47Z
dc.descriptionBoundary equations for the relativistic string with masses at ends are formulated in terms of geometrical invariants of world trajectories of masses at the string ends. In the three--dimensional Minkowski space $E^1_2$, there are two invariants of that sort, the curvature $K$ and torsion $κ$. Curvatures of trajectories of the string ends with masses are always constant, $K_i = γ/m_i (i =1,2,)$, whereas torsions $κ_i(τ)$ obey a system of differential equations with deviating arguments. For these equations with periodic $κ_i(τ+n l)=κ(τ)$, constants of motion are obtained (part I) and exact solutions are presented (part II) for periods $l$ and $2l$ where $l$ is the string length in the plane of parameters $τ$ and $σ\ (σ_1 = 0, σ_2 =l)$.
dc.description15 pages
dc.identifierhttps://arxiv.org/abs/hep-th/9609171
dc.identifierhttp://arxiv.org/abs/hep-th/9609171
dc.identifierJ.Phys.A30:4651-4664,1997
dc.identifierdoi:10.1088/0305-4470/30/13/016
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/187226
dc.subjectHigh Energy Physics - Theory
dc.titleIntegrals of periodic motion and periodic solutions for classical equations of relativistic string with masses at ends. I. Integrals of periodic motion
dc.typetext

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